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1

Red fluorescent proteins: chromophore formation and cellular applications  

E-Print Network [OSTI]

Red fluorescent proteins: chromophore formation and cellular applications Atsushi Miyawaki1,2 , Daria M Shcherbakova3,4 and Vladislav V Verkhusha3,4 In the last decade, a number of red fluorescent proteins (RFPs) that emit orange, red, and far-red fluorescence have been isolated from anthozoans (corals

Verkhusha, Vladislav V.

2

Measurement of the ratio of branching fractions {ital B}({ital D}{sup 0}{r_arrow}{pi}{sup {minus}}{ital e}{sup +}{nu}{sub {ital e}})/{ital B}({ital D}{sup 0}{r_arrow}{ital K}{sup {minus}}{ital e}{sup +}{nu}{sub {ital e}})  

SciTech Connect (OSTI)

Using 3.0 fb{sup {minus}1} of data collected with the CLEO-II detector, we study the Cabibbo-suppressed decay {ital D}{sup 0}{r_arrow}{pi}{sup {minus}}{ital e}{sup +}{nu}{sub {ital e}}. The ratio of the branching fractions {ital B}({ital D}{sup 0}{r_arrow}{pi}{sup {minus}}{ital e}{sup +}{nu}{sub {ital e}})/{ital B}({ital D}{sup 0}{r_arrow}{ital K}{sup {minus}}{ital e}{sup +}{nu}{sub {ital e}}) is measured to be (10.3{plus_minus}3.9{plus_minus}1.3)%, corresponding to an upper limit of 15.6% at the 90% confidence level.

Butler, F.; Fu, X.; Nemati, B.; Ross, W.R.; Skubic, P.; Wood, M.; Bishai, M.; Fast, J.; Gerndt, E.; Hinson, J.W.; McIlwain, R.L.; Miao, T.; Miller, D.H.; Modesitt, M.; Payne, D.; Shibata, E.I.; Shipsey, I.P.J.; Wang, P.N.; Gibbons, L.; Kwon, Y.; Roberts, S.; Thorndike, E.H.; Coan, T.E.; Dominick, J.; Fadeyev, V.; Korolkov, I.; Lambrecht, M.; Sanghera, S.; Shelkov, V.; Skwarnicki, T.; Stroynowski, R.; Volobouev, I.; Wei, G.; Artuso, M.; Gao, M.; Goldberg, M.; He, D.; Horwitz, N.; Moneti, G.C.; Mountain, R.; Muheim, F.; Mukhin, Y.; Playfer, S.; Rozen, Y.; Stone, S.; Xing, X.; Zhu, G.; Bartelt, J.; Csorna, S.E.; Egyed, Z.; Jain, V.; Gibaut, D.; Kinoshita, K.; Pomianowski, P.; Barish, B.; Chadha, M.; Chan, S.; Cowen, D.F.; Eigen, G.; Miller, J.S.; O`Grady, C.; Urheim, J.; Weinstein, A.J.; Wuerthwein, F.; Asner, D.M.; Athanas, M.; Bliss, D.W.; Brower, W.S.; Masek, G.; Paar, H.P.; Gronberg, J.; Korte, C.M.; Kutschke, R.; Menary, S.; Morrison, R.J.; Nakanishi, S.; Nelson, H.N.; Nelson, T.K.; Qiao, C.; Richman, J.D.; Roberts, D.; Ryd, A.; Tajima, H.; Witherell, M.S.; Balest, R.; Cho, K.; Ford, W.T.; Lohner, M.; Park, H.; Rankin, P.; Smith, J.G.; Alexander, J.P.; Bebek, C.; Berger, B.E.; Berkelman, K.; Bloom, K.; Browder, T.E.; Cassel, D.G.; Cho, H.A.; Coffman, D.M.; Crowcroft, D.S.; Dickson, M.; Drell, P.S.; Dumas, D.J.; Ehrlich, R.; Elia, R.; Gaidarev, P.; Garcia-Sciveres, M.; Gittelman, B.; Gray, S.W.; Hartill, D.L.; Heltsley, B.K.; Henderson, S.; Jones, C.D.; Jones, S.L.; Kandaswamy, J.; Katayama, N.; Kim, P.C.; Kreinick, D.L.; Liu, Y.; Ludwig, G.S.; Masui, J.; Mevissen, J.; Mistry, N.B.; Ng, C.R.; Nordberg, E.; Patterson, J.R.; Peterson, D.; Riley, D.; Soffer, A.; Avery, P.; Freyberger, A.; Lingel, K.; Rodriguez, J.; Yang, S.; Yelton, J.; Brandenburg, G.; Cinabro, D.; Liu, T.; Saulnier, M.; Wilson, R.; Yamamoto, H.; Bergfeld, T.; Eisenstein, B.I.; Ernst, J.; Gladding, G.E.; Gollin, G.D.; Palmer, M.; Selen, M.; Thaler, J.J.; Edwards, K.W.; McLean, K.W.; (CLEO Collabor..

1995-09-01T23:59:59.000Z

3

Anisotropic superconductivity: ({ital s}+{ital d})-wave model, ({ital d}+{ital s})-wave model and the effect of normal impurities  

SciTech Connect (OSTI)

We study in three and two dimensions (3D and 2D), some of the superconducting properties of anisotropic hybrid ({ital s}+{ital d})- and ({ital d}+{ital s})-wave superconductor models (depending whether the {ital s} or {ital d} component predominates). The anisotropy is contained in the fermion-fermion pairing interaction as reflecting structural anisotropies of the kind found in layered high-{ital T}{sub {ital c}} cuprates, in particular the orthorhombic ones. We show that even within the weak-coupling formalism and for an isotropic Fermi surface (so that the interaction has a lower symmetry than the Fermi surface), we obtain enhanced values of {Delta}{sub {ital M}}/{ital T}{sub {ital c}} ({Delta}{sub {ital M}} is the maximum value of the gap energy) compared to the BCS one, as well as enhanced {ital T}{sub {ital c}} values. Depending on the anisotropy parameters we can get a four-leaf clover kind of shape for the gap in {bold k} space in 2D, with the size of the leaves in one direction being different from one of those in the perpendicular direction. We also find unusual shapes for the density of states; in particular we can recover the {open_quote}{open_quote}gapless{close_quote}{close_quote} case similar to the one of the purely {ital d}-wave model of the literature. We study two kinds of anisotropic pairings: the first one, in 3D and 2D yields an ({ital s}+{ital d}) pairing; the other one, in 2D, yields a ({ital d}+{ital s}) pairing and is more specifically adapted to orthorhombic high-{ital T}{sub {ital c}} cuprates, the {ital s} component disappearing in the tetragonal case where the distortion is absent and for which the purely {ital d} pairing is recovered. (Abstract Truncated)

Beal-Monod, M.T. [Physique des Solides, Universite de Paris-Sud, 91400 Orsay (France); Maki, K. [Department of Physics and Astronomy, University of Southern California, Los Angeles, California 90089-0484 (United States)

1996-03-01T23:59:59.000Z

4

Measurement of the {ital D}{sup +}{sub {ital s}}{r_arrow}{eta}l{sup +}{nu} and {ital D}{sup +}{sub {ital s}}{r_arrow}{eta}{prime}l{sup +}{nu} branching ratios  

SciTech Connect (OSTI)

Using the CLEO II detector we measure {ital B}({ital D}{sup +}{sub {ital s}}{r_arrow}{eta}{ital e}{sup +}{nu})/{ital B}({ital D}{sup +}{sub {ital s}}{r_arrow}{phi}{ital e}{sup +}{nu}) =1.24{plus_minus}0.12{plus_minus}0.15, {ital B}({ital D}{sup +}{sub {ital s}}{r_arrow}{eta}{prime}{ital e}{sup +}{nu})/{ital B} ({ital D}{sup +}{sub {ital s}}{r_arrow}{phi}{ital e}{sup +}{nu})=0.43{plus_minus}0.11{plus_minus}0.07, and {ital B}({ital D}{sup +}{sub {ital s}}{r_arrow}{eta}{prime}{ital e}{sup +}{nu})/{ital B} ({ital D}{sup +}{sub {ital s}}{r_arrow}{eta}{ital e}{sup +}{nu})=0.35{plus_minus}0.09{plus_minus}0.07. We find the ratio of vector to pseudoscalar final states, {ital B}{bold (}{ital D}{sup +}{sub {ital s}}{r_arrow}{phi}{ital e}{sup +}{nu})/{ital B} ({ital D}{sup +}{sub {ital s}}{r_arrow}({eta}+{eta}{prime}){ital e}{sup +}{nu}{bold )}=0.60{plus_minus}0.06{plus_minus}0.06, which is similar to the ratio found in nonstrange {ital D} decays. {copyright} {ital 1995} {ital The} {ital American} {ital Physical} {ital Society}.

Brandenburg, G.; Cinabro, D.; Liu, T.; Saulnier, M.; Wilson, R.; Yamamoto, H.; Bergfeld, T.; Eisenstein, B.I.; Ernst, J.; Gladding, G.E.; Gollin, G.D.; Palmer, M.; Selen, M.; Thaler, J.J.; Edwards, K.W.; McLean, K.W.; Ogg, M.; Bellerive, A.; Britton, D.I.; Hyatt, E.R.F.; Janicek, R.; MacFarlane, D.B.; Patel, P.M.; Spaan, B.; Sadoff, A.J.; Ammar, R.; Baringer, P.; Bean, A.; Besson, D.; Coppage, D.; Copty, N.; Davis, R.; Hancock, N.; Kotov, S.; Kravchenko, I.; Kwak, N.; Kubota, Y.; Lattery, M.; Momayezi, M.; Nelson, J.K.; Patton, S.; Poling, R.; Savinov, V.; Schrenk, S.; Wang, R.; Alam, M.S.; Kim, I.J.; Ling, Z.; Mahmood, A.H.; O`Neill, J.J.; Severini, H.; Sun, C.R.; Wappler, F.; Crawford, G.; Duboscq, J.E.; Fulton, R.; Fujino, D.; Gan, K.K.; Honscheid, K.; Kagan, H.; Kass, R.; Lee, J.; Sung, M.; White, C.; Wolf, A.; Zoeller, M.M.; Fu, X.; Nemati, B.; Ross, W.R.; Skubic, P.; Wood, M.; Bishai, M.; Fast, J.; Gerndt, E.; Hinson, J.W.; Miao, T.; Miller, D.H.; Modesitt, M.; Shibata, E.I.; Shipsey, I.P.J.; Wang, P.N.; Gibbons, L.; Johnson, S.D.; Kwon, Y.; Roberts, S.; Thorndike, E.H.; Coan, T.E.; Dominick, J.; Fadeyev, V.; Korolkov, I.; Lambrecht, M.; Sanghera, S.; Shelkov, V.; Skwarnicki, T.; Stroynowski, R.; Volobouev, I.; Wei, G.; Artuso, M.; Gao, M.; Goldberg, M.; He, D.; Horwitz, N.; Kopp, S.; Moneti, G.C.; Mountain, R.; Muheim, F.; Mukhin, Y.; Playfer, S.; Stone, S.; Xing, X.; Bartelt, J.; Csorna, S.E.; Jain, V.; Marka, S.; Gibaut, D.; Kinoshita, K.; Pomianowski, P.; Barish, B.; Chadha, M.; Chan, S.; Cowen, D.F.; Eigen, G.; Miller, J.S.; O`Grady, C.; Urheim, J.; Weinstein, A.J.; Wuerthwein, F.; Asner, D.M.; Athanas, M.; Bliss, D.W.; Brower, W.S.; Masek, G.; Paar, H.P.; Gronberg, J.; Korte, C.M.; Kutschke, R.; Menary, S.; Morrison, R.J.; Nakanishi, S.; Nelson, H.N.; Nelson, T.K.; Qiao, C.; Richman, J.D.; Roberts, D.; Ryd, A.; Tajima, H.; Witherell, M.S.; Balest, R.; Cho, K.; Ford, W.T.; Lohner, M.; Park, H.; Rankin, P.; Smith, J.G.; Alexander, J.P.; (CLEO Collaborat..

1995-11-20T23:59:59.000Z

5

Search for {ital CP} violation in {ital D}{sup 0} decay  

SciTech Connect (OSTI)

Using 2.7 fb{sup {minus}1} of data taken with the CLEO II detector, we have searched for {ital CP} violation in the charm system. We looked for asymmetries in the number of decays of {ital D}{sup 0}`s and {ital {bar D}}{sup 0}`s to the {ital CP} eigenstates {ital K}{sup +}{ital K}{sup {minus}}, {ital K}{sub {ital S}}{sup 0}{phi}, and {ital K}{sub {ital S}}{sup 0}{pi}{sup 0}. Confidence intervals (90%) on these asymmetries were found to be {minus}0.020{lt}{ital A}{sub {ital K}{ital K}}{lt}0.180, {minus}0.182{lt}{ital A}{sub {ital K}{ital S}}{sup 0}{phi}{lt}0.126, and {minus}0.067{lt}{ital A}{sub {ital K}{ital S}}{sup 0}{pi}{sup 0}{lt}0.031, respectively.

Bartelt, J.; Csorna, S.E.; Egyed, Z.; Jain, V. [Vanderbilt University, Nashville, Tennessee 37235 (United States)] [Vanderbilt University, Nashville, Tennessee 37235 (United States); Gibaut, D.; Kinoshita, K.; Pomianowski, P. [Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061 (United States)] [Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061 (United States); Barish, B.; Chadha, M.; Chan, S.; Cowen, D.F.; Eigen, G.; Miller, J.S.; O`Grady, C.; Urheim, J.; Weinstein, A.J.; Wuerthwein, F. [California Institute of Technology, Pasadena, California 91125 (United States)] [California Institute of Technology, Pasadena, California 91125 (United States); Asner, D.M.; Athanas, M.; Bliss, D.W.; Brower, W.S.; Masek, G.; Paar, H.P. [University of California, San Diego, La Jolla, California 92093 (United States)] [University of California, San Diego, La Jolla, California 92093 (United States); Gronberg, J.; Korte, C.M.; Kutschke, R.; Menary, S.; Morrison, R.J.; Nakanishi, S.; Nelson, H.N.; Nelson, T.K.; Qiao, C.; Richman, J.D.; Roberts, D.; Ryd, A.; Tajima, H.; Witherell, M.S. [University of California, Santa Barbara, California 93106 (United States)] [University of California, Santa Barbara, California 93106 (United States); Balest, R.; Cho, K.; Ford, W.T.; Lohner, M.; Park, H.; Rankin, P.; Smith, J.G. [University of Colorado, Boulder, Colorado 80309-0390 (United States)] [University of Colorado, Boulder, Colorado 80309-0390 (United States); Alexander, J.P.; Bebek, C.; Berger, B.E.; Berkelman, K.; Bloom, K.; Browder, T.E.; Cassel, D.G.; Cho, H.A.; Coffman, D.M.; Crowcroft, D.S.; Dickson, M.; Drell, P.S.; Dumas, D.J.; Ehrlich, R.; Elia, R.; Gaidarev, P.; Garcia-Sciveres, M.; Gittelman, B.; Gray, S.W.; Hartill, D.L.; Heltsley, B.K.; Henderson, S.; Jones, C.D.; Jones, S.L.; Kandaswamy, J.; Katayama, N.; Kim, P.C.; Kreinick, D.L.; Lee, T.; Liu, Y.; Ludwig, G.S.; Masui, J.; Mevissen, J.; Mistry, N.B.; Ng, C.R.; Nordberg, E.; Patterson, J.R.; Peterson, D.; Riley, D.; Soffer, A. [Cornell University, Ithaca, New York 14853 (United States)] [Cornell University, Ithaca, New York 14853 (United States); Avery, P.; Freyberger, A.; Lingel, K.; Rodriguez, J.; Yang, S.; Yelton, J. [University of Florida, Gainesville, Florida 32611 (United States)] [University of Florida, Gainesville, Florida 32611 (United States); Brandenburg, G.; Cinabro, D.; Liu, T.; Saulnier, M.; Wilson, R.; Yamamoto, H. [Harvard University, Cambridge, Massachusetts 02138 (United States)] [Harvard University, Cambridge, Massachusetts 02138 (United States); Bergfeld, T.; Eisenstein, B.I.; Ernst, J.; (CLEO Collaboration)

1995-11-01T23:59:59.000Z

6

CuIn{sub 1{minus}{ital x}}Ga{sub {ital x}}Se{sub 2} and CdTe PV solar cells  

SciTech Connect (OSTI)

Higher indium proportion in the first precursor was employed to eliminate pits in CuIn{sub 1{minus}{ital x}}Ga{sub {ital x}}Se{sub 2} films prepared by two Se-vapor selenizations of metallic precursors. CuIn{sub 1{minus}{ital x}}Ga{sub {ital x}}Se{sub 2} films had large, faceted grains, and a near-optimum composition Cu:In:Ga:Se 24.25:22.21:4.40:49.14. Ga incorporated using a Cu-Ga(22 at. {percent}) alloy target was enhanced by optimizing the time-temperature profiles of selenizations. CuIn{sub 1{minus}{ital x}}Ga{sub {ital x}}Se{sub 2} solar cells gave {ital V}{sub oc} of 451.8 mV, {ital J}{sub sc} of 34.5 mA, FF of 57.87{percent}, total area efficiency of 9.02{percent}. CdTe thin films were prepared by heat treatment of magnetron-sputtered elemental Cd/Te stacks. Formation of extraneous oxide phases was avoided by optimizing ambients, temperature, and CdCl{sub 2} treatment. CdTe solar cells gave maximum {ital V}{sub oc} of {approximately}600 mV, {ital J}{sub sc} of {approximately}5 mA.cm{sup {minus}2}, very low FF and efficiency probably due to blocking layer or junction away from CdS{backslash}CdTe interface. {copyright} {ital 1996 American Institute of Physics.}

Dhere, N.G. [Florida Solar Energy Center, 300 State Rd 401, Cape Canaveral, Florida 32920-4099 (United States)

1996-01-01T23:59:59.000Z

7

Analysis of {ital D}{sup 0}{r_arrow}{ital K{bar K}X} decays  

SciTech Connect (OSTI)

Using data taken with the CLEO II detector, we have studied the decays of the {ital D}{sup 0} to {ital K}{sup +}{ital K}{sup {minus}}, {ital K}{sup 0}{ital {bar K}}{sup 0}, {ital K}{sup 0}{sub {ital S}}{ital K}{sup 0}{sub {ital S}}{ital K}{sup 0}{sub {ital S}}, {ital K}{sup 0}{sub {ital S}}{ital K}{sup 0}{sub {ital S}}{pi}{sup 0}, {ital K}{sup +}{ital K}{sup {minus}}{pi}{sup 0}. We present significantly improved results for {ital B}({ital D}{sup 0}{r_arrow}{ital K}{sup +}{ital K}{sup {minus}})=(0.454{plus_minus}0.028{plus_minus}0.035){percent}, {ital B}({ital D}{sup 0}{r_arrow}{ital K}{sup 0}{ital {bar K}}{sup 0})=(0.054{plus_minus}0.012{plus_minus}0.010){percent}, and {ital B}({ital D}{sup 0}{r_arrow}{ital K}{sup 0}{sub {ital S}}{ital K}{sup 0}{sub {ital S}}{ital K}{sup 0}{sub {ital S}})=(0.074{plus_minus}0.010{plus_minus}0.015){percent}, where the first errors are statistical and the second errors are the estimate of our systematic uncertainty. We also present a new upper limit {ital B}({ital D}{sup 0}{r_arrow}{ital K}{sup 0}{sub {ital S}}{ital K}{sup 0}{sub {ital S}}{pi}{sup 0}){lt}0.059{percent} at the 90{percent} confidence level and the first measurement of {ital B}({ital D}{sup 0}{r_arrow}{ital K}{sup +}{ital K}{sup {minus}}{pi}{sup 0})=(0.14{plus_minus}0.04){percent}. {copyright} {ital 1996 The American Physical Society.}

Asner, D.M.; Athanas, M.; Bliss, D.W.; Brower, W.S.; Masek, G.; Paar, H.P. [University of California, San Diego, La Jolla, California 92093 (United States)] [University of California, San Diego, La Jolla, California 92093 (United States); Gronberg, J.; Korte, C.M.; Kutschke, R.; Menary, S.; Morrison, R.J.; Nakanishi, S.; Nelson, H.N.; Nelson, T.K.; Qiao, C.; Richman, J.D.; Roberts, D.; Ryd, A.; Tajima, H.; Witherell, M.S. [University of California, Santa Barbara, California 93106 (United States)] [University of California, Santa Barbara, California 93106 (United States); Balest, R.; Cho, K.; Ford, W.T.; Lohner, M.; Park, H.; Rankin, P.; Roy, J.; Smith, J.G. [University of Colorado, Boulder, Colorado 80309-0390 (United States)] [University of Colorado, Boulder, Colorado 80309-0390 (United States); Alexander, J.P.; Bebek, C.; Berger, B.E.; Berkelman, K.; Bloom, K.; Cassel, D.G.; Cho, H.A.; Coffman, D.M.; Crowcroft, D.S.; Dickson, M.; Drell, P.S.; Dumas, D.J.; Ehrlich, R.; Elia, R.; Gaidarev, P.; Gittelman, B.; Gray, S.W.; Hartill, D.L.; Heltsley, B.K.; Jones, C.D.; Jones, S.L.; Kandaswamy, J.; Katayama, N.; Kim, P.C.; Kreinick, D.L.; Lee, T.; Liu, Y.; Ludwig, G.S.; Masui, J.; Mevissen, J.; Mistry, N.B.; Ng, C.R.; Nordberg, E.; Patterson, J.R.; Peterson, D.; Riley, D.; Soffer, A.; Ward, C. [Cornell University, Ithaca, New York 14853 (United States)] [Cornell University, Ithaca, New York 14853 (United States); Avery, P.; Prescott, C.; Yang, S.; Yelton, J. [University of Florida, Gainesville, Florida 32611 (United States)] [University of Florida, Gainesville, Florida 32611 (United States); Brandenburg, G.; Briere, R.A.; Liu, T.; Saulnier, M.; Wilson, R.; Yamamoto, H. [Harvard University, Cambridge, Massachusetts 02138 (United States)] [Harvard University, Cambridge, Massachusetts 02138 (United States); Browder, T.E.; Li, F.; Rodriguez, J.L. [University of Hawaii at Manoa, Honolulu, Hawaii 96822 (United States)] [University of Hawaii at Manoa, Honolulu, Hawaii 96822 (United States); Bergfeld, T.; Eisenstein, B.I.; Ernst, J.; Gladding, G.E.; Gollin, G.D.; Palmer, M.; Selen, M.; Thaler, J.J. [University of Illinois, Champaign-Urbana, Illinois 61801 (United States)] [University of Illinois, Champaign-Urbana, Illinois 61801 (United States); Edwards, K.W.; McLean, K.W.; Ogg, M. [Carleton University, Ottawa, K1S 5B6 (CANADA)] [Carleton University, Ottawa, K1S 5B6 (CANADA); [the Institute of Particle Physics (Canada); Bellerive, A.; Britton, D.I.; Janicek, R.; MacFarlane, D.B.; Patel, P.M.; Spaan, B. [McGill University, Montreal, H3A 2T8 (CANADA)] [McGill University, Montreal, H3A 2T8 (CANADA)

1996-10-01T23:59:59.000Z

8

Stability of Interfaces with Self-Gravity, Relative Flow, and {ital B} Field  

SciTech Connect (OSTI)

Observations with the {ital Hubble} {ital Space} {ital T}{ital elescope} (Hester et al.) of spectacular {open_quotes}fingers{close_quotes} or {open_quotes}elephant trunks{close_quotes} of gas protruding from a large star-forming cloud in the Eagle Nebula stimulate renewed interest in the stability of interfaces between different media in molecular clouds. Instability and nonlinear growth of crenelations of interfaces can lead to mass concentrations that in turn lead to star formation. In an earlier study of the stability of interfaces, we took into account the important physical effects{emdash}the different densities and temperatures of the media, the relative motion (Kelvin-Helmholtz instability), the gravitational acceleration perpendicular to the interface (Rayleigh-Taylor instability), and self-gravity. A new {ital self}-{ital gravitational} {ital instability} of an interface was found that was independent of the wavelength of the perturbation. At short wavelengths, the perturbations are essentially distortional, but compression becomes important as the Jeans length is approached from below. The {ital e}-folding time for the instability is comparable with the free-fall collapse time for the denser fluid. In the present work, we generalize our earlier theory in two ways: by including ordered magnetic fields parallel to the interface, and by examining the stability of long cylindrical interfaces. We show that dynamically important magnetic fields in the media can quench instabilities if the fields are oriented in different directions (that is, crossed); however, for astronomically plausible geometries in which the fields are closer to being parallel, but of different strengths in the two media, instabilities are free to grow in directions normal to the fields. A cylindrical interface between an interior medium of density {rho}{sub 1} and an exterior medium of density {rho}{sub 2} provides a model for the long filaments of dense gas observed in some molecular clouds. We show that such an interface with {rho}{sub 1} {gt} {rho}{sub 2} is stable to {open_quotes}kink modes{close_quotes} but unstable to {open_quotes}sausage modes{close_quotes} owing to self-gravity for long axial wavelengths, {lambda}{sub {ital z}} {gt} 3.8{ital d}, where {ital d} is the diameter of the cylinder. This instability will tend to form prolate ellipsoidal density concentrations aligned with the cylinder axis. {copyright} {ital {copyright} .} {ital The American Astronomical Society}

Hunter, J.H. Jr. [Department of Astronomy, University of Florida, PO Box 112005, Gainesville, FL 32611-2055 (United States)] [Department of Astronomy, University of Florida, PO Box 112005, Gainesville, FL 32611-2055 (United States); Whitaker, R.W. [Los Alamos National Laboratory, EES-8, MS F659, Los Alamos, NM 87545 (United States)] [Los Alamos National Laboratory, EES-8, MS F659, Los Alamos, NM 87545 (United States); Lovelace, R.V. [Department of Astronomy, Cornell University, Ithaca, NY 14853-6801 (United States)] [Department of Astronomy, Cornell University, Ithaca, NY 14853-6801 (United States)

1998-12-01T23:59:59.000Z

9

INTELLIGENT COMPUTING SYSTEM FOR RESERVOIR ANALYSIS AND RISK ASSESSMENT OF THE RED RIVER FORMATION  

SciTech Connect (OSTI)

Integrated software has been written that comprises the tool kit for the Intelligent Computing System (ICS). The software tools in ICS have been developed for characterization of reservoir properties and evaluation of hydrocarbon potential using a combination of inter-disciplinary data sources such as geophysical, geologic and engineering variables. The ICS tools provide a means for logical and consistent reservoir characterization and oil reserve estimates. The tools can be broadly characterized as (1) clustering tools, (2) neural solvers, (3) multiple-linear regression, (4) entrapment-potential calculator and (5) file utility tools. ICS tools are extremely flexible in their approach and use, and applicable to most geologic settings. The tools are primarily designed to correlate relationships between seismic information and engineering and geologic data obtained from wells, and to convert or translate seismic information into engineering and geologic terms or units. It is also possible to apply ICS in a simple framework that may include reservoir characterization using only engineering, seismic, or geologic data in the analysis. ICS tools were developed and tested using geophysical, geologic and engineering data obtained from an exploitation and development project involving the Red River Formation in Bowman County, North Dakota and Harding County, South Dakota. Data obtained from 3D seismic surveys, and 2D seismic lines encompassing nine prospective field areas were used in the analysis. The geologic setting of the Red River Formation in Bowman and Harding counties is that of a shallow-shelf, carbonate system. Present-day depth of the Red River formation is approximately 8000 to 10,000 ft below ground surface. This report summarizes production results from well demonstration activity, results of reservoir characterization of the Red River Formation at demonstration sites, descriptions of ICS tools and strategies for their application.

Mark A. Sippel; William C. Carrigan; Kenneth D. Luff; Lyn Canter

2003-11-12T23:59:59.000Z

10

Insight into the Common Mechanism of the Chromophore Formation in the Red Fluorescent Proteins: The Elusive Blue  

E-Print Network [OSTI]

: The Elusive Blue Intermediate Revealed Ksenia B. Bravaya, Oksana M. Subach, Nadezhda Korovina, Vladislav V calculations identifying the nature of a blue intermediate, a key species in the process of the red chromophore formation in DsRed, TagRFP, fluorescent timers, and PAmCherry. The chromophore of the blue intermediate has

Krylov, Anna I.

11

Excitation and decay of giant resonances in the [sup 40]Ca([ital e],[ital e][prime][ital x]) reaction  

SciTech Connect (OSTI)

The [sup 40]Ca([ital e],[ital e][prime][ital x]) reaction has been investigated for excitation energies between 8 and 26 MeV and momentum transfers from 0.25 to 0.66 fm[sup [minus]1] at the continuous-wave electron accelerators MAMI at Mainz S-DALINAC at Darmstadt. A multipole decomposition of the cross sections reveals strongly fragmented [ital E]2 (plus [ital E]0) strength around 14 and 17 MeV in contrast to all theoretical predictions. Angular correlations of proton decay are described over the entire energy range by a continuum random-phase-approximation approach. A comparison of the branching ratios to statistical model calculations provides information on the dominant damping mechanism.

Diesener, H.; Helm, U.; Herbert, G.; Huck, V.; von Neumann-Cosel, P.; Rangacharyulu, C.; Richter, A.; Schrieder, G.; Stascheck, A.; Stiller, A. (Institut fuer Kernphysik, Technische Hochschule Darmstadt, D-64289 Darmstadt (Germany)); Ryckebusch, J. (Institute for Nuclear Physics, Proeftuinstraat 86, B-9000 Ghent (Belgium)); Carter, J. (Department of Physics, University of the Witwatersrand, P.O. Wits, Johannesburg 2050 (South Africa))

1994-03-28T23:59:59.000Z

12

Depositional environment of lower Green River Formation sandstones (Eocene), Red Wash field (Uinta Basin), Uintah County, Utah  

E-Print Network [OSTI]

DFPOSITIONAL FNVIRONMENT OF LOWER GREEN RIVER FORMATION SANDSTONES (EOCENE), RED WASH FIELD (UINTA BASIN), UINTAH COUNTY, UTAH A Thesis by ANTHONY SCOTT MCCLAIN Submitted to the Graduate College of Texas AAM University in partial fulfillment... of the requirements for the degree of MASTER OF SCIENCE May 1985 Major Subject: Geology OPPOSITIONAL ENVIRONMENT OF LOWFR BPEEN RIVER FORMATION SANDSTONES (EOCFNE. ), RED WASH FIELD (UINTA BASIN), UINTAH COUNTY, UTAH A Thesis by ANTHONY SCOTT MCCLAIN Approved...

McClain, Anthony Scott

1985-01-01T23:59:59.000Z

13

Structure of hot rotating {ital s}-{ital d} shell nuclei  

SciTech Connect (OSTI)

Landau theory of phase transitions is used to determine the shape evolution of even-even {ital s}-{ital d} shell nuclei with temperature and spin. Further in this study, the most important statistical thermal shape fluctuations are also incorporated. The constants appearing in the Landau expression for the free energy are determined by using the free energy surfaces at {omega}=0 calculated by the finite temperature Strutinsky and summation methods. The pairing effect is included at ground state but shown to be of minor importance in shape determination. It is seen that the averaged shapes for the above nuclei at different temperatures and spins are mostly triaxial which are quite different from the most probable shapes, prolate or oblate. Only these averaged shapes can be seen through the study of giant dipole resonance decays of highly excited states.

Shanmugam, G. [Department of Physics, Manonmaniam Sundaranar University, Tirunelveli-627 002 (India)] [Department of Physics, Manonmaniam Sundaranar University, Tirunelveli-627 002 (India); Sankar, K. [Department of Physics, Presidency College, Madras-600 005 (India)] [Department of Physics, Presidency College, Madras-600 005 (India); Ramamurthi, K. [Department of Physics, Bharathidasan University, Tiruchirappalli-620 024 (India)] [Department of Physics, Bharathidasan University, Tiruchirappalli-620 024 (India)

1995-09-01T23:59:59.000Z

14

INTELLIGENT COMPUTING SYSTEM FOR RESERVOIR ANALYSIS AND RISK ASSESSMENT OF THE RED RIVER FORMATION  

SciTech Connect (OSTI)

Integrated software has been written that comprises the tool kit for the Intelligent Computing System (ICS). Luff Exploration Company is applying these tools for analysis of carbonate reservoirs in the southern Williston Basin. The integrated software programs are designed to be used by small team consisting of an engineer, geologist and geophysicist. The software tools are flexible and robust, allowing application in many environments for hydrocarbon reservoirs. Keystone elements of the software tools include clustering and neural-network techniques. The tools are used to transform seismic attribute data to reservoir characteristics such as storage (phi-h), probable oil-water contacts, structural depths and structural growth history. When these reservoir characteristics are combined with neural network or fuzzy logic solvers, they can provide a more complete description of the reservoir. This leads to better estimates of hydrocarbons in place, areal limits and potential for infill or step-out drilling. These tools were developed and tested using seismic, geologic and well data from the Red River Play in Bowman County, North Dakota and Harding County, South Dakota. The geologic setting for the Red River Formation is shallow-shelf carbonate at a depth from 8000 to 10,000 ft.

Kenneth D. Luff

2002-06-30T23:59:59.000Z

15

INTELLIGENT COMPUTING SYSTEM FOR RESERVOIR ANALYSIS AND RISK ASSESSMENT OF THE RED RIVER FORMATION  

SciTech Connect (OSTI)

Integrated software has been written that comprises the tool kit for the Intelligent Computing System (ICS). Luff Exploration Company is applying these tools for analysis of carbonate reservoirs in the southern Williston Basin. The integrated software programs are designed to be used by small team consisting of an engineer, geologist and geophysicist. The software tools are flexible and robust, allowing application in many environments for hydrocarbon reservoirs. Keystone elements of the software tools include clustering and neural-network techniques. The tools are used to transform seismic attribute data to reservoir characteristics such as storage (phi-h), probable oil-water contacts, structural depths and structural growth history. When these reservoir characteristics are combined with neural network or fuzzy logic solvers, they can provide a more complete description of the reservoir. This leads to better estimates of hydrocarbons in place, areal limits and potential for infill or step-out drilling. These tools were developed and tested using seismic, geologic and well data from the Red River Play in Bowman County, North Dakota and Harding County, South Dakota. The geologic setting for the Red River Formation is shallow-shelf carbonate at a depth from 8000 to 10,000 ft.

Kenneth D. Luff

2002-09-30T23:59:59.000Z

16

CP, T, and CPT tests in neutral Kaon decays using tagged {ital K}{sup 0}, {ital K}{sup 0}at LEAR  

SciTech Connect (OSTI)

The CPLEAR experiment at CERN measures particle-antiparticle asymmetries of strangeness-tagged {ital K}{sup 0}, {ital K}{sup 0} decays to two-pion, three-pion, and semileptonic final states. The technique of CPLEAR is an alternative approach to previous CP-violation studies. It provides complementary information with different systematics and gives access to novel measurements. The precision of the CP-violation parameters {eta}{sub +{minus}} for {pi}{sup +}{pi}{sup {minus}}, {eta}{sub +{minus}0} for {pi}{sup +}{pi}{sup {minus}}{pi}{sup 0} and of the T-violation parameter {epsilon}{sub {ital T}} for {pi}{sup {plus_minus}}{ital e}{sup {minus_plus}}{nu} will be discussed for the data taken between 1990--1992. {copyright} {ital 1995} {ital American} {ital Institute} {ital of} {ital Physics}.

Adler, R.; Alhalel, T. [University of Basle (Switzerland); Angelopoulos, A.; Apostolakis, A. [University of Athens (Greece); Aslanides, E. [CPPM, IN2P3-CNRS et Universite d`Aix-Marseille II (France); Backenstoss, G. [University of Basle (Switzerland); Bee, C.P. [CPPM, IN2P3-CNRS et Universite d`Aix-Marseille II (France); Behnke, O. [ETH-ITP Zuerich (Switzerland); Bennet, J. [University of Liverpool (United Kingdom); Bertin, V. [CPPM, IN2P3-CNRS et Universite d`Aix-Marseille II (France); Blanc, F. [University of Fribourg (Germany)]|[Paul-Scherrer-Institut (??); Bloch, P. [CERN (Switzerland); Bula, C. [Paul-Scherrer-Institut (??); Carlson, P. [KTH Stockholm (Sweden); Carroll, M. [University of Liverpool (United Kingdom); Carvalho, J. [LIP and University of Coimbra (Portugal); Cawley, E. [University of Liverpool (United Kingdom); Charalambous, S.; Chardalas, M. [University of Thessaloniki (Greece); Chardin, G. [DAPNIA/SPP, CE Saclay (France); Chertok, M.B. [Boston University (United States); Danielsson, M. [KTH Stockholm (Sweden); Cody, A. [University of Liverpool (United Kingdom); Dedoussis, S. [University of Thessaloniki (Greece); Dejardin, M. [CERN (Switzerland); Derre, J. [DAPNIA/SPP, CE Saclay (France); Dodgson, M. [University of Liverpool (United Kingdom); Duclos, J. [DAPNIA/SPP, CE Saclay (France); Ealet, A. [CPPM, IN2P3-CNRS et Universite d`Aix-Marseille II (France); Eckart, B. [University of Basle (Switzerland); Eleftheriadis, C. [University of Thessaloniki (Greece); Evangelou, I. [University of Ioannina (??); Faravel, L. [University of Fribourg (Germany)]|[CPPM, IN2P3-CNRS et Universite d`Aix-Marseille II (France); Fassnacht, P. [CPPM, IN2P3-CNRS et Universite d`Aix-Marseille II (France); Faure, J.L. [DAPNIA/SPP, CE Saclay (France); Felder, C. [University of Basle (Switzerland); Ferreira-Marques, R. [LIP and University of Coimbra (Portugal); Fetscher, W. [ETH-ITP Zuerich (Switzerland); Fidecaro, M.

1995-05-10T23:59:59.000Z

17

On the RMS anisotropy at 7{degree} and 10{degree} observed in the {ital COBE}-DMR two year sky maps  

SciTech Connect (OSTI)

We summarize the recent results on the observed {ital COBE}-DMR two year sky rms temperature fluctuations. A ``cross-RMS`` statistic is used to infer the {ital Q}{sub {ital rms}-{ital PS}} normalization for a scale-invariant ({ital n}=1) spectral model. The method is extended to the normalization of other cosmological power spectra. {copyright} {ital 1995} {ital American} {ital Institute} {ital of} {ital Physics}.

Banday, A.J.; Gorski, K.M.; Kogut, A.; Hinshaw, G.; Bennett, C. [Code 685, NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771 (United States); Lineweaver, C.H.; Smoot, G.F.; Tenorio, L. [LBL, SSL & CfPA, Bldg 50-351, University of California, Berkeley, California 94720 (United States)

1995-07-01T23:59:59.000Z

18

Formation of Thetis Deep metal-rich sediments in the absence of brines, Red Sea M.C. Pierret a  

E-Print Network [OSTI]

Formation of Thetis Deep metal-rich sediments in the absence of brines, Red Sea M.C. Pierret a , N October 2009 Available online 23 October 2009 Keywords: Pb­Sr­Nd isotopes REE Metal-rich sediments-rich sediments covered by brine pools. It is generally agreed that these metal-rich deposits precipitated from

Demouchy, Sylvie

19

Search for {ital B}{r_arrow}l{bar {nu}}{sub l}  

SciTech Connect (OSTI)

We search for the decays {ital B}{sup {minus}}{r_arrow}l{sup {minus}}{bar {nu}}{sub l} in a sample of 2.2{times}10{sup 6} charged {ital B} decays using the CLEO detector. We see no evidence for a signal in any channel and set upper limits on the branching fractions of {ital B}({ital B}{sup {minus}}{r_arrow}{tau}{sup {minus}}{bar {nu}}{sub {tau}}){lt}2.2{times}10{sup {minus}3}, {ital B}({ital B}{sup {minus}}{r_arrow}{mu}{sup {minus}}{nu}2;m{sub {mu}}){lt}2.1{times}10{sup {minus}5}, and {ital B}({ital B}{sup {minus}}{r_arrow}{ital e}{sup {minus}}{bar {nu}}{sub {ital e}}){lt}1.5{times}10{sup {minus}5} at the 90% confidence level.

Artuso, M.; Gao, M.; Goldberg, M.; He, D.; Horwitz, N.; Moneti, G.C.; Mountain, R.; Muheim, F.; Mukhin, Y.; Playfer, S.; Rozen, Y.; Stone, S.; Xing, X.; Zhu, G.; Bartelt, J.; Csorna, S.E.; Egyed, Z.; Jain, V.; Gibaut, D.; Kinoshita, K.; Pomianowski, P.; Barish, B.; Chadha, M.; Chan, S.; Cowen, D.F.; Eigen, G.; Miller, J.S.; O`Grady, C.; Urheim, J.; Weinstein, A.J.; Wuerthwein, F.; Asner, D.M.; Athanas, M.; Bliss, D.W.; Brower, W.S.; Masek, G.; Paar, H.P.; Gronberg, J.; Korte, C.M.; Kutschke, R.; Menary, S.; Morrison, R.J.; Nakanishi, S.; Nelson, H.N.; Nelson, T.K.; Qiao, C.; Richman, J.D.; Roberts, D.; Ryd, A.; Tajima, H.; Witherell, M.S.; Balest, R.; Cho, K.; Ford, W.T.; Lohner, M.; Park, H.; Rankin, P.; Smith, J.G.; Alexander, J.P.; Bebek, C.; Berger, B.E.; Berkelman, K.; Bloom, K.; Browder, T.E.; Cassel, D.G.; Cho, H.A.; Coffman, D.M.; Crowcroft, D.S.; Dickson, M.; Drell, P.S.; Dumas, D.J.; Ehrlich, R.; Elia, R.; Gaidarev, P.; Galik, R.S.; Garcia-Sciveres, M.; Gittelman, B.; Gray, S.W.; Hartill, D.L.; Heltsley, B.K.; Henderson, S.; Jones, C.D.; Jones, S.L.; Kandaswamy, J.; Katayama, N.; Kim, P.C.; Kreinick, D.L.; Liu, Y.; Ludwig, G.S.; Masui, J.; Mevissen, J.; Mistry, N.B.; Ng, C.R.; Nordberg, E.; Patterson, J.R.; Peterson, D.; Riley, D.; Soffer, A.; Avery, P.; Freyberger, A.; Lingel, K.; Rodriguez, J.; Yang, S.; Yelton, J.; Brandenburg, G.; Cinabro, D.; Liu, T.; Saulnier, M.; Wilson, R.; Yamamoto, H.; Bergfeld, T.; Eisenstein, B.I.; Ernst, J.; Gladding, G.E.; Gollin, G.D.; Palmer, M.; Selen, M.; Thaler, J.J.; Edwards, K.W.; McLean, K.W.; Ogg, M.; Bellerive, A.; Britton, D.I.; Hyatt, E.R.F.; Janicek, R.; MacFarlane, D.B.; Patel, P.M.; Spaan, B.; Sadoff, A.J.; Ammar, R.; Baringer, P.; Bean, A.; Besson, D.; Coppage, D.; Copty, N.; Davis, R.; Hancock, N.; Kelly, M.; Kotov, S.; Kravchenko, I.; Kwak, N.; Lam, H.; Kubota, Y.; Lattery, M.; Momayezi, M.; Nelson, J.K.; Patton, S.; Poling, R.; Savinov, V.; Schrenk, S.; Wang, R.; Alam, M.S.; Kim, I.J.; Ling, Z.; (CLEO Co..

1995-07-31T23:59:59.000Z

20

Conditions for uniform growth of GaAs/sub 1-//sub x-italic/P/sub x-italic/ superlattices  

SciTech Connect (OSTI)

Nonplanar morphology and compositional inhomogeneity are observed in GaAs/sub 1-//sub x-italic/P/sub x-italic/ superlattices when the phosphorus content is substantially different in adjacent sublayers. The main characteristic feature of the distortion is a series of ribbonlike regions running through the superlattice which etch at a faster rate and contain more phosphorus than the surrounding material and are also the source of clusters of dislocations. Morphological stability and a general decrease in dislocation density can be effected by decreasing the interlayer strain, i.e., compositional difference, between the superlattice sublayers.

Blakeslee, A.E.; Kibbler, A.; Wanlass, M.W.; Biefeld, R.M.

1986-08-01T23:59:59.000Z

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


21

Lateral Drilling and Completion Technologies for Shallow-Shelf Carbonates of the Red River and Ratcliffe Formations, Williston Basin  

SciTech Connect (OSTI)

Luff Exploration Company (LEC) focused on involvement in technologies being developed utilizing horizontal drilling concepts to enhance oil- well productivity starting in 1992. Initial efforts were directed toward high-pressure lateral jetting techniques to be applied in existing vertical wells. After involvement in several failed field attempts with jetting technologies, emphasis shifted to application of emerging technologies for drilling short-radius laterals in existing wellbores and medium-radius technologies in new wells. These lateral drilling technologies were applied in the Mississippi Ratcliffe and Ordovician Red River formations at depths of 2590 to 2890 m (8500 to 9500 ft) in Richland Co., MT; Bowman Co., ND; and Harding Co., SD.

David Gibbons; Larry A. Carrell; Richard D. George

1997-07-31T23:59:59.000Z

22

3D Hydrodynamical Simulations of Surface Convection in Red Giant Stars. Impact on spectral line formation and abundance analysis  

E-Print Network [OSTI]

We investigate the impact of 3D hydrodynamical model atmospheres of red giant stars at different metallicities on the formation of spectral lines of a number of ions and molecules. We carry out realistic 3D simulations of surface convection in red giant stars with varying stellar parameters. We use the simulations as time-dependent hydrodynamical model stellar atmospheres to compute atomic (Li, O, Na, Mg, Ca, Fe) and molecular (CH, NH, OH) spectral lines under the assumption of local thermodynamic equilibrium (LTE). We compare the line strengths computed in 3D with the results of analogous line formation calculations for 1D, hydrostatic, plane-parallel MARCS model atmospheres in order to estimate the impact of 3D models on the derivation of elemental abundances. The temperature and density inhomogeneities and correlated velocities in 3D models, as well as the differences between the 1D and mean 3D structures significantly affect the predicted line strengths. Under the assumption of LTE, the low atmospheric temperatures of very metal-poor 3D model atmospheres cause the lines from neutral species and molecules to appear stronger than in 1D. Therefore, elemental abundances derived from these lines using 3D models are significantly lower than according to 1D analyses. Differences between 3D and 1D abundances of C, N, and O derived from CH, NH, and OH weak low-excitation lines are found to be in the range -0.5 dex to -1.0 dex for the the red giant stars at [Fe/H]=-3 considered here. At this metallicity, large negative corrections (about -0.8 dex) are also found for weak low-excitation Fe I lines. We caution, however, that departures from LTE might be significant for these and other elements and comparable to the effects due to stellar granulation.

Remo Collet; Martin Asplund; Regner Trampedach

2007-03-26T23:59:59.000Z

23

The {ital COBE} Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background. I. Limits and Detections  

SciTech Connect (OSTI)

The Diffuse Infrared Background Experiment (DIRBE) on the Cosmic Background Explorer ({ital COBE}) spacecraft was designed primarily to conduct a systematic search for an isotropic cosmic infrared background (CIB) in 10 photometric bands from 1.25 to 240 {mu}m. The results of that search are presented here. Conservative limits on the CIB are obtained from the minimum observed brightness in all-sky maps at each wavelength, with the faintest limits in the DIRBE spectral range being at 3.5 {mu}m ({nu}{ital I}{sub {nu}} {lt} 64 nW m{sup {minus}2} sr{sup {minus}1}, 95{percent} confidence level) and at 240 {mu}m ({nu}{ital I}{sub {nu}} {lt} 28 nW m{sup {minus}2} sr{sup {minus}1}, 95{percent} confidence level). The bright foregrounds from interplanetary dust scattering and emission, stars, and interstellar dust emission are the principal impediments to the DIRBE measurements of the CIB. These foregrounds have been modeled and removed from the sky maps. Assessment of the random and systematic uncertainties in the residuals and tests for isotropy show that only the 140 and 240 {mu}m data provide candidate detections of the CIB. The residuals and their uncertainties provide CIB upper limits more restrictive than the dark sky limits at wavelengths from 1.25 to 100 {mu}m. No plausible solar system or Galactic source of the observed 140 and 240 {mu}m residuals can be identified, leading to the conclusion that the CIB has been detected at levels of {nu}{ital I}{sub {nu}} = 25 {plus_minus} 7 and 14 {plus_minus} 3 nW m{sup {minus}2} sr{sup {minus}1} at 140 and 240 {mu}m, respectively. The integrated energy from 140 to 240 {mu}m, 10.3 nW m{sup {minus}2} sr{sup {minus}1}, is about twice the integrated optical light from the galaxies in the Hubble Deep Field, suggesting that star formation might have been heavily enshrouded by dust at high redshift. The detections and upper limits reported here provide new constraints on models of the history of energy-releasing processes and dust production since the decoupling of the cosmic microwave background from matter. {copyright} {ital {copyright} 1998.} {ital The American Astronomical Society}

Hauser, M.G. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)] [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Arendt, R.G. [Raytheon STX, Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)] [Raytheon STX, Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Kelsall, T.; Dwek, E. [Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)] [Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Odegard, N.; Weiland, J.L.; Freudenreich, H.T. [Raytheon STX, Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)] [Raytheon STX, Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Reach, W.T. [California Institute of Technology, IPAC/JPL, MS 100-22, Pasadena, CA 91125 (United States)] [California Institute of Technology, IPAC/JPL, MS 100-22, Pasadena, CA 91125 (United States); Silverberg, R.F.; Moseley, S.H. [Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)] [Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Pei, Y.C. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)] [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Lubin, P. [Physics Department, University of California at Santa Barbara, Santa Barbara, CA 93106 (United States)] [Physics Department, University of California at Santa Barbara, Santa Barbara, CA 93106 (United States); Mather, J.C.; Shafer, R.A. [Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)] [Code 685, NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Smoot, G.F. [Lawrence Berkeley Laboratory, Space Sciences Laboratory, Department of Physics, UC Berkeley, CA 94720 (United States)] [Lawrence Berkeley Laboratory, Space Sciences Laboratory, Department of Physics, UC Berkeley, CA 94720 (United States); Weiss, R. [Massachusetts Institute of Technology, Room 20F-001, Department of Physics, Cambridge, MA 02139 (United States)] [Massachusetts Institute of Technology, Room 20F-001, Department of Physics, Cambridge, MA 02139 (United States); Wilkinson, D.T. [Princeton University, Department of Physics, Jadwin Hall, Box 708, Princeton, NJ 08544 (United States)] [Princeton University, Department of Physics, Jadwin Hall, Box 708, Princeton, NJ 08544 (United States); Wright, E.L. [UCLA, Astronomy Department, Los Angeles, CA 90024-1562 (United States)] [UCLA, Astronomy Department, Los Angeles, CA 90024-1562 (United States)

1998-11-01T23:59:59.000Z

24

The correlation of open-circuit voltage with bandgap in amorphous silicon-based {ital pin} solar cells  

SciTech Connect (OSTI)

We briefly review the correlation of open-circuit voltages {ital V}{sub OC} with the bandgap of the intrinsic layer in amorphous silicon based {ital pin} solar cells. We discuss two mechanisms which limit {ital V}{sub OC}: intrinsic layer recombination, and the built-in potential {ital V}{sub BI}. In particular we discuss Li{close_quote}s proposal that the open-circuit voltages in higher bandgap cells ({ital E}{sub G}{gt}1.9 eV) are {ital V}{sub BI}-limited. Based on computer simulations of {ital pin} solar cells we propose that {ital V}{sub BI} limitation occurs when the recombination limit to {ital V}{sub OC} exceeds the cell{close_quote}s field-reversal voltage {ital V}{sub R}. For {ital a}-Si:H based cells this field-reversal voltage occurs at about {ital V}{sub BI}-0.3 V. This proposal would account for the observation that {ital V}{sub BI} limitation occurs for {ital V}{sub OC} significantly smaller than {ital V}{sub BI}. {copyright} {ital 1996 American Institute of Physics.}

Crandall, R.S. [National Renewable Energy Laboratory, Golden, Colorado 80401 (United States); Schiff, E.A. [Department of Physics, Syracuse University, Syracuse, New York 13244-1130 (United States)

1996-01-01T23:59:59.000Z

25

Search for the Decays {ital B}{sup 0}{r_arrow}{ital D}{sup ({asterisk})+}{ital D}{sup ({asterisk}){minus}}  

SciTech Connect (OSTI)

Using the CLEO-II data set we have searched for the decays B{sup 0}{r_arrow}D{sup (*)+}D{sup (* ){minus}} . We observe one candidate signal event for the decay B{sup 0}{r_arrow}D{sup *+}D{sup *{minus}} with an expected background of 0.022{plus_minus}0.011 events. This yield corresponds to a branching fraction of B(B{sup 0}{r_arrow}D{sup *+}D{sup *{minus}} )=[5.3{sup +7.1}{sub {minus}3.7}(stat ){plus_minus}1.0(syst)]{times} 10{sup {minus}4} and an upper limit of B(B{sup 0}{r_arrow}D{sup *+}D{sup *{minus}} ){lt}2.2{times}10{sup {minus}3} at the 90% C.L. We see no significant excess of signal above the expected background level in the other modes, and we calculate the 90% C.L.upper limits on the branching fractions to be B(B{sup 0}{r_arrow}D{sup *{plus_minus}}D{sup {minus_plus}}){lt}1.8{times}10{sup {minus}3} and B(B{sup 0}{r_arrow}D{sup +}D{sup {minus}}){lt}1.2{times}10{sup {minus}3} . {copyright} {ital 1997} {ital The American Physical Society}

Asner, D.M.; Bliss, D.W.; Brower, W.S.; Masek, G.; Paar, H.P.; Sharma, V. [University of California, San Diego, La Jolla, California 92093 (United States)] [University of California, San Diego, La Jolla, California 92093 (United States); Gronberg, J.; Kutschke, R.; Lange, D.J.; Menary, S.; Morrison, R.J.; Nelson, H.N.; Nelson, T.K.; Qiao, C.; Richman, J.D.; Roberts, D.; Ryd, A.; Witherell, M.S. [University of California, Santa Barbara, California 93106 (United States)] [University of California, Santa Barbara, California 93106 (United States); Balest, R.; Behrens, B.H.; Cho, K.; Ford, W.T.; Park, H.; Rankin, P.; Roy, J.; Smith, J.G. [University of Colorado, Boulder, Colorado 80309-0390 (United States)] [University of Colorado, Boulder, Colorado 80309-0390 (United States); Alexander, J.P.; Bebek, C.; Berger, B.E.; Berkelman, K.; Bloom, K.; Cassel, D.G.; Cho, H.A.; Coffman, D.M.; Crowcroft, D.S.; Dickson, M.; Drell, P.S.; Ecklund, K.M.; Ehrlich, R.; Elia, R.; Foland, A.D.; Gaidarev, P.; Gittelman, B.; Gray, S.W.; Hartill, D.L.; Heltsley, B.K.; Hopman, P.I.; Kandaswamy, J.; Katayama, N.; Kim, P.C.; Kreinick, D.L.; Lee, T.; Liu, Y.; Ludwig, G.S.; Masui, J.; Mevissen, J.; Mistry, N.B.; Ng, C.R.; Nordberg, E.; Ogg, M.; Patterson, J.R.; Peterson, D.; Riley, D.; Soffer, A.; Ward, C. [Cornell University, Ithaca, New York 14853 (United States)] [Cornell University, Ithaca, New York 14853 (United States); Athanas, M.; Avery, P.; Jones, C.D.; Lohner, M.; Prescott, C.; Yang, S.; Yelton, J.; Zheng, J. [University of Florida, Gainesville, Florida 32611 (United States)] [University of Florida, Gainesville, Florida 32611 (United States); Brandenburg, G.; Briere, R.A.; Gao, Y.S.; Kim, D.Y.; Wilson, R.; Yamamoto, H. [Harvard University, Cambridge, Massachusetts 02138 (United States)] [Harvard University, Cambridge, Massachusetts 02138 (United States); Browder, T.E.; Li, F.; Li, Y.; Rodriguez, J.L. [University of Hawaii at Manoa, Honolulu, Hawaii 96822 (United States)] [University of Hawaii at Manoa, Honolulu, Hawaii 96822 (United States); Bergfeld, T.; Eisenstein, B.I.; Ernst, J.; Gladding, G.E.; Gollin, G.D.; Hans, R.M.; Johnson, E.; Karliner, I.; Marsh, M.A.; Palmer, M.; Selen, M.; Thaler, J.J. [University of Illinois, Champaign-Urbana, Illinois 61801 (United States)] [University of Illinois, Champaign-Urbana, Illinois 61801 (United States); Edwards, K.W. [Carleton University, Ottawa, Ontario, K1S 5B6 (Canada)] [Carleton University, Ottawa, Ontario, K1S 5B6 (Canada); Bellerive, A.; Janicek, R.; MacFarlane, D.B.; McLean, K.W.; Patel, P.M. [McGill University, Montreal, Quebec, (Canada)] [McGill University, Montreal, Quebec, (Canada)

1997-08-01T23:59:59.000Z

26

First Observation of Inclusive {ital B} Decays to the Charmed Strange Baryons {Xi}{sup 0}{sub {ital c}} and {Xi}{sup +}{sub {ital c}}  

SciTech Connect (OSTI)

Using data collected in the region of the {Upsilon}(4S) resonance with the CLEO II detector operating at the Cornell Electron Storage Ring (CESR), we present the first observation of B mesons decaying into the charmed strange baryons {Xi}{sup 0}{sub c} and {Xi}{sup +}{sub c} . We find 79{plus_minus}27 {Xi}{sup 0}{sub c} and 125{plus_minus}28 {Xi}{sup +}{sub c} candidates from B decays, leading to product branching fractions of B({bar B}{r_arrow}{Xi}{sup 0}{sub c}X)B({Xi}{sup 0}{sub c}{r_arrow}{Xi}{sup {minus}}{pi}{sup +})= (0.144{plus_minus}0.048 {plus_minus}0.021) {times}10{sup {minus}3} and B({bar B}{r_arrow}{Xi}{sup +}{sub c}X)B({Xi}{sup +}{sub C}{r_arrow} {Xi}{sup {minus}}{pi}{sup +}{pi}{sup +}) =(0.453{plus_minus} 0.096{sup +0.085}{sub {minus}0.065}){times} 10{sup {minus}3} . {copyright} {ital 1997} {ital The American Physical Society}

Barish, B.; Chadha, M.; Chan, S.; Eigen, G.; Miller, J.S.; OGrady, C.; Schmidtler, M.; Urheim, J.; Weinstein, A.J.; Wuerthwein, F. [California Institute of Technology, Pasadena, California 91125 (United States)] [California Institute of Technology, Pasadena, California 91125 (United States); Asner, D.M.; Bliss, D.W.; Brower, W.S.; Masek, G.; Paar, H.P.; Prell, S.; Sharma, V. [University of California, San Diego, La Jolla, California 92093 (United States)] [University of California, San Diego, La Jolla, California 92093 (United States); Gronberg, J.; Hill, T.S.; Kutschke, R.; Lange, D.J.; Menary, S.; Morrison, R.J.; Nelson, H.N.; Nelson, T.K.; Qiao, C.; Richman, J.D.; Roberts, D.; Ryd, A.; Witherell, M.S. [University of California, Santa Barbara, California 93106 (United States)] [University of California, Santa Barbara, California 93106 (United States); Balest, R.; Behrens, B.H.; Cho, K.; Ford, W.T.; Park, H.; Rankin, P.; Roy, J.; Smith, J.G. [University of Colorado, Boulder, Colorado 80309-0390 (United States)] [University of Colorado, Boulder, Colorado 80309-0390 (United States); Alexander, J.P.; Bebek, C.; Berger, B.E.; Berkelman, K.; Bloom, K.; Cassel, D.G.; Cho, H.A.; Coffman, D.M.; Crowcroft, D.S.; Dickson, M.; Drell, P.S.; Ecklund, K.M.; Ehrlich, R.; Elia, R.; Foland, A.D.; Gaidarev, P.; Gittelman, B.; Gray, S.W.; Hartill, D.L.; Heltsley, B.K.; Hopman, P.I.; Kandaswamy, J.; Kim, P.C.; Kreinick, D.L.; Lee, T.; Liu, Y.; Ludwig, G.S.; Masui, J.; Mevissen, J.; Mistry, N.B.; Ng, C.R.; Nordberg, E.; Ogg, M.; Patterson, J.R.; Peterson, D.; Riley, D.; Soffer, A.; Valant-Spaight, B.; Ward, C. [Cornell University, Ithaca, New York 14853 (United States)] [Cornell University, Ithaca, New York 14853 (United States); Athanas, M.; Avery, P.; Jones, C.D.; Lohner, M.; Prescott, C.; Yelton, J.; Zheng, J. [University of Florida, Gainesville, Florida 32611 (United States)] [University of Florida, Gainesville, Florida 32611 (United States); Brandenburg, G.; Briere, R.A.; Gao, Y.S.; Kim, D.Y.; Wilson, R.; Yamamoto, H. [Harvard University, Cambridge, Massachusetts 02138 (United States)] [Harvard University, Cambridge, Massachusetts 02138 (United States); Browder, T.E.; Li, F.; Li, Y.; Rodriguez, J.L. [University of Hawaii at Manoa, Honolulu, Hawaii 96822 (United States)] [University of Hawaii at Manoa, Honolulu, Hawaii 96822 (United States); Bergfeld, T.; Eisenstein, B.I.; Ernst, J.; Gladding, G.E.; Gollin, G.D.; Hans, R.M.; Johnson, E.; Karliner, I.; Marsh, M.A.; Palmer, M.; Selen, M.; Thaler, J.J.; and others

1997-11-01T23:59:59.000Z

27

Polygynous colony formation in the red imported fire ant, Solenopsis invicta Buren (Hymenoptera: Formicidae)  

E-Print Network [OSTI]

, probably on nursery root stock. S. invicta spread quickly throughout the southeastern United States. The black imported fire ant, ~sol** ' ' ht ' p 1, rl d ' 1 f h' earlier, before 1918, but did not spread as widely as the red imported fire ant... 1908; Peacock et al. 1955; Rettenmeyer & Watkins 1978; Scherba 1961; West- Eberhard 1978; Wilson 1971). In Solenopsis, S. ~x loni Id 1 1976) d 6. 9 t IAd t 1. 1976) I polygynous colonies. The phylogenetically distinct order Isoptera, the termites...

Stamps, William Terrell

1989-01-01T23:59:59.000Z

28

A Study of External Galaxies Detected by the {ital COBE} Diffuse Infrared Background Experiment  

SciTech Connect (OSTI)

A comparison of the {ital COBE} Diffuse Infrared Background Experiment (DIRBE) all-sky survey with the locations of known galaxies in the {ital IRAS} Catalog of Extragalactic Objects and the Center for Astrophysics Catalog of Galaxies led to the detection of as many as 57 galaxies. In this paper, we present the photometric data for these galaxies and an analysis of the seven galaxies that were detected at {lambda} {gt} 100 {mu}m. Estimates of the ratio of the mass of the cold dust (CD) component detected at {ital T}{sub {ital d}} = 20{endash}30 K to a very cold dust (VCD) component with {ital T}{sub {ital d}} {approx} 10{endash}15 K suggest that between 2{percent}{endash}100{percent} of the cirrus-like CD mass can also exist in many of these galaxies as VCD. In one galaxy, M33, the DIRBE photometry at 240 {mu}m suggests as much as 26 times as much VCD may be present as compared to the cirrus-like component. Further submillimeter measurements of this galaxy are required to verify such a large population of VCD. We also present 10 galaxies that were detected in the sky region not previously surveyed by {ital IRAS} and that can be used to construct a flux-limited all-sky catalog of galaxies brighter than 1000 Jy with a modest completeness limit of about 65{percent}. {copyright} {ital {copyright} 1998.} {ital The American Astronomical Society}

Odenwald, S. [Raytheon STX, Code 630.0, Goddard SFC, Greenbelt, MD 20771 (United States)] [Raytheon STX, Code 630.0, Goddard SFC, Greenbelt, MD 20771 (United States); Newmark, J. [Applied Research Corporation, Landover, MD 20785 (United States)] [Applied Research Corporation, Landover, MD 20785 (United States); Smoot, G. [Lawrence Berkeley Laboratory, University of California, Berkeley, CA 94720 (United States)] [Lawrence Berkeley Laboratory, University of California, Berkeley, CA 94720 (United States)

1998-06-01T23:59:59.000Z

29

Pressure contact probe for resistivity measurements in the temperature range 77 K/lt//ital T//lt/200 K  

SciTech Connect (OSTI)

We have designed and built a sample probe that is particularly well suited for measuring the resistivity and superconducting transition temperature /ital T//sub /ital c// of bulk high-/ital T//sub /ital c// materials of nonuniform shape, in the temperature range 77 K/lt//ital T//lt/200 K. The probe uses spring-loaded indium pressure contacts and allows electrical contact to be made without altering or contaminating the sample. The probe is relatively efficient because of its short turn-around time in mounting of samples and cylcing of temperature. The resistivity and /ital T//sub /ital c// of a bulk Y/sub 1/Ba/sub 2/Cu/sub 3/minus///sub /ital x//Ag/sub /ital x//O/sub 7/ sample was measured and the results compared with those from a more elaborate sample probe and Dewar system.

Tritt, T. M.; Ehrlich, A. C.; Davis, H. S.

1989-05-01T23:59:59.000Z

30

Reservoir characterization of the Ordovician Red River Formation in southwest Williston Basin Bowman County, ND and Harding County, SD  

SciTech Connect (OSTI)

This topical report is a compilation of characterizations by different disciplines of the Red River Formation in the southwest portion of the Williston Basin and the oil reservoirs which it contains in an area which straddles the state line between North Dakota and South Dakota. Goals of the report are to increase understanding of the reservoir rocks, oil-in-place, heterogeneity, and methods for improved recovery. The report is divided by discipline into five major sections: (1) geology, (2) petrography-petrophysical, (3) engineering, (4) case studies and (5) geophysical. Interwoven in these sections are results from demonstration wells which were drilled or selected for special testing to evaluate important concepts for field development and enhanced recovery. The Red River study area has been successfully explored with two-dimensional (2D) seismic. Improved reservoir characterization utilizing 3-dimensional (3D) and has been investigated for identification of structural and stratigraphic reservoir compartments. These seismic characterization tools are integrated with geological and engineering studies. Targeted drilling from predictions using 3D seismic for porosity development were successful in developing significant reserves at close distances to old wells. Short-lateral and horizontal drilling technologies were tested for improved completion efficiency. Lateral completions should improve economics for both primary and secondary recovery where low permeability is a problem and higher density drilling is limited by drilling cost. Low water injectivity and widely spaced wells have restricted the application of waterflooding in the past. Water injection tests were performed in both a vertical and a horizontal well. Data from these tests were used to predict long-term injection and oil recovery.

Sippel, M.A.; Luff, K.D.; Hendricks, M.L.; Eby, D.E.

1998-07-01T23:59:59.000Z

31

Relationship of the superoxide dismutase genes, sodA and sodB, to the iron uptake (/ital fur/) regulon in /ital Escherichia coli/ K-12  

SciTech Connect (OSTI)

Expression of sodA, as indicated by MnSod activity is normal in /ital fur/ mutants. This suggests that sodA is not a member of the /ital fur/ regulon and that the putative Fe-binding, regulatory protein of sodA, suggested by Moody and Hassan is not the Fur protein. by contrast, expression of sodB, as indicated by FeSod activity, is completely blocked in /ital fur/ mutants and the effect is restored by transformation with a plasmid having a normal /ital fur/ locus. The observations suggest that Fur, either directly or indirectly, controls SodB biosynthesis. Additional observations are described which indicate that SodB and Fur act together in a complicated fashion to control the biosynthesis of enterobactin. 26 refs., 3 tabs.

Niederhoffer, E.C.; Naranjo, C.M.; Fee, J.A.

1988-01-01T23:59:59.000Z

32

Two-deuteron correlation functions in [sup 14]N+[sup 27]Al collisions at [ital E]/[ital A]=75 MeV  

SciTech Connect (OSTI)

Both two-deuteron and two-proton correlation functions, at small relative momenta, have been measured for [sup 14]N+[sup 27]Al collisions at [ital E]/[ital A]=75 MeV. Data are compared to the predictions of a microscopic transport model which incorporates deuteron production and Coulomb interactions. The results indicate that deuterons are emitted over a shorter time span than protons.

Gong, W.G.; Danielewicz, P.; Gelbke, C.K.; Carlin, N.; de Souza, R.T.; Kim, Y.D.; Lynch, W.G.; Murakami, T.; Poggi, G.; Tsang, M.B.; Xu, H.M. (National Superconducting Cyclotron Laboratory and Department of Physics Astronomy, Michigan State University, East Lansing, Michigan 48824 (United States)); Pratt, S. (Department of Physics, University of Wisconsin, Madison, Wisconsin 53706 (United States)); Kwiatkowski, K.; Viola, V.E. Jr.; Yennello, S.J. (Indiana University Cyclotron Facility, Indiana University, Bloomington, Indiana 47405 (United States)); Shillcock, J.C. (Department of Physics, Simon Fraser University, Burnaby, British Columbia, V5A1S6 (Canada))

1993-02-01T23:59:59.000Z

33

Study of the high-[ital j] states in [sup 249]Cm  

SciTech Connect (OSTI)

We have performed the reaction [sup 248]Cm([sup 4]He,[sup 3]He) using 98.5-MeV alpha particles from the IUCF cyclotron to populate high-[ital j] states in [sup 249]Cm. A tentative assignment of the k[sub 17/2] component of the 1/2[sup +][880] Nilsson state has been made. [copyright] [ital 1998 American Institute of Physics.

Ahmad, I.; Back, B.B.; Chasman, R.R.; Greene, J.P.; Ishii, T.; Morss, L.R. (Argonne National Laboratory, Argonne, Illinois 60439 (United States)); Foster, C.C.; Lozowski, W.R.; Schmitt, W.; Stephenson, E.J.; Yamanaka, T. (Indiana University Cyclotron Facility, Bloomington, Indiana 47405 (United States))

1998-12-01T23:59:59.000Z

34

Determination of {sup 13}C NMR isotropic Knight shift and deviation from BCS relation in {ital A}{sub 3}C{sub 60} superconductors  

SciTech Connect (OSTI)

We determined the isotropic {sup 13}C NMR hyperfine coupling constant as {ital a}{sub iso}/2{pi}=0.69{plus_minus}0.06 MHz for the C{sub 60}{sup 3{minus}} ion near room temperature (RT). On this basis, the spin susceptibility at RT, {chi}{sub {ital s}}(RT), was estimated in various alkali-metal doped C{sub 60} compounds {ital A}{sub 3}C{sub 60}, which is approximately proportional to the lattice constant {ital a}{sub 0}; we found {ital d}{chi}{sub {ital s}}/{ital da}{sub 0}=(0.61{plus_minus}0.06){times}10{sup {minus}3} (emu/moleC{sub 60})/A . The correlation between the superconducting transition temperature {ital T}{sub {ital c}} and {chi}{sub {ital s}}(RT) was determined. It was found that {ital T}{sub {ital c}} of Na{sub 2}RbC{sub 60}, Na{sub 2}KC{sub 60}, Li{sub 2}CsC{sub 60}, and ammoniated {ital A}{sub 3}C{sub 60} is significantly lower than that expected from the BCS relation based on {chi}{sub {ital s}}(RT). {copyright} {ital 1996 The American Physical Society.}

Maniwa, Y.; Sugiura, D.; Kume, K. [Department of Physics, Tokyo Metropolitan University, Minami-osawa, Hachi-oji, Tokyo 192-03 (Japan)] [Department of Physics, Tokyo Metropolitan University, Minami-osawa, Hachi-oji, Tokyo 192-03 (Japan); Kikuchi, K.; Suzuki, S.; Achiba, Y. [Department of Chemistry, Tokyo Metropolitan University, Minami-osawa, Hachi-oji, Tokyo 192-03 (Japan)] [Department of Chemistry, Tokyo Metropolitan University, Minami-osawa, Hachi-oji, Tokyo 192-03 (Japan); Hirosawa, I.; Tanigaki, K. [NEC Corporation, 34 miyukigaoka, Tsukuba 305 (Japan)] [NEC Corporation, 34 miyukigaoka, Tsukuba 305 (Japan); Shimoda, H.; Iwasa, Y. [Japan Advanced Institute of Science and Technology, Tatsunokuchi, Ishikawa 923-12 (Japan)] [Japan Advanced Institute of Science and Technology, Tatsunokuchi, Ishikawa 923-12 (Japan)

1996-09-01T23:59:59.000Z

35

{ital S}-matrix analysis of heavy-ion elastic scattering  

SciTech Connect (OSTI)

A procedure to minimize {chi}{sup 2} is described which explores the fact that the {chi}{sup 2} distribution is of the fourth degree in the {ital S}-matrix elements. The fact that all three roots of the scale parameter for the minimum of {chi}{sup 2} in its gradient direction are algebraically determined gives the present procedure some global features that previous methods did not contemplate. The automatic search procedure also preserves the unitary bound constraint of the {ital S}-matrix at every step. When the search in the gradient direction slows down, the procedure reverts to the traditional quadratic approximation with zero-order regularization. The method is applied to the elastic scattering of the {sup 12}C+{sup 16}O reaction near the Coulomb barrier. {copyright} {ital 1996 The American Physical Society.}

Chiste, V.; Lichtenthaeler, R.; Villari, A.C.; Gomes, L.C. [Departamento de Fisica Nuclear, Laboratorio do Pelletron, Instituto de Fisica, Universidade de Sao Paulo, Caixa Postal 66318, 05389-970 - Sao Paulo, SP, (Brasil)

1996-08-01T23:59:59.000Z

36

Limit on the Two-Photon Production of the Glueball Candidate {ital f}{sub {ital J}}(2220) at the Cornell Electron Storage Ring  

SciTech Connect (OSTI)

We use the CLEO detector at the Cornell e{sup +}e{sup {minus}} storage ring, CESR, to search for the two-photon production of the glueball candidate f{sub J}(2220) in its decay to K{sub s}K{sub s} . We present a restrictive upper limit on the product of the two-photon partial width and the K{sub s}K{sub s} branching fraction, ({Gamma}{sub {gamma}{gamma}}B{sub K{sub s}K{sub s}}){sub f{sub J(2220) }} . We use this limit to calculate a lower limit on the stickiness, which is a measure of the two-gluon coupling relative to the two-photon coupling. This limit on stickiness indicates that the f{sub J}(2220) has substantial glueball content. {copyright} {ital 1997} {ital The American Physical Society}

Godang, R.; Kinoshita, K.; Lai, I.C.; Pomianowski, P.; Schrenk, S. [Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061 (United States)] [Virginia Polytechnic Institute and State University, Blacksburg, Virginia 24061 (United States); Bonvicini, G.; Cinabro, D.; Greene, R.; Perera, L.P.; Zhou, G.J. [Wayne State University, Detroit, Michigan 48202 (United States)] [Wayne State University, Detroit, Michigan 48202 (United States); Barish, B.; Chadha, M.; Chan, S.; Eigen, G.; Miller, J.S.; OGrady, C.; Schmidtler, M.; Urheim, J.; Weinstein, A.J.; Wuerthwein, F. [California Institute of Technology, Pasadena, California 91125 (United States)] [California Institute of Technology, Pasadena, California 91125 (United States); Asner, D.M.; Bliss, D.W.; Brower, W.S.; Masek, G.; Paar, H.P.; Prell, S.; Sivertz, M.; Sharma, V. [University of California, San Diego, La Jolla, California 92093 (United States)] [University of California, San Diego, La Jolla, California 92093 (United States); Gronberg, J.; Hill, T.S.; Kutschke, R.; Lange, D.J.; Menary, S.; Morrison, R.J.; Nelson, H.N.; Nelson, T.K.; Qiao, C.; Richman, J.D.; Roberts, D.; Ryd, A.; Witherell, M.S. [University of California, Santa Barbara, California 93106 (United States)] [University of California, Santa Barbara, California 93106 (United States); Balest, R.; Behrens, B.H.; Cho, K.; Ford, W.T.; Park, H.; Rankin, P.; Roy, J.; Smith, J.G. [University of Colorado, Boulder, Colorado 80309-0390 (United States)] [University of Colorado, Boulder, Colorado 80309-0390 (United States); Alexander, J.P.; Bebek, C.; Berger, B.E.; Berkelman, K.; Bloom, K.; Cassel, D.G.; Cho, H.A.; Coffman, D.M.; Crowcroft, D.S.; Dickson, M.; Drell, P.S.; Ecklund, K.M.; Ehrlich, R.; Elia, R.; Foland, A.D.; Gaidarev, P.; Galik, R.S.; Gittelman, B.; Gray, S.W.; Hartill, D.L.; Heltsley, B.K.; Hopman, P.I.; Kandaswamy, J.; Katayama, N.; Kim, P.C.; Kreinick, D.L.; Lee, T.; Liu, Y.; Ludwig, G.S.; Masui, J.; Mevissen, J.; Mistry, N.B.; Ng, C.R.; Nordberg, E.; Ogg, M.; Patterson, J.R.; Peterson, D.; Riley, D.; Soffer, A.; Ward, C. [Cornell University, Ithaca, New York 14853 (United States)] [Cornell University, Ithaca, New York 14853 (United States); Athanas, M.; Avery, P.; Jones, C.D.; Lohner, M.; Prescott, C.; Yelton, J.; Zheng, J. [University of Florida, Gainesville, Florida 32611 (United States)] [University of Florida, Gainesville, Florida 32611 (United States); Brandenburg, G.; Briere, R.A.; Gao, Y.S.; Kim, D.Y.; Wilson, R.; Yamamoto, H. [Harvard University, Cambridge (United States)] [Harvard University, Cambridge (United States)

1997-11-01T23:59:59.000Z

37

Multiplicity dependence of azimuthal distributions for [sup 36]Ar+[sup 197]Au collisions at [ital E]/[ital A]=35 MeV  

SciTech Connect (OSTI)

Collisions between [sup 36]Ar projectile and [sup 197]Au target nuclei at [ital E]/[ital A]=35 MeV have been studied with the Michigan State University Miniball, a 4[pi] phoswich array with a low detection threshold. Azimuthal distributions of charged particles with respect to the reaction plane are determined via the transverse-momentum-tensor method. Dependence on the kinetic energy of the emitted particles, the collision geometry, and the associated charged particle multiplicity is investigated. Corrections for the intrinsic resolution of the experimental reaction plane determination are applied. Scaling implied by the coalescence model is explored and the data are compared to the results of microscopic calculations within the Boltzmann-Uehling-Uhlenbeck theory.

Tsang, M.B.; Bowman, D.R.; Carlin, N.; Danielewicz, P.; Gelbke, C.K.; Gong, W.G.; Kim, Y.D.; Lynch, W.G.; Phair, L.; de Souza, R.T.; Zhu, F. (National Superconducting Cyclotron Laboratory and Department of Physics Astronomy, Michigan State University, East Lansing, Michigan 48824 (United States))

1993-06-01T23:59:59.000Z

38

Overrelaxation phenomena during the formation of reversed-field pinch plasmas  

SciTech Connect (OSTI)

Experiments on the Extrap T1 reversed-field pinch (RFP) [Phys. Scr. {bold 49}, 224 (1994)] have shown that the formation of the RFP configuration is quite sensitive to the relative programming of the toroidal field and Ohmic heating circuits. In this paper, new measurements of the evolution of the current density profile and of the spectral structure of the fluctuations during the setup phase of RFP plasmas in the T1 experiment are presented. These measurements improve the understanding of the role of different spectral components in the dynamics of RFP formation. Under unfavorable (slow) setup conditions, comparatively high energy is accumulated in {ital m}=1 internal kinks prior to reversal of the edge toroidal field. At reversal, nonlinearly driven {ital m}=0 modes trigger a rapid broadening of the {ital m}=1 spectrum. This behavior is associated with a violent suppression of the current density in the core, leading to an overrelaxation of the discharge involving a hollowing of the parallel current density profile. The setup conditions are found to affect the volt-second consumption and plasma/wall interaction during RFP formation, as well as the flat-top discharge performance. {copyright} {ital 1995} {ital American} {ital Institute} {ital of} {ital Physics}.

Mazur, S.; Nordlund, P. [Division of Fusion Plasma Physics (Association EURATOM-NFR), Alfven Laboratory, Royal Institute of Technology, S-100 44 Stockholm (Sweden)] [Division of Fusion Plasma Physics (Association EURATOM-NFR), Alfven Laboratory, Royal Institute of Technology, S-100 44 Stockholm (Sweden)

1995-10-01T23:59:59.000Z

39

Log-derived evaluation of gas-bearing Cherokee, Red Fork, and Morrow formations, Custer County, OK  

SciTech Connect (OSTI)

Medium to low porosity and rather tight Cherokee, Red Fork and Morrow sands, located in Oklahoma, contain significant hydrocarbon resources. To evaluate the commercial importance of wells drilled in Custer County, Oklahoma, an innovative digital shaly sand analysis approach (CLASS - Epilog) has been applied, which provides information on total and effective reservoir porosity, total and effective fluid distribution based on the Waxman-Smits equation, shaliness, clay typing, and reservoir productivity. Several field case examples are presented and discussed based on (1) open hole logging suite, consisting of induction, compensated density/neutron and Spectralog, (2) CLASS analysis, (3) well completion and stimulation data, and (4) the resulting production test results.

Busch, E.A.; Fertl, W.H.; Neill, B.E.; Sinha, A.K.; Sobkowich, K.N.

1985-03-01T23:59:59.000Z

40

Spin and charge dynamics of the two-dimensional {ital t}-{ital J} model at intermediate electron densities: Absence of spin-charge separation  

SciTech Connect (OSTI)

We present an exact diagonalization study of the dynamical spin and density correlation functions in small clusters of the {ital t}-{ital J} model, focusing on the regime of intermediate and low electron densities, {rho}{sub {ital e}}{lt}0.5. In two dimensions (2D) both correlation functions agree remarkably well with the convolution of the single-particle spectral function, i.e., the simplest estimate possible within a Fermi-liquid picture. Deviations from the convolution are shown to originate from symmetry-related selection rules, which are unaccounted for in the convolution estimate. For all fillngs under consideration, we show that the low-energy peaks originate from particle-hole excitations between the Fermi momenta, as expected for a Fermi liquid. We contrast this with the behavior in 1D, where spin and density correlation function show the differences characteristic of spin-charge separation and where neither correlation function is approximated well by the convolution.

Eder, R.; Ohta, Y. [Department of Applied Physics, Nagoya University, Nagoya 464-01 (Japan)] [Department of Applied Physics, Nagoya University, Nagoya 464-01 (Japan)

1995-05-01T23:59:59.000Z

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
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41

Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger  

E-Print Network [OSTI]

Mergers of binary neutron stars (NSs) usually result in the formation of a hypermassive neutron star (HMNS). Whether- and when this remnant collapses to a black hole (BH) depends primarily on the equation of state and on angular momentum transport processes, both of which are uncertain. Here we show that the lifetime of the merger remnant may be directly imprinted in the radioactively powered kilonova emission following the merger. We employ axisymmetric, time-dependent hydrodynamic simulations of remnant accretion disks orbiting a HMNS of variable lifetime, and characterize the effect of this delay to BH formation on the disk wind ejecta. When BH formation is relatively prompt (~ 100 ms), outflows from the disk are sufficiently neutron rich to form heavy r-process elements, resulting in ~ week-long emission with a spectral peak in the near-infrared (NIR), similar to that produced by the dynamical ejecta. In contrast, delayed BH formation allows neutrinos from the HMNS to raise the electron fraction in the polar direction to values such that potentially Lanthanide-free outflows are generated. The lower opacity would produce a brighter, bluer, and shorter-lived ~ day-long emission (a `blue bump') prior to the late NIR peak from the dynamical ejecta and equatorial wind. This new diagnostic of BH formation should be useful for events with a signal to noise lower than that required for direct detection of gravitational waveform signatures.

Brian D. Metzger; Rodrigo Fernndez

2014-05-02T23:59:59.000Z

42

THE ASYMPTOTIC GIANT BRANCH AND THE TIP OF THE RED GIANT BRANCH AS PROBES OF STAR FORMATION HISTORY: THE NEARBY DWARF IRREGULAR GALAXY KKH 98  

SciTech Connect (OSTI)

We investigate the utility of the asymptotic giant branch (AGB) and the red giant branch (RGB) as probes of the star formation history (SFH) of the nearby (D = 2.5 Mpc) dwarf irregular galaxy, KKH 98. Near-infrared (near-IR) Keck Laser Guide Star Adaptive Optics (AO) images resolve 592 IR-bright stars reaching over 1 mag below the tip of the RGB. Significantly deeper optical (F475W and F814W) Hubble Space Telescope images of the same field contain over 2500 stars, reaching to the red clump and the main-sequence turnoff for 0.5 Gyr old populations. Compared to the optical color-magnitude diagram (CMD), the near-IR CMD shows significantly tighter AGB sequences, providing a good probe of the intermediate-age (0.5-5 Gyr) populations. We match observed CMDs with stellar evolution models to recover the SFH of KKH 98. On average, the galaxy has experienced relatively constant low-level star formation (5 x 10{sup -4} M{sub sun} yr{sup -1}) for much of cosmic time. Except for the youngest main-sequence populations (age <0.1 Gyr), which are typically fainter than the AO data flux limit, the SFH estimated from the 592 IR-bright stars is a reasonable match to that derived from the much larger optical data set. Differences between the optical- and IR-derived SFHs for 0.1-1 Gyr populations suggest that current stellar evolution models may be overproducing the AGB by as much as a factor of 3 in this galaxy. At the depth of the AO data, the IR-luminous stars are not crowded. Therefore, these techniques can potentially be used to determine the stellar populations of galaxies at significantly further distances.

Melbourne, J. [Caltech Optical Observatories, Division of Physics, Mathematics and Astronomy, Mail Stop 301-17, California Institute of Technology, Pasadena, CA 91125 (United States); Williams, B.; Dalcanton, J. [Department of Astronomy, Box 351580, University of Washington, Seattle, WA 98195 (United States); Ammons, S. M.; Max, C.; Koo, D. C. [University of California Observatories/Lick Observatory, Department of Astronomy and Astrophysics, University of California at Santa Cruz, 1156 High Street, Santa Cruz, CA 95064 (United States); Girardi, Leo [Osservatorio Astronomico di Padova-INAF, Padova (Italy); Dolphin, A., E-mail: jmel@caltech.ed, E-mail: ben@astro.washington.ed, E-mail: jd@astro.washington.ed, E-mail: ammons@ucolick.or, E-mail: max@ucolick.or, E-mail: koo@ucolick.or, E-mail: leo.girardi@oapd.inaf.i, E-mail: adolphin@raytheon.co [Raytheon, 1151 E. Hermans Road, Tucson, AZ 85706 (United States)

2010-03-20T23:59:59.000Z

43

Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger  

E-Print Network [OSTI]

Mergers of binary neutron stars (NSs) usually result in the formation of a hypermassive neutron star (HMNS). Whether- and when this remnant collapses to a black hole (BH) depends primarily on the equation of state and on angular momentum transport processes, both of which are uncertain. Here we show that the lifetime of the merger remnant may be directly imprinted in the radioactively powered kilonova emission following the merger. We employ axisymmetric, time-dependent hydrodynamic simulations of remnant accretion disks orbiting a HMNS of variable lifetime, and characterize the effect of this delay to BH formation on the disk wind ejecta. Our models follow the system evolution over several seconds, and include the effect of nuclear recombination, viscous heating, and neutrino irradiation by both the HMNS and the disk. When BH formation is relatively prompt ( 140, resulting in ~week-long emission with a spectral peak in the near-infrared (NIR), similar to that produced by the dynamical ejecta. In contrast, de...

Metzger, Brian D

2014-01-01T23:59:59.000Z

44

The {ital b} Distribution and the Velocity Structure of Absorption Peaks in the Ly{alpha} Forest  

SciTech Connect (OSTI)

A theory is developed that relates the observed {ital b} parameter of a Ly{alpha} absorption line to the velocity curvature of the corresponding peak in the optical depth fluctuation. Its relation to the traditional interpretation of {ital b} as the thermal broadening width is discussed. It is demonstrated that, independent of the details of the cosmological model, the differential {ital b} distribution has a high-{ital b} asymptote of dN/db{proportional_to}b{sup {minus}m}, where m{ge}5, when we make the reasonable assumption that low-curvature fluctuations are statistically favored over high-curvature ones. There in general always exist lines much broader than the thermal width. We develop a linear perturbative analysis of the optical depth fluctuation, which yields a single-parameter prediction for the full {ital b} distribution. In addition to exhibiting the high-velocity tail, it qualitatively explains the observed sharp low-{ital b} cutoff{emdash}a simple reflection of the fact that high-curvature fluctuations are relatively rare. Although the existence of the high-{ital b} asymptote, which is independent of the validity of the linear expansion, is consistent with the observed {ital b} distribution, a detailed comparison of the linear prediction with six observational data sets indicates that higher order corrections are not negligible. The perturbative analysis nonetheless offers valuable insights into the dependence of the {ital b} distribution on cosmological parameters such as {Omega} and the power spectrum. A key parameter is the effective smoothing scale of the optical depth fluctuation, which is in turn determined by three scales: the thermal broadening width, the baryon smoothing scale (approximately the Jeans scale), and the observation/simulation resolution. The first two are determined by reionization history, but are comparable in general, whereas the third varies by about an order of magnitude in current hydrodynamic simulations. Studies with non{endash}resolution-dominated {ital b} distributions can be used to probe the reionization history of the universe. {copyright} {ital {copyright} 1999.} {ital The American Astronomical Society}

Hui, L. [NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States)] [NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States); Rutledge, R.E. [Max-Planck-Institut fuer extraterrestrische Physik, Postfach 1603, D-85740 Garching (Germany)] [Max-Planck-Institut fuer extraterrestrische Physik, Postfach 1603, D-85740 Garching (Germany)

1999-06-01T23:59:59.000Z

45

The [ital b] Distribution and the Velocity Structure of Absorption Peaks in the Ly[alpha] Forest  

SciTech Connect (OSTI)

A theory is developed that relates the observed [ital b] parameter of a Ly[alpha] absorption line to the velocity curvature of the corresponding peak in the optical depth fluctuation. Its relation to the traditional interpretation of [ital b] as the thermal broadening width is discussed. It is demonstrated that, independent of the details of the cosmological model, the differential [ital b] distribution has a high-[ital b] asymptote of dN/db[proportional to]b[sup [minus]m], where m[ge]5, when we make the reasonable assumption that low-curvature fluctuations are statistically favored over high-curvature ones. There in general always exist lines much broader than the thermal width. We develop a linear perturbative analysis of the optical depth fluctuation, which yields a single-parameter prediction for the full [ital b] distribution. In addition to exhibiting the high-velocity tail, it qualitatively explains the observed sharp low-[ital b] cutoff[emdash]a simple reflection of the fact that high-curvature fluctuations are relatively rare. Although the existence of the high-[ital b] asymptote, which is independent of the validity of the linear expansion, is consistent with the observed [ital b] distribution, a detailed comparison of the linear prediction with six observational data sets indicates that higher order corrections are not negligible. The perturbative analysis nonetheless offers valuable insights into the dependence of the [ital b] distribution on cosmological parameters such as [Omega] and the power spectrum. A key parameter is the effective smoothing scale of the optical depth fluctuation, which is in turn determined by three scales: the thermal broadening width, the baryon smoothing scale (approximately the Jeans scale), and the observation/simulation resolution. The first two are determined by reionization history, but are comparable in general, whereas the third varies by about an order of magnitude in current hydrodynamic simulations. Studies with non[endash]resolution-dominated [ital b] distributions can be used to probe the reionization history of the universe. [copyright] [ital [copyright] 1999.] [ital The American Astronomical Society

Hui, L. (NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510 (United States)); Rutledge, R.E. (Max-Planck-Institut fuer extraterrestrische Physik, Postfach 1603, D-85740 Garching (Germany))

1999-06-01T23:59:59.000Z

46

Benchmark single-differential ionization cross section results for the {ital s}-wave model of electron-hydrogen scattering  

SciTech Connect (OSTI)

Exterior complex scaling enables one to compute the outgoing wave portion of the wave function for three charged particles without explicitly imposing the asymptotic boundary condition for three-body breakup. This technique is used in connection with a high-order finite difference scheme to provide numerically accurate single-differential ionization cross sections for the Temkin-Poet ({ital s}-wave) model of e-H scattering. These benchmark values are compared with results obtained from several recent close-coupling approaches that employ pseudostates to discretize the ionization continuum, but use a strictly two-body scattering formalism. {copyright} {ital 1999} {ital The American Physical Society}

Baertschy, M. [Department of Applied Science, University of California--Davis, Livermore, California 94550 (United States)] [Department of Applied Science, University of California--Davis, Livermore, California 94550 (United States); Rescigno, T.N. [Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)] [Lawrence Livermore National Laboratory, Livermore, California 94550 (United States); Isaacs, W.A.; McCurdy, C.W. [Lawrence Berkeley National Laboratory, Berkeley, California 94720 (United States)] [Lawrence Berkeley National Laboratory, Berkeley, California 94720 (United States)

1999-07-01T23:59:59.000Z

47

GALAXY-SCALE STAR FORMATION ON THE RED SEQUENCE: THE CONTINUED GROWTH OF S0s AND THE QUIESCENCE OF ELLIPTICALS  

SciTech Connect (OSTI)

This paper examines star formation (SF) in relatively massive, primarily early-type galaxies (ETGs) at z {approx} 0.1. A sample is drawn from bulge-dominated Galaxy Evolution Explorer/Sloan Digital Sky Survey (GALEX/SDSS) galaxies on the optical red sequence with strong UV excess and yet quiescent SDSS spectra. High-resolution far-UV imaging of 27 such ETGs using Hubble Space Telescope Advanced Camera for Surveys/Solar Blind Channel (ACS/SBC) reveals structured UV morphology in 93% of the sample, consistent with low-level ongoing SF ({approx}0.5 M{sub Sun} yr{sup -1}). In 3/4 of the sample the SF is extended on galaxy scales (25-75 kpc), while the rest contains smaller (5-15 kpc) SF patches in the vicinity of an ETG-presumably gas-rich satellites being disrupted. Optical imaging reveals that all ETGs with galaxy-scale SF in our sample have old stellar disks (mostly S0 type). None is classified as a true elliptical. In our sample, galaxy-scale SF takes the form of UV rings of varying sizes and morphologies. For the majority of such objects we conclude that the gas needed to fuel current SF has been accreted from the intergalactic medium, probably in a prolonged, quasi-static manner, leading in some cases to additional disk buildup. The remaining ETGs with galaxy-scale SF have UV and optical morphologies consistent with minor merger-driven SF or with the final stages of SF in fading spirals. Our analysis excludes that all recent SF on the red sequence resulted from gas-rich mergers. We find further evidence that galaxy-scale SF is almost exclusively an S0 phenomenon ({approx}20% S0s have SF) by examining the overall optically red SDSS ETGs. Conclusion is that significant number of field S0s maintain or resume low-level SF because the preventive feedback is not in place or is intermittent. True ellipticals, on the other hand, stay entirely quiescent even in the field.

Salim, Samir [Department of Astronomy, Indiana University, Bloomington, IN 47404 (United States); Fang, Jerome J.; Faber, S. M. [University of California Observatories/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States); Rich, R. Michael [Department of Physics and Astronomy, University of California, Los Angeles, CA 90095 (United States); Thilker, David A., E-mail: salims@indiana.edu [Center for Astrophysical Sciences, Johns Hopkins University, Baltimore, MD 21218 (United States)

2012-08-20T23:59:59.000Z

48

Lateral drilling and completion technologies for shallow-shelf carbonates of the Red River and Ratcliffe Formations, Williston Basin. Topical report, July 1997  

SciTech Connect (OSTI)

Luff Exploration Company (LEC) focused on involvement in technologies being developed utilizing horizontal drilling concepts to enhance oil-well productivity starting in 1992. Initial efforts were directed toward high-pressure lateral jetting techniques to be applied in existing vertical wells. After involvement in several failed field attempts with jetting technologies, emphasis shifted to application of emerging technologies for drilling short-radius lateral in existing wellbores and medium-radius technologies in new wells. These lateral drilling technologies were applied in the Mississippi Ratcliffe and Ordovician Red River formations at depths of 2,590 to 2,890 m in Richland County, MT; Bowman County, ND; and Harding County, SD. In theory, all of the horizontal drilling techniques explored in this project have merit for application fitting specific criteria. From a realistic point of view, the only relatively trouble-free, adequately-proven technology employed was the medium-radius steered motor/MWD technology. The slim-tool steered motor/MWD re-entry technology has been used extensively but appears to still be significantly in developmental stages. This technology will probably always be more troublesome than the technology used to drill new wells because the smaller diameter required for the tools contributes to both design and operational complexities. Although limited mechanical success has been achieved with some of the lateral jetting technologies and the Amoco tools, their predictability and reliability is unproven. Additionally, they appear to be limited to shallow depths and certain rock types. The Amoco technology probably has the most potential to be successfully developed for routinely reliable, field applications. A comparison of the various horizontal drilling technologies investigated is presented.

Carrell, L.A.; George, R.D.; Gibbons, D.

1998-07-01T23:59:59.000Z

49

Red Sky with Red Mesa  

ScienceCinema (OSTI)

The Red Sky/Red Mesa supercomputing platform dramatically reduces the time required to simulate complex fuel models, from 4-6 months to just 4 weeks, allowing researchers to accelerate the pace at which they can address these complex problems. Its speed also reduces the need for laboratory and field testing, allowing for energy reduction far beyond data center walls.

None

2014-06-23T23:59:59.000Z

50

Red Giant Red Giant White Giant  

E-Print Network [OSTI]

Red Giant Red Giant White Giant Red Giant White Giant White Giant Blue Giant Blue Giant Blue Giant. Proxima Centauri, the closest star to the Sun, is a red giant. Mass: 1- 4 Solar Mass StarPower Points: 7

Bechtold, Jill

51

{sup 6}Li({pi}{sup +}, {ital pp}){sup 4}He{sub g.s.} reaction at 100 and 165 MeV incident pion energies  

SciTech Connect (OSTI)

Differential and total cross sections for {pi}{sup +} absorption on {sup 6}Li leading to the {ital pp}+{sup 4}He{sub g.s} final state are presented at incident pion energies of 100 and 165 MeV. The narrow width of the {ital pp} angular correlation is observed and reported.

Papandreou, Z.; Huber, G.; Lolos, G.; Cormier, J.; Mathie, E.; Naqvi, S. [Department of Physics, University of Regina, Regina, Saskatchewan, S4S 0A2 (Canada)] [Department of Physics, University of Regina, Regina, Saskatchewan, S4S 0A2 (Canada); Ottewell, D.; Tacik, R.; Walden, P. [TRIUMF, Vancouver, British Columbia, V6T 2A3 (Canada)] [TRIUMF, Vancouver, British Columbia, V6T 2A3 (Canada); Jones, G.; Trelle, R. [Department of Physics, University of British Columbia, Vancouver, British Columbia, V6T 2A6 (Canada)] [Department of Physics, University of British Columbia, Vancouver, British Columbia, V6T 2A6 (Canada); Aslanoglou, X. [Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701 (United States)] [Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701 (United States); Humphrey, D. [Department of Physics and Astronomy, Western Kentucky University, Bowling Green, Kentucky 42101 (United States)] [Department of Physics and Astronomy, Western Kentucky University, Bowling Green, Kentucky 42101 (United States)

1995-06-01T23:59:59.000Z

52

Equatorial spread {ital F} effects on an HF path: Doppler spread, spatial coherence, and frequency coherence  

SciTech Connect (OSTI)

In August 1990 we participated in the Equatorial Ionospheric Studies sounding rocket campaign near Kwajalein Atoll in the equatorial Pacific region. The campaign included measurements of plasma density using rocket probes and coherent and incoherent scatter radar. During the campaign we fielded high-frequency ionospheric sounders over a bistatic path between Maloelap Atoll and Bikini Atoll in the Marshall Islands. The distance between the transmitters and receivers was 700 km; the ionospheric-reflection region was at 10.18; {degree}N, 168.40;{degree}E, near the magnetic equator. We made three types of measurements: Doppler spread and spatial coherence for a single-frequency CW path; frequency coherence of multiple CW paths; and Doppler spread and time-delay spread for a 60-kHz bandwidth path. We obtained such data over a period of 2 weeks for approximately 2 hours each evening; during this period spread {ital F} was common. Fifty percent of the evenings showed Doppler spread of greater than 6 Hz at the {minus}10 dB level (relative to the peak signal power) and greater than 15 Hz at the {minus}30 dB level. Forty percent of the evenings showed spatial coherence distance of less than 180 m in the direction normal to the bistatic path; 40{percent} of the evenings showed spatial coherence of less than 75 m in the direction parallel to the path. Seventy-five percent of the evenings showed coherence bandwidths of less than 1.5 kHz. {copyright} 1999 American Geophysical Union

Fitzgerald, T.J.; Argo, P.E.; Carlos, R.C. [Los Alamos National Laboratory, Los Alamos, New Mexico (United States)] [Los Alamos National Laboratory, Los Alamos, New Mexico (United States)

1999-01-01T23:59:59.000Z

53

Red Cabbage Smoothie Ingredients  

E-Print Network [OSTI]

Red Cabbage Smoothie Ingredients · 1 1/2 cups cold water · 1/2 small head red cabbage, quartered: http://www.accordingtoelle.com/2014/05/red-cabbage-smoothie/ Recipe provided by former chef

Myers, Lawrence C.

54

Red River Compact (Texas)  

Broader source: Energy.gov [DOE]

The Red River Compact Commission administers the Red River Compact to ensure that Texas receives its equitable share of quality water from the Red River and its tributaries as apportioned by the...

55

Code Red 2 kills off Code Red 1  

E-Print Network [OSTI]

#12;#12;Code Red 2 kills off Code Red 1 Code Red 2 settles into weekly pattern Nimda enters the ecosystem Code Red 2 dies off as programmed CR 1 returns thanks to bad clocks #12;Code Red 2 dies off as programmed Nimda hums along, slowly cleaned up With its predator gone, Code Red 1 comes back, still

Paxson, Vern

56

Mechanical alloying of Si and Ge in a planetary ball mill: Milling parameters and microscopic evolution of alloy formation  

SciTech Connect (OSTI)

The external parameters geometry and frequency of a planetary ball mill were adjusted in order to minimize the duration of mechanically induced Si-Ge alloy formation. Experimental results were compared with theoretical calculations on impact energies and milling power. It was found that a planetary ball mill with a ratio of the planetary to the system wheel`s frequency of {minus}3 delivers the best milling performance for vial sizes between 0.2 and 0.33 that of the system wheel size. Microstructural investigations on powder compacts revealed that a solid state diffusion mechanism of Ge into the harder Si seems to be the responsible process for realizing a homogeneous Si-Ge alloy. Crystallite sizes of the processed powders were 30 nm. The knowledge of the influence of external milling parameters on the comminution and alloying behavior of substances and the resulting internal structure of the processed ingots may help in a future correlation between thermoelectrical properties and microstructure. {copyright} {ital 1995} {ital American} {ital Institute} {ital of} {ital Physics}.

Schilz, J.; Pixius, K.; Amend, W. [Institute of Materials Research, German Aerospace Research Establishment (DLR), Linder Hoehe, 51147 Koehn (Germany); Plate, M.; Meyer, H. [Retsch Co., Rheinische Str. 36, 42781 Haan (Germany)

1994-08-10T23:59:59.000Z

57

69. Red Butte-Red Fir Ridge (Shasta Red Fir) (Imper 1988b, Cheng 1996d)  

E-Print Network [OSTI]

69. Red Butte-Red Fir Ridge (Shasta Red Fir) (Imper 1988b, Cheng 1996d) Location This established (fig. 139). Ecological subsection ­ High Cascades (M261Df). Target Element Red Fir (Abies magnifica) Distinctive Features Shasta Red Fir Forest: Taxonomically, the description of Shasta red fir (Abies magnifica

Standiford, Richard B.

58

Buoyancy-driven circulation in the Red Sea  

E-Print Network [OSTI]

This thesis explores the buoyancy-driven circulation in the Red Sea, using a combination of observations, as well as numerical modeling and analytical method. The first part of the thesis investigates the formation mechanism ...

Zhai, Ping, Ph. D. Massachusetts Institute of Technology

2014-01-01T23:59:59.000Z

59

Red Pepper Sauce  

E-Print Network [OSTI]

... chopped 2 cloves garlic, minced 1/4 cup water 1/2 Tbs. white wine vinegar 1/8 tsp. crushed red pepper 1/8 tsp. white pepper dash or two Tabasco sauce 1/2 to...

60

Ayrshire Red Squirrel Group Squirrelpox  

E-Print Network [OSTI]

Ayrshire Red Squirrel Group SSG Report 1st March 2012 Squirrelpox Sero-positive grey squirrels. Concerns are also rising that there may be outbreaks of pox in red squirrel populations which have gone

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


61

Are red 2MASS QSOs young?  

E-Print Network [OSTI]

We use photometric data from Spitzer to explore the mid- and far-IR properties of 10 red QSOs (J-K>2, R-K>5) selected by combining the 2MASS in the NIR with the SDSS at optical wavelengths. Optical and/or near-infrared spectra are available for 8/10 sources. Modeling the SED from UV to far-IR shows that moderate dust reddening (A_V=1.3-3.2) can explain the red optical and near-IR colours of the sources in the sample. There is also evidence that red QSOs have 60/12micron luminosity ratio higher than PG QSOs (97% significance). This can be interpreted as a higher level of star-formation in these systems (measured by the 60micron luminosity) for a given AGN power (approximated by the 12micron luminosity). This is consistent with a picture where red QSOs represent an early phase of AGN evolution, when the supermassive black hole is enshrouded in dust and gas clouds, which will eventually be blown out (possibly by AGN driven outflows) and the system will appear as typical optically luminous QSO. There is also tentative evidence significant at the 96% level that red 2MASS QSOs are more often associated with radio emission than optically selected SDSS QSOs. This may indicate outflows, also consistent with the young AGN interpretation. We also estimate the space density of red QSOs relative to optically selected SDSS QSOs, taking into account the effect of dust extinction and the intrinsic luminosity of the sources. We estimate that the fraction of red QSOs in the overall population increases from 3% at M_K=-27.5mag to 12% at M_K=-29.5mag. This suggests that reddened QSOs become more important at the bright end of the Luminosity Function. If red QSOs are transition objects on the way to becoming typical optically luminous QSOs, the low fractions above suggest that these systems spent <12% of their lifetime at the "reddened" stage.

A. Georgakakis; D. L. Clements; G. Bendo; M. Rowan-Robinson; K. Nandra; M. S. Brotherton

2008-12-10T23:59:59.000Z

62

Red-black Tree Jingjing Xia  

E-Print Network [OSTI]

Advanced Algorithm Design Red-black Tree Jingjing Xia #12;Red-Black Tree A red-black tree is a binary search tree, and each node contains one extra field: its color, it can be either black or red of the binary search tree. If a binary search tree satisfies all the following red-black properties, it is a red

Chen, Yangjun

63

www.vopen.net 1994 Young Mark Ewing Red Hat Red H  

E-Print Network [OSTI]

www.vopen.net Linux --- 1994 Young Mark Ewing Red Hat Red H at Linux Linux Red Hat Linux Red Hat Linux Red Hat Linux MandrakeSOT BestConnectivaAbit KondaraRed Hat Linux 2001 4 16 Red Hat Red Hat Linux 7.1 Red Hat Linux 1 1.1 1 Linux 2.4.2 2 Xfree86 4.0.3 3 4 Big5 5 CPU CPU 4

Li, Tiejun

64

OBSERVATIONAL CONSTRAINTS ON RED AND BLUE HELIUM BURNING SEQUENCES  

SciTech Connect (OSTI)

We derive the optical luminosity, colors, and ratios of the blue and red helium burning (HeB) stellar populations from archival Hubble Space Telescope observations of nineteen starburst dwarf galaxies and compare them with theoretical isochrones from Padova stellar evolution models across metallicities from Z = 0.001 to 0.009. We find that the observational data and the theoretical isochrones for both blue and red HeB populations overlap in optical luminosities and colors and the observed and predicted blue to red HeB ratios agree for stars older than 50 Myr over the time bins studied. These findings confirm the usefulness of applying isochrones to interpret observations of HeB populations. However, there are significant differences, especially for the red HeB population. Specifically, we find (1) offsets in color between the observations and theoretical isochrones of order 0.15 mag (0.5 mag) for the blue (red) HeB populations brighter than M{sub V} {approx} -4 mag, which cannot be solely due to differential extinction; (2) blue HeB stars fainter than M{sub V} {approx} -3 mag are bluer than predicted; (3) the slope of the red HeB sequence is shallower than predicted by a factor of {approx}3; and (4) the models overpredict the ratio of the most luminous blue to red HeB stars corresponding to ages {approx}< 50 Myr. Additionally, we find that for the more metal-rich galaxies in our sample (Z {approx}> 0.5 Z{sub sun}), the red HeB stars overlap with the red giant branch stars in the color-magnitude diagrams, thus reducing their usefulness as indicators of star formation for ages {approx}> 100 Myr.

McQuinn, Kristen B. W.; Skillman, Evan D. [Department of Astronomy, School of Physics and Astronomy, 116 Church Street, S.E., University of Minnesota, Minneapolis, MN 55455 (United States); Dalcanton, Julianne J.; Weisz, Daniel R.; Williams, Benjamin F. [Department of Astronomy, Box 351580, University of Washington, Seattle, WA 98195 (United States); Dolphin, Andrew E. [Raytheon Company, 1151 E. Hermans Road, Tucson, AZ 85706 (United States); Holtzman, Jon, E-mail: kmcquinn@astro.umn.edu [Department of Astronomy, New Mexico State University, Box 30001-Department 4500, 1320 Frenger Street, Las Cruces, NM 88003 (United States)

2011-10-10T23:59:59.000Z

65

Ambiguous Red Shifts  

E-Print Network [OSTI]

A one-parameter conformal invariance of Maxwell's equations allows the wavelengths of electromagnetic waves to change as they propagate, and do so even in otherwise field-free space. This produces an ambiguity in interpretations of stellar red shifts. Experiments that will determine the value of the group parameter, and thereby remove the ambiguity, are proposed. They are based on an analysis of the anomalous frequency shifts uncovered in the Pioneer 10 and 11 spacecraft studies, and physical interpretation of an isomorphism discovered by E. L. Hill. If the group parameter is found to be non-zero, Hubble's relations will have to be reinterpreted and space-time metrics will have to be altered. The cosmological consequences of the transformations are even more extensive because, though they change frequencies, they do not alter the energy and momentum conservations laws of classical and quantum-electrodynamical fields established by Cunningham and by Bialynicki-Birula.

Carl E. Wulfman

2010-10-11T23:59:59.000Z

66

Red Means Go Structural Engineering  

E-Print Network [OSTI]

Red Means Go Structural Engineering: An Overview of Global Directions Marc Hoit, Ph.D. Vice Chancellor for IT Professor of Civil Engineering #12;Red Means Go Overview · Global trends affecting on advanced degrees · Educate for the "Smile" Creativity as fundamental education Entrepreneurs ­ Need

67

Red Raider Orientation COLLEGE DISMISSAL  

E-Print Network [OSTI]

and Management Wildlife Science #12;RED RAIDER ORIENTATION University Studies University Studies Wind Energy Center, City of Lubbock · Information Sessions and Campus Resource Fair · Dinner on your own and Parent Communications, etc.) #12;#12;RED RAIDER ORIENTATION Business Administration Accounting Energy Commerce

Rock, Chris

68

White Baneberry and Red Baneberry  

E-Print Network [OSTI]

1 White Baneberry and Red Baneberry Actaea pachypoda and Actaea rubra buttercup family (ranunculaceae) both white baneberry and red baneberry are poisonous plants native to the northeast inhabit swamps. Range: white baneberry--parts of the canadian mari- times and the southern border

Landweber, Laura

69

Red Rice Research and Control.  

E-Print Network [OSTI]

s cu l t iva ted white r i c e , Oryza sativa L. Red r i c e crosses read i ly .- with white r i c e and i s very s i m i l a r t o it i n appearance. The main morpho- logical d i f ferences t h a t d i s t ingu i sh it from white r i c... l e s i n white r i c e . Since these characters can be t r ans fe r red by crossing, new red r i c e types can and do appear. Red r i c e i s undesirable because: 1. Red r i c e p l a n t s compete with cu l t iva ted r i c e...

Baker, John B.; Baldwin, Ford L.; Bourgeois, W.J.; Cox, Clodis H.; Craigmiles, Julian P.; Dishman, William D.; Eastin, E. Ford; Helpert, Charles W.; Hill, Lewis C.; Huey, Bobby A.; Klosterboer, Arlen D.; Sonnier, Earl A.

1980-01-01T23:59:59.000Z

70

The red and blue galaxy populations in the GOODS field: evidence for an excess of red dwarfs  

E-Print Network [OSTI]

We study the evolution of the galaxy population up to z\\sim3 as a function of its colour properties. In particular, luminosity functions and luminosity densities have been derived as a function of redshift for the blue/late and red/early populations. We use data from the GOODS-MUSIC catalogue which have typical magnitude limits zred/early subsamples. The LFs of the blue/late and total samples are well represented by steep Schechter functions evolving in luminosity with increasing redshifts. The volume density of the LFs of the red/early populations decreases with increasing redshift. The shape of the red/early LFs shows an excess of faint red dwarfs with respect to the extrapolation of a flat Schechter function and can be represented by the sum of two Schechter functions. Our model for galaxy formation in the hierarchical clustering scenario, which also includes external feedback due to a diffuse UV background, shows a general broad agreement with the LFs of both populations, the larger discrepancies being present at the faint end for the red population. Hints on the nature of the red dwarf population are given on the basis of their stellar mass and spatial distributions.

S. Salimbeni; E. Giallongo; N. Menci; M. Castellano; A. Fontana; A. Grazian; L. Pentericci; D. Trevese; S. Cristiani; M. Nonino; E. Vanzella

2007-10-19T23:59:59.000Z

71

SCOTTISH RED SQUIRREL ACTION PLAN  

E-Print Network [OSTI]

SCOTTISH RED SQUIRREL ACTION PLAN 2006­2011 #12;#12;S C O T T I S H R E D S Q U I R R E L A C T I O.1 Background 1 1.2 Action Plan Working Group 1 1.3 Issues affecting the conservation of the red squirrel 1 1.2 Timescale and partnership working 3 2.3 Rationale 3 2.4 Key actions 4 2.4.1 Establish and monitor the red

72

Jamaican red clay tobacco pipes  

E-Print Network [OSTI]

JAMAICAN RED CLAY TOBACCO PIPES A Thesis by KENAN PAUL HEIDTKE Submitted to the Office of Graduate Studies of Texas A&M University in partial fulfillment of the requirements for the degree of MASTER OF ARTS December 1992 Major Subject...: Anthropology JAMAICAN RED CLAY TOBACCO PIPES A Thesis by KENAN PAUL HEIDTKE Approved as to style and content by: Dorm L. Hamilton (Chair of Committee) Frederick H. van Doorninck, J (Member) enry C. Schmidt (Member) Vaughn M. Bryant (Head...

Heidtke, Kenan Paul

1992-01-01T23:59:59.000Z

73

Automatic Red Eye Removal for Digital Photography  

E-Print Network [OSTI]

Chapter 1 Automatic Red Eye Removal for Digital Photography FRANCESCA GASPARINI DISCo, Dipartimento The red eye effect is a well known problem in photography. It is often seen in amateur shots taken with a built-in flash, but the problem is also well known to professional photographers. Red eye is the red

Schettini, Raimondo

74

Gradual Ordering in Red Abalone Nacre  

SciTech Connect (OSTI)

Red abalone (Haliotis rufescens) nacre is a layered composite biomineral that contains crystalline aragonite tablets confined by organic layers. Nacre is intensely studied because its biologically controlled microarchitecture gives rise to remarkable strength and toughness, but the mechanisms leading to its formation are not well understood. Here we present synchrotron spectromicroscopy experiments revealing that stacks of aragonite tablet crystals in nacre are misoriented with respect to each other. Quantitative measurements of crystal orientation, tablet size, and tablet stacking direction show that orientational ordering occurs not abruptly but gradually over a distance of 50 {micro}m. Several lines of evidence indicate that different crystal orientations imply different tablet growth rates during nacre formation. A theoretical model based on kinetic and gradual selection of the fastest growth rates produces results in qualitative and quantitative agreement with the experimental data and therefore demonstrates that ordering in nacre is a result of crystal growth kinetics and competition either in addition or to the exclusion of templation by acidic proteins as previously assumed. As in other natural evolving kinetic systems, selection of the fastest-growing stacks of tablets occurs gradually in space and time. These results suggest that the self-ordering of the mineral phase, which may occur completely independently of biological or organic-molecule control, is fundamental in nacre formation.

Gilbert, P. U. P. A.; Metzler, Rebecca A.; Zhou, Dong; Scholl, Andreas; Doran, Andrew; Young, Anthony; Kunz, Martin; Tamura, Nobumichi; Coppersmith, Susan N.

2008-09-03T23:59:59.000Z

75

Red Mesa | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revisionEnvReviewNonInvasiveExplorationUT-g Grant of Access Permit5-ID-aRECRaton,RFPs Home NameRecurrentRedRed

76

Red-Black Trees 1 2004 Goodrich, Tamassia Red-Black Trees  

E-Print Network [OSTI]

Red-Black Trees 1© 2004 Goodrich, Tamassia Red-Black Trees 6 3 8 4 v z #12;Red-Black Trees 2© 2004 Goodrich, Tamassia From (2,4) to Red-Black Trees A red-black tree is a representation of a (2,4) tree by means of a binary tree whose nodes are colored red or black In comparison with its associated (2,4) tree

Alechina, Natasha

77

RED with ACK Spoofing Dept. of Electrical Engineering  

E-Print Network [OSTI]

RED with ACK Spoofing Zhong Xu Dept. of Electrical Engineering University of California, Riverside Early Detection (RED). Using simulation, we compare RED/Spoofing with Tail Drop, RED, and RED/ECN. Our results show that RED/Spoofing performs as well as RED/ECN, even though it avoids ECN's deployment problem

Molle, Mart

78

EA-1692: Red River Environmental Products, LLC Activated Carbon...  

Broader source: Energy.gov (indexed) [DOE]

2: Red River Environmental Products, LLC Activated Carbon Manufacturing Facility, Red River Parish, LA EA-1692: Red River Environmental Products, LLC Activated Carbon Manufacturing...

79

Red Band Needle Blight TERMS OF REFERENCE  

E-Print Network [OSTI]

Red Band Needle Blight TERMS OF REFERENCE Purpose 1. The Programme Board has been formed to have an overview of the administration and science of Red Band Needle Blight (RBNB), to underpin decisions made

80

3, 383408, 2006 The northern Red  

E-Print Network [OSTI]

BGD 3, 383­408, 2006 The northern Red Sea ­ A system in balance? C. H¨ase et al. Title Page in balance? ­ Implications of deep vertical mixing for the nitrogen budget in the northern Red Sea, including The northern Red Sea ­ A system in balance? C. H¨ase et al. Title Page Abstract Introduction Conclusions

Paris-Sud XI, Université de

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We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


81

Tuning RED for Web Traffic* Mikkel Christiansen,**  

E-Print Network [OSTI]

139 Tuning RED for Web Traffic* Mikkel Christiansen,** Kevin Jeffay, David Ott, F. Donelson Smith http://www.cs.unc.edu/Research/dirt Abstract We study the effects of RED on the performance of Web -- response time for HTTP request-response pairs. We empirically evaluate RED across a range of parameter

Jeffay, Kevin

82

Conservation Plan for Red Squirrels in Wales  

E-Print Network [OSTI]

#12;Conservation Plan for Red Squirrels in Wales Meeting the challenge to keep reds in Wales to enable effective red squir- rel conservation and grey squirrel management in Wales. The Wales Squirrel squirrel conservation and grey squirrel management in Wales. The Forum and Partnership are currently

83

Italian Herb Red Potato Salad Ingredients  

E-Print Network [OSTI]

Italian Herb Red Potato Salad Ingredients: 1 1/2 pounds red potatoes 1 green pepper 1 red onion 1/4 teaspoon garlic powder 1/4 teaspoon ground black pepper Directions 1. Wash potatoes, and cut into quarters. Place potatoes in sauce pan with cool water, cover and bring to a boil, turn to low and cook until

Liskiewicz, Maciej

84

Far-Red Fluorescent Protein Excitable with Red Lasers for Flow Cytometry and Superresolution STED Nanoscopy  

E-Print Network [OSTI]

Far-Red Fluorescent Protein Excitable with Red Lasers for Flow Cytometry and Superresolution STED Biology, Yale University School of Medicine, New Haven, Connecticut ABSTRACT Far-red fluorescent proteins are required for deep-tissue and whole-animal imaging and multicolor labeling in the red wavelength range

Verkhusha, Vladislav V.

85

Adaptive RED: An Algorithm for Increasing the Robustness of RED's Active Queue Management  

E-Print Network [OSTI]

Adaptive RED: An Algorithm for Increasing the Robustness of RED's Active Queue Management Sally, under submission Abstract The RED active queue management algorithm allows net- work operators is quite sensitive to the level of congestion and to the RED parameter settings, and is therefore not pre

Floyd, Sally

86

Red Band Needle Blight Programme Red Band Needle Blight of Pine Programme Group  

E-Print Network [OSTI]

Red Band Needle Blight Programme Group Red Band Needle Blight of Pine Programme Group Minutes Support Welcome and introduction 1. Jim thanked everyone for attending the first meeting of the Red Band and that the private 1 | Paper 1 - Minutes | Debbie Erskine | 23/01/2009 #12;Red Band Needle Blight Programme Group

87

Adaptive RED: An Algorithm for Increasing the Robustness of RED's Active Queue Management  

E-Print Network [OSTI]

Adaptive RED: An Algorithm for Increasing the Robustness of RED's Active Queue Management Sally, under submission Abstract The RED active queue management algorithm allows net­ work operators is quite sensitive to the level of congestion and to the RED parameter settings, and is therefore not pre

Floyd, Sally

88

Red-black Trees To know what a red-black tree is (10.1).  

E-Print Network [OSTI]

809 CHAPTER 10 Red-black Trees Objectives · To know what a red-black tree is (§10.1). · To convert a red-black tree to a 2-4 tree and vice versa (§10.2). · To design the RBTree class that extends the BinaryTree class (§10.3). · To insert an element in a red-black tree and resolve the double red problem

Liang, Y. Daniel

89

Sandia National Laboratories: Red LED  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear Security Administration the1 -theErik SpoerkeSolar Regional TestClimateResearchRecovery Act (ARRA) ProjectsRed

90

The Star Formation History of NGC 6822  

E-Print Network [OSTI]

Images of five fields in the Local Group dwarf irregular galaxy NGC 6822 obtained with the {\\it Hubble Space Telescope} in the F555W and F814W filters are presented. Photometry for the stars in these images was extracted using the Point-Spread-Function fitting program HSTPHOT/MULTIPHOT. The resulting color-magnitude diagrams reach down to $V\\approx26$, a level well below the red clump, and were used to solve quantitatively for the star formation history of NGC 6822. Assuming that stars began forming in this galaxy from low-metallicity gas and that there is little variation in the metallicity at each age, the distribution of stars along the red giant branch is best fit with star formation beginning in NGC 6822 12-15 Gyr ago. The best-fitting star formation histories for the old and intermediate age stars are similar among the five fields and show a constant or somewhat increasing star formation rate from 15 Gyr ago to the present except for a possible dip in the star formation rate from 3 to 5 Gyr ago. The main differences among the five fields are in the higher overall star formation rate per area in the bar fields as well as in the ratio of the recent star formation rate to the average past rate. These variations in the recent star formation rate imply that stars formed within the past 0.6 Gyr are not spatially very well mixed throughout the galaxy.

Ted K. Wyder

2001-07-31T23:59:59.000Z

91

Red-Black Trees 11/26/2007 11:09 AM Red-Black Trees 1 2004 Goodrich, Tamassia  

E-Print Network [OSTI]

Red-Black Trees 11/26/2007 11:09 AM 1 Red-Black Trees 1© 2004 Goodrich, Tamassia Red-Black Trees 6 3 8 4 v z Red-Black Trees 2© 2004 Goodrich, Tamassia From (2,4) to Red-Black Trees A red-black tree is a representation of a (2,4) tree by means of a binary tree whose nodes are colored red or black In comparison

Alechina, Natasha

92

Red-Black Trees 11/11/2004 10:02 AM Red-Black Trees 1 2004 Goodrich, Tamassia  

E-Print Network [OSTI]

Red-Black Trees 11/11/2004 10:02 AM 1 Red-Black Trees 1© 2004 Goodrich, Tamassia Red-Black Trees 6 3 8 4 v z Red-Black Trees 2© 2004 Goodrich, Tamassia From (2,4) to Red-Black Trees A red-black tree is a representation of a (2,4) tree by means of a binary tree whose nodes are colored red or black In comparison

Alechina, Natasha

93

Red blood cell malformations Cell shapes Modeling and simulation of red blood cell light scattering  

E-Print Network [OSTI]

that have a "sickle" appearance (see figure to left). This malformed geometry prevents cells from traveling Red blood cell malformations Cell shapes Modeling and simulation of red blood cell light to various diseases and acute conditions, the shape and composition of erythrocytes (red blood cells

California at Berkeley, University of

94

Do red giants have short mode lifetimes?  

E-Print Network [OSTI]

We show evidence that the red giant star ksi Hya has an oscillation mode lifetime, tau, of about 2 days significantly shorter than predicted by theory (tau = 17 days, Houdek & Gough 2002). If this is a general trend of red giants it would limit the prospects of asteroseismology on these stars because of poor coherence of the oscillations.

D. Stello; H. Kjeldsen; T. R. Bedding; D. Buzasi

2005-10-18T23:59:59.000Z

95

*Please do NOT put out food if both red and grey squirrels are present* Feeding red squirrels  

E-Print Network [OSTI]

*Please do NOT put out food if both red and grey squirrels are present* Feeding red squirrels The UK Red Squirrel Group does not generally recommend that people put out food for red squirrels, there are risks to red squirrels by enticing them into your garden, or other premises. These include disease

96

On bitcoin and red balloons  

E-Print Network [OSTI]

Many large decentralized systems rely on information propagation to ensure their proper function. We examine a common scenario in which only participants that are aware of the information can compete for some reward, and thus informed participants have an incentive not to propagate information to others. One recent example in which such tension arises is the 2009 DARPA Network Challenge (finding red balloons). We focus on another prominent example: Bitcoin, a decentralized electronic currency system. Bitcoin represents a radical new approach to monetary systems. It has been getting a large amount of public attention over the last year, both in policy discussions and in the popular press [Davis 2011; Surowiecki 2011]. Its cryptographic fundamentals have largely held up even as its usage has become increasingly widespread. We find, however, that it exhibits a fundamental problem of a different nature, based on how its incentives are structured. We propose a modification to the protocol that can eliminate this problem. Bitcoin relies on a peer-to-peer network to track transactions that are performed with the currency. For this purpose, every transaction a node learns about should be transmitted to its neighbors in the network. As the protocol is currently defined and implemented, it does not provide an incentive for nodes to broadcast transactions they are aware of. In fact, it provides an incentive not to do so. Our solution is to augment the

Moshe Babaioff; Silicon Valley; Shahar Dobzinski; Sigal Oren

2012-01-01T23:59:59.000Z

97

On Bitcoin and Red Balloons  

E-Print Network [OSTI]

We study scenarios in which the goal is to ensure that some information will propagate through a large network of nodes. In these scenarios all nodes that are aware of the information compete for the same prize, and thus have an incentive not to propagate information. One example for such a scenario is the 2009 DARPA Network Challenge (finding red balloons). We give special attention to a second domain, Bitcoin, a decentralized electronic currency system. Bitcoin, which has been getting a large amount of public attention over the last year, represents a radical new approach to monetary systems which has appeared in policy discussions and in the popular press. Its cryptographic fundamentals have largely held up even as its usage has become increasingly widespread. We find, however, that it exhibits a fundamental problem of a different nature, based on how its incentives are structured. We propose a modification to the protocol that can fix this problem. Bitcoin relies on a peer-to-peer network to track transac...

Babaioff, Moshe; Oren, Sigal; Zohar, Aviv

2011-01-01T23:59:59.000Z

98

T-678: Red Hat Enterprise Virtualization Hypervisor VLAN Packet...  

Broader source: Energy.gov (indexed) [DOE]

8: Red Hat Enterprise Virtualization Hypervisor VLAN Packet Processing Flaw Lets Remote Users Deny Service T-678: Red Hat Enterprise Virtualization Hypervisor VLAN Packet...

99

T-649: Red Hat Network Satellite Server Request Validation Flaw...  

Broader source: Energy.gov (indexed) [DOE]

49: Red Hat Network Satellite Server Request Validation Flaw Permits Cross-Site Request Forgery Attacks T-649: Red Hat Network Satellite Server Request Validation Flaw Permits...

100

U-200: Red Hat Directory Server Information Disclosure Security...  

Broader source: Energy.gov (indexed) [DOE]

0: Red Hat Directory Server Information Disclosure Security Issue and Vulnerability U-200: Red Hat Directory Server Information Disclosure Security Issue and Vulnerability June 27,...

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


101

Star Formation and the Growth of Stellar Mass  

E-Print Network [OSTI]

Recent observations have demonstrated a significant growth in the integrated stellar mass of the red sequence since z=1, dominated by a steadily increasing number of galaxies with stellar masses M* 3x10^10 M_sun blue galaxies would also be overproduced; i.e., most of the new stars formed in blue cloud galaxies are in the massive galaxies. We explore a simple truncation scenario in which these `extra' blue galaxies have their star formation suppressed by an unspecified mechanism or mechanisms; simple cessation of star formation in these extra blue galaxies is approximately sufficient to build up the red sequence at M*<10^11 M_sun.

Eric F. Bell; Xian Zhong Zheng; Casey Papovich; Andrea Borch; Christian Wolf; Klaus Meisenheimer

2007-04-23T23:59:59.000Z

102

THE TEMPERATURES OF RED SUPERGIANTS  

SciTech Connect (OSTI)

We present a re-appraisal of the temperatures of red supergiants (RSGs) using their optical and near-infrared spectral energy distributions (SEDs). We have obtained data of a sample of RSGs in the Magellanic Clouds using VLT+XSHOOTER, and we fit MARCS model atmospheres to different regions of the spectra, deriving effective temperatures for each star from (1) the TiO bands, (2) line-free continuum regions of the SEDs, and (3) the integrated fluxes. We show that the temperatures derived from fits to the TiO bands are systematically lower than the other two methods by several hundred kelvin. The TiO fits also dramatically overpredict the flux in the near-IR, and imply extinctions which are anomalously low compared to neighboring stars. In contrast, the SED temperatures provide good fits to the fluxes at all wavelengths other than the TiO bands, are in agreement with the temperatures from the flux integration method, and imply extinctions consistent with nearby stars. After considering a number of ways to reconcile this discrepancy, we conclude that three-dimensional effects (i.e., granulation) are the most likely cause, as they affect the temperature structure in the upper layers where the TiO lines form. The continuum, however, which forms at much deeper layers, is apparently more robust to such effects. We therefore conclude that RSG temperatures are much warmer than previously thought. We discuss the implications of this result for stellar evolution and supernova progenitors, and provide relations to determine the bolometric luminosities of RSGs from single-band photometry.

Davies, Ben [Astrophysics Research Institute, Liverpool John Moores University, Egerton Wharf, Birkenhead CH41 1LD (United Kingdom)] [Astrophysics Research Institute, Liverpool John Moores University, Egerton Wharf, Birkenhead CH41 1LD (United Kingdom); Kudritzki, Rolf-Peter; Gazak, Zach [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)] [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Plez, Bertrand [Laboratoire Univers et Particules de Montpellier, Universite Montpellier 2, CNRS, F-34095 Montpellier (France)] [Laboratoire Univers et Particules de Montpellier, Universite Montpellier 2, CNRS, F-34095 Montpellier (France); Trager, Scott [Kapteyn Institute, University of Groningen, P.O. Box 800, 9700-AV Groningen (Netherlands)] [Kapteyn Institute, University of Groningen, P.O. Box 800, 9700-AV Groningen (Netherlands); Lancon, Ariane [Observatoire Astronomique and CNRS UMR 7550, Universite de Strasbourg, F-67000 Strasbourg (France)] [Observatoire Astronomique and CNRS UMR 7550, Universite de Strasbourg, F-67000 Strasbourg (France); Bergemann, Maria [Max-Planck-Institute for Astrophysics, Karl-Schwarzschild-Str. 1, D-85741 Garching (Germany)] [Max-Planck-Institute for Astrophysics, Karl-Schwarzschild-Str. 1, D-85741 Garching (Germany); Evans, Chris [UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom)] [UK Astronomy Technology Centre, Royal Observatory Edinburgh, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Chiavassa, Andrea [CNRS Laboratoire Lagrange, Universite de Nice Sophia-Antipolis, Observatoire de la Cote d'Azur, BP 4229, F-06304 Nice Cedex 4 (France)] [CNRS Laboratoire Lagrange, Universite de Nice Sophia-Antipolis, Observatoire de la Cote d'Azur, BP 4229, F-06304 Nice Cedex 4 (France)

2013-04-10T23:59:59.000Z

103

Redding Electric- Earth Advantage Rebate Program  

Broader source: Energy.gov [DOE]

The Earth Advantage Rebate Program was designed to offer rebates to residential and business customers of Redding Electric Utility (REU) for solar PV, solar thermal, and geothermal heat pump...

104

Viscoelastic transient of confined Red Blood Cells  

E-Print Network [OSTI]

The unique ability of a red blood cell to flow through extremely small microcapillaries depends on the viscoelastic properties of its membrane. Here, we study in vitro the response time upon flow startup exhibited by red blood cells confined into microchannels. We show that the characteristic transient time depends on the imposed flow strength, and that such a dependence gives access to both the effective viscosity and the elastic modulus controlling the temporal response of red cells. A simple theoretical analysis of our experimental data, validated by numerical simulations, further allows us to compute an estimate for the two-dimensional membrane viscosity of red blood cells, $\\eta_{mem}^{2D}\\sim 10^{-7}$ N$\\cdot$s$\\cdot$m$^{-1}$. By comparing our results with those from previous studies, we discuss and clarify the origin of the discrepancies found in the literature regarding the determination of $\\eta_{mem}^{2D}$, and reconcile seemingly conflicting conclusions from previous works.

Gal Prado; Alexander Farutin; Chaouqi Misbah; Lionel Bureau

2014-09-17T23:59:59.000Z

105

Right Turn on Red! | Department of Energy  

Broader source: Energy.gov (indexed) [DOE]

benefits for the country, helping us all save money by saving energy. Prior to the 1970's, some states already allowed drivers to turn right on a red light, but many others -...

106

POPULATION BIOLOGY OF RED ABAWNES, HALIOTIS RUFESCENS, IN SOUTHERN CALIFORNIA AND MANAGEMENT OF THE RED AND  

E-Print Network [OSTI]

ABSTRACT Population dynamics of red abalones. Hal·wti.s rufeSC611,8 Swainson. were studied at Johnsons Lee

107

Newtonian gravity, red shift, confinement, asymptotic freedom and quarks oscillations  

E-Print Network [OSTI]

Quarks oscillations give the Newtonian gravity law, the red shift, the confinement and the asymptotic freedom.

G. Quznetsov

2008-10-18T23:59:59.000Z

108

Improved ``Optical Highlighter'' Probes Derived from Discosoma Red Fluorescent Protein  

E-Print Network [OSTI]

, Minneapolis, Minnesota ABSTRACT The tetrameric red fluorescent protein, DsRed, undergoes a rapid red to green-emitting species of DsRed and an enhancement of emission from the ``immature'' green species, likely caused by dequenching of fluorescence resonance energy transfer occurring within the protein tetramer. Here, we have

Marchant, Jonathan

109

Bureau of Commercial Fisheries Symposium on Red Tide  

E-Print Network [OSTI]

21 Bureau of Commercial Fisheries Symposium on Red Tide By James E. Sykes Marine Biological, Donald L. McKernan, Director Bureau of Commercial Fisheries Symposium on Red Tide By James E. Sykes causing Red-Tide blooms as deduced from field observations 2 Red- Tide research at the Florida State

110

Red giant variables: OGLE--II and MACHO  

E-Print Network [OSTI]

We review the recent impact of microlensing projects on our understanding of pulsating red giant stars. Discussed are red giant stars' pulsation properties (period--luminosity relations, period changes, mode switchings), Red Giant Branch pulsations, metallicity effects and the use of red giant variables to explore galactic structure.

L. L. Kiss; P. Lah

2005-09-21T23:59:59.000Z

111

A monomeric red fluorescent protein Robert E. Campbell*, Oded Tour*  

E-Print Network [OSTI]

A monomeric red fluorescent protein Robert E. Campbell*, Oded Tour* , Amy E. Palmer*, Paul A, and the obligate tetramerization of the red fluorescent protein from Discosoma (DsRed). Although the weak, the obligate tet- ramerization of DsRed has greatly hindered its use as a genetically encoded fusion tag. We

Tsien, Roger Y.

112

RED Revisited Tuan Anh Trinh and Sandor Molnar  

E-Print Network [OSTI]

RED Revisited Tuan Anh Trinh and S´andor Moln´ar High Speed Networks Laboratory Department- ternet is RED. However, research results on RED perfor- mance are highly mixed, especially in the field of tuning its parameters. In this paper, we revisit some features in RED and study them in greater details

Molnár, Sándor

113

UK Red Squirrel Group Terms of Reference Introduction  

E-Print Network [OSTI]

UK Red Squirrel Group Terms of Reference Introduction The red squirrel Sciurus vulgaris has of the Bern Convention, is Lower Risk ­near threatened on the IUCN Red List and is protected under Schedules 5-ordinate, support and provide advice on the implementation of conservation measures for the red squirrel in the UK

114

Guide to Red Fluorescent Proteins and Biosensors for Flow Cytometry  

E-Print Network [OSTI]

CHAPTER 17 Guide to Red Fluorescent Proteins and Biosensors for Flow Cytometry Kiryl D. PiatkevichH Stability of Fluorescence F. Optimization of Nucleotide and Amino Acid Sequences III. Modern Advanced Red-Shifted FPs A. Orange Fluorescent Proteins B. Red Fluorescent Proteins C. Far-Red Fluorescent Proteins IV

Verkhusha, Vladislav V.

115

RED Revisited Tuan Anh Trinh and Sandor Molnar  

E-Print Network [OSTI]

RED Revisited Tuan Anh Trinh and S??andor Moln??ar High Speed Networks Laboratory Department­ ternet is RED. However, research results on RED perfor­ mance are highly mixed, especially in the field of tuning its parameters. In this paper, we revisit some features in RED and study them in greater details

Molnár, Sándor

116

UK RED SQUIRREL GROUP WEDNESDAY 7 OCTOBER 2009  

E-Print Network [OSTI]

1 UK RED SQUIRREL GROUP WEDNESDAY 7 OCTOBER 2009 Northumberland Wildlife Trust Newcastle MINUTES in conjunction with grey squirrel culling, the outcome for the red squirrel has substantially improved.with 11 red squirrels and 24 grey squirrels recorded in 2004 changing to 103 red squirrels and 3 grey

117

MFR PAPER 1229 Red Snappers of the Carolina Coast  

E-Print Network [OSTI]

Coast to the Campeche Banks. A closely related species, the Caribbean red snapper, Lutjanus pur- pureus

118

THE SIZE DIFFERENCE BETWEEN RED AND BLUE GLOBULAR CLUSTERS IS NOT DUE TO PROJECTION EFFECTS  

SciTech Connect (OSTI)

Metal-rich (red) globular clusters in massive galaxies are, on average, smaller than metal-poor (blue) globular clusters. One of the possible explanations for this phenomenon is that the two populations of clusters have different spatial distributions. We test this idea by comparing clusters observed in unusually deep, high signal-to-noise images of M87 with a simulated globular cluster population in which the red and blue clusters have different spatial distributions, matching the observations. We compare the overall distribution of cluster effective radii as well as the relationship between effective radius and galactocentric distance for both the observed and simulated red and blue sub-populations. We find that the different spatial distributions does not produce a significant size difference between the red and blue sub-populations as a whole or at a given galactocentric distance. These results suggest that the size difference between red and blue globular clusters is likely due to differences during formation or later evolution.

Webb, Jeremy J.; Harris, William E.; Sills, Alison, E-mail: webbjj@mcmaster.ca [Department of Physics and Astronomy, McMaster University, Hamilton ON L8S 4M1 (Canada)

2012-11-10T23:59:59.000Z

119

Utility Formation  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear SecurityTensile Strain Switched Ferromagnetism inS-4500II Field EmissionFunctional MaterialsRobertUtility-Formation

120

Conserving Scotland's Red Squirrels Scotland supports an estimated 75% of the UK red squirrel population. Although one  

E-Print Network [OSTI]

Conserving Scotland's Red Squirrels Scotland supports an estimated 75% of the UK red squirrel population. Although one of the most popular mammal species in the country, red squirrels currently face a number of ecological problems and their range within the UK has been much reduced. It means that the red

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


121

CUTTING SOLAR RED TAPECUTTING SOLAR RED TAPE Evergreen State Solar PartnershipEvergreen State Solar Partnership  

E-Print Network [OSTI]

CUTTING SOLAR RED TAPECUTTING SOLAR RED TAPE Evergreen State Solar PartnershipEvergreen State Solar Partnership Rooftop Solar Challenge 1 Sunshot #12;WASHINGTON PV CONTEXTWASHINGTON PV CONTEXT 285 cities, 39 Installations happen where process is easier #12;EVERGREEN STATE SOLAR PARTNERSHIP Commerce NWSEEDEdmonds

122

7X performance results - final report : ASCI Red vs Red Storm.  

SciTech Connect (OSTI)

The goal of the 7X performance testing was to assure Sandia National Laboratories, Cray Inc., and the Department of Energy that Red Storm would achieve its performance requirements which were defined as a comparison between ASCI Red and Red Storm. Our approach was to identify one or more problems for each application in the 7X suite, run those problems at multiple processor sizes in the capability computing range, and compare the results between ASCI Red and Red Storm. The first part of this report describes the two computer systems, the applications in the 7X suite, the test problems, and the results of the performance tests on ASCI Red and Red Storm. During the course of the testing on Red Storm, we had the opportunity to run the test problems in both single-core mode and dual-core mode and the second part of this report describes those results. Finally, we reflect on lessons learned in undertaking a major head-to-head benchmark comparison.

Dinge, Dennis C. (Cray Inc., Albuquerque, NM); Davis, Michael E. (Cray Inc., Albuquerque, NM); Haskell, Karen H.; Ballance, Robert A.; Gardiner, Thomas Anthony; Stevenson, Joel O.; Noe, John P.

2011-04-01T23:59:59.000Z

123

Red mud characterization using nuclear analytical techniques  

SciTech Connect (OSTI)

Red mud is a toxic waste left as a byproduct in aluminum production Bayer process. Since it contains significant concentrations of other chemical elements interesting for industry, including REE, it is also potential secondary ore source. Recent events in some countries have shown that red mud presents a serious environmental hazard if not properly stored. The subject of our study is the red mud from an ex-aluminum plant in Obrovac, Croatia, left from processing of bauxite mined during late 70's and early 80's at the eastern Adriatic coast and since than stored in open concrete basins for more than 30 years. We have used energy dispersive x-ray fluorescence analysis (both tube and radioactive source excitation), fast neutron activation analysis and passive gamma spectrometry to identify a number of elements present in the red mud, their concentration levels and radioactivity in the red mud. The high concentrations of Al, Si, Ca, Ti and Fe have been measured. Chemical elements Sc, Cr, Mn, Co, Ni, Cu, Zn, Ga, As, Se, Br, Y, La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Pb, Th and U were found in lower concentrations. No significant levels of radioactivity have been measured. (authors)

Obhodas, J.; Sudac, D.; Matjacic, L. [Dept. of Experimental Physics, Inst. Ruder Boskovic, Zagreb (Croatia); Valkovic, V. [A.C.T.d.o.o., Prilesje 4, Zagreb (Croatia)

2011-07-01T23:59:59.000Z

124

Red River Biodiesel Ltd | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revisionEnvReviewNonInvasiveExplorationUT-g Grant of Access Permit5-ID-aRECRaton,RFPs Home NameRecurrentRedRedLtd

125

The FIRST-2MASS Red Quasar Survey  

SciTech Connect (OSTI)

Combining radio observations with optical and infrared color selection--demonstrated in our pilot study to be an efficient selection algorithm for finding red quasars--we have obtained optical and infrared spectroscopy for 120 objects in a complete sample of 156 candidates from a sky area of 2716 square degrees. Consistent with our initial results, we find our selection criteria--J-K > 1.7,R-K > 4.0--yield a {approx} 50% success rate for discovering quasars substantially redder than those found in optical surveys. Comparison with UVX- and optical color-selected samples shows that {approx}> 10% of the quasars are missed in a magnitude-limited survey. Simultaneous two-frequency radio observations for part of the sample indicate that a synchrotron continuum component is ruled out as a significant contributor to reddening the quasars spectra. We go on to estimate extinctions for our objects assuming their red colors are caused by dust. Continuum fits and Balmer decrements suggest E(B-V) values ranging from near zero to 2.5 magnitudes. Correcting the K-band magnitudes for these extinctions, we find that for K {le} 14.0, red quasars make up between 25% and 60% of the underlying quasar population; owing to the incompleteness of the 2MASS survey at fainter K-band magnitudes, we can only set a lower limit to the radio-detected red quasar population of > 20-30%.

Glikman, E; Helfand, D J; White, R L; Becker, R H; Gregg, M D; Lacy, M

2007-06-28T23:59:59.000Z

126

The Red Planet Mars is noticeable  

E-Print Network [OSTI]

the melting polar ice, and to distribute the water among the oases #12;Camille Flammarion (1884) #12;Chesley Viewed through a telescope: Mars has white polar caps Mars has dark (greenish) and bright (red;Northern Polar Cap in Spring #12;The Facts of Mars mass = 0.11M radius = 0.53 R density = 3.9 gm/cm3

Walter, Frederick M.

127

Early and later diagenetic alteration of Ordovician Red River carbonates, Tioga Deep field, Williston basin, North Dakota  

SciTech Connect (OSTI)

The Ordovician Red River Formation in the Williston basin is generally subdivided into three restrictive-upward cycles referred to as 'A,' 'B,' and 'C' zones in descending order. Most Red River production in western North Dakota and eastern Montana comes from dolomitized burrowed and laminated members of the C-cycle. Four cores taken by Amerada Hess Corporation within the Tioga Deep field, Williams and Montrail Counties, North Dakota, were studied in detail to establish depositional and diagenetic controls on porosity distribution within the Red River. Dolomitized portions of the Red River C member are genetically related to downward-descending Mg-rich brines derived from hypersaline basin waters depleted of their sulfate content throught attendant precipitation of gypsum. Calcite associated with this early dolomitization phase occupied intercrystalline positions between dolomite rhombs. Following burial, limestones tended to chemically compact through pressure solution, whereas late stage fractures were localized in the more brittle dolomitic portions of the Red River. These fractures served as conduits for late stage leaching fluids, possibly associated with hydrocarbon generation, that enhanced porosity in the dolomites through the removal of associated calcite. Late-stage leaching is reflected in 'overly porous' dolomite haloes around cemented burrow centers and highly porous dolomite seams along stylolitic contacts. Previous models proposed to explain porosity distribution within Red River reservoirs should be modified to include the overprint of deep diagenetic effects.

Perkins, R.D. (Duke Univ., Durham, NC (United States))

1991-03-01T23:59:59.000Z

128

E-Print Network 3.0 - aux red oils Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Environmental Sciences and Ecology 22 Red Leaf Resources and the Commercialization of Oil Shale Summary: Red Leaf Resources and the Commercialization of Oil Shale 12;About Red...

129

Nationwide: Slashing Red Tape To Speed Solar Deployment for Homes...  

Energy Savers [EERE]

Slashing Red Tape To Speed Solar Deployment for Homes and Businesses Nationwide: Slashing Red Tape To Speed Solar Deployment for Homes and Businesses January 24, 2014 - 12:00am...

130

Cation Uptake and Allocation by Red Pine Seedlings under Cation...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Uptake and Allocation by Red Pine Seedlings under Cation-Nutrient Stress in a Column Growth Experiment. Cation Uptake and Allocation by Red Pine Seedlings under Cation-Nutrient...

131

Sun-Sentinel Red hot email heats up Wasserman Schultz,  

E-Print Network [OSTI]

Sun-Sentinel Red hot email heats up Wasserman Schultz, West rift South Florida members of Congress take feud public July 20, 2011|By Anthony Man, Sun Sentinel Congressman Allen West's red hot response

Belogay, Eugene A.

132

WHEN THE BLUE-GREEN WATERS TURN RED  

E-Print Network [OSTI]

WHEN THE BLUE-GREEN WATERS TURN RED Historical Flooding in Havasu Creek, Arizona U.S. GEOLOGICAL OF RECLAMATION #12;WHEN THE BLUE-GREEN WATERS TURN RED Historical Flooding in Havasu Creek, Arizona By THEODORE S

133

Thyroid Hormone Regulation of Deiodinase in Red Drum (Sciaenops ocellatus)  

E-Print Network [OSTI]

thyroxine (T4) in the red drum (Sciaenops ocellatus), a commercially important fish species. Immersion experiments were performed, where red drum were kept in 20-gallon glass tanks with either T4-treated or control solution-treated tank water...

Ron, Laura

2011-05-04T23:59:59.000Z

134

THE MID-INFRARED AND NEAR-ULTRAVIOLET EXCESS EMISSIONS OF QUIESCENT GALAXIES ON THE RED SEQUENCE  

SciTech Connect (OSTI)

We study the mid-infrared (IR) and near-ultraviolet (UV) excess emissions of spectroscopically selected quiescent galaxies on the optical red sequence. We use the Wide-field Infrared Survey Explorer mid-IR and Galaxy Evolution Explorer near-UV data for a spectroscopic sample of galaxies in the Sloan Digital Sky Survey Data Release 7 to study the possible connection between quiescent red-sequence galaxies with and without mid-IR/near-UV excess. Among 648 12 {mu}m detected quiescent red-sequence galaxies without H{alpha} emission, 26% and 55% show near-UV and mid-IR excess emissions, respectively. When we consider only bright (M{sub r} < -21.5) galaxies with an early-type morphology, the fraction of galaxies with recent star formation is still 39%. The quiescent red-sequence galaxies with mid-IR and near-UV excess emissions are optically fainter and have slightly smaller D{sub n} 4000 than those without mid-IR and near-UV excess emissions. We also find that mid-IR weighted mean stellar ages of quiescent red-sequence galaxies with mid-IR excess are larger than those with near-UV excess, and smaller than those without mid-IR and near-UV excess. The environmental dependence of the fraction of quiescent red-sequence galaxies with mid-IR and near-UV excess seems strong even though the trends of quiescent red-sequence galaxies with near-UV excess differ from those with mid-IR excess. These results indicate that the recent star formation traced by near-UV ({approx}< 1 Gyr) and mid-IR ({approx}< 2 Gyr) excess is not negligible among nearby, quiescent, red, early-type galaxies. We suggest a possible evolutionary scenario of quiescent red-sequence galaxies from quiescent red-sequence galaxies with near-UV excess to those with mid-IR excess to those without near-UV and mid-IR excess.

Ko, Jongwan; Lee, Jong Chul [Korea Astronomy and Space Science Institute, Daejeon 305-348 (Korea, Republic of)] [Korea Astronomy and Space Science Institute, Daejeon 305-348 (Korea, Republic of); Hwang, Ho Seong [Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138 (United States)] [Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138 (United States); Sohn, Young-Jong, E-mail: jwko@kasi.re.kr [Department of Astronomy, Yonsei University, Seoul 120-749 (Korea, Republic of)] [Department of Astronomy, Yonsei University, Seoul 120-749 (Korea, Republic of)

2013-04-10T23:59:59.000Z

135

Red de compensacin al trabajador Recibo de Informacin  

E-Print Network [OSTI]

Red de compensación al trabajador Recibo de Información He recibido la Notificación de los requisitos para utilizar la Red que me explica cómo obtener atención médica a través de la Red de información, entiendo que: 1. Debo elegir un médico tratante de la lista de médicos pertenecientes a la red de

Yang, Zong-Liang

136

Spectroscopic Survey of Red Giants in the SMC. I: Kinematics  

E-Print Network [OSTI]

We present a spectroscopic survey of 2046 red giant stars, distributed over the central 4x2 kpc of the Small Magellanic Cloud (SMC). After fitting and removing a small velocity gradient across the SMC (7.9 km/s/deg oriented at 10 deg E of N), we measure an rms velocity scatter of 27.5+-0.5 km/s. The line of sight velocity distribution is well-characterized by a Gaussian and the velocity dispersion profile is nearly constant as a function of radius. We find no kinematic evidence of tidal disturbances. Without a high-precision measurement of the SMC's proper motion, it is not possible to constrain the SMC's true rotation speed from our measured radial-velocity gradient. However, even with conservative assumptions, we find that v < sigma and hence that the SMC is primarily supported by its velocity dispersion. We find that the shape of the SMC, as measured from the analysis of the spatial distribution of its red giant stars, is consistent with the degree of rotational flattening expected for the range of allowed v/sigma values. As such, the properties of the SMC are consistent with similar low luminosity spheroidal systems. We conclude that the SMC is primarily a low luminosity spheroid whose irregular visual appearance is dominated by recent star formation. A simple virial analysis using the measured kinematics implies an enclosed mass within 1.6 kpc of between 1.4 and 1.9x10^9 Mo, and a less well constrained mass within 3 kpc of between 2.7 and 5.1x10^9 Mo.

Jason Harris; Dennis Zaritsky

2006-01-02T23:59:59.000Z

137

UK RED SQUIRREL GROUP WEDNESDAY 22 APRIL 2009  

E-Print Network [OSTI]

1 UK RED SQUIRREL GROUP WEDNESDAY 22 APRIL 2009 SNH, Silvan House Edinburgh MINUTES Present Tony, have led to divergence in the philosophy and focus on a red squirrel conservation strategy. Evidence. Also, FCE grant-aid supported red squirrel conservation work in reserves #12;2 and surrounding buffer

138

UK Red Squirrel Group Minutes Tuesday 15th  

E-Print Network [OSTI]

UK Red Squirrel Group Minutes Tuesday 15th January 2013 1 Welcome and apologies S Bailey Attendee for protocol on red squirrel translocations to SM ­ see renewed AP1 AP2 ALL to visit new RSNE website to BM - complete General consensus that veterinary checks were required for red squirrel translocations

139

UK Red Squirrel Group Minutes Thursday 24th  

E-Print Network [OSTI]

UK Red Squirrel Group Minutes Thursday 24th November 2011 1 Welcome and apologies B Mayle BM Country updates Country reps SCOTLAND JB, JR, SE General update: The `Management Guidance for Red Squirrel Strategy for Red Squirrel Conservation ­ reflecting that many of the existing action plans and projects

140

Release of 'Red Dragon' Ornamental Hazelnut March 15, 2008  

E-Print Network [OSTI]

Release of 'Red Dragon' Ornamental Hazelnut March 15, 2008 The Oregon Agricultural Experiment Station announces the release of a new hazelnut (Corylus avellana L.) cultivar 'Red Dragon' for the ornamental market with red leaves, contorted growth habit, and complete resistance to eastern filbert blight

Tullos, Desiree

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


141

716 Langdon St 2nd Floor Red Gym  

E-Print Network [OSTI]

716 Langdon St 2nd Floor Red Gym Madison WI 53706 (608) 262-4503 http://msc.wisc.edu 1 FOLLOW OUR of witnesses may always go before you and walk beside you. We bestow a red and white kente stole upon all of our graduates. Red, for passion and sacrifice. White, for initiation and new beginnings. Each stole

Sheridan, Jennifer

142

Ridgeview Publishing Company Indeterminism and the Thin Red Line  

E-Print Network [OSTI]

Ridgeview Publishing Company Indeterminism and the Thin Red Line Author(s): Nuel Belnap INDETERMINISM AND THE THIN RED LINE NuelBelnapandMitchellGreen Universityof Pittsburgh 1. Introduction 2,settledness,andactualityin branchingtime 5. The AssertionProblem 6. TheThinRedLine 7. Time's wingedchariothurriesnear 1. Introduction

Belnap, Nuel

143

American Red Cross VOLUNTEER SERVICE AGREEMENT FOR DISASTER OPERATIONS  

E-Print Network [OSTI]

American Red Cross VOLUNTEER SERVICE AGREEMENT FOR DISASTER OPERATIONS I and maintenance costs will be reimbursed by the American Red Cross, pursuant to Staff Reimbursement Procedures the American Red Cross while I am performing disaster relief work. Furthermore, I understand and accept that

Wu, Shin-Tson

144

Verifying Red-Black Trees Paolo Baldan1  

E-Print Network [OSTI]

Verifying Red-Black Trees Paolo Baldan1 , Andrea Corradini2 , Javier Esparza3 , Tobias Heindel3,heindets,koenigba,koziouvi}@fmi.uni-stuttgart.de Abstract. We show how to verify the correctness of insertion of ele- ments into red-black trees--a form of balanced search trees--using anal- ysis techniques developed for graph rewriting. We first model red

Baldan, Paolo

145

Use of red ochre by early Neandertals Wil Roebroeksa,1  

E-Print Network [OSTI]

Use of red ochre by early Neandertals Wil Roebroeksa,1 , Mark J. Siera,b,c , Trine Kellberg older iron oxide finds that constitute the earliest documented use of red ochre by Neandertals. These finds were small concen- trates of red material retrieved during excavations at Maastricht- Belvédère

Utrecht, Universiteit

146

Is the Missing Ultra-Red Material Colorless Ice?  

E-Print Network [OSTI]

The extremely red colors of some transneptunian objects and Centaurs are not seen among the Jupiter family comets which supposedly derive from them. Could this mismatch result from sublimation loss of colorless ice? Radiative transfer models show that mixtures of volatile ice and nonvolatile organics could be extremely red, but become progressively darker and less red as the ice sublimates away.

W. M. Grundy

2008-11-14T23:59:59.000Z

147

Brief Communication 809 Photoactivation turns green fluorescent protein red  

E-Print Network [OSTI]

Brief Communication 809 Photoactivation turns green fluorescent protein red Michael B. Elowitz gene was first cloned, the Aequorea victoria green fluorescent protein (GFP) has become a powerful tool- wavelength (red) fluorescence has remained elusive. Here we describe a red-emitting, green

Elowitz, Michael

148

Red Leaf Resources and the Commercialization of Oil Shale  

E-Print Network [OSTI]

Red Leaf Resources and the Commercialization of Oil Shale #12;About Red Leaf Resources 2006 Company commercial development field activities #12;Highlights Proven, Revolutionary Oil Shale Extraction Process Technology Significant Owned Oil Shale Resource #12;· The executive management team of Red Leaf Resources

Utah, University of

149

The plasma protein fibrinogen stabilizes clusters of red blood cells in microcapillary flows  

E-Print Network [OSTI]

The supply of oxygen and nutrients and the disposal of metabolic waste in the organs depend strongly on how blood, especially red blood cells, flow through the microvascular network. Macromolecular plasma proteins such as fibrinogen cause red blood cells to form large aggregates, called rouleaux, which are usually assumed to be disaggregated in the circulation due to the shear forces present in bulk flow. This leads to the assumption that rouleaux formation is only relevant in the venule network and in arterioles at low shear rates or stasis. Thanks to an excellent agreement between combined experimental and numerical approaches, we show that despite the large shear rates present in microcapillaries, the presence of either fibrinogen or the synthetic polymer dextran leads to an enhanced formation of robust clusters of red blood cells, even at haematocrits as low as 1%. Robust aggregates are shown to exist in microcapillaries even for fibrinogen concentrations within the healthy physiological range. These persistent aggregates should strongly affect cell distribution and blood perfusion in the microvasculature, with putative implications for blood disorders even within apparently asymptomatic subjects.

M. Brust; O. Aouane; M. Thiebaud; D. Flormann; C. Verdier; L. Kaestner; M. W. Laschke; H. Selmi; A. Benyoussef; T. Podgorski; G. Coupier; C. Misbah; C. Wagner

2014-02-25T23:59:59.000Z

150

Red Shift from Gravitational Back Reaction  

E-Print Network [OSTI]

Deviations from geodesic motion caused by gravitational radiation have been discussed in the last decades to describe the motion of particles or photons in strong fields around collapsed objects. On cosmological scale this effect, which in the first order is caused by the finite speed of gravitational interaction, is important also in the weak field limit. In this paper the energy loss by transfer to the gravitational potential is determined in a quasi-Newtonian approximation for the examples of a static Einstein universe and for an expanding universe with flat metric. In both cases the resulting red shift is a considerable fraction of the total red shift and requires an adjustment of the age and the matter composition in our models of the universe.

Ernst Fischer

2007-03-30T23:59:59.000Z

151

Star Formation in the Local Universe  

E-Print Network [OSTI]

We present preliminary results of a long-term study aimed at answering a number of open questions on the evolution of starbursts in local galaxies. The project employes mainly HST data from the ultraviolet to the red of the stellar continuum and of the nebular emission from the galaxies. Here we concentrate on NGC5253 and NGC5236 (M83), that form a dwarf--massive galaxy pair at about 4 Mpc distance. The recent star formation history of the centers of the two galaxies is investigated in order to identify similarities and differences in the evolution of their central starbursts.

Daniela Calzetti; Jason Harris

2001-11-28T23:59:59.000Z

152

Blue, green, orange, and red upconversion laser  

DOE Patents [OSTI]

A laser for outputting visible light at the wavelengths of blue, green, orange and red light. This is accomplished through the doping of a substrate, such as an optical fiber or waveguide, with Pr.sup.3+ ions and Yb.sup.3+ ions. A light pump such as a diode laser is used to excite these ions into energy states which will produce lasing at the desired wavelengths. Tuning elements such as prisms and gratings can be employed to select desired wavelengths for output.

Xie, Ping (San Jose, CA); Gosnell, Timothy R. (Sante Fe, NM)

1998-01-01T23:59:59.000Z

153

Blue, green, orange, and red upconversion laser  

DOE Patents [OSTI]

A laser is disclosed for outputting visible light at the wavelengths of blue, green, orange and red light. This is accomplished through the doping of a substrate, such as an optical fiber or waveguide, with Pr{sup 3+} ions and Yb{sup 3+} ions. A light pump such as a diode laser is used to excite these ions into energy states which will produce lasing at the desired wavelengths. Tuning elements such as prisms and gratings can be employed to select desired wavelengths for output. 11 figs.

Xie, P.; Gosnell, T.R.

1998-09-08T23:59:59.000Z

154

Red Canyon Wind Farm | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revisionEnvReviewNonInvasiveExplorationUT-g Grant of Access Permit5-ID-aRECRaton,RFPs Home NameRecurrentRed Canyon

155

Red Hills Wind Farm | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revisionEnvReviewNonInvasiveExplorationUT-g Grant of Access Permit5-ID-aRECRaton,RFPs Home NameRecurrentRed

156

The ERE of the "Red Rectangle" revisited  

E-Print Network [OSTI]

We present in this paper high signal-to-noise long-slit optical spectra of the Extended Red Emission (ERE) in the "Red Rectangle" (RR) nebula. These spectra, obtained at different positions in the nebula, reveal an extremely complex emission pattern on top of the broad ERE continuum. It is well known that three features converge at large distance from the central object, in wavelength and profile to the diffuse interstellar bands (DIBs) at 5797, 5849.8 and 6614 ang., (e.g. Sarre et al., 1995). In this paper we give a detailed inventory of all spectral subfeatures observed in the 5550--6850 ang. spectral range. Thanks to our high S/N spectra, we propose 5 new features in the RR that can be associated with DIBs. For the 5550--6200 ang. spectral range our slit position was on top of the NE spike of the X shaped nebula. A detailed description of the spatial profile-changes is given of the strongest features revealing that even far out in the nebula at 24 arcsec from the central star, there remains a small shift in wavelength of 1 respectively 2 ang between the ERE subfeatures and the DIB wavelengths of 5797.11 and 5849.78 ang.

Hans Van Winckel; Martin Cohen; Ted R. Gull

2002-04-26T23:59:59.000Z

157

Age and growth of the red snapper, Lutjanus campechanus, and the vermilion snapper, Rhomboplites aurorubens, from the northwestern Gulf of Mexico  

E-Print Network [OSTI]

). Red snapper are found from Cape Hatteras, N. C. , south to Key West in the Atlantic and along the coastal Gulf of Mexico to the Campeche Banks The style and format of this thesis follows that of Transactions of the American Fisheries ~gociet...

Zastrow, Colleen Elizabeth

1984-01-01T23:59:59.000Z

158

Integrated Culture of Seaweeds and Red Abalone in Monterey Harbor  

E-Print Network [OSTI]

Project Hypotheses (1) Red algae and kelp can be effectivelydiets are superior to all kelp diets in enhancing farmedlaboratory methods for seeding kelp zoospores onto string

Graham, Michael H.

2008-01-01T23:59:59.000Z

159

aqaba northern red: Topics by E-print Network  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

for a population of extremely red stellar objects extracted from the point-source catalogue of the INT Photometric H-Alpha Survey (IPHAS) of the northern galactic...

160

Redding Electric- Residential and Commercial Energy Efficiency Rebate Program  

Broader source: Energy.gov [DOE]

Redding Electric Utility offers a variety of financial incentives for energy efficiency through its Earth Advantage Rebate Program. Rebates are for weatherization measures, HVAC equipment, and...

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


161

Red Fish, Blue Fish, One Fish Becomes By Chandra Shekhar  

E-Print Network [OSTI]

could impact speciation, says Carleton: Water pollution, for example, could destroy the color gradients Victoria, whereas red males dwell in deeper water. CREDIT: OLE SEEHAUSEN ADVERTISEMENT ADVERTISEMENT Home

162

Red Shift in a Laboraory Environment  

E-Print Network [OSTI]

A hypotheses of energy loss for polarization of e-e+ vacuum by a photon passing interstellar space is considered. An excitation and relaxation of vacuum can't run with speed of light due to very small but finite fraction of e-e+ pair mass that creates a retardment in recuperation of deposited energy back to photon. This "forgotten" by many photons energy is finally splashed out in real space as a Relic Radiation. An assumption that such energy loss is proportional to a photon energy conforms to Hubble low of Red Shift and experimental data treated as accelerated expansion of Universe. A possibility of an observation of this type energy loss is considered at high-energy accelerators where energy deposition may reach up hundreds MeV in second.

Yuriy A. Yatsunenko; Julian A. Budagov

2011-03-04T23:59:59.000Z

163

Intelligent Computing System for Reservoir Analysis and Risk Assessment of Red River Formation, Class Revisit  

SciTech Connect (OSTI)

Integrated software was written that comprised the tool kit for the Intelligent Computing System (ICS). The software tools in ICS are for evaluating reservoir and hydrocarbon potential from various seismic, geologic and engineering data sets. The ICS tools provided a means for logical and consistent reservoir characterization. The tools can be broadly characterized as (1) clustering tools, (2) neural solvers, (3) multiple-linear regression, (4) entrapment-potential calculator and (5) combining tools. A flexible approach can be used with the ICS tools. They can be used separately or in a series to make predictions about a desired reservoir objective. The tools in ICS are primarily designed to correlate relationships between seismic information and data obtained from wells; however, it is possible to work with well data alone.

Sippel, Mark A.

2002-09-24T23:59:59.000Z

164

Formatted: Footer, Left Formatted: Font: 10 pt  

E-Print Network [OSTI]

Formatted: Space Before: 12 pt, Border: Bottom: (Single solid line, Auto, 0.5 pt Line width) Deleted: Angelis ­ Sacramento Municipal Utility District Anne Gillette ­ California Public Utilities Commission Steven Kelly

165

ACARYOCHLORIS EXPLAINING THE RIDDLE OF CHLOROPHYLL D IN RED ALGAE AND EXPANDING PAR FOR OXYGENIC PHOTOSYNTHESIS  

E-Print Network [OSTI]

ACARYOCHLORIS ­ EXPLAINING THE RIDDLE OF CHLOROPHYLL D IN RED ALGAE AND EXPANDING PAR FOR OXYGENIC strain is shown to live epi- phytically on the red alga Gelidium caulacantheum, which itself is harvested by the red alga. Availability of far red light, however, is relatively unaffected by DOM or red

Oregon, University of

166

INHIBITION OF PHOTOSYNTHESIS IN CERTAIN ALGAE BY EXTREME RED LIGHT  

E-Print Network [OSTI]

INHIBITION OF PHOTOSYNTHESIS IN CERTAIN ALGAE BY EXTREME RED LIGHT GOVINDJEE, EUGENE RABINOWITCH. INTRODUCTION It was shown in preceding papers (9, 10) that when the unicellular red alga Por- phyridium), these algae, when exposed to monochromatic light (bands isolated by a grating monochromator, band half

Govindjee

167

MEMORIA DE LA RED DE INVESTIGACIN PARA LA DOCENCIA UNIVERSITARIA  

E-Print Network [OSTI]

Psicología Social Facultad de Ciencias Económicas y Empresariales Universidad de Alicante Red de Creatividad profesores docentes de asignaturas relacionadas con la creatividad publicitaria en el Grado de Publicidad y;1. INTRODUCCI?N La red aglutina profesores docentes de asignaturas afines con la creatividad publicitaria que

Escolano, Francisco

168

Ris-R-1513(EN) The "Red" Decline of Norway  

E-Print Network [OSTI]

Risø-R-1513(EN) The "Red" Decline of Norway Spruce or "Røde Rødgraner" ­ Is it Ammonium Overload. Engvild Title: The "Red" Decline of Norway Spruce or "Røde Rødgraner" ­ Is it Ammonium Overload or Top" decline of Norway spruce (Picea abies) became a serious problem in plantations in Jutland on poor, sandy

169

Anisotropic light scattering of individual sickle red blood cells  

E-Print Network [OSTI]

Anisotropic light scattering of individual sickle red blood cells Youngchan Kim John M. Higgins blood cells (RBCs) from a patient with sickle cell disease (SCD). To measure light scattering spectra: red blood cell; sickle cell disease; light scattering; quantita- tive phase microscopy. Paper 11736L

Suresh, Subra

170

Fife Red Squirrel Project Phase II Summary Sophie Eastwood The Fife Red Squirrel Group was established in 2006 by the Fife Countryside Ranger Service to address  

E-Print Network [OSTI]

Fife Red Squirrel Project Phase II Summary Sophie Eastwood The Fife Red Squirrel Group to red squirrel conservation in Fife. The first phase of the project centred around two pilot forests, Devilla and Ladybank. Red Squirrel Project Officer Sophie Eastwood embarked on the next stage

171

Three-dimensional hydrodynamical CO5BOLD model atmospheres of red giant stars. IV. Oxygen diagnostics in extremely metal-poor red giants with infrared OH lines  

E-Print Network [OSTI]

Context. Although oxygen is an important tracer of Galactic chemical evolution, measurements of its abundance in the atmospheres of the oldest Galactic stars are still scarce and rather imprecise. At the lowest end of the metallicity scale, oxygen can only be measured in giant stars and in most of cases such measurements rely on a single forbidden [O I] 630 nm line that is very weak and frequently blended with telluric lines. Although molecular OH lines located in the ultraviolet and infrared could also be used for the diagnostics, oxygen abundances obtained from the OH lines and the [O I] 630 nm line are usually discrepant to a level of ~0.3-0.4 dex. Aims. We study the influence of convection on the formation of the infrared (IR) OH lines and the forbidden [O I] 630 nm line in the atmospheres of extremely metal-poor (EMP) red giant stars. Methods. We used high-resolution and high signal-to-noise ratio spectra of four EMP red giant stars obtained with the VLT CRIRES spectrograph. For each EMP star, 4-14 IR OH...

Dobrovolskas, V; Bonifacio, P; Caffau, E; Ludwig, H -G; Steffen, M; Spite, M

2015-01-01T23:59:59.000Z

172

V-072: Red Hat update for java-1.7.0-openjdk | Department of...  

Broader source: Energy.gov (indexed) [DOE]

2: Red Hat update for java-1.7.0-openjdk V-072: Red Hat update for java-1.7.0-openjdk January 18, 2013 - 6:00am Addthis PROBLEM: Red Hat has issued an update for...

173

E-Print Network 3.0 - adjunct red blood Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

adjunct red blood Search Powered by Explorit Topic List Advanced Search Sample search results for: adjunct red blood Page: << < 1 2 3 4 5 > >> 1 Always Needed The American Red...

174

RedSeal Comments on "Smart Grid RFI: Addressing Policy and Logistical...  

Broader source: Energy.gov (indexed) [DOE]

RedSeal Comments on "Smart Grid RFI: Addressing Policy and Logistical Challenges. RedSeal Comments on "Smart Grid RFI: Addressing Policy and Logistical Challenges. RedSeal Comments...

175

E-Print Network 3.0 - azoene fast red Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

profile vs. Reference Dataset Summary: -of-fit chi-squared statistic values for the train, test, large (LgRed), medium (MdRed), and small (SmRed... level. Numbers in the Ref,...

176

Studies on reaction runaways for Urex/Purex solvent-nitric acid and red-oil synthesis  

SciTech Connect (OSTI)

In PUREX/UREX processes for recycling of spent nuclear fuels, 30% TBP solvent is used, This solvent has a small solubility in the aqueous phase. During concentration of the process solutions by an evaporation route, a runaway reaction between TBP and nitric acid is initiated at above 130 deg. C, leading to rapid pressurization and finally containment failure if proper venting is not provided. Red oil was synthesized for the first time in India, and its physical properties as well as thermodynamic parameters for the reaction were determined. It was experimentally established that the presence of metallic nitrates was not essential for red-oil formation as thought earlier. Various experiments have been completed for single-phase as well as two-phase runs. The most important finding of this work was lowering of the limiting acid concentration from the conventional values. In fact, in these experiments, red oil could be formed even at 2 N aqueous acidity. Thus, safety guidelines based on the classical literature are obsolete. New guidelines for the red-oil-safety are required. (authors)

Kumar, Shekhar; Kumar, Rajnish; Koganti, S.B. [Reprocessing R and D Division, Reprocessing Group, Indira Gandhi Centre for Atomic Research, Kalpakkam 603102 (India)

2008-07-01T23:59:59.000Z

177

Ordovician Red River {open_quotes}B{close_quotes}: Horizontal oil play in the southern Williston basin  

SciTech Connect (OSTI)

Recent application of horizontal drilling technology to the Ordovician Red River {open_quotes}B{close_quotes} zone in the southern Williston basin has resulted in a successful oil play, with more than 100 wells drilled in 1995 and 1996. The Red River {open_quotes}B{close_quotes} reservoir is a dolomitized laminated carbonate with microsucrosic porosity of 8-25% and permeabilities in the range of 1-66 md. It occurs within the middle of three depositional cycles ({open_quotes}A,{close_quotes} {open_quotes}B,{close_quotes} and {open_quotes}C{close_quotes}) that form the upper Red River Formation. Each cycle consists of a lower burrowed limestone, middle laminated member, and capping anhydrite or lime mudstone. The {open_quotes}B{close_quotes} reservoir is confined to the {open_quotes}B{close_quotes} laminated member and consists of an upper portion, characterized by better reservoir quality, and a lower, less permeable portion. Horizontal drilling has the advantage of significantly increasing well-bore exposure to the upper, more permeable portion. Well data indicate the total Red River {open_quotes}B{close_quotes} porosity zone has remarkable extent over parts of southwestern North Dakota, southeastern Montana, and northwestern South Dakota. Productivity from horizontal well displays considerable variation that can be correlated with structure/tectonic patterns and with reservoir petrophysical character.

Montgomery, S.L.

1997-04-01T23:59:59.000Z

178

Formation of mixed oxide powders in flames: Part II. SiO sub 2 --GeO sub 2 and Al sub 2 O sub 3 --TiO sub 2  

SciTech Connect (OSTI)

SiO{sub 2}--GeO{sub 2} and Al{sub 2}O{sub 3}--TiO{sub 2} mixed oxide powders were synthesized using a counterflow diffusion flame burner. SiCl{sub 4}, GeCl{sub 4}, Al(CH{sub 3}){sub 3}, and TiCl{sub 4} were used as source materials for the formation of oxide particles in hydrogen-oxygen flames. {ital In} {ital situ} particle sizes were determined using dynamic light-scattering. Powders were collected using two different methods, a thermophoretic method (particles are collected onto carbon coated TEM grids) and an electrophoretic method (particles are collected onto stainless steel strips). Their size, morphology, and crystalline form were examined using a transmission electron microscope and an x-ray diffractometer. A photomultiplier at 90{degree} to the argon ion laser beam was used to measure the light-scattering intensity. The formation of the mixed oxides was investigated using Si to Ge and Al to Ti ratios of 3:5 and 1:1, respectively. Heterogeneous nucleation of the SiO{sub 2} on the surface of the GeO{sub 2} was observed. In Al{sub 2}O{sub 3}--TiO{sub 2} mixtures, both oxide particles form at the same temperature. X-ray diffraction analysis of particles sampled at temperatures higher than 1553 K showed the presence of rutile, {gamma}--Al{sub 2}O{sub 3}, and aluminum titanate. Although the particle formation processes for SiO{sub 2}--GeO{sub 2} is very different from that for Al{sub 2}O{sub 3}--TiO{sub 2}, both mixed oxides result in very uniform mixtures.

Hung, C.; Miquel, P.F.; Katz, J.L. (Department of Chemical Engineering, The Johns Hopkins University, Baltimore, Maryland 21218 (United States))

1992-07-01T23:59:59.000Z

179

Red Galaxy Growth and the Halo Occupation Distribution  

E-Print Network [OSTI]

We have traced the past 7 Gyr of red galaxy stellar mass growth within dark matter halos. We have determined the halo occupation distribution, which describes how galaxies reside within dark matter halos, using the observed luminosity function and clustering of 40,696 0.2red galaxies in Bootes. Half of 10^{11.9} Msun/h halos host a red central galaxy, and this fraction increases with increasing halo mass. We do not observe any evolution of the relationship between red galaxy stellar mass and host halo mass, although we expect both galaxy stellar masses and halo masses to evolve over cosmic time. We find that the stellar mass contained within the red population has doubled since z=1, with the stellar mass within red satellite galaxies tripling over this redshift range. In cluster mass halos most of the stellar mass resides within satellite galaxies and the intra-cluster light, with a minority of the stellar mass residing within central galaxies. The stellar masses of the most luminous red central galaxies are proportional to halo mass to the power of a third. We thus conclude that halo mergers do not always lead to rapid growth of central galaxies. While very massive halos often double in mass over the past 7 Gyr, the stellar masses of their central galaxies typically grow by only 30%.

Michael J. I. Brown; Zheng Zheng; Martin White; Arjun Dey; Buell T. Jannuzi; Andrew J. Benson; Kate Brand; Mark Brodwin; Darren J. Croton

2008-04-15T23:59:59.000Z

180

U-159: Red Hat Enterprise MRG Messaging Qpid Bug Lets Certain...  

Broader source: Energy.gov (indexed) [DOE]

9: Red Hat Enterprise MRG Messaging Qpid Bug Lets Certain Remote Users Bypass Authentication U-159: Red Hat Enterprise MRG Messaging Qpid Bug Lets Certain Remote Users Bypass...

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


181

A Red Cy3-Based Biarsenical Fluorescent Probe Targeted to a Complement...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Red Cy3-Based Biarsenical Fluorescent Probe Targeted to a Complementary Binding Peptide. A Red Cy3-Based Biarsenical Fluorescent Probe Targeted to a Complementary Binding Peptide....

182

Oscillating red-giant stars in eccentric binary systems  

E-Print Network [OSTI]

The unparalleled photometric data obtained by NASA's Kepler Space Telescope has led to improved understanding of red-giant stars and binary stars. We discuss the characterization of known eccentric system, containing a solar-like oscillating red-giant primary component. We also report several new binary systems that are candidates for hosting an oscillating companion. A powerful approach to study binary stars is to combine asteroseimic techniques with light curve fitting. Seismology allows us to deduce the properties of red giants. In addition, by modeling the ellipsoidal modulations we can constrain the parameters of the binary system. An valuable independent source are ground-bases, high-resolution spectrographs.

Beck, P G; Vos, J; Kallinger, T; Garcia, R A; Mathur, S; Houmani, K

2014-01-01T23:59:59.000Z

183

Properties of Luminous Red Galaxies in the Sloan Digital Sky Survey  

E-Print Network [OSTI]

We perform population synthesis modelling of a magnitude-limited sample of 4391 Luminous Red Galaxies selected from the Sloan Digital Sky Survey Data Release 4 (SDSS DR4). We fit measured spectral indices using a large library of high resolution spectra, covering a wide range of metallicities and assuming an exponentially decaying star-formation rate punctuated by bursts, to obtain median-likelihood estimates for the light-weighted age, metallicity, stellar mass and extinction for the galaxies. The ages lie in the range 4-10 Gyr, peaking near 6 Gyr, with metallicities in the range -0.4<[Z/H]<0.4, peaking at [Z/H] ~ 0.2. Only a few per cent of the spectra are better fit allowing for a burst in addition to continuous star-formation. The total stellar masses of all the galaxies are confined to a very narrow range. Our results broadly agree with those of previous groups using an independent population synthesis code. We find, however, that our choice in priors results in ages 1-2 Gyr smaller, decreasing the peak star formation epoch from z=2.3 to z=1.3. We develop a metal evolution model incorporating stochastic star-formation quenching motivated by recent attempts to solve the `anti-hierarchical' formation problem of ellipticals. Two scenarios emerge, a closed box with an effective stellar yield of 0.26, and an accreting box with an effective stellar yield of 0.10. Both scenarios require an IMF weighted towards massive stars and characteristic star-formation quenching times of about 100 Myr, the expected lifetime of luminous QSOs. The models predict an anti-correlation between the age and mean metallicity similar to that observed.

T. Barber; A. Meiksin; T. Murphy

2006-11-02T23:59:59.000Z

184

Inert plug formation in the DDT of granular energetic materials  

SciTech Connect (OSTI)

A mechanism is proposed to explain the {open_quotes}plugs{close_quotes} that have been observed in deflagration-to-detonation transition (DDT) of granular explosives. Numerical simulations are performed that demonstrate the proposed mechanism. Observed trends are reproduced. {copyright} {ital 1996 American Institute of Physics.}

Son, S.F.; Asay, B.W.; Bdzil, J.B. [Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States of America)

1996-05-01T23:59:59.000Z

185

Red River Valley REA- Heat Pump Loan Program  

Broader source: Energy.gov [DOE]

The Red River Valley Rural Electric Association (RRVREA) offers a loan program to its members for air-source and geothermal heat pumps. Loans are available for geothermal heat pumps at a 5% fixed...

186

Western Red-tailed Skink Distribution in Southern Nevada  

SciTech Connect (OSTI)

This slide show reports a study to: determine Western Red-tailed Skink (WRTS) distribution on Nevada National Security Site (NNSS); identify habitat where WRTS occur; learn more about WRTS natural history; and document distribution of other species.

Hall, D. B. and Gergor, P. D.

2011-11-01T23:59:59.000Z

187

Regulation of Pituitary Thyrotropin Production in Red Drum  

E-Print Network [OSTI]

of pituitary hormone production and secretion is accomplished by a portal system which delivers thyrotropin-releasing hormone to positively stimulate the pituitary to release more TSH. However, in teleost fish such as the red drum (Sciaenops ocellatus), TSH...

Drone, Elizabeth

2011-01-11T23:59:59.000Z

188

Red Sequence Cluster Finding in the Millennium Simulation  

E-Print Network [OSTI]

We investigate halo mass selection properties of red-sequence cluster finders using galaxy populations of the Millennium Simulation (MS). A clear red sequence exists for MS galaxies in massive halos at redshifts z red sequence and confusion from a larger number of intermediate mass halos hosting bright red galaxies of magnitude similar to those in higher mass halos. Our method produces catalogs of cluster candidates whose halo mass selection function, p(M|\\Ngal,z), is characterized by a bimodal log-normal model with a dominant component that reproduces well the real-space distribution, and a redshift-dependent tail that is broader and displaced by a factor ~2 lower in mass. We discuss implications for X-ray properties of optically selected clusters and offer ideas for improving both mock catalogs and cluster-finding in future surveys.

J. D. Cohn; A. E. Evrard; M. White; D. Croton; E. Ellingson

2007-09-17T23:59:59.000Z

189

Anisotropic light scattering of individual sickle red blood cells  

E-Print Network [OSTI]

We present the anisotropic light scattering of individual red blood cells (RBCs) from a patient with sickle cell disease (SCD). To measure light scattering spectra along two independent axes of elongated-shaped sickle RBCs ...

Kim, Youngchan

190

Deformability of Plasmodium falciparum parasitized red blood cells  

E-Print Network [OSTI]

The biophysical properties of the human red blood cell (RBC) permit large deformations required for passage through narrow capillaries and spleen sinusoids. Several pathologic conditions alter RBC deformability that can ...

Mills, John Philip, Ph. D. Massachusetts Institute of Technology

2007-01-01T23:59:59.000Z

191

Red Ink : open source financial analytics for people & communities  

E-Print Network [OSTI]

Red Ink is an open source social-financial web-service that enables people to share, aggregate, analyze, visualize and publish their financial transactions as individuals and ad-hoc groups, through data sharing campaigns. ...

O'Toole, Ryan (Ryan Michael)

2010-01-01T23:59:59.000Z

192

Entrance-channel mass-asymmetry dependence of compound nucleus formation time in light heavy-ion reactions  

SciTech Connect (OSTI)

The entrance-channel mass-asymmetry dependence of the compound nucleus formation time in light heavy-ion reactions has been investigated within the framework of semiclassical dissipative collision models. The model calculations have been applied successfully to the formation of the {sup 38}Ar compound nucleus as populated via the {sup 9}Be+{sup 29}Si, {sup 11}B+{sup 27}Al, {sup 12}C+{sup 26}Mg, and {sup 19}F+{sup 19}F entrance channels. The shape evolution of several other light composite systems appears to be consistent with the so-called {open_quote}{open_quote}Fusion Inhibition Factor{close_quote}{close_quote} which has been observed experimentally. As found previously in more massive systems for the fusion-evaporation process, the entrance-channel mass-asymmetry degree of freedom appears to determine the competition between the different mechanisms as well as the time scales involved. {copyright} {ital 1996 The American Physical Society.}

Szanto de Toledo, A. [Instituto de Fisica da Universidade de Sao Paulo, Departamento de Fisica Nuclear-Laboratorio, Pelletron, Caixa Postal 66318-05389-970 Sao Paulo, (Brasil)] [Instituto de Fisica da Universidade de Sao Paulo, Departamento de Fisica Nuclear-Laboratorio, Pelletron, Caixa Postal 66318-05389-970 Sao Paulo, (Brasil); Carlson, B.V. [Departamento de Fisica, Instituto Tecnologico da Aeronautica, Centro Tecnico Aerospacial, 12228-900 Sao Jose dos Campos, (Brasil)] [Departamento de Fisica, Instituto Tecnologico da Aeronautica, Centro Tecnico Aerospacial, 12228-900 Sao Jose dos Campos, (Brasil); Beck, C. [Centre de Recherches Nucleaires, Institut National de Physique Nucleaire et de Physique des Particules-Centre National de la Recherche Scientifique/Universite Louis Pasteur, Boite Postale 28, F-67037 Strasbourg Cedex 2 (France)] [Centre de Recherches Nucleaires, Institut National de Physique Nucleaire et de Physique des Particules-Centre National de la Recherche Scientifique/Universite Louis Pasteur, Boite Postale 28, F-67037 Strasbourg Cedex 2 (France); Thoennessen, M. [National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824 (United States)] [National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824 (United States)

1996-12-01T23:59:59.000Z

193

Red Storm usage model :Version 1.12.  

SciTech Connect (OSTI)

Red Storm is an Advanced Simulation and Computing (ASC) funded massively parallel supercomputer located at Sandia National Laboratories (SNL). The Red Storm Usage Model (RSUM) documents the capabilities and the environment provided for the FY05 Tri-Lab Level II Limited Availability Red Storm User Environment Milestone and the FY05 SNL Level II Limited Availability Red Storm Platform Milestone. This document describes specific capabilities, tools, and procedures to support both local and remote users. The model is focused on the needs of the ASC user working in the secure computing environments at Los Alamos National Laboratory (LANL), Lawrence Livermore National Laboratory (LLNL), and SNL. Additionally, the Red Storm Usage Model maps the provided capabilities to the Tri-Lab ASC Computing Environment (ACE) requirements. The ACE requirements reflect the high performance computing requirements for the ASC community and have been updated in FY05 to reflect the community's needs. For each section of the RSUM, Appendix I maps the ACE requirements to the Limited Availability User Environment capabilities and includes a description of ACE requirements met and those requirements that are not met in that particular section. The Red Storm Usage Model, along with the ACE mappings, has been issued and vetted throughout the Tri-Lab community.

Jefferson, Karen L.; Sturtevant, Judith E.

2005-12-01T23:59:59.000Z

194

Red inalmbrica de la Universidad de Alicante La Red Inalmbrica de la UA (eduroam) es una extensin de la red local, disponible en el 99% del Campus de San  

E-Print Network [OSTI]

Red inalámbrica de la Universidad de Alicante La Red Inalámbrica de la UA (eduroam) es una extensión de la red local, disponible en el 99% del Campus de San Vicente. eduroam (Educational Roaming) es no puedan utilizarse en la red wireless de la UA o sufran problemas de navegación o conexión. No se ofrecerá

Escolano, Francisco

195

Assessment of Biomass Energy Opportunities for the Red Lake Band of Chippewa Indians  

SciTech Connect (OSTI)

Assessment of biomass energy and biobased product manufacturing opportunities for the Red Lake Tribe.

Scott Haase (McNeil Technologies, Inc)

2005-09-30T23:59:59.000Z

196

AbstractThe red porgy, Pagrus pag rus, is an important reef fish in several  

E-Print Network [OSTI]

81 Abstract­The red porgy, Pagrus pag rus, is an important reef fish in several offshore fisheries a fishery-independent source. Red porgy attain a maximum age of at least 18 years and 733 mm total length revealed a difference in mean length at age of red porgy from the three sources. Red porgy in fishery

197

Red-Black Relaxed Plan Heuristics Michael Katz and Jorg Hoffmann  

E-Print Network [OSTI]

Red-Black Relaxed Plan Heuristics Michael Katz and J¨org Hoffmann Saarland University Saarbr the red-black planning frame- work, where red variables take the relaxed semantics (accu- mulating their values), while black variables take the regular semantics. Provided the red variables are chosen so

Domshlak, Carmel

198

Red Hat Enterprise Linux 3 The Next Generation Of Enterprise Class Linux  

E-Print Network [OSTI]

Page 1 Red Hat Enterprise Linux 3 The Next Generation Of Enterprise Class Linux Ken Crandall Engineer, Red Hat Version: 3.7ICCAD #12;Page 2 Agenda Why Red Hat Enterprise Linux Workstations High Performance Computing Summary Q & A #12;Page 3 Why Red Hat Enterprise Linux? Version: 3.7ICCAD #12;Page 4

199

Red drum, Sciaenops ocellatus, is an estuary-dependent marine spe-  

E-Print Network [OSTI]

730 Red drum, Sciaenops ocellatus, is an estuary-dependent marine spe- cies found in coastal to Vera Cruz, Mexico (Yokel, 1966, 1980). Red drum are highly sought after as food and gamefish. Annual the sale of red drum was pro- hibited. Recreational fishing effort directed toward red drum in Florida has

200

The Red Queen and the Court Jester: Species Diversity and the Role of Biotic  

E-Print Network [OSTI]

REVIEW The Red Queen and the Court Jester: Species Diversity and the Role of Biotic and Abiotic Factors Through Time Michael J. Benton Evolution may be dominated by biotic factors, as in the Red Queen the Red Queen or the Court Jester. The Red Queen model (1) stems from Darwin, who viewed evo- lution

Benton, Michael

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


201

Red variables in the OGLE-II data base -- III. Constraints on the three-dimensional structures of the LMC and SMC  

E-Print Network [OSTI]

We present an analysis of the 3-D structure of the Magellanic Clouds, using period-luminosity (P-L) relations of pulsating red giants in the OGLE-II sample. By interpreting deviations from the mean P-L relations as distance modulus variations, we examine the three-dimensional distributions of the sample. The results for the Large Magellanic Cloud, based solely on stars below the tip of the Red Giant Branch, confirm previous results on the inclined and possibly warped bar of the LMC. The depth variation across the OGLE-II field is about 2.4 kpc, interpreted as the distance range of a thin but inclined structure. The inclination angle is about 29 deg. A comparison with OGLE-II red clump distances revealed intriguing differences that seem to be connected to the red clump reddening correction. A spatially variable red clump population in the LMC can explain the deviations, which may have a broader impact on our understanding of the LMC formation history. For the Small Magellanic Cloud, we find a complex structure showing patchy distribution scattered within 3.2 kpc of the mean. However, the larger range of the overall depth on every line-of-sight is likely to smooth out significantly the real variations.

P. Lah; L. L. Kiss; T. R. Bedding

2005-02-22T23:59:59.000Z

202

Unlayered graphenes in red-giant starsmoke  

E-Print Network [OSTI]

Electron diffraction, imaging, and energy loss provide evidence for unlayered graphene sheets in the core of certain interstellar graphite onions (from the meteorite Murchison) whose isotopes indicate formation in the atmosphere of late-stage asymptotic giant branch stars (like those which nucleo-synthesized much of the earth's carbon). The data are compared to structural models loosely associated with atom-by-atom, molecule-by-molecule, and dendritic-droplet solidification processes. In this context the observed density, diffraction peak-shapes, and edge-on sheet patterns, along with theoretical limits on time for growth in the presence of outgoing radiation pressure, suggest nucleation of hexagonal sheets from pentagons, perhaps from a supercooled melt. These results warrant a closer examination of specimen structure, the energetics of unlayered graphene nucleation, and processes such as jets in late star atmospheres.

Eric Mandell; Nathaniel Hunton; P. Fraundorf

2006-06-04T23:59:59.000Z

203

AMPLITUDES OF SOLAR-LIKE OSCILLATIONS: CONSTRAINTS FROM RED GIANTS IN OPEN CLUSTERS OBSERVED BY KEPLER  

SciTech Connect (OSTI)

Scaling relations that link asteroseismic quantities to global stellar properties are important for gaining understanding of the intricate physics that underpins stellar pulsations. The common notion that all stars in an open cluster have essentially the same distance, age, and initial composition implies that the stellar parameters can be measured to much higher precision than what is usually achievable for single stars. This makes clusters ideal for exploring the relation between the mode amplitude of solar-like oscillations and the global stellar properties. We have analyzed data obtained with NASA's Kepler space telescope to study solar-like oscillations in 100 red giant stars located in either of the three open clusters, NGC 6791, NGC 6819, and NGC 6811. By fitting the measured amplitudes to predictions from simple scaling relations that depend on luminosity, mass, and effective temperature, we find that the data cannot be described by any power of the luminosity-to-mass ratio as previously assumed. As a result we provide a new improved empirical relation which treats luminosity and mass separately. This relation turns out to also work remarkably well for main-sequence and subgiant stars. In addition, the measured amplitudes reveal the potential presence of a number of previously unknown unresolved binaries in the red clump in NGC 6791 and NGC 6819, pointing to an interesting new application for asteroseismology as a probe into the formation history of open clusters.

Stello, Dennis; Huber, Daniel; Bedding, Timothy R.; Benomar, Othman [Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, NSW 2006 (Australia); Kallinger, Thomas [Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1 (Canada); Basu, Sarbani [Department of Astronomy, Yale University, P.O. Box 208101, New Haven, CT 06520-8101 (United States); Mosser, BenoIt [LESIA, CNRS, Universite Pierre et Marie Curie, Universite Denis Diderot, Observatoire de Paris, 92195 Meudon (France); Hekker, Saskia [Astronomical Institute 'Anton Pannekoek', University of Amsterdam, P.O. Box 94249, 1090 GE Amsterdam (Netherlands); Mathur, Savita [High Altitude Observatory, NCAR, P.O. Box 3000, Boulder, CO 80307 (United States); GarcIa, Rafael A. [Laboratoire AIM, CEA/DSM-CNRS, Universite Paris 7 Diderot, IRFU/SAp, Centre de Saclay, 91191 Gif-sur-Yvette (France); Kjeldsen, Hans; Grundahl, Frank; Christensen-Dalsgaard, Joergen [Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, 8000 Aarhus C (Denmark); Gilliland, Ronald L. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Verner, Graham A.; Chaplin, William J.; Elsworth, Yvonne P. [School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT (United Kingdom); Meibom, Soeren [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Molenda-Zakowicz, Joanna [Instytut Astronomiczny Uniwersytetu Wroclawskiego, ul. Kopernika 11, 51-622 Wroclaw (Poland); Szabo, Robert [Konkoly Observatory of the Hungarian Academy of Sciences, Konkoly Thege Miklos ut 15-17, H-1121 Budapest (Hungary)

2011-08-10T23:59:59.000Z

204

Vegetation's Red Edge: A Possible Spectroscopic Biosignature of Extraterrestrial Plants  

E-Print Network [OSTI]

Earth's deciduous plants have a sharp order-of-magnitude increase in leaf reflectance between approximately 700 and 750 nm wavelength. This strong reflectance of Earth's vegetation suggests that surface biosignatures with sharp spectral features might be detectable in the spectrum of scattered light from a spatially unresolved extrasolar terrestrial planet. We assess the potential of Earth's step-function-like spectroscopic feature, referred to as the "red edge", as a tool for astrobiology. We review the basic characteristics and physical origin of the red edge and summarize its use in astronomy: early spectroscopic efforts to search for vegetation on Mars and recent reports of detection of the red edge in the spectrum of Earthshine (i.e., the spatially integrated scattered light spectrum of Earth). We present Earthshine observations from Apache Point Observatory to emphasize that time variability is key to detecting weak surface biosignatures such as the vegetation red edge. We briefly discuss the evolutionary advantages of vegetation's red edge reflectance, and speculate that while extraterrestrial "light harvesting organisms" have no compelling reason to display the exact same red edge feature as terrestrial vegetation, they might have similar spectroscopic features at different wavelengths than terrestrial vegetation. This implies that future terrestrial-planet-characterizing space missions should obtain data that allow time-varying, sharp spectral features at unknown wavelengths to be identified. We caution that some mineral reflectance edges are similar in slope and strength to vegetation's red edge (albeit at different wavelengths); if an extrasolar planet reflectance edge is detected care must be taken with its interpretation.

Sara Seager; Edwin L. Turner; Justin Schafer; Eric B. Ford

2005-03-14T23:59:59.000Z

205

Experimental and theoretical study of red-shifted solitonic resonant radiation in photonic crystal fibers and generation of radiation seeded Raman solitons  

E-Print Network [OSTI]

The red shifted solitonic resonant radiation is a fascinating phase matching phenomenon that occurs when an optical pulse, launched in the normal dispersion regime of photonic crystal fiber, radiates across the zero dispersion wavelength. The formation of such phase-matched radiation is independent of the generation of any optical soliton and mainly governed by the leading edge of input pump which forms a shock front. The radiation is generated at the anomalous dispersion regime and found to be confined both in time and frequency domain. We experimentally investigate the formation of such radiations in photonic crystal fibers with detailed theoretical analysis. Our theoretical predictions corroborate well with experimental results. Further we extend our study for long length fiber and investigate the interplay between red-shifted solitonic resonant radiation and intrapulse Raman scattering (IPRS). It is observed that series of radiation-seeded Raman solitons are generated in anomalous dispersion regime.

Bose, Surajit; Chattopadhyay, Rik; Pal, Mrinmay; Bhadra, Shyamal K

2015-01-01T23:59:59.000Z

206

The Suitable Geological Formations for Spent Fuel Disposal in Romania  

SciTech Connect (OSTI)

Using the experience in the field of advanced countries and formerly Romanian program data, ANDRAD, the agency responsible for the disposal of radioactive wastes, started the program for spent fuel disposal in deep geological formations with a documentary analysis at the national scale. The potential geological formations properly characterized elsewhere in the world: salt, clay, volcanic tuff, granite and crystalline rocks,. are all present in Romania. Using general or specific selection criteria, we presently consider the following two areas for candidate geological formations: 1. Clay formations in two areas in the western part of Romania: (1) The Pannonian basin Socodor - Zarand, where the clay formation is 3000 m thick, with many bentonitic strata and undisturbed structure, and (2) The Eocene Red Clay on the Somes River, extending 1200 m below the surface. They both need a large investigation program in order to establish and select the required homogeneous, dry and undisturbed zones at a suitable depth. 2. Old platform green schist formations, low metamorphosed, quartz and feldspar rich rocks, in the Central Dobrogea structural unit, not far from Cernavoda NPP (30 km average distance), 3000 m thick and including many homogeneous, fine granular, undisturbed, up to 300 m thick layers. (authors)

Marunteanu, C. [Bucharest Univ. (Romania); Ionita, G. [ANDRAD, Bucharest (Romania); Durdun, I. [S.C. GEOTEC S.A., Bucharest (Romania)

2007-07-01T23:59:59.000Z

207

Effects of Gossypol Consumption on the Growth Traits of Red Deer Stags and Supplemental Melatonin for Advancement of Estrous Cycles in Red Deer Hinds.  

E-Print Network [OSTI]

EFFECTS OF GOSSYPOL CONSUMPTION ON GROWTH TRAITS OF RED DEER STAGS AND SUPPLEMENTAL MELATONIN FOR ADVANCEMENT OF ESTROUS CYCLES IN RED DEER HINDS A Thesis by SHANE LEE MORGAN Submitted to the Office of Graduate Studies of Texas A... Stags and Supplemental Melatonin for Advancement of Estrous Cycles in Red Deer Hinds Copyright 2011 Shane Lee Morgan EFFECTS OF GOSSYPOL CONSUMPTION ON GROWTH TRAITS OF RED DEER STAGS AND SUPPLEMENTAL MELATONIN FOR ADVANCEMENT OF ESTROUS...

Morgan, Shane

2011-08-08T23:59:59.000Z

208

Red Fork sandstone of Oklahoma: depositional history and reservoir distribution  

SciTech Connect (OSTI)

The Middle Pennsylvanian Red Fork sandstone formed as a result of progradation across eastern Kansas and most of Oklahoma. The Red Fork is one of several transgressive-regressive sequences (cyclothems) developed within the Desmoinesian Cherokee Group. Sea level changes, together with varying subsidence, were dominant factors controlling the general stratigraphic (correlative) characteristics of the Red Fork interval. Progradation was episodic, with sand deposition in the more active part of the basin during lower sea level stands and valley-fill deposition in the more stable areas during sea level rises. A map of Red Fork sand trends reveals an alluvial-deltaic complex covering most of Oklahoma. The Red Fork consists primarily of alluvial-valley and plain (fluvial) bodies in the northernmost part of northeastern Oklahoma, alluvial-deltaic bodies in most of the remaining parts of the shelf area, and off-shelf submarine-fan and slope basinal-floor complexes within the deeper part of the Anadarko basin. Determination of reservoir trend and genesis requires integration of rock and log data. Logs need to be calibrated to cores in order to estimate depositional environments accurately and to make a reasonable assessment of diagenetic overprints. Much of the oil and gas has been trapped in stratigraphic traps, and a significant amount of oil is in channel sandstones with trends at high angles to the structural grain. In some areas, secondary clay, in particular chloritic clay, has resulted in microporosity, high water saturation, and correspondingly low resistivities in oil reserves.

Shelton, J.W.; Fritz, R.D.; Johnson, C.

1989-03-01T23:59:59.000Z

209

Red phosphors for use in high CRI fluorescent lamps  

DOE Patents [OSTI]

Novel red emitting phosphors for use in fluorescent lamps resulting in superior color rendering index values compared to conventional red phosphors. Also disclosed is a fluorescent lamp including a phosphor layer comprising blends of one or more of a blue phosphor, a blue-green phosphor, a green phosphor and a red a phosphor selected from the group consisting of SrY.sub.2 O.sub.4 :Eu.sup.3+, (Y,Gd)Al.sub.3 B.sub.4 O.sub.12 :Eu.sup.3+, and [(Y.sub.1-x-y-m La.sub.y)Gd.sub.x ]BO.sub.3 :Eu.sub.m wherein y<0.50 and m=0.001-0.3. The phosphor layer can optionally include an additional deep red phosphor and a yellow emitting phosphor. The resulting lamp will exhibit a white light having a color rendering index of 90 or higher with a correlated color temperature of from 2500 to 10000 Kelvin. The use of the disclosed red phosphors in phosphor blends of lamps results in high CRI light sources with increased stability and acceptable lumen maintenance over the course of the lamp life.

Srivastava, Alok; Comanzo, Holly; Manivannan, Vankatesan; Setlur, Anant Achyut

2005-11-15T23:59:59.000Z

210

Red River play, Gulf Canada deal boost Williston basin  

SciTech Connect (OSTI)

High levels of activity in the Williston basin are assured this year with an expanding horizontal drilling play for oil in Ordovician Red River. The Red River play, like the Mississippian Lodgepole mound play, is centered in North Dakota. But the Red River play is much larger, extending into eastern Montana and northwestern South Dakota. More than 500 Red River B wells have been staked. One of the most recent companies to position itself in both plays is Gulf Canada Resources Ltd. The company forged an agreement with the Assiniboine and Sioux Indian tribes. The agreement initially provides Gulf access to about 800,000 acres on the Fort Peck Indian Reservation, mostly in Roosevelt County, Mont., on the western slope of the Williston basin. Under an option, Gulf`s access could later expand to cover the reservation`s remaining 1.3 million acres. The paper discusses the extent of the Red River play, and Gulf Canada`s role in its development.

NONE

1997-01-20T23:59:59.000Z

211

Ages of White Dwarf-Red Subdwarf Systems  

E-Print Network [OSTI]

We provide the first age estimates for two recently discovered white dwarf-red subdwarf systems, LHS 193AB and LHS 300AB. These unusual systems provide a new opportunity for linking the reliable age estimates for the white dwarfs to the (measurable) metallicities of the red subdwarfs. We have obtained precise photometry in the $V_{J}R_{KC}I_{KC}JH$ bands and spectroscopy covering from 6000\\AA to 9000\\AA for the two new systems, as well as for a comparison white dwarf-main sequence red dwarf system, GJ 283 AB. Using model grids available in the literature, we estimate the cooling age as well as temperature, surface gravity, mass, progenitor mass and {\\it total} lifetimes of the white dwarfs. The results indicate that the two new systems are probably ancient thick disk objects with ages of at least 6-9 Gyr. We also conduct searches of red dwarf and white dwarf compendia from SDSS data and the L{\\'e}pine Shara Proper Motion (LSPM) catalog for additional common proper motion white dwarf-red subdwarf systems. Only seven new candidate systems are found, which indicates the rarity of these systems.

Hektor Monteiro; Wei-Chun Jao; Todd Henry; John Subasavage; Thom Beaulieu

2005-10-12T23:59:59.000Z

212

Energy conditions in the epoch of galaxy formation  

E-Print Network [OSTI]

The energy conditions of Einstein gravity (classical general relativity) do not require one to fix a specific equation of state. In a Friedmann-Robertson-Walker universe where the equation of state for the cosmological fluid is uncertain, the energy conditions provide simple, model-independent, and robust bounds on the behaviour of the density and look-back time as a function of red-shift. Current observations suggest that the "strong energy condition" is violated sometime between the epoch of galaxy formation and the present. This implies that no possible combination of "normal" matter is capable of fitting the observational data.

Visser, Matt

2015-01-01T23:59:59.000Z

213

Radiolabeled red blood cells: status, problems, and prospects  

SciTech Connect (OSTI)

Radionuclidic labels for red cells can be divided into two main categories - cohort or pulse labels, and random labels. The random labels are incorporated into circulating cells of all ages and the labeling process is usually carried out in vitro. The red cell labels in predominant use involve random labeling and employ technetium-99m, chromium-51, indium-111, and gallium-68, roughly in that order. The extent of usefulness depends on the properties of the label such as the half-life, decay mode, and in-vivo stability, etc. Labeled cells can be used for red cell survival measurements when the half-life of the radionuclide is sufficiently long. The major portion of this article deals with random labels.

Srivastava, S.C.

1983-01-01T23:59:59.000Z

214

Red rice control in rice using herbicides plus safeners  

E-Print Network [OSTI]

of the herbicide was a stand reduc- TABLE I Effect of Preplant Incorporated Applications of Alachlor, DCPA, and Molinate on Red Rice Rate No. coleoptiles Fr. Wt. * Herbicide (kg/ha) emerged of Check % Control Alachlor Check 1. 12 2. 24 3. 36 0 0 0 22... for the TABLE II Effect of Molinate Applied Preplant Incorporated at 5. 60 kg/ha on Red Rice Planted At Different Soil Depths Planting Depth (cm) No. Coleoptiles Fr. Wt. * I Control Emerged of Check 0 2. 54 3. 81 5. 08 6. 35 Check 12 9 9 7 11 22...

Price, James Bain

1977-01-01T23:59:59.000Z

215

Dietary phosphorus requirement of juvenile red drum, Sciaenops ocellatus  

E-Print Network [OSTI]

DIETARy PHOSPHORUS REQUIREMENT OF JUVENILE RED DRUNK ~CIAO)PS QCELIA~K A Thesis by DONALD ALLEN DAVIS Submitted to the Graduate College of Texas A a N University in partial fulfillment of the requirements for the degree of 1%STER OF SCIENCE... ~r 1986 Najor Subject: Wildlife and Fisheries Sciences DIETARY PHOSPHORUS REQUIRENENT FOR JUVENILE RED DRUN, jKIMgllLPS ~CCEUAlU . A Thesis by Approved as to style and content by: Edwin H. Robinson (Chairman of Committee) Kirk Strawn (Nenber...

Davis, Donald Allen

1986-01-01T23:59:59.000Z

216

Method for determining properties of red blood cells  

DOE Patents [OSTI]

A method for quantifying the concentration of hemoglobin in a cell, and indicia of anemia, comprises determining the wavelength of the longitudinal mode of a liquid in a laser microcavity; determining the wavelength of the fundamental transverse mode of a red blood cell in the liquid in the laser microcavity; and determining if the cell is anemic from the difference between the wavelength of the longitudinal mode and the fundamental transverse mode. In addition to measuring hemoglobin, the invention includes a method using intracavity laser spectroscopy to measure the change in spectra as a function of time for measuring the influx of water into a red blood cell and the cell's subsequent rupture.

Gourley, Paul L. (Albuquerque, NM)

2001-01-01T23:59:59.000Z

217

Varieties of Cotton in the Red Prairies of Northwest Texas.  

E-Print Network [OSTI]

. NORTHCUTT. JR., B. S.. Feed Inspedor SIDNEY D. REYNOLDS. JR.. Feed Inspector P. A. MOORE, Feed Inspector SUBSTATIONS No. 1 Beerille, Bee County: R. A. HALL, B. S.. Superintendent o. 10. Ftsdfng and Breeding Station. near College Station. Brazos Connty... OF COTTON IN THE RED PRAIRIES OF NORTH- WEST TEXAS Substation No. 12 of the Texas Agricultural Experiment Station is located in the eastern part of Hardeman County southwest of Chilli- cothe about midway between the Red and Pease Rivers, and in the seo...

Quinby, John Roy

1927-01-01T23:59:59.000Z

218

Genetic endangerment of wild Red Junglefowl *Gallus gallus*?  

E-Print Network [OSTI]

in organizing an d com- puterizing data and Davi d Watso n inspected critica l specimens in Europea n museums. This study was supported in part by Financial Assistance Award No DE-FC09-96SR18546 from th e U.S. Department o f Energy to the University of Georgia...Bird Conservation International (1999) 9:387-394. BirdLife International 199 9 Genetic endangerment of wild Red Junglefowl Gallus gallus? A. TOWNSEND PETERSON and I. LEHR BRISBIN, JR Summary Domestic chickens were derived from the wild Red...

Peterson, A. Townsend; Brisbin, I. Lehr Jr

1998-01-01T23:59:59.000Z

219

Observing Massive Galaxy Formation  

E-Print Network [OSTI]

A major goal of contemporary astrophysics is understanding the origin of the most massive galaxies in the universe, particularly nearby ellipticals and spirals. Theoretical models of galaxy formation have existed for many decades, although low and high redshift observations are only beginning to put constraints on different ideas. We briefly describe these observations and how they are revealing the methods by which galaxies form by contrasting and comparing fiducial rapid collapse and hierarchical formation model predictions. The available data show that cluster ellipticals must have rapidly formed at z > 2, and that up to 50% of all massive galaxies at z ~ 2.5 are involved in major mergers. While the former is consistent with the monolithic collapse picture, we argue that hierarchal formation is the only model that can reproduce all the available observations.

Christopher J. Conselice

2002-12-20T23:59:59.000Z

220

JPEG File Interchange Format  

E-Print Network [OSTI]

interchange format compressed image representation PC or Mac or Unix workstation compatible Standard color space: one or three components. For three components, YCbCr (CCIR 601-256 levels) APP0 marker used to specify Units, X pixel density, Y pixel... by the Macintosh but not by PCs or workstations. JPEG File Interchange Format, Version 1.02 2 Standard color space The color space to be used is YCbCr as defined by CCIR 601 (256 levels). The RGB components calculated by linear conversion from YCbCr shall...

Hamilton, Eric

2004-03-30T23:59:59.000Z

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


221

Isolating Triggered Star Formation  

SciTech Connect (OSTI)

Galaxy pairs provide a potentially powerful means of studying triggered star formation from galaxy interactions. We use a large cosmological N-body simulation coupled with a well-tested semi-analytic substructure model to demonstrate that the majority of galaxies in close pairs reside within cluster or group-size halos and therefore represent a biased population, poorly suited for direct comparison to 'field' galaxies. Thus, the frequent observation that some types of galaxies in pairs have redder colors than 'field' galaxies is primarily a selection effect. We use our simulations to devise a means to select galaxy pairs that are isolated in their dark matter halos with respect to other massive subhalos (N= 2 halos) and to select a control sample of isolated galaxies (N= 1 halos) for comparison. We then apply these selection criteria to a volume-limited subset of the 2dF Galaxy Redshift Survey with M{sub B,j} {le} -19 and obtain the first clean measure of the typical fraction of galaxies affected by triggered star formation and the average elevation in the star formation rate. We find that 24% (30.5 %) of these L* and sub-L* galaxies in isolated 50 (30) h{sup -1} kpc pairs exhibit star formation that is boosted by a factor of {approx}> 5 above their average past value, while only 10% of isolated galaxies in the control sample show this level of enhancement. Thus, 14% (20 %) of the galaxies in these close pairs show clear triggered star formation. Our orbit models suggest that 12% (16%) of 50 (30) h{sup -1} kpc close pairs that are isolated according to our definition have had a close ({le} 30 h{sup -1} kpc) pass within the last Gyr. Thus, the data are broadly consistent with a scenario in which most or all close passes of isolated pairs result in triggered star formation. The isolation criteria we develop provide a means to constrain star formation and feedback prescriptions in hydrodynamic simulations and a very general method of understanding the importance of triggered star formation in a cosmological context.

Barton, Elizabeth J.; Arnold, Jacob A.; /UC, Irvine; Zentner, Andrew R.; /KICP, Chicago /Chicago U., EFI; Bullock, James S.; /UC, Irvine; Wechsler, Risa H.; /KIPAC, Menlo

2007-09-12T23:59:59.000Z

222

New red phosphor for near-ultraviolet light-emitting diodes with high color-purity  

SciTech Connect (OSTI)

New red phosphors, Na{sub 5}Eu(MoO{sub 4}){sub 4} doped with boron oxide were prepared by the solid-state reaction. Their structure and photo-luminescent properties were investigated. With the introduction of boron oxide, the red emission intensity of the phosphors under 395 nm excitation is strengthened, with high color-purity (x = 0.673, y = 0.327). The single red light-emitting diode was obtained by combining InGaN chip with the red phosphor, bright red light can be observed by naked eyes from the red light-emitting diodes under a forward bias of 20 mA.

Wang, Zhengliang, E-mail: wzhl_ww@yahoo.com.cn [School of Chemistry and Biotechnology, Yunnan Nationalities University, Kunming, Yunnan 650031 (China)] [School of Chemistry and Biotechnology, Yunnan Nationalities University, Kunming, Yunnan 650031 (China); He, Pei; Wang, Rui [School of Chemistry and Chemical Engineering, Sun Yat-sen University, Guangzhou, Guangdong 510275 (China)] [School of Chemistry and Chemical Engineering, Sun Yat-sen University, Guangzhou, Guangdong 510275 (China); Zhao, Jishou [School of Chemistry and Biotechnology, Yunnan Nationalities University, Kunming, Yunnan 650031 (China)] [School of Chemistry and Biotechnology, Yunnan Nationalities University, Kunming, Yunnan 650031 (China); Gong, Menglian [School of Chemistry and Chemical Engineering, Sun Yat-sen University, Guangzhou, Guangdong 510275 (China)] [School of Chemistry and Chemical Engineering, Sun Yat-sen University, Guangzhou, Guangdong 510275 (China)

2010-02-15T23:59:59.000Z

223

Introduction Format Proprietaire -Standard  

E-Print Network [OSTI]

Code for Information Interchange) 4. Unicode IFT-1215 Stefan Monnier 7 #12;BCD IFT-1215 Stefan MonnierSOMMAIRE Introduction Format Propri´etaire -Standard Code Alphanum´erique Entr´ee Alphanum : !, ?, ", (, . . . · Caract`eres sp´eciaux : *, $, ¿, . . . Quelques standards utilis´es pour les coder en binaires 1. BCD

Monnier, Stefan

224

Hair follicle Formation of  

E-Print Network [OSTI]

Hair follicle Formation of new follicles Bud Healed skin Hair bulge Open wound Epidermis a b Dermis 1950s and help to explain the controversy. What is the origin of the cells that make up these new hair follicles? Are they derived from existing hair follicles located at the wound edge

Chuong, Cheng-Ming

225

The Ultraviolet-Optical Color-Magnitude Diagram III: Constraints on Evolution from the Blue to Red Sequence  

E-Print Network [OSTI]

We introduce a new quantity, the mass flux density of galaxies evolving from the blue sequence to the red sequence. We propose a simple technique for constraining this mass flux using the volume corrected number density in the extinction-corrected UV-optical color magnitude distribution, the stellar age indexes H-delta-a and D_n(4000), and a simple prescription for spectral evolution using a quenched star formation history. We exploit the excellent separation of red and blue sequences in the NUV-r band color-magnitude diagram. The final value we measure, 0.033 M_sun yr^-1 Mpc^-3, is strictly speaking an upper limit due to the possible contributions of bursting, composite, and extincted galaxies. However, it compares favorably with estimates of the average mass flux that we make based on the red luminosity function evolution derived from the DEEPII and COMBO-17 surveys (Bell et al 2004; Faber et al. 2005), 0.034 M_sun yr^-1 Mpc^-3. We find that the blue sequence mass has remained roughly constant since z=1 (mass flux 0.01 M_sun yr^-1 Mpc^-3) but the average on-going star formation of 0.037$ M_sun yr^-1 Mpc^-3 over 0

D. Christopher Martin; Ted K. Wyder; David Schiminovich; Tom A. Barlow; Karl Forster; Peter G. Friedman; Patrick Morrissey; Susan G. Neff; Mark Seibert; Todd Small; Barry Y. Welsh; Luciana Bianchi; Jose Donas; Timothy M. Heckman; Young-Wook Lee; Barry F. Madore; Bruno Milliard; R. Michael Rich; Alex S. Szalay; Sukyoung K. Yi

2007-03-12T23:59:59.000Z

226

Analysis of records of embryo production in Red Brahman cows  

E-Print Network [OSTI]

Records of embryo production in Red Brahman donor cows (n=50) and F1 recipients (n=531) were evaluated from the collection day to the birth of the embryo produced. The effects of the sire of the donor and the embryo, protocol, season...

Riano Rocha, Edgar Hernando

2005-11-01T23:59:59.000Z

227

The Hermeneutics and Genesis of the Red Cow Ritual  

E-Print Network [OSTI]

HTR 105:3 (2012) 35171 The Hermeneutics and Genesis of the Red Cow Ritual* Nathan MacDonald University of Gttingen / University of St. Andrews Q#3;Introduction 7KH#3;GLIFXOWLHV#3;ZLWK#3;WKH#3;UHG#3;FRZ#3;ULWXDO#3;KDYH#3;ORQJ#3;H[HUFLVHG#3;UHDGHUV...

MacDonald, Nathan

2012-07-11T23:59:59.000Z

228

HISTORY OF RED LAKES FISHERY, With Observations on  

E-Print Network [OSTI]

was presented of the artificial propagation of the walleye and whitefish from 1918 through 1938. NOTE Average catch per lift 20 The walleyes of Lower Red Lake 25 Length -frequency distributions 25 Rate bass 50 Artificial propagation 50 Walleye 51 Whitefish 57 Brook, brown, rainbow, and lake trout 60

229

Red Halos of Galaxies - Reservoirs of Baryonic Dark Matter?  

E-Print Network [OSTI]

Deep optical/near-IR surface photometry of galaxies outside the Local Group have revealed faint and very red halos around objects as diverse as disk galaxies and starbursting dwarf galaxies. The colours of these structures are too extreme to be reconciled with stellar populations similar to those seen in the stellar halos of the Milky Way or M31, and alternative explanations like dust reddening, high metallicities or nebular emission are also disfavoured. A stellar population obeying an extremely bottom-heavy initial mass function (IMF), is on the other hand consistent with all available data. Because of its high mass-to-light ratio, such a population would effectively behave as baryonic dark matter and could account for some of the baryons still missing in the low-redshift Universe. Here, we give an overview of current red halo detections, alternative explanations for the origin of the red colours and ongoing searches for red halos around types of galaxies for which this phenomenon has not yet been reported. A number of potential tests of the bottom-heavy IMF hypothesis are also discussed.

E. Zackrisson; N. Bergvall; C. Flynn; G. Ostlin; G. Micheva; B. Caldwell

2007-08-06T23:59:59.000Z

230

InsideBauer RED Labs: Start Me Up  

E-Print Network [OSTI]

: Lithuania 38 Bauer Recognized for Exemplary Internal Audit Program 41 RED Labs: Start Me Up 42 A Unique Adrenaline Rush 62 Cover: The Changing Landscape of Higher Education 64 A Whole New Venture 68 Energy Lecture Opens Doors 72 Bauer's Sales Excellence Institute Named Top University Sales Program 73 Our

Azevedo, Ricardo

231

Alcian Blue Alizarin Red Skeletal Staining October 2003  

E-Print Network [OSTI]

Alcian Blue ­ Alizarin Red Skeletal Staining October 2003 Eddy M. De Robertis 1. Dissect mice damage. 3. Replace 95% ethanol with Alcian blue staining solution for 1-3 days slowly rocking at room days. 4. Replace Alcian blue solution with 95% ethanol for 6 hours slowly rocking at room temperature

De Robertis, Eddy M.

232

INTEGRATED LIDAR & PHOTOGRAMMETRIC DOCUMENTATION OF THE RED GULCH DINOSAUR  

E-Print Network [OSTI]

101 INTEGRATED LIDAR & PHOTOGRAMMETRIC DOCUMENTATION OF THE RED GULCH DINOSAUR TRACKSITE (WYOMING Resource Technology Section, National Operations Center, Bu- reau of Land Management, Bldg. 50 Denver, CO of successful schemes is testament to the advances made in attitudes and approaches to fossil site management

Falkingham, Peter

233

A theoretical analysis of the systematic errors in the Red Clump distance to the LMC  

E-Print Network [OSTI]

We present a detailed analysis of the uncertainty on the theoretical population corrections to the LMC Red Clump (RC) absolute magnitude, by employing a population synthesis algorithm to simulate theoretically the photometric and spectroscopic properties of RC stars, under various assumptions about the LMC Star Formation Rate (SFR) and Age Metallicity Relationship (AMR). A comparison of the outcome of our simulations with observations of evolved low-intermediate mass stars in the LMC allows one to select the combinations of SFR and AMR that bracket the real LMC star formation history, and to estimate the systematic error on the associated RC population corrections. The most accurate estimate of the LMC distance modulus from the RC method (adopting the OGLE-II reddening maps for the LMC) is obtained from the K-band magnitude, and provides (m-M)_{0, LMC}=18.47 +/-0.01(random) +0.05/-0.06(systematic). Distances obtained from the I-band, or from the multicolour RC technique which determines at the same time reddening and distance, both agree (albeit with a slightly larger error bar) with this value.

Maurizio Salaris; Susan Percival; Leo Girardi

2003-07-17T23:59:59.000Z

234

FCS Guidance Note 33: Forest operations and red squirrels: November 2006 Forest operations and red squirrels in Scottish forests  

E-Print Network [OSTI]

protection were introduced by the Nature Conservation (Scotland) Act 2004. These are introduced in the FCS by the introduced grey squirrel. Scotland now holds at least 75% of the UK red squirrel population, ie about 120 squirrels have been protected against intentional acts of damage or disturbance since 1981 under the UK

235

E-Print Network 3.0 - acquired pure red Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

for Data-Centric Synchronization Summary: Acquire Bitmap (CAB register) 1 ld B ld Z stack " CAB CAB " 0 ... Owned Colors Array ld T Blue Red Green... ,B,C color red A,B...

236

E-Print Network 3.0 - amphiuma red blood Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

red blood Search Powered by Explorit Topic List Advanced Search Sample search results for: amphiuma red blood Page: << < 1 2 3 4 5 > >> 1 JOURNAL OF MORPHOLOGY 211:63-72 (1992)...

237

T-671: Red Hat system-config-firewall Lets Local Users Gain Root...  

Broader source: Energy.gov (indexed) [DOE]

1: Red Hat system-config-firewall Lets Local Users Gain Root Privileges T-671: Red Hat system-config-firewall Lets Local Users Gain Root Privileges July 19, 2011 - 2:42pm Addthis...

238

E-Print Network 3.0 - adsol-preserved red blood Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

adsol-preserved red blood Search Powered by Explorit Topic List Advanced Search Sample search results for: adsol-preserved red blood Page: << < 1 2 3 4 5 > >> 1 Always Needed The...

239

U-230: Sudo on Red Hat Enterprise Linux %postun Symlink Flaw...  

Broader source: Energy.gov (indexed) [DOE]

0: Sudo on Red Hat Enterprise Linux %postun Symlink Flaw Lets Local Users Gain Elevated Privileges U-230: Sudo on Red Hat Enterprise Linux %postun Symlink Flaw Lets Local Users...

240

At science, he's a natural; Retiring J-Lab leader discusses red...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

hes-natural-retiring-j-lab-leader-discusses-red-tape-and-pursuit-knowledge-in... At science, he's a natural Retiring J-Lab leader discusses red tape and the pursuit of knowledge By...

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


241

E-Print Network 3.0 - auroral red arc Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

red arc Search Powered by Explorit Topic List Advanced Search Sample search results for: auroral red arc Page: << < 1 2 3 4 5 > >> 1 Annales Geophysicae, 23, 15231531, 2005...

242

E-Print Network 3.0 - aqaba red sea Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

& COMPANY THE RED SEA, THE NILE VALLEY AND THE HOLY LAND ABOARD THE EXCLUSIVELY... Egypt, Jordan and Israel. Join us as we sail along the ancient trade routes of the Red Sea...

243

Evaluation of Critical Habitat for the California red-legged frog (Rana aurora draytonii)  

E-Print Network [OSTI]

With Comparisons to Rana Aurora and Rana Pretiosa. Copeia.M. Jennings. May 1996. Rana aurora- Red -legged Frog [WebRed- Legged Frog, Rana aurora, Tadpoles. Animal Behaviour

Allen, Michael F.; Tennant, Tracy

2000-01-01T23:59:59.000Z

244

Evaluation of various sulphur amino acid compounds in the diet of red drum, Sciaenops ocellatus  

E-Print Network [OSTI]

Refinement of diet formulations to enhance the efficiency of red drum production continues to be pursued. Based on previous studies, the sulfur amino acid (SAA) requirement of red drum for methionine plus cystine appears to be most limiting, which...

Goff, Jonathan B

2003-01-01T23:59:59.000Z

245

Adaptive Tuning of RED Using On-line Simulation Tao Ye, Shivkumar Kalyanaraman  

E-Print Network [OSTI]

on the proposed RED optimization scheme, a general automatic network management system, i.e., on-line simulation

Kalyanaraman, Shivkumar

246

Young red supergiants and the near infrared light appearance of disk galaxies  

E-Print Network [OSTI]

Disk galaxies often show prominent nonaxisymmetric features at near-infrared wavelengths. Such features may indicate variations in the surface density of stellar mass, contributions from young red supergiants in star forming regions, or substantial dust obscuration. To distinguish among these possibilities, we have searched for spatial variations in the 2.3 micron photometric CO index within the disks of three nearby galaxies (NGC 278, NGC 2649, & NGC 5713). This index measures the strength of the absorption bands of molecular CO in stellar atmospheres, and is strong in cool, low surface-gravity stars, reaching the largest values for red supergiants. We observe significant spatial CO index variations in two galaxies (NGC 278 & NGC 5713), indicating that the dominant stellar population in the near-infrared is not everywhere the same. Central CO index peaks are present in two galaxies; these could be due to either metallicity gradients or recent star formation activity. In addition, significant azimuthal CO index variations are seen in NGC 278. Because strong azimuthal metallicity gradients are physically implausible in disk galaxies, these features are most naturally explained by the presence of a young stellar population. The fraction of 2 micron light due to young stellar populations in star forming regions can be calculated from our data. Overall, young stellar populations can contribute ~3% of a (normal) galaxy's near infrared flux. Locally, this fraction may rise to ~33%. Thus, young stars do not dominate the total near infrared flux, but can be locally dominant in star forming regions, and can bias estimates of spiral arm amplitude or other nonaxisymmetric structures in galaxies' mass distributions.

James E. Rhoads

1997-10-17T23:59:59.000Z

247

Red Algae Lose Key Mitochondrial Genes in Response to Becoming Parasitic  

E-Print Network [OSTI]

Red Algae Lose Key Mitochondrial Genes in Response to Becoming Parasitic Lillian Hancock1 , Lynda independently evolved hundreds of times among the floridiophyte red algae. Much is known about the life history class of red algae, Plocamiocolax puvinata, has lost the atp8 gene entirely, indicating that this gene

Lane, Chris

248

SPECIAL ISSUE ORIGINAL ARTICLE Biophotonic techniques for the study of malaria-infected red blood  

E-Print Network [OSTI]

SPECIAL ISSUE ­ ORIGINAL ARTICLE Biophotonic techniques for the study of malaria-infected red blood for Medical and Biological Engineering 2010 Abstract Investigation of the homeostasis of red blood cells upon infection by Plasmodium falciparum poses complex experimental challenges. Changes in red cell shape, volume

Cicuta, Pietro

249

Evolution of Red Algal Plastid Genomes: Ancient Architectures, Introns, Horizontal Gene Transfer, and  

E-Print Network [OSTI]

Evolution of Red Algal Plastid Genomes: Ancient Architectures, Introns, Horizontal Gene Transfer, Station Biologique, Roscoff, France Abstract Red algae have the most gene-rich plastid genomes known across all available red algal plastid genomes we show they all share a highly compact and slowly

Martone, Patrick T.

250

Code-Red: a case study on the spread and victims of an Internet worm  

E-Print Network [OSTI]

Code-Red: a case study on the spread and victims of an Internet worm David Moore, Colleen Shannon infected with the Code- Red (CRv2) worm in less than 14 hours. The cost of this epidemic, including subsequent strains of Code-Red, is es- timated to be in excess of $2.6 billion. Despite the global damage

Somayaji, Anil

251

RED SQUIRRELS OF THE HIGHLANDS Scottish Squirrel Group Update March 2012  

E-Print Network [OSTI]

RED SQUIRRELS OF THE HIGHLANDS Scottish Squirrel Group Update March 2012 Strongholds Update the Highlands and their main task will be to be the main local red squirrel contact within their region. We had-ordination and website Website www.redsquirrelsofthehighlands.co.uk This site serves as a vital link to all red squirrel

252

AbstractThe red snapper (Lutjanus campechanus) is currently under rig  

E-Print Network [OSTI]

653 Abstract­The red snapper (Lutjanus campechanus) is currently under rig orous federal and state of annuli in otolith thin sections have been used to age many species of fish, including red snapper. However, the utility of this method for aging red snapper has been questioned by those who dispute both

253

Red-Tide Research Summarized to 1964 Including an Annotated Bibliography  

E-Print Network [OSTI]

535^ Red-Tide Research Summarized to 1964 Including an Annotated Bibliography By George A, Harold E. Crowther, Acting Director Red-Tide Research Summarized to 1964 Including an Annotated Historical 2 General conditions during red-tide outbreaks 3 Temperature 3 Salinity 3 Rainfall 4 Wind 4 Light

254

The flow of red blood cells through a narrow spleen-like slit Jonathan B. Freund  

E-Print Network [OSTI]

The flow of red blood cells through a narrow spleen-like slit Jonathan B. Freund Citation: Phys OF FLUIDS 25, 110807 (2013) The flow of red blood cells through a narrow spleen-like slit Jonathan B are perhaps the smallest blood passages in the body, and red blood cells must deform significantly to pass

Freund, Jonathan B.

255

Larval red snapper (Lutjanus cam-pechanus) spend approximately 26 days  

E-Print Network [OSTI]

366 Larval red snapper (Lutjanus cam- pechanus) spend approximately 26 days in the plankton, prior diet differences from shifts that are due to habitat. Previous red snapper diet studies have focused and Bryan, 1975). Camber (1955) described the diets of 15 "small red snapper" from Campeche Banks

256

Appendix 15 Red and Blue-Listed Vertebrate and Vascular Plant Species The  

E-Print Network [OSTI]

Appendix 15 Red and Blue-Listed Vertebrate and Vascular Plant Species The report that follows lists red- and blue-listed species occurring in the Cranbrook Forest District and in the Southern Rocky risk' as either vulnerable in BC (Blue-listed), or endangered or threatened (Red-listed). The species

257

The red porgy, Pagrus pagrus, occurs in the eastern Atlantic from the Brit-  

E-Print Network [OSTI]

723 The red porgy, Pagrus pagrus, occurs in the eastern Atlantic from the Brit- ish Isles south and Vergara, 1978). In the Gulf of Mexico (GOM), red porgy are usu- ally found near hard-bottom areas off that red porgies are most common over inshore live-bottom habitats and over shelf-edge, rocky-rub- ble

258

Red-emitting fluorescent Organic Light emitting Diodes with low sensitivity to self-quenching  

E-Print Network [OSTI]

Red-emitting fluorescent Organic Light emitting Diodes with low sensitivity to self-quenching S, France *E-mail : sebastien.forget@univ-paris13.fr Keywords: OLED, quenching, doping, red-emitting organic. We herein report on Organic Light-Emitting Diodes (OLEDs) based on a fluorescent amorphous red

Paris-Sud XI, Université de

259

Tuning RED for Web Traffic * Mikkel Christiansen, ** Kevin Jeffay, David Ott, F. Donelson Smith  

E-Print Network [OSTI]

139 Tuning RED for Web Traffic * Mikkel Christiansen, ** Kevin Jeffay, David Ott, F. Donelson Smith http://www.cs.unc.edu/Research/dirt Abstract We study the effects of RED on the performance of Web --- response time for HTTP request­response pairs. We empirically evaluate RED across a range of parameter

Jeffay, Kevin

260

23 Figure 3.1: Color transition from purple/maroon argillites into bright red  

E-Print Network [OSTI]

;#12;#12;#12;#12;#12;#12;#12;#12;23 Figure 3.1: Color transition from purple/maroon argillites into bright red argillites. This transition weathering, possibly sideritic layer in the lower part of the picture. The fine grained overlying red Island Section, lower maroon and purple part in red unit (level: 9 meter; Figure 3.3); south shore Gull

Kidd, William S. F.

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


261

Perth & Kinross Red Squirrel Group update for SSG National Lottery: Community Wildlife fund  

E-Print Network [OSTI]

Perth & Kinross Red Squirrel Group ­ update for SSG National Lottery: Community Wildlife fund PKRSG's Red squirrel conservation efforts were significantly boosted by receipt of a funding award from and 23rd ) and with the help of the Royal Mail some 36,470 `Reds on your doorstep' leaflets were

262

SEASONAL V A R IA TIONS IN STRUCTURE AND CIRCULATION IN THE RED SEA  

E-Print Network [OSTI]

SEASONAL V A R IA TIONS IN STRUCTURE AND CIRCULATION IN THE RED SEA A DISSERTATION SUBMITTE D and surface circulation in the Red Sea, occur r ing along the north-south axis of the Sea and extending fr om on in the northern Red Sea is frorn the nor th-northwest throughout the year' during the winter ( fr om October

Luther, Douglas S.

263

Annual variation in primary moult parameters in Cape Weavers, Southern Masked Weavers and Southern Red  

E-Print Network [OSTI]

and Southern Red Bishops in the Western Cape, South Africa #12;160 #12;161 Annual variation in primary moult parameters in Cape Weavers, Southern Masked Weavers and Southern Red Bishops in the Western Cape, South Africa Abstract Duration of primary moult was similar in Cape Weavers and Southern Red Bishops (96 days

de Villiers, Marienne

264

Evolutionary Ecology, 1987, 1, 59-94 Red Queens and ESS  

E-Print Network [OSTI]

Evolutionary Ecology, 1987, 1, 59-94 Red Queens and ESS: the coevolution of evolutionary rates coevolutionary rates of zero is that of evolutio- narily stable strategies (ESS). Red Queen assumes that the more of such a phenotypic trait value. Such traits are the key to the Red Queen prediction of progressive coevolution. ESS

Brown, Joel S.

265

Original article Normal and sickle red blood cell dynamics under venular flow  

E-Print Network [OSTI]

1 Original article Normal and sickle red blood cell dynamics under venular flow C. Allayousa , A these notions are found in sickle cell disease where sickle red blood cells become more rigid, leading. Thus, normal and sickle red blood cells are classified into different sub-groups, showing

Paris-Sud XI, Université de

266

Getting simultaneous red and near infrared bands from a single digital camera for plant monitoring applications  

E-Print Network [OSTI]

Getting simultaneous red and near infrared bands from a single digital camera for plant monitoring including red and near-infrared bands have proved their efficiency for vegetation-soil discrimination an original solution to obtain simultaneously the near-infrared and red bands from a standard RGB camera

Paris-Sud XI, Université de

267

Understanding Blue-to-Red Conversion in Monomeric Fluorescent Timers and Hydrolytic Degradation of Their  

E-Print Network [OSTI]

Understanding Blue-to-Red Conversion in Monomeric Fluorescent Timers and Hydrolytic Degradation-FT (chromophore Met66-Tyr67-Gly68) and its precursor with blocked blue-to- red conversion Blue102 (chromophore Leu data suggest that blue-to-red conversion, taking place in Fast-FT and in related FTs, is associated

Verkhusha, Vladislav V.

268

Alternate Explosions: Collapse and Accretion Events with Red Holes instead of Black Holes  

E-Print Network [OSTI]

A red hole is "just like a black hole" except it lacks an event horizon and a singularity. As a result, a red hole emits much more energy than a black hole during a collapse or accretion event. We consider how a red hole solution can solve the "energy crisis" and power extremely energetic gamma ray bursts and hypernovae.

James S. Graber

1999-08-10T23:59:59.000Z

269

Using species distribution models to inform IUCN Red List assessments  

E-Print Network [OSTI]

to these as SRLI species because the occurrence data for these came from the plant component of the Sampled Red List Index (SRLI), an indicator to measure the current rate of loss of biodiversity by tracking trends in the conservation status of 6 a randomly... the Mesoamerica biodiversity hotspot (Myers et al. 2000). Many species in this region are poorly represented in the worlds herbaria, so limited knowledge of their true distribution exists; nonetheless, conservation assessments are urgently needed...

Syfert, Mindy M.; Joppa, Lucas; Smith, Matthew J.; Coomes, David A.; Bachman, Steven P.; Brummitt, Neil A.

2014-07-26T23:59:59.000Z

270

Red River Hot Springs Geothermal Area | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to: navigation, search RAPIDColoradosourceRausWyoming: Energy Resources6072302°,Red River

271

Formation of Carbon Dwarfs  

E-Print Network [OSTI]

We consider the formation of dwarf carbon stars via accretion from a carbon AGB companion in light of the new 107 object sample of Downes et al. (2004). This sample is now large enough to allow good mass determination via comparison of a composite spectrum to theoretical atmospheric models. Carbon dwarfs of spectral type M are indeed main sequence M dwarfs with enhanced metallicity and carbon abundance. We also calculate the predicted abundance of both M and of F/G carbon dwarfs, and show that the latter should be falsifiable in the near future.

Charles L. Steinhardt; Dimitar D. Sasselov

2012-01-27T23:59:59.000Z

272

Level Diagram Format Choice  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmospheric Optical Depth7-1D: VegetationEquipment Surfaces and Interfaces Sample6, 2011 LawrenceE C HLester toRecalcitrantWhich format

273

Planning and Search Exam format  

E-Print Network [OSTI]

is the frame problem. Revision 5 #12;Exam topics: planning Classical planning. How the problem definitionPlanning and Search Revision Revision 1 #12;Outline Exam format Exam topics How to revise Revision 2 #12;Exam format 4 questions out of 6 same format as 2010-2011 and 2011-2012 exams (on G52PAS

Alechina, Natasha

274

WHAT DETERMINES THE SIZES OF RED EARLY-TYPE GALAXIES?  

SciTech Connect (OSTI)

The sizes of galaxies are known to be closely related with their masses, luminosities, redshifts, and morphologies. However, when we fix these quantities and morphology, we still find large dispersions in the galaxy size distribution. We investigate the origin of these dispersions for red early-type galaxies using two SDSS-based catalogs. We find that the sizes of faint galaxies (log (M{sub dyn}/M{sub Sun }) {approx}< 10.3 or {sup 0.1} M{sub r} {approx}> -19.5, where {sup 0.1} M{sub r} is the r-band absolute magnitude, k-corrected to z = 0.1) are affected more significantly by luminosity, while the sizes of bright galaxies (log (M{sub dyn}/M{sub Sun }) {approx}> 11.4 or {sup 0.1} M{sub r} {approx}< -21.4) are by dynamical mass. At fixed mass and luminosity, the sizes of low-mass galaxies (log (M{sub dyn}/M{sub Sun }) {approx} 10.45 and {sup 0.1} M{sub r} {approx} -19.8) are relatively less sensitive to their colors, color gradients, and axis ratios. On the other hand, the sizes of intermediate-mass (log (M{sub dyn}/M{sub Sun }) {approx} 10.85 and {sup 0.1} M{sub r} {approx} -20.4) and high-mass (log (M{sub dyn}/M{sub Sun }) {approx} 11.25 and {sup 0.1} M{sub r} {approx} -21.0) galaxies significantly depend on those parameters, in the sense that larger red early-type galaxies have bluer colors, more negative color gradients (bluer outskirts), and smaller axis ratios. These results indicate that the sizes of intermediate- and high-mass red early-type galaxies are significantly affected by their recent minor mergers or rotations, whereas the sizes of low-mass red early-type galaxies are affected by some other mechanisms. Major dry mergers also seem to have influenced on the size growth of high-mass red early-type galaxies.

Lee, Joon Hyeop; Kim, Minjin; Ree, Chang Hee; Kim, Sang Chul; Lee, Jong Chul; Lee, Hye-Ran; Jeong, Hyunjin; Seon, Kwang-Il; Kyeong, Jaemann [Korea Astronomy and Space Science Institute, Daejeon 305-348 (Korea, Republic of); Oh, Kyuseok, E-mail: jhl@kasi.re.kr [Department of Astronomy, Yonsei University, Seoul 120-749 (Korea, Republic of)

2013-01-01T23:59:59.000Z

275

Method using CO for extending the useful shelf-life of refrigerated red blood cells  

DOE Patents [OSTI]

A method is disclosed using CO for extending the useful shelf-life of refrigerated red blood cells. Carbon monoxide is utilized for stabilizing hemoglobin in red blood cells to be stored at low temperature. Changes observed in the stored cells are similar to those found in normal red cell aging in the body, the extent thereof being directly related to the duration of refrigerated storage. Changes in cell buoyant density, vesiculation, and the tendency of stored cells to bind autologous IgG antibody directed against polymerized band 3 IgG, all of which are related to red blood cell senescence and increase with refrigerated storage time, have been substantially slowed when red blood cells are treated with CO. Removal of the carbon monoxide from the red blood cells is readily and efficiently accomplished by photolysis in the presence of oxygen so that the stored red blood cells may be safely transfused into a recipient. 5 figs.

Bitensky, M.W.

1995-12-19T23:59:59.000Z

276

Method using CO for extending the useful shelf-life of refrigerated red blood cells  

DOE Patents [OSTI]

Method using CO for extending the useful shelf-life of refrigerated red blood cells. Carbon monoxide is utilized for stabilizing hemoglobin in red blood cells to be stored at low temperature. Changes observed in the stored cells are similar to those found in normal red cell aging in the body, the extent thereof being directly related to the duration of refrigerated storage. Changes in cell buoyant density, vesiculation, and the tendency of stored cells to bind autologous IgG antibody directed against polymerized band 3 IgG, all of which are related to red blood cell senescence and increase with refrigerated storage time, have been substantially slowed when red blood cells are treated with CO. Removal of the carbon monoxide from the red blood cells is readily and efficiently accomplished by photolysis in the presence of oxygen so that the stored red blood cells may be safely transfused into a recipient.

Bitensky, Mark W. (Los Alamos, NM)

1995-01-01T23:59:59.000Z

277

A comparison between the responses of neutral red and acridine orange: Acridine orange should be preferential and alternative to neutral red as a dye  

E-Print Network [OSTI]

be preferential and alternative to neutral red as a dye for the monitoring of contaminants by means of biological (AO) and neutral red (NR) dyes, commonly used as probes to measure the internal pH in acidic vesicles, are compared in this article. The comparison between the two dyes (arising from cal- culations taking

Canberra, University of

278

Abstract Red is a common colour signal in both aposematic warning displays, and in fruit displays. One common feature is that red is conspicuous against the natural  

E-Print Network [OSTI]

Abstract Red is a common colour signal in both aposematic warning displays, and in fruit displays. One common feature is that red is conspicuous against the natural background of the prey and fruits. However, there is a potential conflict between fruits and aposematic prey in how a bird predator should

Tullberg, Birgitta

279

Formation, characterization and reactivity of adsorbed oxygen...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Formation, characterization and reactivity of adsorbed oxygen on BaOPt(111). Formation, characterization and reactivity of adsorbed oxygen on BaOPt(111). Abstract: The formation...

280

Inhibition of Photosynthesis in Some Algae by Extreme-Red Light Author(s): Eugene Rabinowitch, Govindjee, Jan B. Thomas  

E-Print Network [OSTI]

Inhibition of Photosynthesis in Some Algae by Extreme-Red Light Author(s): Eugene Rabinowitch://www.jstor.org #12;Inhibition of Photosynthesis in Some Algae by Extreme"Red Light Abstract. Photosynthesis produced by far-red light (about 700 m,b) is reversibly inhibited in some algae by extreme-red light ( 750 m

Govindjee

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


281

FM13 Glastir woodland creation appeals form 3 December, 2010 Glastir Woodland Creation Appeals Process-Red Areas  

E-Print Network [OSTI]

Process-Red Areas Glastir Woodland Creation Appeals Process ­ Red Areas This should only be used where you: What is the reason/s for the RED designation? Why do you think that the area has been incorrectly the boundary of the area that you wish to plant in the red areas in question Project Officer

282

(Non) formation of methanol by direct hydrogenation of formate...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

produces significant quantities of methanol, although decomposition of formate to carbon dioxide and hydrogen remains the dominant reaction pathway. Simultaneous production...

283

On the cosmic ray spectrum from type II Supernovae expanding in their red giant presupernova wind  

E-Print Network [OSTI]

While from the energetic point of view SNRs are viable sources of Galactic CRs, the issue of whether they can accelerate protons up to PeV remains unsolved. Here we discuss particle acceleration at the forward shock of SN and discuss the possibility that the escaping particle current may excite a non-resonant instability that in turn leads to the formation of resonant modes confining particles close to the shock and increasing the maximum energy. This mechanism works throughout the expansion of the SN explosion, from the ejecta dominated (ED) to the Sedov-Taylor (ST) phase. Because of their higher explosion rate,we focus on type II SNae expanding in the slow, dense red supergiant wind. When the explosion occurs in such winds, the transition between the ED and the ST phase is likely to take place within a few tens of years. As a result, the spectrum of accelerated particles shows a break in the slope, at the maximum energy (Em) achieved at the beginning of the ST phase. Above this energy, the spectrum becomes ...

Cardillo, Martina; Blasi, Pasquale

2015-01-01T23:59:59.000Z

284

Tungsten-incorporation induced red-shift in the bandgap of gallium oxide thin films  

SciTech Connect (OSTI)

Tungsten (W) incorporated Ga{sub 2}O{sub 3} films were produced by co-sputter deposition. W-concentration was varied by the applied sputtering-power. The structure and optical properties of W-incorporated Ga{sub 2}O{sub 3} films were evaluated using X-ray diffraction, scanning electron microscopy, and spectrophotometric measurements. No secondary phase formation was observed in W-incorporated Ga{sub 2}O{sub 3} films. W-induced effects were significant on the structure and optical properties of Ga{sub 2}O{sub 3} films. The bandgap of Ga{sub 2}O{sub 3} films without W-incorporation was {approx}5 eV. Red-shift in the bandgap was noted with increasing W-concentration indicating the electronic structure changes in W-Ga{sub 2}O{sub 3} films. A functional relationship between W-concentration and optical property is discussed.

Rubio, E. J.; Ramana, C. V. [Department of Mechanical Engineering, University of Texas at El Paso, El Paso, Texas 79968 (United States)] [Department of Mechanical Engineering, University of Texas at El Paso, El Paso, Texas 79968 (United States)

2013-05-13T23:59:59.000Z

285

Fe and Al Abundances for 180 Red Giants in the Globular Cluster Omega Centauri (NGC 5139)  

E-Print Network [OSTI]

We present radial velocities, Fe, and Al abundances for 180 red giant branch (RGB) stars in the Galactic globular cluster Omega Centauri ($\\omega$ Cen). The majority of our data lie in the range 11.0$Al/Fe] ratios exhibit large star--to--star scatter for all populations, with the more than 1.0 dex range of [Al/Fe] decreasing for stars more metal--rich than [Fe/H]$\\sim$--1.4. The minimum [Al/Fe] abundance observed for all metallicity populations is [Al/Fe]$\\sim$+0.15. The maximum abundance of log $\\epsilon$(Al) is reached for stars with [Fe/H]$\\sim$--1.4 and does not increase further with stellar metallicity. We interpret these results as evidence for type II SNe providing the minimum [Al/Fe] ratio and a mass spectrum of intermediate mass asymptotic giant branch stars causing the majority of the [Al/Fe] scatter. These results seem to fit in the adopted scheme that star formation occurred in $\\omega$ Cen over $>$1 Gyr.

Christian I. Johnson; Catherine A. Pilachowski; Jennifer Simmerer; Dustin Schwenk

2008-04-16T23:59:59.000Z

286

Population Effects on the Metallicity Distribution Function Derived From the Red Giant Branch  

E-Print Network [OSTI]

We have tested the reliability of the red giant branch (RGB) as a metallicity indicator accounting for observational errors as well as the complexity of star formation histories (SFHs) and chemical evolution histories observed in various stellar systems. We generate model color-magnitude diagrams (CMDs) produced with a variety of evolutionary histories and compare the resultant metallicity estimates from the colors and magnitudes of RGB stars to the true input metallicities. We include realistic models for photometric errors and completeness in our synthetic CMDs. As expected, for simple simple stellar populations dominated by old stars, the RGB provides a very accurate estimate of the modular metallicity value for a population. An error in the age of a system targeted for this type of study may produce metallicity errors of a few tenths of a dex. The size of this metallicity error depends linearly on the age error, and we find this dependence to be stronger with more precise photometry. If the population has...

Ordoez, Antonio J

2015-01-01T23:59:59.000Z

287

Overview of ''Red Oil'' Frequency Analyses for F-Canyon  

SciTech Connect (OSTI)

A very small potential exists in the Savannah River Site (SRS) separations operations for an uncontrolled reaction between tri-n-butyl phosphate (TBP) and nitric acid that could result in unacceptable damage to separations facilities and a significant release of radioactive materials. The recent ''red oil'' (TBP and nitric acid) accident in Tomsk, Russia, resulted in considerable damage and radioactive release. Explosions have also occurred at SRS during the early years of operations. While the SRS separations facilities have operated without incident for many years, it is prudent to revisit the SRS defense-in-depth approach to preventing such an accident and to upgrade preventive procedures and hardware as appropriate.

Lux, C.R.

2000-07-19T23:59:59.000Z

288

Earth fissures of the Red Light Bolson, Hudspeth County, Texas  

E-Print Network [OSTI]

in the laboratory techniques used during the soil analyses. Finally, I would like to thank the people of Sierra Blanca who went out of their way to make me feel welcome. A very special and heart-felt thanks goes to the family of R. Ramirez. The Ramirez household... in engineering design. Studies of the life history of individual or sets of fissures can lead to designing preemptive mitigation measures. Earth fissures are actively forming in the Red Light Bolson south of Sierra Blanca, Texas, the county seat of Hudspeth...

Sherrier, Michael Perry

1994-01-01T23:59:59.000Z

289

Red Lake Electric Coop, Inc | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating Solar PowerstoriesNrelPartnerType Jump to:Co JumpRETScreenJam Home NameRed Lake

290

Red River Valley Coop Pwr Assn | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating Solar PowerstoriesNrelPartnerType Jump to:Co JumpRETScreenJam Home NameRed LakeAssn

291

EA-1692: Red River Environmental Products, LLC Activated Carbon  

Office of Environmental Management (EM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "of EnergyEnergy CooperationRequirements Matrix U.S.7685 Vol. 76, No.5-FEB.Draft0:Manufacturing Facility, Red

292

EERE: VTO - Red Leaf PNG Image | Department of Energy  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE:YearRound-UpHeat Pump Models |Conduct,Final9:Department of EnergyQCJuly 2015 < prevRed Leaf

293

Sigurd Red Butte No2 | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to:Seadov Pty Ltd Jump to: navigation,Pvt LtdShrub Oak, New York:Siemens° LoadingSigurd Red

294

MHK Technologies/RED HAWK | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to:46 - 429Lacey,(MonasterLowell Point,ECO Auger < MHK Technologies JumpProteusRED HAWK

295

Red Cliffs Campground, Cedar City District, Utah | Department of Energy  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE:Year in3.pdfEnergyDepartmentEnergy DataRemediated | DepartmentRecruit MilitaryRed Cliffs

296

RedShift Systems Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to: navigation, search RAPIDColoradosourceRausWyoming: EnergyElec Assn Jump to:RedShift

297

Town of Red Springs, North Carolina (Utility Company) | Open Energy  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating SolarElectric Coop, IncTipmont RuralMiddletown Place:Information Red Springs Town

298

Red Cliffs Campground, Cedar City District, Utah | Department of Energy  

Office of Environmental Management (EM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "of EnergyEnergyENERGY TAXBalancedDepartment ofColumbusReport # INL/EXT-06-11478RailcarsJune 7,AboutRed

299

American Red Cross Blood Drive Hanford Health and Safety Exposition  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsruc DocumentationP-Series to someone by E-mail ShareRed Cross Blood Drive Hanford Health and Safety

300

The Occurrence of the Moody's Branch Formation at Four Surface Localities Between the Red River and the Brazos River  

E-Print Network [OSTI]

'idee D- . h - ~h. h Discorbis globule-~s inosa D~d- + d 'll E~d* l *k S~i honina jacksonensis Cushman Cushman Cushman Cushman and App'in Cushman and Applin Family Cassidulanidae Cassidulinoades hower Cushman Family Globe. ge"znadae Glob~i sp...

Pitzer, Carroll Dale

1960-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


301

A Generalized {ital K} Correction for Type Ia Supernovae: Comparing {ital R}-band Photometry Beyond {ital z=9.2} with B,V, and {ital R}-band Nearby Photometry  

E-Print Network [OSTI]

spectroscopically peculiar supernovae, and to search for anyK Correction for Type Ia Supernovae: Comparing R-bandK Correction for Type Ia Supernovae: Comparing R-band

Goodbar, Ariel

2008-01-01T23:59:59.000Z

302

QUENCHING STAR FORMATION AT INTERMEDIATE REDSHIFTS: DOWNSIZING OF THE MASS FLUX DENSITY IN THE GREEN VALLEY  

SciTech Connect (OSTI)

The bimodality in galaxy properties has been observed at low and high redshifts, with a clear distinction between star-forming galaxies in the blue cloud and passively evolving objects in the red sequence; the absence of galaxies with intermediate properties indicates that the quenching of star formation and subsequent transition between populations must happen rapidly. In this paper, we present a study of over 100 transiting galaxies in the so-called green valley at intermediate redshifts (z {approx} 0.8). By using very deep spectroscopy with the DEIMOS instrument at the Keck telescope we are able to infer the star formation histories of these objects and measure the stellar mass flux density transiting from the blue cloud to the red sequence when the universe was half its current age. Our results indicate that the process happened more rapidly and for more massive galaxies in the past, suggesting a top-down scenario in which the massive end of the red sequence is forming first. This represents another aspect of downsizing, with the mass flux density moving toward smaller galaxies in recent times.

Goncalves, Thiago S.; Menendez-Delmestre, Karin [Observatorio do Valongo, Universidade Federal do Rio de Janeiro, Ladeira Pedro Antonio, 43, Saude 20080-090 Rio de Janeiro (Brazil); Martin, D. Christopher; Wyder, Ted K. [California Institute of Technology, MC 278-17, Pasadena, CA 91125 (United States); Koekemoer, Anton, E-mail: tsg@astro.ufrj.br [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States)

2012-11-01T23:59:59.000Z

303

FORMATION GESTION DU STRESS CONTEXTE, PUBLIC, FINALITE DE LA FORMATION  

E-Print Network [OSTI]

FORMATION GESTION DU STRESS CONTEXTE, PUBLIC, FINALITE DE LA FORMATION La vie moderne et le stress : mettre en place des stratgies de gestion , tudier quelques aspects essentiels de la et cas cliniques composs par les participants ou fournis par le formateur . - Jeux de rle en sous

Brest, Universit de

304

NLTE Strontium and Barium in metal poor red giant stars  

E-Print Network [OSTI]

We present atmospheric models of red giant stars of various metallicities, including extremely metal poor (XMP, [Fe/H]Strontium (Sr) and Barium (Ba), treated in Non-Local Thermodynamic Equilibrium (NLTE) with various degrees of realism. We conclude that 1) for all lines that are useful Sr and Ba abundance diagnostics the magnitude and sense of the computed NLTE effect on the predicted line strength is metallicity dependent, 2) the indirect NLTE effect of overlap between Ba and Sr transitions and transitions of other species that are also treated in NLTE non-negligibly enhances NLTE abundance corrections for some lines, 3) the indirect NLTE effect of NLTE opacity of other species on the equilibrium structure of the atmospheric model is not significant, 4) the computed NLTE line strengths differ negligibly if collisional b-b and b-f rates are an order of magnitude smaller or larger than those calculated with standard analytic formulae, and 5) the effect of NLTE upon the resonance line of Ba II at 4554.03 AA is independent of whether that line is treated with hyperfine splitting. As a result, the derivation of abundances of Ba and Sr for metal-poor red giant stars with LTE modeling that are in the literature should be treated with caution.

C. I. Short; P. H. Hauschildt

2006-01-10T23:59:59.000Z

305

Magnesium Isotope Ratios in omega Centauri Red Giants  

E-Print Network [OSTI]

We have used high resolution observations obtained at the AAT with UHRF (R ~ 100,000) and at Gemini-S with b-HROS (R ~ 150,000) to determine magnesium isotope ratios for seven omega Centauri red giants that cover a range in iron abundance from [Fe/H] = --1.78 to --0.78 dex, and for two red giants in M4 (NGC 6121). The omega Centauri stars sample both the "primordial" (i.e., O-rich, Na and Al-poor) and the "extreme" (O-depleted, Na and Al-rich) populations in the cluster. The primordial population stars in both omega Centauri and M4 show (25Mg, 26Mg)/24 Mg isotopic ratios that are consistent with those found for the primordial population in other globular clusters with similar [Fe/H] values. The isotopic ratios for the omega Centauri extreme stars are also consistent with those for extreme population stars in other clusters. The results for the extreme population stars studied indicate that the 26Mg/24Mg ratio is highest at intermediate metallicities ([Fe/H] < --1.4 dex), and for the highest [Al/Fe] values....

Da Costa, G S; Yong, David

2013-01-01T23:59:59.000Z

306

Compositional changes in red and violet smoke mixes after combustion  

SciTech Connect (OSTI)

Anthraquinone-derived dyes are commonly used in colored dye mixes prepared for signal smoke grenades. Biological studies have shown, however, that a number of these dyes exhibit bacterial mutagenicity. In addition, these dyes are similar in structure to several polycyclic aromatic hydrocarbons which are well-known carcinogens. The grenades contain not only anthraquinone-derived dyes, but also a pyrotechnic fuel and cooling and starting mixes consisting primarily of potassium chlorate and nitrate, sodium bicarbonate, and sulfur. These dyes are volatilized at temperatures up to 550/sup 0/C during the detonation of the grenade, which could subject the dyes to oxidative and pyrolytic reactions that could result in a variety of reaction by-products. As part of a program to investigate possible environmental and occupational risks of the colored smoke dyes and in signal grenades, two colored smoke mixes, red and violet, have been studied both before and after detonation to evaluate any differences in composition due to the combustion process. This report focuses primarily on the separation and identification of the components of the original and combusted red and violet smoke mixes. The conditions for the detonation of the smoke grenades and sampling of the combusted smoke mixes are also discussed.

Buchanan, M.V.; Rubin, I.B.; Moneyhun, J.H.

1983-01-01T23:59:59.000Z

307

E-Print Network 3.0 - amphiuma tridactylum red Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

bones). My request is still tangled in red tape. Fortunately, we now Source: Staton, Joe - Belle W. Baruch Institute for Marine Biology and Coastal Research, University of...

308

E-Print Network 3.0 - argentinean red wine Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

of all German wines were red wines in 2006, according to the German Wine Institute. In Germany... of sugar because German consumers have ... Source: California at Davis, University...

309

E-Print Network 3.0 - australian red meat Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Collection: Renewable Energy ; Geosciences 24 China's Agriculture, Smallholders and Trade: Driven by the Livestock Revolution? Summary: , poultry and red meats (milk was not...

310

Energy Department Invests $12 Million to Slash Red Tape and Speed...  

Energy Savers [EERE]

generation once again by 2020, the Energy Department today announced eight teams to spur solar power deployment by cutting red tape for residential and small commercial rooftop...

311

Star Formation and Galaxy Environment  

E-Print Network [OSTI]

The dependence of star formation rate on galaxian environment is a key issue in the understanding of galaxy formation and evolution. However, the study of this subject is complex and observationally challenging. This paper reviews some of the current results, drawing mostly from recent large redshift surveys such the LCRS, the MORPH collaboration, and the CNOC1 and CNOC2 redshift surveys.

H. K. C. Yee

2000-04-05T23:59:59.000Z

312

Exploring the associations of maternal red blood cell fatty acids, infant body composition, and quality of infant growth  

E-Print Network [OSTI]

(21:0) and infant FM (r = 0.23, p = 0.049). Vaccenic acid (18:1n-7t) showed an association that approached significance (presented in italics in Table 3). Table 3. Correlation Matrix of Significant Fatty Acids for Visit 1 Fatty Acid (%) Percentage... expression (12). Research currently has studied associations between essential fatty acids such as the omega-3 (n-3) fatty acids docosahexaenoic acid (DHA) and eicosapentaenoic acid (EPA), and omega-6 (n-6) fatty acid arachidonic acid (AA) in maternal...

Newbold, Emily A.

2014-05-31T23:59:59.000Z

313

The Star Formation Histories of Four Fields Spanning the Minor Axis of NGC 6822  

E-Print Network [OSTI]

The star formation histories of four fields within the Local Group dwarf irregular galaxy NGC 6822 are presented. Each of the fields was imaged by the WFPC2 aboard the {\\it Hubble Space Telescope} and were used to obtain $VI$ color-magnitude diagrams for each field reaching $V\\simeq26$. The magnitude of the tip of the red giant branch and the red clump were used to determine distances to NGC 6822 that are consistent with previous ground-based measurements. The distance, extinction and star formation history were also determined by fitting the entire color-magnitude diagram in each field. The distances from these fits are consistent with the other determinations within the estimated errors once the systematic effects of uncertainties in the age-metallicity relation are taken into account. The extinction varies among the four fields from approximately the foreground Galactic value to $\\approx 0.4$ mag higher in $V$ and roughly correlates with the $60\\micron$ surface brightness. The star formation histories in the four fields are similar for ages $\\gtrsim 1$ Gyr and are relatively constant or somewhat increasing with time. These old star formation rates are comparable to that expected from the typical gas surface densities at these galactocentric radii and suggest that no large scale redistribution of gas or stars is required to account for the inferred star formation rates. Three of the fields show a drop of a factor of $\\sim 2-4$ in the star formation rate about 600 Myr ago while the remaining field centered on the bar shows an increase.

Ted K. Wyder

2003-03-10T23:59:59.000Z

314

Infra-red divergences in the large-N expansion  

E-Print Network [OSTI]

We investigate a vectorial O(N) model with a generic nearest-neighbor interaction W(\\bsigma_i\\cdot \\bsigma_j) (depending on {\\cal N} tunable parameters), a Yukawa (and Gross Neveu) model with N_f fermions at finite temperature and the vectorial \\phi^6 model, in the large N (N_f) limit. All this models exhibit a Mean Field critical point for N=\\infinity. When 1/N fluctuations are included, infra red divergences appear near the critical point. In the framework of a generalized 1/N expansion we show that these divergences are related to a universal crossover mechanism between the Mean Field universality class (N=\\infinity) and the nonclassical one for N<\\infinity. For the generic nearest-neighbor interaction multicritical points are also investigated.

Bortolo Matteo Mognetti

2007-03-20T23:59:59.000Z

315

MAGNESIUM ISOTOPE RATIOS IN {omega} CENTAURI RED GIANTS  

SciTech Connect (OSTI)

We have used the high-resolution observations obtained at the Anglo-Australian Telescope with Ultra-High Resolution Facility (R {approx} 100,000) and at Gemini-S with b-HROS (R {approx} 150,000) to determine magnesium isotope ratios for seven {omega} Cen red giants that cover a range in iron abundance from [Fe/H] = -1.78 to -0.78 dex, and for two red giants in M4 (NGC 6121). The {omega} Cen stars sample both the ''primordial'' (i.e., O-rich, Na- and Al-poor) and the ''extreme'' (O-depleted, Na- and Al-rich) populations in the cluster. The primordial population stars in both {omega} Cen and M4 show ({sup 25}Mg, {sup 26}Mg)/{sup 24}Mg isotopic ratios that are consistent with those found for the primordial population in other globular clusters with similar [Fe/H] values. The isotopic ratios for the {omega} Cen extreme stars are also consistent with those for extreme population stars in other clusters. The results for the extreme population stars studied indicate that the {sup 26}Mg/{sup 24}Mg ratio is highest at intermediate metallicities ([Fe/H] < -1.4 dex), and for the highest [Al/Fe] values. Further, the relative abundance of {sup 26}Mg in the extreme population stars is notably higher than that of {sup 25}Mg, in contrast to model predictions. The {sup 25}Mg/{sup 24}Mg isotopic ratio in fact does not show any obvious dependence on either [Fe/H] or [Al/Fe] nor, intriguingly, any obvious difference between the primordial and extreme population stars.

Da Costa, G. S.; Norris, John E.; Yong, David [Research School of Astronomy and Astrophysics, Australian National University, Canberra, ACT 0200 (Australia)

2013-05-20T23:59:59.000Z

316

Kit for the selective labeling of red blood cells in whole blood with .sup.9 TC  

DOE Patents [OSTI]

Disclosed herein are a method and kit for the preparation of .sup.99m Tc labeled red blood cells using whole blood in a closed sterile system containing stannous tin in a form such that it will enter the red blood cells and be available therein for reduction of technetium.

Srivastava, Suresh C. (Setauket, NY); Babich, John W. (Redhill Surrey, GB2); Straub, Rita (Brookhaven, NY); Richards, Powell (New Bern, NC)

1992-01-01T23:59:59.000Z

317

Kit for the selective labeling of red blood cells in whole blood with [sup 99]Tc  

DOE Patents [OSTI]

Disclosed herein are a method and kit for the preparation of [sup 99m]Tc labeled red blood cells using whole blood in a closed sterile system containing stannous tin in a form such that it will enter the red blood cells and be available therein for reduction of technetium. No Drawings

Srivastava, S.C.; Babich, J.W.; Straub, R.; Richards, P.

1992-05-26T23:59:59.000Z

318

CHANGES IN QUANTUM YIELD OF PHOTOSYNTHESIS IN THE RED ALGA Porphyridium cruentum  

E-Print Network [OSTI]

CHANGES IN QUANTUM YIELD OF PHOTOSYNTHESIS IN THE RED ALGA Porphyridium cruentum CAUSED BY STEPWISE From the Photosynthesis Research Laboratory, Botany Department, University of Illinois, Urbana. Dr of photosynthesis in the red alga Porphyridium cruentum, and the spectral compo- sition of light, changed

Govindjee

319

Regulation of Thyrotropin mRNA Expression in Red Drum, Sciaenops ocellatus  

E-Print Network [OSTI]

, circulates with a robust daily rhythm in the sciaenid fish, red drum. Previous research has suggested that the red drum T? cycle is circadian in nature, driven by TSH secretion in the early photophase and inhibited by T? feedback in the early scotophase...

Jones, Richard Alan

2012-10-19T23:59:59.000Z

320

Bioluminescent and Red-Fluorescent Lures in a Deep-Sea Siphonophore  

E-Print Network [OSTI]

Bioluminescent and Red-Fluorescent Lures in a Deep-Sea Siphonophore Steven H. D. Haddock,1 * Casey stalk (Fig. 1, B and C). The transpar- ent stalk terminates in a bulb containing white spots, historical surrounded by red fluorescent material (Fig. 1C). This substance produced a multimodal fluorescence emis

Dunn, Casey

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


321

Sandwiches come with the following: Mayo or mustard, lettuce, tomatoes, red onions, pickles, pepperoncinis, salt & pepper.  

E-Print Network [OSTI]

and chile-lime tortilla strips, Romaine and Spring Mix, Buttermilk Ranch dressing. Chicken Caesar - Chicken Chicken All natural chicken with BBQ sauce, lettuce, tomatoes, red onions, Ranch dressing and chile & SWEETS SALADS & SALAD WRAPS FAVORITES BBQ Ranch Chicken - Chicken, BBQ sauce, red onions, tomatoes

de Lijser, Peter

322

On Bitcoin and Red Balloons Moshe Babaioff, Microsoft Research, Silicon Valley.  

E-Print Network [OSTI]

X On Bitcoin and Red Balloons Moshe Babaioff, Microsoft Research, Silicon Valley. moshe (finding red balloons). We focus on another prominent scenario: Bitcoin, a decentralized electronic currency system. Bitcoin represents a radical new approach to monetary systems. It has been getting a large

Fiat, Amos

323

INTRODUCTION Red wood ants play an important role in the ecology of  

E-Print Network [OSTI]

INTRODUCTION Red wood ants play an important role in the ecology of woodland ecosystems by virtue the ecological impor- tance of red wood ants (Gsswald, 1989) and the conser- vation concern for some species.borkin@clear.net.nz 2 Royal Society for the Protection of Birds, Etive House, Beechwood Park, Inverness, IV2 3BW, UK; e

Thomas, Len

324

NESTING WITH THE WASP ROPALIDIA CINCTA INCREASES NEST SUCCESS OF RED-CHEEKED CORDONBLEU  

E-Print Network [OSTI]

1022 NESTING WITH THE WASP ROPALIDIA CINCTA INCREASES NEST SUCCESS OF RED-CHEEKED CORDONBLEU costs or benefits to associated hymenopterans. We followed the nesting cycles of an estrildid finch, the Red-cheeked Cordonbleu (Uraeginthus bengalus), and a common nesting associate, the wasp Ropalidia

Beier, Paul

325

"Red Sore Disease"in Game Fish1 Peggy Reed and Ruth Francis-Floyd2  

E-Print Network [OSTI]

frequently affected are game fish, particularly bluegill (bream), largemouth bass, and striped bass and itsVM85 "Red Sore Disease"in Game Fish1 Peggy Reed and Ruth Francis-Floyd2 1. This document is VM85 fish is generically referred to as "red sore disease." This problem usually occurs in the spring

Watson, Craig A.

326

Some Constraints On the Effects of Age and Metallicity on the Low Mass X-ray Binary Formation Rate  

E-Print Network [OSTI]

We have studied the low mass X-ray binary (LMXB) populations within and outside globular clusters (GC) in NGC 4365 and NGC 3115. Using published age and metallicity constraints from optical and IR observations of their GCs, we do not find any evidence for an increase in the LMXB formation rate in the intermediate age cluster population of NGC 4365, as has been proposed in some scenarios of dynamical LMXB formation in GCs. The old, metal-rich, red population of GCs in NGC 3115 on the other hand is {\\it at least} three times as efficient at creating LMXBs as the old, metal-poor, blue clusters. These data suggest that the higher formation efficiency of LMXBs in the red GC subsystems of many galaxies is largely a consequence of their higher metallicity. A comparison of the densities of field LMXBs in different galaxies does not reveal an obvious correlation with the age of the field stars as predicted by models in which the LMXB formation rate in the field drops monotonically with time after an initial burst. This suggests that either a significant fraction of the field LMXBs are created in GCs and subsequently injected into the field, or the LMXB formation rate has a more complex time evolution pattern.

Arunav Kundu; Thomas J. Maccarone; Stephen E. Zepf; Thomas H. Puzia

2003-04-24T23:59:59.000Z

327

Treating tar sands formations with karsted zones  

DOE Patents [OSTI]

Methods for treating a tar sands formation are described herein. The tar sands formation may have one or more karsted zones. Methods may include providing heat from one or more heaters to one or more karsted zones of the tar sands formation to mobilize fluids in the formation. At least some of the mobilized fluids may be produced from the formation.

Vinegar, Harold J. (Bellaire, TX); Karanikas, John Michael (Houston, TX)

2010-03-09T23:59:59.000Z

328

Use-driven concept formation  

E-Print Network [OSTI]

When faced with a complex task, humans often identify domain-specific concepts that make the task more tractable. In this thesis, I investigate the formation of domain-specific concepts of this sort. I propose a set of ...

Roberts, Jennifer M. (Jennifer Marie)

2010-01-01T23:59:59.000Z

329

Absence of Red Structural Color in Photonic Glasses, Bird Feathers and Certain Beetles  

E-Print Network [OSTI]

Colloidal glasses, bird feathers, and beetle scales can all show structural colors arising from short-ranged spatial correlations between scattering centers. Unlike the structural colors arising from Bragg diffraction in ordered materials like opals, the colors of these photonic glasses are independent of orientation, owing to their disordered, isotropic microstructures. However, there are few examples of photonic glasses with angle-independent red colors in nature, and colloidal glasses with particle sizes chosen to yield structural colors in the red show weak color saturation. Using scattering theory, we show that the absence of angle-independent red color can be explained by the tendency of individual particles to backscatter light more strongly in the blue. We discuss how the backscattering resonances of individual particles arise from cavity-like modes, and how they interact with the structural resonances to prevent red. Finally, we use the model to develop design rules for colloidal glasses with red, angle-independent structural colors.

Sofia Magkiriadou; Jin-Gyu Park; Young-Seok Kim; Vinothan N. Manoharan

2014-11-14T23:59:59.000Z

330

Policy Experimentation and the Search for Institutional Change: The Politics of Red-Green Reform in Germany  

E-Print Network [OSTI]

the first four years of Germany first Red-Green coalition.OF RED-GREEN REFORM IN GERMANY June 2006 J. Nicholas Zieglercoalition government in Germany between Social Democrats and

Ziegler, J. Nicholas; Leslie, John C.

2006-01-01T23:59:59.000Z

331

An early Miocene age for a high-temperature event in gneisses from Zabargad Island (Red Sea, Egypt): mantle diapirism?  

E-Print Network [OSTI]

An early Miocene age for a high-temperature event in gneisses from Zabargad Island (Red Sea, Egypt outcropping on Zabargad Island (Red Sea, Egypt). This island, though of limited size (& 4 km2 ), has an almost

Demouchy, Sylvie

332

Post-fire recovery and successional dynamics of an old growth red spruce forest in the southern Appalachian Mountains  

E-Print Network [OSTI]

of fire in a mesic ecosystem, specifically a high-elevation red spruce (Picea rubens Sarg.) forest on Whitetop Mountain in the southern Appalachian Mountains. Six plots were established in a high elevation red spruce stand to characterize the stand...

Krustchinsky, Adam R.

2009-05-15T23:59:59.000Z

333

Red grouper is an economically important species of the southeast United States and in particular the Gulf of Mexico. Red grouper are highly territorial and often remain at the same site for long periods of  

E-Print Network [OSTI]

Red grouper is an economically important species of the southeast United States and in particular the Gulf of Mexico. Red grouper are highly territorial and often remain at the same site for long periods of time. We now know Red grouper are also engineering marvels for their ability to modify habitat through

Watson, Craig A.

334

ARM: Shortwave Array Spectroradiometer-Hemispheric, Near-InfraRed channel, low-sun angles [a0 data is uncalibrated  

DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

Shortwave Array Spectroradiometer-Hemispheric, Near-InfraRed channel, low-sun angles [a0 data is uncalibrated

Flynn, Connor

335

ARM: Shortwave Array Spectroradiometer-Hemispheric, Near-InfraRed channel, high-sun angles [a0 data is uncalibrated  

DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

Shortwave Array Spectroradiometer-Hemispheric, Near-InfraRed channel, high-sun angles [a0 data is uncalibrated

Flynn, Connor

336

ARM: Shortwave Array Spectroradiometer-Hemispheric, Near-InfraRed channel, low-sun angles [a0 data is uncalibrated  

SciTech Connect (OSTI)

Shortwave Array Spectroradiometer-Hemispheric, Near-InfraRed channel, low-sun angles [a0 data is uncalibrated

Flynn, Connor

2011-03-22T23:59:59.000Z

337

ARM: Shortwave Array Spectroradiometer-Hemispheric, Near-InfraRed channel, high-sun angles [a0 data is uncalibrated  

SciTech Connect (OSTI)

Shortwave Array Spectroradiometer-Hemispheric, Near-InfraRed channel, high-sun angles [a0 data is uncalibrated

Flynn, Connor

2011-03-22T23:59:59.000Z

338

JURO Application Editing Sample Please edit the following passage for style and content. Make edits in red or blue ink.  

E-Print Network [OSTI]

in red or blue ink. American citizens eat unhealthily all the time. America increasing rely on foreign

Arnold, Jonathan

339

Ice Formation in Gas-Diffusion Layers  

E-Print Network [OSTI]

the University of California. Ice Formation in Gas-Diffusionsub-freezing conditions, ice forms in the gas-diffusionstrategies exist to prevent ice formation, there is little

Dursch, Thomas

2013-01-01T23:59:59.000Z

340

AOAC Meeting and Exposition, Orlando, FL HPLC-PDA-Fluorescence-MS Analysis of Flavonoids in Red and White Cranberry  

E-Print Network [OSTI]

in Red and White Cranberry Introduction Cranberries (Vaccinium macrocarpon) exist in red and white stages of maturity. While consumption of red cranberries is much higher than white stage cranberries it is useful to know how they compare in regard to relative composition and biological effect. Cranberries contain high

Heller, Barbara

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


341

UBC Social Ecological Economic Development Studies (SEEDS) Student Report An Investigation into the Red Listed Material: Pressure Treated Wood  

E-Print Network [OSTI]

into the Red Listed Material: Pressure Treated Wood (Preservative Infused) and Possible Alternatives Abby Yuen of a project/report". #12;APSC 261 An Investigation into the Red Listed Material: Pressure Treated Wood. Pressure treated wood, a commonly used building material in British Columbia, is a red-listed material

342

Types of red cell potassium in seven Spanish native breeds Paquita GONZALEZ Maria Jess TUON M. VALLEJO  

E-Print Network [OSTI]

Note Types of red cell potassium in seven Spanish native breeds of cattle Paquita GONZALEZ Maria Madrid, Spain Summary The distribution of red-cell potassium was studied in seven Spanish native breeds-equiv/1. For HK animals the means ranged from 50.8 to 66.1 m-equiv/1. Key word : red cell potassium

Paris-Sud XI, Université de

343

Red blood cell dynamics: from spontaneous fluctuations to non-linear response Young Zoon Yoon,ab  

E-Print Network [OSTI]

Red blood cell dynamics: from spontaneous fluctuations to non-linear response Young Zoon Yoon DOI: 10.1039/c0sm01117g We studied experimentally the mechanical properties of the red blood cell and microtubules: generally they confer rigidity to cells, and to tissues at larger scales.3,4 The red blood cell

Cicuta, Pietro

344

Red1p, a MEK1-dependent Phosphoprotein That Physically Interacts with Hop1p during Meiosis in Yeast*  

E-Print Network [OSTI]

Red1p, a MEK1-dependent Phosphoprotein That Physically Interacts with Hop1p during Meiosis in Yeast two meiosis-spe- cific components of AEs in S. cerevisiae, HOP1 and RED1, is critical for proper that Red1p is a MEK1-dependent phosphopro- tein. Co-immunoprecipitation experiments demon- strated

Hollingsworth, Nancy Marie

345

MITAC Red Sox Ticket Lottery 2012: Rules & Instructions ONLINE TICKET PAYMENT! Those selected to purchase tickets will be  

E-Print Network [OSTI]

MITAC Red Sox Ticket Lottery 2012: Rules & Instructions ONLINE TICKET PAYMENT! Those selected contact us at 617-253-7990 or mitac-office@mit.edu. HOW TO ENTER THE RED SOX LOTTERY · ELIGIBILITY: Web certificates will be required to enter the lottery. Entry in the Red Sox Lottery gives MIT employees, students

Seager, Sara

346

Is the Extended Red Emission due to CO? Philip D. Bennett, Graham M. Harper, and Alexander Brown  

E-Print Network [OSTI]

Is the Extended Red Emission due to CO? Philip D. Bennett, Graham M. Harper, and Alexander Brown. The Extended Red Emission (ERE) is a broad emission feature ob­ served between 5000 and 8000 š A in a large to be correct. The strongest known source of the ERE is the bipolar nebula (the ``Red Rect­ angle'') associated

Harper, Graham

347

A Red-Shifted, Fast-Relaxing Azobenzene Photoswitch for Visible Light Control of an Ionotropic Glutamate Receptor  

E-Print Network [OSTI]

A Red-Shifted, Fast-Relaxing Azobenzene Photoswitch for Visible Light Control of an Ionotropic cores with a red-shifted cis-to-trans isomerization have been previously described, they have not yet ligand (PTL) approach. We report the synthesis and characterization of a red-shifted PTL, L-MAG0460

Trauner, Dirk

348

Red tide detection and tracing using MODIS fluorescence data: A regional example in SW Florida coastal waters  

E-Print Network [OSTI]

Red tide detection and tracing using MODIS fluorescence data: A regional example in SW Florida-time data from the MODIS satellite sensor was used to detect and trace a harmful algal bloom (HAB), or red to interferences of other water constituents. The red tide that formed from November to December 2004 off SW

349

Using Event Based Data to Assess Vehicle Pedestrian Crash Risk in the Absence of All-Red  

E-Print Network [OSTI]

Using Event Based Data to Assess Vehicle Pedestrian Crash Risk in the Absence of All-Red Phase decision making at a signalized intersection? ? How effective is the signal timing (particularly "All-Red lane.) #12;4 4 ?Data analyzed between 10:30 am to 5 pm. ?Typical Yellow duration = 3 secs, All-Red

Minnesota, University of

350

Red Squirrels in South Scotland Project Update 96 landowners have been successfully recruited onto SRDP and are receiving funding  

E-Print Network [OSTI]

Red Squirrels in South Scotland Project Update 96 landowners have been successfully recruited squirrels have moved. In December 2011 a new red squirrel pox outbreak occurred along the River Tweed at Paxton House in Berwickshire. To date 2 poxed red squirrels have been found (1 confirmed case

351

Red Squirrels in South Scotland Project Update 34 new SRDP applications have been written and submitted. If all applications are  

E-Print Network [OSTI]

Red Squirrels in South Scotland Project Update 34 new SRDP applications have been written. In response to this worrying influx of grey squirrels, Red Squirrels in Northern England (RSNE resurfaced with the confirmation of 4 poxed red squirrels found between April 2011 to present. Grey

352

Red Quasars in the Las Campanas Infrared Survey Frank Masci, Carol Lonsdale, Perry Hacking, the LCIR collaboraton...  

E-Print Network [OSTI]

Red Quasars in the Las Campanas Infrared Survey Frank Masci, Carol Lonsdale, Perry Hacking, the LCIR collaboraton... Summary We propose to search for red quasars in the Las Campanas Infrared (LCIR/near-IR appearence prior to spectroscopic follow- up. Our method will preferentially select red quasars at z>2

Masci, Frank

353

The red rain phenomenon of Kerala and its possible extraterrestrial origin  

E-Print Network [OSTI]

A red rain phenomenon occurred in Kerala, India starting from 25th July 2001, in which the rainwater appeared coloured in various localized places that are spread over a few hundred kilometers in Kerala. Maximum cases were reported during the first 10 days and isolated cases were found to occur for about 2 months. The striking red colouration of the rainwater was found to be due to the suspension of microscopic red particles having the appearance of biological cells. These particles have no similarity with usual desert dust. An estimated minimum quantity of 50,000 kg of red particles has fallen from the sky through red rain. An analysis of this strange phenomenon further shows that the conventional atmospheric transport processes like dust storms etc. cannot explain this phenomenon. The electron microscopic study of the red particles shows fine cell structure indicating their biological cell like nature. EDAX analysis shows that the major elements present in these cell like particles are carbon and oxygen. Strangely, a test for DNA using Ethidium Bromide dye fluorescence technique indicates absence of DNA in these cells. In the context of a suspected link between a meteor airburst event and the red rain, the possibility for the extraterrestrial origin of these particles from cometary fragments is discussed.

Godfrey Louis; A. Santhosh Kumar

2006-01-02T23:59:59.000Z

354

The Photophysics of the Carrier of Extended Red Emission  

E-Print Network [OSTI]

Interstellar dust contains a component which reveals its presence by emitting a broad, unstructured band of light in the 540 to 950 nm wavelength range, referred to as Extended Red Emission (ERE). The presence of interstellar dust and ultraviolet photons are two necessary conditions for ERE to occur. This is the basis for suggestions which attribute ERE to an interstellar dust component capable of photoluminescence. In this study, we have collected all published ERE observations with absolute-calibrated spectra for interstellar environments, where the density of ultraviolet photons can be estimated reliably. In each case, we determined the band-integrated ERE intensity, the wavelength of peak emission in the ERE band, and the efficiency with which absorbed ultraviolet photons are contributing to the ERE. The data show that radiation is not only driving the ERE, as expected for a photoluminescence process, but is modifying the ERE carrier as manifested by a systematic increase in the ERE band's peak wavelength and a general decrease in the photon conversion efficiency with increasing densities of the prevailing exciting radiation. The overall spectral characteristics of the ERE and the observed high quantum efficiency of the ERE process are currently best matched by the recently proposed silicon nanoparticle (SNP) model. Using the experimentally established fact that ionization of semiconductor nanoparticles quenches their photoluminescence, we proceeded to test the SNP model by developing a quantitative model for the excitation and ionization equilibrium of SNPs under interstellar conditions for a wide range of radiation field densities.

Tracy L. Smith; Adolf N. Witt

2001-09-26T23:59:59.000Z

355

The pulsation modes, masses and evolution of luminous red giants  

E-Print Network [OSTI]

The period-luminosity sequences and the multiple periods of luminous red giant stars are examined using the OGLE III catalogue of long-period variables in the Large Magellanic Cloud. It is shown that the period ratios in individual multimode stars are systematically different from the ratios of the periods at a given luminosity of different period-luminosity sequences. This leads to the conclusion that the masses of stars at the same luminosity on the different period-luminosity sequences are different. An evolutionary scenario is used to show that the masses of stars on adjacent sequences differ by about 16-26% at a given luminosity, with the shorter period sequence being more massive. The mass is also shown to vary across each sequence by a similar percentage, with the mass increasing to shorter periods. On one sequence, sequence B, the mass distribution is shown to be bimodal. It is shown that the small amplitude variables on sequences A', A and B pulsate in radial and nonradial modes of angular degree l=0...

Wood, P R

2015-01-01T23:59:59.000Z

356

The Unidentified InfraRed Features after ISO  

E-Print Network [OSTI]

The Infrared Space Observatory (ISO) has provided the first complete mid-IR spectra for a wide range of objects. Almost all of these spectra are dominated by the well-known infrared emission features at 3.3, 6.2, 7.7, and 11.2 $\\mu$m, the so-called Unidentified Infra-Red (UIR) features. Besides the major features, there is an array of minor features and broad plateaux stretching from 3 to 20 $\\mu$m which reveal subtle details of conditions in the emission zones and properties of the carriers. Generally attributed to the vibrational relaxation of UV-pumped Polycyclic Aromatic Hydrocarbon molecules (PAHs) containing some 50--100 C-atoms, these UIR spectra are a treasure trove of information. The ISO spectra have, for the first time, allowed a systematic analysis of the spectral characteristics of the UIR features in a wide variety of environments. The peak positions, profiles, and relative strengths of the major features vary from source to source and spatially within sources. These specific profiles are not unique to certain object types but can occur within each individual source. Here, we review ISO and recent ground-based observations and assess some of their implications.

E. Peeters; L. J. Allamandola; D. M. Hudgins; S. Hony; A. G. G. M. Tielens

2003-12-06T23:59:59.000Z

357

YELLOW AND RED SUPERGIANTS IN THE LARGE MAGELLANIC CLOUD  

SciTech Connect (OSTI)

Due to their transitionary nature, yellow supergiants (YSGs) provide a critical challenge for evolutionary modeling. Previous studies within M31 and the Small Magellanic Cloud show that the Geneva evolutionary models do a poor job at predicting the lifetimes of these short-lived stars. Here, we extend this study to the Large Magellanic Cloud (LMC) while also investigating the galaxy's red supergiant (RSG) content. This task is complicated by contamination by Galactic foreground stars that color and magnitude criteria alone cannot weed out. Therefore, we use proper-motions and the LMC's large systemic radial velocity ({approx}278 km s{sup -1}) to separate out these foreground dwarfs. After observing nearly 2000 stars, we identified 317 probable YSGs, 6 possible YSGs, and 505 probable RSGs. Foreground contamination of our YSG sample was {approx}80%, while that of the RSG sample was only 3%. By placing the YSGs on the Hertzsprung-Russell diagram and comparing them against the evolutionary tracks, we find that new Geneva evolutionary models do an exemplary job at predicting both the locations and the lifetimes of these transitory objects.

Neugent, Kathryn F.; Massey, Philip; Skiff, Brian [Lowell Observatory, 1400 W Mars Hill Road, Flagstaff, AZ 86001 (United States); Meynet, Georges, E-mail: kneugent@lowell.edu, E-mail: phil.massey@lowell.edu, E-mail: bas@lowell.edu, E-mail: georges.meynet@unige.ch [Geneva Observatory, Geneva University, CH-1290 Versoix (Switzerland)

2012-04-20T23:59:59.000Z

358

Hydrodynamic Simulations of Galaxy Formation  

E-Print Network [OSTI]

We have developed an accurate, one-dimensional, spherically symmetric, Lagrangian hydrodynamics/gravity code, designed to study the effects of radiative cooling and photo-ionization on the formation of protogalaxies. We examine the ability of collapsing perturbations to cool within the age of the universe. In contrast to some studies based on order-of-magnitude estimates, we find that cooling arguments alone cannot explain the sharp upper cutoff observed in the galaxy luminosity function. We also look at the effect of a photoionizing background on the formation of low-mass galaxies.

A. A. Thoul

1994-12-09T23:59:59.000Z

359

Where the Blue Stragglers Roam: Searching for a Link Between Formation and Environment  

E-Print Network [OSTI]

The formation of blue stragglers is still not completely understood, particularly the relationship between formation environment and mechanism. We use a large, homogeneous sample of blue stragglers in the cores of 57 globular clusters to investigate the relationships between blue straggler populations and their environments. We use a consistent definition of "blue straggler" based on position in the color-magnitude diagram, and normalize the population relative to the number of red giant branch stars in the core. We find that the previously determined anti-correlation between blue straggler frequency and total cluster mass is present in the purely core population. We find some weak correlations with central velocity dispersion and with half-mass relaxation time. The blue straggler frequency does not show any trend with any other cluster parameter. Even though collisions may be expected to be a dominant blue straggler formation process in globular cluster cores, we find no correlation between the frequency of blue stragglers and the collision rate in the core. We also investigated the blue straggler luminosity function shape, and found no relationship between any cluster parameter and the distribution of blue stragglers in the color-magnitude diagram. Our results are inconsistent with some recent models of blue straggler formation that include collisional formation mechanisms, and may suggest that almost all observed blue stragglers are formed in binary systems.

Nathan Leigh; Alison Sills; Christian Knigge

2008-08-15T23:59:59.000Z

360

Method for extending the useful shelf-life of refrigerated red blood cells by flushing with inert gas  

DOE Patents [OSTI]

A method is disclosed using oxygen removal for extending the useful shelf-life of refrigerated red blood cells. A cost-effective, 4 C storage procedure that preserves red cell quality and prolongs post-transfusion in vivo survival is described. Preservation of adenosine triphosphate levels and reduction in hemolysis and in membrane vesicle production of red blood cells stored at 4 C for prolonged periods of time is achieved by removing oxygen from the red blood cells at the time of storage; in particular, by flushing with an inert gas. Adenosine triphosphate levels of the stored red blood cells are boosted in some samples by addition of ammonium phosphate. 4 figs.

Bitensky, M.W.; Yoshida, Tatsuro

1997-04-29T23:59:59.000Z

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


361

Structurally Electromagnetic Formation Flight (EMFF)  

E-Print Network [OSTI]

Structurally connected secondary mirror EMFF secondary mirror EMFF Design Electromagnetic Formation for a smaller, simpler system. µEMFF investigates the use of conventional conductors, capacitors, and solar propellants that often limit lifetime, the EMFF system uses solar power to energize a magnetic field

de Weck, Olivier L.

362

Earth and Terrestrial Planet Formation  

E-Print Network [OSTI]

The growth and composition of Earth is a direct consequence of planet formation throughout the Solar System. We discuss the known history of the Solar System, the proposed stages of growth and how the early stages of planet formation may be dominated by pebble growth processes. Pebbles are small bodies whose strong interactions with the nebula gas lead to remarkable new accretion mechanisms for the formation of planetesimals and the growth of planetary embryos. Many of the popular models for the later stages of planet formation are presented. The classical models with the giant planets on fixed orbits are not consistent with the known history of the Solar System, fail to create a high Earth/Mars mass ratio, and, in many cases, are also internally inconsistent. The successful Grand Tack model creates a small Mars, a wet Earth, a realistic asteroid belt and the mass-orbit structure of the terrestrial planets. In the Grand Tack scenario, growth curves for Earth most closely match a Weibull model. The feeding zon...

Jacobson, Seth A

2015-01-01T23:59:59.000Z

363

Cloud Formation, Evolution and Destruction  

E-Print Network [OSTI]

Chapter 4 Cloud Formation, Evolution and Destruction We now begin to trace the journey towards a star. How long does this take? The answer is surprisingly short: a good many clouds already contain new stars and these stars tend to be young. The typical cloud cannot spend long, if any time at all

Estalella, Robert

364

VEHICLE NETWORKS: ACHIEVING REGULAR FORMATION  

E-Print Network [OSTI]

VEHICLE NETWORKS: ACHIEVING REGULAR FORMATION MADALENA CHAVES, ROBERT DAY, LUCIA GOMEZ a network of vehicles exchanging information among themselves with the intention of achieving a specified the performance of the vehicle network. A stochastic model for information flow is also considered, allowing

365

Method to inhibit deposit formation  

SciTech Connect (OSTI)

A process is described for inhibiting deposit formation on the contact surfaces of structures confining heated hydrocarbon fluid which exhibits substantial fouling. The process consists of introducing into the hydrocarbon fluid at least an inhibiting amount of thiophene-containing polycondensed aromatic/naphthenic compounds of number average molecular weight (M-bar n) from 200 to 1,000.

Dickakian, G.B.

1986-10-28T23:59:59.000Z

366

Method of fracturing a geological formation  

DOE Patents [OSTI]

An improved method of fracturing a geological formation surrounding a well bore is disclosed. A relatively small explosive charge is emplaced in a well bore and the bore is subsequently hydraulically pressurized to a pressure less than the formation breakdown pressure and preferably greater than the fracture propagation pressure of the formation. The charge is denoted while the bore is so pressurized, resulting in the formation of multiple fractures in the surrounding formation with little or no accompanying formation damage. Subsequent hydraulic pressurization can be used to propagate and extend the fractures in a conventional manner. The method is useful for stimulating production of oil, gas and possibly water from suitable geologic formations.

Johnson, James O. (2679-B Walnut, Los Alamos, NM 87544)

1990-01-01T23:59:59.000Z

367

The Ratchet and the Red Queen: the maintenance of sex in parasites  

E-Print Network [OSTI]

The Ratchet and the Red Queen: the maintenance of sex in parasites R. S. HOWARD* & C. M. LIVELY for the stochastic accumulation of mutations in the finite parasite populations (Muller's Ratchet). We found that

Howard, Stephen

368

The Red Squirrel (Sciurus vulgaris L.) in relation to its food resource  

E-Print Network [OSTI]

1. A study of the ecology of the native red squirrel (Sciurus vulgaris leucorus) was carried out in a mature Scots pine (Pinus sylvestris) plantation in East Scotland. 2. The aims of this study were:- 1)To determine the ...

Tittensor, Andrew M

369

Mapping red squirrel (Sciurus vulgaris) habitat suitability using GIS and remote sensing techniques  

E-Print Network [OSTI]

The British red squirrel population has dramatically declined in the last years. The survival of the species in the UK may depend on the careful selection and management of suitable habitats. A deep understanding of its habitat requirements...

de Lamo, Xavier

2010-01-01T23:59:59.000Z

370

E-Print Network 3.0 - american red cross Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Powered by Explorit Topic List Advanced Search Sample search results for: american red cross Page: << < 1 2 3 4 5 > >> 1 University Human Resources 57 U.S. Highway 1 New...

371

Development of Digital Techniques for Analysis of Hormone Regulation of Melanophore Activity in Red Drum  

E-Print Network [OSTI]

results, and reduce subjectivity in procedures to more accurately analyze hormone interaction. To accomplish this, digital cameras were used to photograph scales of red drum (Sciaenops ocellatus), which were then analyzed using ImageJ software...

Russey, William Andrew

2008-08-19T23:59:59.000Z

372

The Agricultural Benefits of Salinity Control on the Red River of Texas and Oklahoma  

E-Print Network [OSTI]

Salinity of the waters from the Red River and its major tributaries has virtually eliminated its use for irrigation of agricultural crops in Texas and Oklahoma. A chloride control project has been proposed whereby the source salt waters...

Laughlin, D. H.; Lacewell, R. D.; Moore, D. S.

373

Red Blood cell Alloimmunization in Sickle Cell Disease: Pathophysiology, Risk Factors, and Transfusion Management  

E-Print Network [OSTI]

1 Red Blood cell Alloimmunization in Sickle Cell Disease: Pathophysiology, Risk Factors; email: france.noizat-pirenne@efs.sante.fr Keywords: sickle cell disease, alloimmunization, DHTR with sickle cell disease (SCD). Transfusions can lead to erythrocyte alloimmunization, however, with serious

Boyer, Edmond

374

E-Print Network 3.0 - acidic red soil Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

S-1--SOIL PHYSICS Visualizing Preferential Flow Paths using Ammonium Carbonate and a pH Indicator Summary: to purple-red, while the unaffected soil be- comes light yellow. The...

375

Characteristics of warm season precipitating storms in the ArkansasRed River basin  

E-Print Network [OSTI]

[1] Analysis of a multisensor precipitation product enables us to extract the precipitation from individual storms in the ArkansasRed River drainage basin over a period of 11 years. We examine the year-to-year and ...

Tucker, Donna F.; Li, Xingong

2009-07-16T23:59:59.000Z

376

E-Print Network 3.0 - adult red deer Sample Search Results  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

found in farmed Red deer in New Zealand. But these are very rare. More... antlers. White tails will also shed those antlers earlier in the year. ... Source: Buckel, Jeffrey A....

377

E-Print Network 3.0 - antibody-mediated pure red Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

antibody-mediated immunofluorescence co... is crucial for mature red blood cell production. The murine EpoR can also be activated by the envelope Source: Engelman, Donald M.-...

378

Feeding and feed-processing by red drum (Sciaenops ocellatus) fed natural and formluated diets  

E-Print Network [OSTI]

Experiments with juvenile red drum, Sciaenops ocellatus, estimated 1) digestibility, 2) feed consumption and growth, and 3) gastric evacuation rate (GER) for two diets: shrimp tail-meat ("Shrimp"), representing natural forage and a commercially...

Grey, Michael Steven

2003-01-01T23:59:59.000Z

379

E-Print Network 3.0 - adjustable red-green-blue led Sample Search...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Powered by Explorit Topic List Advanced Search Sample search results for: adjustable red-green-blue led Page: << < 1 2 3 4 5 > >> 1 The Spectrum of Clean Energy Innovationinnovati...

380

Microsoft Word - CX-Franklin-BadgerCanyonGrandview-RedMtnsDisconnectSw...  

Broader source: Energy.gov (indexed) [DOE]

8, 2012 REPLY TO ATTN OF: KEPR-4 SUBJECT: Environmental Clearance Memorandum Richard Heredia Project Manager - TEP-TPP-1 Proposed Action: Franklin-Badger Canyon and Grandview-Red...

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


381

Identification of vaccine candidates against the Poultry Red Mite, Dermanyssus gallinae  

E-Print Network [OSTI]

The poultry red mite Dermanyssus gallinae (De Geer) is a blood feeding ectoparasite that infests many bird species. Economically it is the most important parasite affecting egg-laying hens. The aim of this study was to identify vaccine candidate...

Wright, Harry Watmore

2011-07-05T23:59:59.000Z

382

The relevance of red blood cell deformability in the pathophysiology of blood disorders  

E-Print Network [OSTI]

Red blood cells (RBCs) play a crucial role in delivering oxygen to the body tissues. During the 120 days of their lifespan, average RBCs would circulate for approximately 500,000 times and undergo repeated deformations in ...

Huang, Sha, Ph. D. Massachusetts Institute of Technology

2014-01-01T23:59:59.000Z

383

Formation,  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

observed graphitization of nanodiamonds into multi-shell onion like carbon nano-structures, also called carbon onions, using reactive force-fields, which include...

384

Treating tar sands formations with dolomite  

DOE Patents [OSTI]

Methods for treating a tar sands formation are described herein. The tar sands formation may include dolomite and hydrocarbons. Methods may include providing heat at less than the decomposition temperature of dolomite from one or more heaters to at least a portion of the formation. At least some of the hydrocarbon fluids are mobilized in the formation. At least some of the hydrocarbon fluids may be produced from the formation.

Vinegar, Harold J.; Karanikas, John Michael

2010-06-08T23:59:59.000Z

385

A Preliminary Microsatellite Linkage Map of the Red Drum (Sciaenops ocellatus)  

E-Print Network [OSTI]

A PRELIMINARY MICROSATELLITE LINKAGE MAP OF THE RED DRUM (SCIAENOPS OCELLATUS) Major: Biology April 2009 Submitted to the Office of Undergraduate Research Texas A&M University in partial fulfillment of the requirements... for the designation as UNDERGRADUATE RESEARCH SCHOLAR A Senior Scholars Thesis by CHRISTOPHER M. HOLLENBECK A PRELIMINARY MICROSATELLITE LINKAGE MAP OF THE RED DRUM (SCIAENOPS OCELLATUS) Approved by: Research Advisor: John R. Gold Associate...

Hollenbeck, Christopher

2011-01-11T23:59:59.000Z

386

Effects of ionizing radiation on the response of certain photosensitive seeds to red light  

E-Print Network [OSTI]

and molecular oxygen. Studies of phosphate metabolism (Surrey and Gordon, 1962) and phosphorylation (Gordon and Surrey, 1961) indicate that energy transfer through phosphate esterification plays an important role and may be the key enzymatic reaction in red... spectrum promoting the germination of light-sensitive lettuce seed. Smithsonian Inst. Pubis. Misc. Collections 96: 1-8 ~ 11. Gordon, S. A. , and K. Surrey. 1961. Phosphorylation and red-spectrum photomorphogenesis. ~n Effects of ionizing radiations...

Richardson, Billy

2012-06-07T23:59:59.000Z

387

RED TERICA, EVOLUCIN TERICA Y HOLONES EN ARQUEOLOGA Autor: Magster. Mara Virginia Ferro  

E-Print Network [OSTI]

1 RED TE?RICA, EVOLUCI?N TE?RICA Y HOLONES EN ARQUEOLOGÍA Autor: Magster. María Virginia Ferro desde conceptos de evolución teórica, redes teóricas y holones en el desarrollo de la arqueología. Primera Parte: Evolución y red teórica; holones desde metateoría. Siguiendo a Balzer, Moulines y Sneed

Boyer, Edmond

388

Blueshift Without Blueshift: Red Hole Gamma-Ray Burst Models Explain the Peak energy Distribution  

E-Print Network [OSTI]

Gamma-ray bursts are still a puzzle. In particular, the central engine, the total energy and the very narrow distribution of peak energies challenge model builders. We consider here an extreme model of gamma-ray bursts based on highly red- and blue-shifted positron annihilation radiation. The burst emerges from inside the red hole created by the complete gravitational collapse of the GRB progenitor.

James S. Graber

1999-12-15T23:59:59.000Z

389

Mixed modes in red-giant stars observed with CoRoT  

E-Print Network [OSTI]

The CoRoT mission has provided thousands of red-giant light curves. The analysis of their solar-like oscillations allows us to characterize their stellar properties. Up to now, the global seismic parameters of the pressure modes remain unable to distinguish red-clump giants from members of the red-giant branch. As recently done with Kepler red giants, we intend to analyze and use the so-called mixed modes to determine the evolutionary status of the red giants observed with CoRoT. We also aim at deriving different seismic characteristics depending on evolution. The complete identification of the pressure eigenmodes provided by the red-giant universal oscillation pattern allows us to aim at the mixed modes surrounding the l=1 expected eigenfrequencies. A dedicated method based on the envelope autocorrelation function is proposed to analyze their period separation. We have identified the mixed-mode signature separation thanks to their pattern compatible with the asymptotic law of gravity modes. We have shown tha...

Mosser, B; Montalb, J; Beck, P G; Miglio, A; Belkacem, K; Goupil, M J; Hekker, S; De Ridder, J; Dupret, M A; Elsworth, Y; Noels, A; Baudin, F; Michel, E; Samadi, R; Auvergne, M; Baglin, A; Catala, C

2011-01-01T23:59:59.000Z

390

The Optical Gravitational Lensing Experiment. Red Clump Stars as a Distance Indicator  

E-Print Network [OSTI]

We present relation of the mean I-band brightness of red clump stars on metallicity. Red clump stars were proposed to be a very attractive standard candle for distance determination. The calibration is based on 284 nearby red giant stars whose high quality spectra allowed to determine accurate individual metal abundances. High quality parallaxes (\\sigma_\\pi / \\pi < 10%) and photometry of these very bright stars come from Hipparcos measurements. Metallicity of the sample covers a large range: -0.6<[Fe/H]<+0.2 dex. We find a weak dependence of the mean I-band brightness on metallicity (about 0.13 mag/dex). What is more important, the range of metallicity of the Hipparcos sample partially overlaps with metallicity of field giants in the LMC, thus making it possible to determine the distance to the LMC by almost direct comparison of brightness of the local Hipparcos red clump giants with that of LMC stars. Photometry of field red clump giants in nine low extinction fields of the LMC halo collected during the OGLE-II microlensing survey compared with the Hipparcos red clump stars data yields the distance modulus to the LMC: (m-M)_LMC=18.24+/-0.08 mag.

A. Udalski

2000-01-14T23:59:59.000Z

391

Star Formation and AGN activity in Galaxies classified using the 1.6 {\\mu}m Bump and PAH features at $z = 0.4-2$  

E-Print Network [OSTI]

We have studied the star-formation and AGN activity of massive galaxies in the redshift range $z=0.4-2$, which are detected in a deep survey field using the AKARI InfraRed (IR) astronomical satellite and {\\em Subaru} telescope toward the North Ecliptic Pole (NEP). The AKARI/IRC Mid-InfraRed (MIR) multiband photometry is used to trace their star-forming activities with the Polycyclic-Aromatic Hydrocarbon (PAH) emissions, which is also used to distinguish star-forming populations from AGN dominated ones and to estimate the Star Formation Rate (SFR) derived from their total emitting IR (TIR) luminosities. In combination with analyses of their stellar components, we have studied the MIR SED features of star-forming and AGN-harboring galaxies.

Hanami, Hitoshi; Fujishiro, Naofumi; Nakanishi, Kouichiro; Miyaji, Takamitsu; Krumpe, Mirko; Umetsu, Keiichi; Ohyama, Youichi; Shim, Hyun Jin; Im, Myungshin; Lee, Hyoung Mok; Lee, Myung Gyoon; Serjeant, Stephen; White, Glenn J; Willmer, Christopher N; Goto, Tomotsugu; Oyabu, Shinki; Takagi, Toshinobu; Wada, Takehiko; Matsuhara, Hideo

2011-01-01T23:59:59.000Z

392

SUPERNOVA 2008bk AND ITS RED SUPERGIANT PROGENITOR  

SciTech Connect (OSTI)

We have obtained limited photometric and spectroscopic data for supernova (SN) 2008bk in NGC 7793, primarily at {approx}> 150 days after explosion. We find that it is a Type II-Plateau (II-P) SN that most closely resembles the low-luminosity SN 1999br in NGC 4900. Given the overall similarity between the observed light curves and colors of SNe 2008bk and 1999br, we infer that the total visual extinction to SN 2008bk (A{sub V} = 0.065 mag) must be almost entirely due to the Galactic foreground, similar to what has been assumed for SN 1999br. We confirm the identification of the putative red supergiant (RSG) progenitor star of the SN in high-quality g'r'i' images we had obtained in 2007 at the Gemini-South 8 m telescope. Little ambiguity exists in this progenitor identification, qualifying it as the best example to date, next to the identification of the star Sk -69 Degree-Sign 202 as the progenitor of SN 1987A. From a combination of photometry of the Gemini images with that of archival, pre-SN, Very Large Telescope JHK{sub s} images, we derive an accurate observed spectral energy distribution (SED) for the progenitor. We find from nebular strong-intensity emission-line indices for several H II regions near the SN that the metallicity in the environment is likely subsolar (Z Almost-Equal-To 0.6 Z{sub Sun }). The observed SED of the star agrees quite well with synthetic SEDs obtained from model RSG atmospheres with effective temperature T{sub eff} = 3600 {+-} 50 K. We find, therefore, that the star had a bolometric luminosity with respect to the Sun of log (L{sub bol}/L{sub Sun} ) = 4.57 {+-} 0.06 and radius R{sub *} = 496 {+-} 34 R{sub Sun} at {approx}6 months prior to explosion. Comparing the progenitor's properties with theoretical massive-star evolutionary models, we conclude that the RSG progenitor had an initial mass in the range of 8-8.5 M{sub Sun }. This mass is consistent with, albeit at the low end of, the inferred range of initial masses for SN II-P progenitors. It is also consistent with the estimated upper limit on the initial mass of the progenitor of SN 1999br, and it agrees with the low initial masses found for the RSG progenitors of other low-luminosity SNe II-P.

Van Dyk, Schuyler D.; Elias-Rosa, Nancy [Spitzer Science Center/Caltech, Mailcode 220-6, Pasadena, CA 91125 (United States); Davidge, Tim J., E-mail: vandyk@ipac.caltech.edu, E-mail: tim.davidge@nrc.ca [Herzberg Institute of Astrophysics, National Research Council of Canada, Victoria, B.C., V9E 2E7 (Canada); and others

2012-01-15T23:59:59.000Z

393

Photophoresis boosts giant planet formation  

E-Print Network [OSTI]

In the core accretion model of giant planet formation, a solid protoplanetary core begins to accrete gas directly from the nebula when its mass reaches about 5 earth masses. The protoplanet has at most a few million years to reach runaway gas accretion, as young stars lose their gas disks after 10 million years at the latest. Yet gas accretion also brings small dust grains entrained in the gas into the planetary atmosphere. Dust accretion creates an optically thick protoplanetary atmosphere that cannot efficiently radiate away the kinetic energy deposited by incoming planetesimals. A dust-rich atmosphere severely slows down atmospheric cooling, contraction, and inflow of new gas, in contradiction to the observed timescales of planet formation. Here we show that photophoresis is a strong mechanism for pushing dust out of the planetary atmosphere due to the momentum exchange between gas and dust grains. The thermal radiation from the heated inner atmosphere and core is sufficient to levitate dust grains and to ...

Teiser, Jens

2013-01-01T23:59:59.000Z

394

Formation of polar ring galaxies  

E-Print Network [OSTI]

Polar ring galaxies are peculiar systems in which a gas rich, nearly polar ring surrounds an early-type or elliptical host galaxy. Two formation scenarios for these objects have been proposed: they are thought to form either in major galaxy mergers or by tidal accretion of the polar material from a gas rich donor galaxy. Both scenarios are studied through N-body simulations including gas dynamics and star formation. Constraints on physical parameters are drawn out, in order to determine which scenario is the most likely to occur. Polar ring galaxies from each scenario are compared with observations and we discuss whether the accretion scenario and the merging scenario account for observational properties of polar ring galaxies. The conclusion of this study is that the accretion scenario is both the most likely and the most supported by observations. Even if the merging scenario is rather robust, most polar ring galaxies are shown to be the result of tidal gas accretion events.

F. Bournaud; F. Combes

2003-02-04T23:59:59.000Z

395

Rapid gas hydrate formation process  

DOE Patents [OSTI]

The disclosure provides a method and apparatus for forming gas hydrates from a two-phase mixture of water and a hydrate forming gas. The two-phase mixture is created in a mixing zone which may be wholly included within the body of a spray nozzle. The two-phase mixture is subsequently sprayed into a reaction zone, where the reaction zone is under pressure and temperature conditions suitable for formation of the gas hydrate. The reaction zone pressure is less than the mixing zone pressure so that expansion of the hydrate-forming gas in the mixture provides a degree of cooling by the Joule-Thompson effect and provides more intimate mixing between the water and the hydrate-forming gas. The result of the process is the formation of gas hydrates continuously and with a greatly reduced induction time. An apparatus for conduct of the method is further provided.

Brown, Thomas D.; Taylor, Charles E.; Unione, Alfred J.

2013-01-15T23:59:59.000Z

396

Kinetic models of opinion formation  

E-Print Network [OSTI]

We introduce and discuss certain kinetic models of (continuous) opinion formation involving both exchange of opinion between individual agents and diffusion of information. We show conditions which ensure that the kinetic model reaches non trivial stationary states in case of lack of diffusion in correspondence of some opinion point. Analytical results are then obtained by considering a suitable asymptotic limit of the model yielding a Fokker-Planck equation for the distribution of opinion among individuals.

G. Toscani

2006-05-17T23:59:59.000Z

397

Structure and red shift of optical band gap in CdOZnO nanocomposite synthesized by the sol gel method  

SciTech Connect (OSTI)

The structure and the optical band gap of CdOZnO nanocomposites were studied. Characterization using X-ray diffraction (XRD), transmission electron microscopy (TEM) and diffuse reflectance spectroscopy (DRS) analysis confirms that CdO phase is present in the nanocomposites. TEM analysis confirms the formation of spheroidal nanoparticles and nanorods. The particle size was calculated from DebeySherrer?s formula and corroborated by TEM images. FTIR spectroscopy shows residual organic materials (aromatic/Olefinic carbon) from nanocomposites surface. CdO content was modified in the nanocomposites in function of polyvinylalcohol (PVA) added. The optical band gap is found to be red shift from 3.21 eV to 3.11 eV with the increase of CdO content. Photoluminescence (PL) measurements reveal the existence of defects in the synthesized CdOZnO nanocomposites. - Graphical abstract: Optical properties of ZnO, CdO and ZnO/CdO nanoparticles. Display Omitted - Highlights: TEM analysis confirms the presence of spherical nanoparticles and nanorods. The CdO phase is present in the nanocomposites. The band gap of the CdOZnO nanocomposites is slightly red shift with CdO content. PL emission of CdOZnO nanocomposite are associated to structural defects.

Mosquera, Edgar, E-mail: edemova@ing.uchile.cl [Laboratorio de Materiales a Nanoescala, Departamento de Ciencia de los Materiales, Facultad de Ciencias Fsicas y Matemticas, Universidad de Chile, Av. Tupper 2069, Santiago (Chile); Pozo, Ignacio del, E-mail: ignacio.dpf@gmail.com [Facultad de Ciencias Naturales, Matemticas y del Medio Ambiente, Universidad Tecnolgica Metropolitana, Av. Jos Pedro Alessandri 1242, Santiago (Chile); Morel, Mauricio, E-mail: mmorel@ing.uchile.cl [Laboratorio de Materiales a Nanoescala, Departamento de Ciencia de los Materiales, Facultad de Ciencias Fsicas y Matemticas, Universidad de Chile, Av. Tupper 2069, Santiago (Chile)

2013-10-15T23:59:59.000Z

398

UV Star Formation Rates in the Local Universe  

E-Print Network [OSTI]

We measure star formation rates of ~50,000 optically-selected galaxies in the local universe (z~0.1), spanning a range from gas-rich dwarfs to massive ellipticals. We obtain dust-corrected SFRs by fitting the GALEX (UV) and SDSS (optical) photometry to a library of population synthesis models that include dust attenuation. For star-forming galaxies, our UV-based SFRs compare remarkably well with those derived from SDSS H alpha. Deviations from perfect agreement between these two methods are due to differences in the dust attenuation estimates. In contrast to H alpha, UV provides reliable SFRs for galaxies with weak or no H alpha emission, and where H alpha is contaminated with an emission from an AGN. We use full-SED SFRs to calibrate a simple prescription that uses GALEX UV magnitudes to produce good SFRs for normal star-forming galaxies. The specific SFR is considered as a function of stellar mass for (1) star-forming galaxies with no AGN, (2) those hosting an AGN, and for (3) galaxies without H alpha emission. We find that the three have distinct star formation histories, with AGN lying intermediate between the star-forming and the quiescent galaxies. Normal star forming galaxies (without an AGN) lie on a relatively narrow linear sequence. Remarkably, galaxies hosting a strong AGN appear to represent the massive continuation of this sequence. Weak AGN, while also massive, have lower SFR, sometimes extending to the realm of quiescent galaxies. We propose an evolutionary sequence for massive galaxies that smoothly connects normal star-forming galaxies to quiescent (red sequence) galaxies via strong and weak AGN. We confirm that some galaxies with no H alpha emission show signs of SF in the UV. We derive a UV-based cosmic SFR density at z=0.1 with smaller total error than previous measurements (abridged).

Samir Salim; R. Michael Rich; Stphane Charlot; Jarle Brinchmann; Benjamin D. Johnson; David Schiminovich; Mark Seibert; Ryan Mallery; Timothy M. Heckman; Karl Forster; Peter G. Friedman; D. Christopher Martin; Patrick Morrissey; Susan G. Neff; Todd Small; Ted K. Wyder; Luciana Bianchi; Jose Donas; Young-Wook Lee; Barry F. Madore; Bruno Milliard; Alex S. Szalay; Barry Y. Welsh; Sukyoung K. Yi

2007-05-07T23:59:59.000Z

399

Star Formation at Redshift One: Preliminary results from an H-alpha Survey  

E-Print Network [OSTI]

We present the first successful demonstration of multi-object near-infrared spectroscopy on high redshift galaxies. Our objective is to address the true star formation history of the universe at z~1, a crucial epoch which some have suggested is the peak of star formation activity. By using H-alpha -the same robust star formation indicator used at low-z - redshifted into the J- and H-bands, we can trace star formation without the systematic uncertainties of different calibrators, or the extreme dust extinction in the rest-UV, which have plagued previous efforts. We are using the instrument CIRPASS (the Cambridge Infra-Red PAnoramic Survey Spectrograph), in multi-object mode, which has been successfully demonstrated on the Anglo-Australian Telescope (AAT) and the William Herschel Telescope (WHT). CIRPASS has 150 fibres deployable over \\~40arcmin on the AAT and ~15arcmin on the WHT. Here we present preliminary results from one of our fields observed with the WHT: H-alpha detections of z~1 galaxies in the Hubble Deep Field North.

M. Doherty; A. Bunker; R. Sharp; G. Dalton; I. Parry; I. Lewis; E. MacDonald; C. Wolf

2004-07-12T23:59:59.000Z

400

Formation damage in underbalanced drilling operations  

E-Print Network [OSTI]

Formation damage has long been recognized as a potential source of reduced productivity and injectivity in both horizontal and vertical wells. From the moment that the pay zone is being drilled until the well is put on production, a formation...

Reyes Serpa, Carlos Alberto

2003-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


401

SAR polar format implementation with MATLAB.  

SciTech Connect (OSTI)

Traditional polar format image formation for Synthetic Aperture Radar (SAR) requires a large amount of processing power and memory in order to accomplish in real-time. These requirements can thus eliminate the possible usage of interpreted language environments such as MATLAB. However, with trapezoidal aperture phase history collection and changes to the traditional polar format algorithm, certain optimizations make MATLAB a possible tool for image formation. Thus, this document's purpose is two-fold. The first outlines a change to the existing Polar Format MATLAB implementation utilizing the Chirp Z-Transform that improves performance and memory usage achieving near realtime results for smaller apertures. The second is the addition of two new possible image formation options that perform a more traditional interpolation style image formation. These options allow the continued exploration of possible interpolation methods for image formation and some preliminary results comparing image quality are given.

Martin, Grant D.; Doerry, Armin Walter

2005-11-01T23:59:59.000Z

402

Proportional structural effects of formative indicators  

E-Print Network [OSTI]

Formative constructs must influence two or more distinct outcome variables for meaningful tests of the formative conceptualization. Because the construct mediates the effects of its indicators, the indicators must have ...

Franke, George R.; Preacher, K. J.; Rigdon, Ed E.

2009-03-15T23:59:59.000Z

403

Structure formation: Models, Dynamics and Status  

E-Print Network [OSTI]

The constraints on the models for the structure formation arising from various cosmological observations at different length scales are reviewed. The status of different models for structure formation is examined critically in the light of these observations.

T. Padmanabhan

1995-08-25T23:59:59.000Z

404

Treating nahcolite containing formations and saline zones  

DOE Patents [OSTI]

A method for treating a nahcolite containing subsurface formation includes removing water from a saline zone in or near the formation. The removed water is heated using a steam and electricity cogeneration facility. The heated water is provided to the nahcolite containing formation. A fluid is produced from the nahcolite containing formation. The fluid includes at least some dissolved nahcolite. At least some of the fluid is provided to the saline zone.

Vinegar, Harold J

2013-06-11T23:59:59.000Z

405

Depositional framework and reservoir distribution of Red Fork sandstone in Oklahoma  

SciTech Connect (OSTI)

The Middle Pennsylvanian Red Fork sandstone formed as a result of southward progradation across most of Oklahoma. The Red Fork is one of several cyclothemic (transgressive-regressive) sequences developed within the Desmoinesian Cherokee Group. Sea level changes and stability of the depositional area were dominant factors in determining the general stratigraphic characteristics of the Red Fork interval. Progradation was episodic, with sand deposition in the distal, more subsident part of the basin during lower sea level stands, and valley-fill deposition in the more stable areas during sea level rises. Red Fork sandstone trends depict an alluvial-deltaic complex covering most of Oklahoma. The Red Fork consists primarily of alluvial-valley and plain (fluvial) bodies in the northern part of northeastern Oklahoma, alluvial-deltaic bodies in most of the remaining parts of the shelf area, and off-shelf submarine-fan and slope/basin-floor complexes within the deeper part of the Anadarko basin. Determination of reservoir trend and genesis requires integration of rock data and log data, with logs calibrated to cores for estimating depositional environments and assessing diagenetic overprints. Much of the oil and gas has been trapped in stratigraphic traps, some of which represent channelized sandstones with trends at high angles to the structural grain. Secondary chlorite, in particular, is associated locally with development of productive reservoirs showing microporosity, high water saturation, and correspondingly low resistivities.

Shelton, J.W.; Fritz, R.D.; Johnson, C. (Masera Corp., Tulsa, OK (USA))

1989-08-01T23:59:59.000Z

406

Red-Shift Distribution of Gamma-ray Bursts and Their Progenitors  

E-Print Network [OSTI]

Gamma ray bursts have been divided into two classes, long-soft gamma ray burst and short-hard gamma ray burst according to the bimodal distribution in duration time. Due to the harder spectrum and the lack of afterglows of short-hard bursts in optical and radio observations, different progenitors for short-hard bursts and long-soft bursts have been suggested. Based on the X-ray afterglow observation and the cumulative red-shift distribution of short-hard bursts, Nakar et al. (2006) found that the progenitors of short-hard bursts are consistent with old populations, such as mergers of binary neutron stars. Recently, the existence of two subclasses in long-soft bursts has been suggested after considering multiple characteristics of gamma-ray bursts, including fluences and the duration time. In this work, we extended the analysis of cumulative red-shift distribution to two possible subclasses in L-GRBs. We found that two possible subclass GRBs show different red-shift distributions, especially for red-shifts z > 1. Our results indicate that the accumulative red-shift distribution can be used as a tool to constrain the progenitor characteristics of possible subclasses in L-GRBs.

Soomin Jeong; Chang-Hwan Lee

2007-10-08T23:59:59.000Z

407

Petrophysical evaluation of subterranean formations  

DOE Patents [OSTI]

Methods and systems are provided for evaluating petrophysical properties of subterranean formations and comprehensively evaluating hydrate presence through a combination of computer-implemented log modeling and analysis. Certain embodiments include the steps of running a number of logging tools in a wellbore to obtain a variety of wellbore data and logs, and evaluating and modeling the log data to ascertain various petrophysical properties. Examples of suitable logging techniques that may be used in combination with the present invention include, but are not limited to, sonic logs, electrical resistivity logs, gamma ray logs, neutron porosity logs, density logs, NRM logs, or any combination or subset thereof.

Klein, James D; Schoderbek, David A; Mailloux, Jason M

2013-05-28T23:59:59.000Z

408

Gas Cooling Through Galaxy Formations  

E-Print Network [OSTI]

Abstract-- Gas cooling was studied in two different boxes of sizes and by simulation at same redshifts. The gas cooling is shown in four different redshifts (z=1.15, 0.5, 0.1 and 0). In the simulation the positions of the clumps of cooled gas were studied with slices of the two volumes and also the density of cooled gas of the two volumes shown in the simulation. From the process of gas cooling it is clear that this process gives different results in the two cases. Index Term- Gas Cooling, Simulation, galaxy Formation. I.

Mariwan A. Rasheed; Mohamad A. Brza

409

Format for Federal Register Notice  

Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE: AlternativeEnvironment, Safety and HealthDepartmentFindings of NoFleetFood andDepartment ofFormat

410

Electrochemical formation of field emitters  

DOE Patents [OSTI]

Electrochemical formation of field emitters, particularly useful in the fabrication of flat panel displays. The fabrication involves field emitting points in a gated field emitter structure. Metal field emitters are formed by electroplating and the shape of the formed emitter is controlled by the potential imposed on the gate as well as on a separate counter electrode. This allows sharp emitters to be formed in a more inexpensive and manufacturable process than vacuum deposition processes used at present. The fabrication process involves etching of the gate metal and the dielectric layer down to the resistor layer, and then electroplating the etched area and forming an electroplated emitter point in the etched area.

Bernhardt, Anthony F. (Berkeley, CA)

1999-01-01T23:59:59.000Z

411

Autonomous Helicopter Formation using Model Predictive Control  

E-Print Network [OSTI]

Autonomous Helicopter Formation using Model Predictive Control Hoam Chung and S. Shankar Sastry are required to fly in tight formations and under harsh conditions. The starting point for safe autonomous into a formation, so that each vehicle can safely maintain sufficient space between it and all other vehicles

Sastry, S. Shankar

412

Electromagnetic Formation Flight of Satellite Arrays  

E-Print Network [OSTI]

Electromagnetic Formation Flight of Satellite Arrays Daniel W. Kwon and David W. Miller February 2005 SSL # 2-05 #12;#12;Electromagnetic Formation Flight of Satellite Arrays By DANIEL W. KWON S;#12;Electromagnetic Formation Flight of Satellite Arrays by DANIEL W. KWON Submitted to the Department of Aeronautics

413

The Observer March 2003 page 3 CSU Fresno 16" SCT at f/38 & Jupiter's Great Red Spot  

E-Print Network [OSTI]

The Observer March 2003 page 3 CSU Fresno 16" SCT at f/38 & Jupiter's Great Red Spot By Greg Morgan in March that the Great Red Spot will be making a central meridian crossing along with the shadow of one in the region of the Great Red Spot. Similarly, on Tuesday evening April 1st , from 10:24 PM to 1:48 AM PDT, Io

Ringwald, Frederick A.

414

U-217: Red Hat Certificate System Bugs Let Remote Users Conduct Cross-Site Scripting and Denial of Service Attacks  

Broader source: Energy.gov [DOE]

Two vulnerabilities were reported in Red Hat Certificate System. A remote user can conduct cross-site scripting attacks. A remote authenticated user can revoke the CA certificate.

415

Method for extending the useful shelf-life of refrigerated red blood cells by flushing with inert gas  

DOE Patents [OSTI]

Method using oxygen removal for extending the useful shelf-life of refrigerated red blood cells. A cost-effective, 4.degree. C. storage procedure that preserves red cell quality and prolongs post-transfusion in vivo survival is described. Preservation of adenosine triphosphate levels and reduction in hemolysis and in membrane vesicle production of red blood cells stored at 4.degree. C. for prolonged periods of time is achieved by removing oxygen therefrom at the time of storage; in particular, by flushing with an inert gas. Adenosine triphosphate levels of the stored red blood cells are boosted in some samples by addition of ammonium phosphate.

Bitensky, Mark W. (Los Alamos, NM); Yoshida, Tatsuro (Los Alamos, NM)

1997-01-01T23:59:59.000Z

416

U-230: Sudo on Red Hat Enterprise Linux %postun Symlink Flaw Lets Local Users Gain Elevated Privileges  

Broader source: Energy.gov [DOE]

An updated sudo package that fixes one security issue and several bugs is now available for Red Hat Enterprise Linux 5.

417

Coring in deep hardrock formations  

SciTech Connect (OSTI)

The United States Department of Energy is involved in a variety of scientific and engineering feasibility studies requiring extensive drilling in hard crystalline rock. In many cases well depths extend from 6000 to 20,000 feet in high-temperature, granitic formations. Examples of such projects are the Hot Dry Rock well system at Fenton Hill, New Mexico and the planned exploratory magma well near Mammoth Lakes, California. In addition to these programs, there is also continuing interest in supporting programs to reduce drilling costs associated with the production of geothermal energy from underground sources such as the Geysers area near San Francisco, California. The overall progression in these efforts is to drill deeper holes in higher temperature, harder formations. In conjunction with this trend is a desire to improve the capability to recover geological information. Spot coring and continuous coring are important elements in this effort. It is the purpose of this report to examine the current methods used to obtain core from deep wells and to suggest projects which will improve existing capabilities. 28 refs., 8 figs., 2 tabs.

Drumheller, D.S.

1988-08-01T23:59:59.000Z

418

Formula for red-shift of light signals coming from distant galaxies  

E-Print Network [OSTI]

Relying on the obtained results in Rev.[1](physics/0505035), we derive the formula relating the red-shift of light signals coming from distant galaxies to the distance of these galaxies from us and the time of detecting of these light signals. The red-shift coefficient, instead of the Hubble parameter, is introduced. It varies with time and positive at all times. Its nowadays value equals the Hubble parameter. It increases forever as time is running from the past to the future. The derived formula enables us to estimate the nowadays increasing rate of the red-shift coefficient, which is nothing but the nowadays value of the "acceleration of the expansion of the Universe".

Jian-Miin Liu

2005-05-04T23:59:59.000Z

419

Prolonged cold storage of red blood cells by oxygen removal and additive usage  

DOE Patents [OSTI]

Prolonged cold storage of red blood cells by oxygen removal and additive usage. A cost-effective, 4.degree. C. storage procedure that preserves red cell quality and prolongs post-transfusion in vivo survival is described. The improved in vivo survival and the preservation of adenosine triphosphate levels, along with reduction in hemolysis and membrane vesicle production of red blood cells stored at 4.degree. C. for prolonged periods of time, is achieved by reducing the oxygen level therein at the time of storage; in particular, by flushing the cells with an inert gas, and storing them in an aqueous solution which includes adenine, dextrose, mannitol, citrate ion, and dihydrogen phosphate ion, but no sodium chloride, in an oxygen-permeable container which is located in an oxygen-free environment containing oxygen-scavenging materials.

Bitensky, Mark W. (Boston, MA); Yoshida, Tatsuro (Newton, MA)

1998-01-01T23:59:59.000Z

420

Prolonged cold storage of red blood cells by oxygen removal and additive usage  

DOE Patents [OSTI]

Prolonged cold storage of red blood cells by oxygen removal and additive usage. A cost-effective, 4 C storage procedure that preserves red cell quality and prolongs post-transfusion in vivo survival is described. The improved in vivo survival and the preservation of adenosine triphosphate levels, along with reduction in hemolysis and membrane vesicle production of red blood cells stored at 4 C for prolonged periods of time, is achieved by reducing the oxygen level therein at the time of storage; in particular, by flushing the cells with an inert gas, and storing them in an aqueous solution which includes adenine, dextrose, mannitol, citrate ion, and dihydrogen phosphate ion, but no sodium chloride, in an oxygen-permeable container which is located in an oxygen-free environment containing oxygen-scavenging materials. 8 figs.

Bitensky, M.W.; Yoshida, Tatsuro

1998-08-04T23:59:59.000Z

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


421

Heating tar sands formations while controlling pressure  

DOE Patents [OSTI]

Methods for treating a tar sands formation are described herein. Methods may include heating at least a section of a hydrocarbon layer in the formation from a plurality of heaters located in the formation. A pressure in the majority of the section may be maintained below a fracture pressure of the formation. The pressure in the majority of the section may be reduced to a selected pressure after the average temperature reaches a temperature that is above 240.degree. C. and is at or below pyrolysis temperatures of hydrocarbons in the section. At least some hydrocarbon fluids may be produced from the formation.

Stegemeier, George Leo (Houston, TX) [Houston, TX; Beer, Gary Lee (Houston, TX) [Houston, TX; Zhang, Etuan (Houston, TX) [Houston, TX

2010-01-12T23:59:59.000Z

422

Hydrothermal synthesis and characteristics of anions-doped calcium molybdate red powder phosphors  

SciTech Connect (OSTI)

Graphical abstract: - Highlights: Four anion-doped CaMoO{sub 4}:Eu{sup 3+} red phosphors were prepared by hydrothermal approach. Some samples exhibit nearly spherical morphology and well-distributed fine particles. The red luminescence can be obviously enhanced after certain amount of anion doping. The improved phosphor system is a potential candidate for white LED applications. - Abstract: Applying hydrothermal and subsequent heat-treatment process, CaMoO{sub 4}:Eu{sup 3+} was doped with four anions (SiO{sub 3}{sup 2?}, PO{sub 4}{sup 3?}, SO{sub 4}{sup 2?} and ClO{sub 3}{sup ?}) to prepare fine red powder phosphors. The introduction of small amount of anions into the host had little influence on the structure, which was confirmed by X-ray diffraction patterns. The anion-doped phosphor samples (except SiO{sub 3}{sup 2?}) exhibited nearly spherical morphology, and the particle sizes were in the range of 0.30.4 ?m for SO{sub 4}{sup 2?}-doped samples, and 0.81.2 ?m for PO{sub 4}{sup 3?} and ClO{sub 3}{sup ?}-doped samples. Excited with 395 nm near-UV light, all samples showed typical Eu{sup 3+} red emission at 615 nm, and PO{sub 4}{sup 3?}, SO{sub 4}{sup 2?} and ClO{sub 3}{sup ?}-doped samples enhanced the red luminescence as compared with the individual CaMoO{sub 4}:Eu{sup 3+} sample. In particular, relative emission intensity for optimum ClO{sub 3}{sup ?}-doped phosphors reached more than 6-fold that of the commercial red phosphor, which is highly desirable for the powder phosphors used in the solid-state lighting industry.

Shi, Shikao, E-mail: ssk02@mails.tsinghua.edu.cn [College of Chemistry and Materials Science, Hebei Normal University, Shijiazhuang 050024 (China); Zhang, Yan; Liu, Qing [College of Chemistry and Materials Science, Hebei Normal University, Shijiazhuang 050024 (China); Zhou, Ji [State Key Laboratory of New Ceramics and Fine Processing, Tsinghua University, Beijing 100084 (China)

2013-10-15T23:59:59.000Z

423

GRANULATION IN RED GIANTS: OBSERVATIONS BY THE KEPLER MISSION AND THREE-DIMENSIONAL CONVECTION SIMULATIONS  

SciTech Connect (OSTI)

The granulation pattern that we observe on the surface of the Sun is due to hot plasma rising to the photosphere where it cools down and descends back into the interior at the edges of granules. This is the visible manifestation of convection taking place in the outer part of the solar convection zone. Because red giants have deeper convection zones than the Sun, we cannot a priori assume that their granulation is a scaled version of solar granulation. Until now, neither observations nor one-dimensional analytical convection models could put constraints on granulation in red giants. With asteroseismology, this study can now be performed. We analyze {approx}1000 red giants that have been observed by Kepler during 13 months. We fit the power spectra with Harvey-like profiles to retrieve the characteristics of the granulation (timescale {tau}{sub gran} and power P{sub gran}). We search for a correlation between these parameters and the global acoustic-mode parameter (the position of maximum power, {nu}{sub max}) as well as with stellar parameters (mass, radius, surface gravity (log g), and effective temperature (T{sub eff})). We show that {tau}{sub eff}{proportional_to}{nu}{sup -0.89}{sub max} and P{sub gran}{proportional_to}{nu}{sup -1.90}{sub max}, which is consistent with the theoretical predictions. We find that the granulation timescales of stars that belong to the red clump have similar values while the timescales of stars in the red giant branch are spread in a wider range. Finally, we show that realistic three-dimensional simulations of the surface convection in stars, spanning the (T{sub eff}, log g) range of our sample of red giants, match the Kepler observations well in terms of trends.

Mathur, S. [High Altitude Observatory, NCAR, P.O. Box 3000, Boulder, CO 80307 (United States); Hekker, S. [Astronomical Institute 'Anton Pannekoek', University of Amsterdam, P.O. Box 94249, 1090 GE Amsterdam (Netherlands); Trampedach, R. [JILA, University of Colorado and National Institute of Standards and Technology, 440 UCB, Boulder, CO 80309 (United States); Ballot, J. [Institut de Recherche en Astrophysique et Planetologie, CNRS, 14 avenue E. Belin, 31400 Toulouse (France); Kallinger, T. [Institute for Astronomy (IfA), University of Vienna, Tuerkenschanzstrasse 17, 1180 Vienna (Austria); Buzasi, D. [Eureka Scientific, 2452 Delmer Street Suite 100, Oakland, CA 94602-3017 (United States); Garcia, R. A. [Laboratoire AIM, CEA/DSM-CNRS-Universite Paris Diderot-IRFU/SAp, 91191 Gif-sur-Yvette Cedex (France); Huber, D.; Bedding, T. R.; Stello, D. [Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006 (Australia); Jimenez, A.; Regulo, C. [Dpto de Astrofisica, Universidad de La Laguna, 38206, Tenerife (Spain); Mosser, B. [LESIA, UMR8109, Universite Pierre et Marie Curie, Universite Denis Diderot, Obs. de Paris, 92195 Meudon Cedex (France); Elsworth, Y.; Chaplin, W. J.; Hale, S. J. [School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT (United Kingdom); De Ridder, J. [Instituut voor Sterrenkunde, K.U. Leuven, Celestijnenlaan 200D, 3001 Leuven (Belgium); Kinemuchi, K. [Bay Area Environmental Research Inst./NASA Ames Research Center, Moffett Field, CA 94035 (United States); Kjeldsen, H. [Danish AsteroSeismology Centre, Department of Physics and Astronomy, University of Aarhus, 8000 Aarhus C (Denmark); Mullally, F. [SETI Institute/NASA Ames Research Center, Moffett Field, CA 94035 (United States)

2011-11-10T23:59:59.000Z

424

Crystallographic study of red fluorescent protein eqFP578 and its far-red variant Katushka reveals opposite pH-induced isomerization of chromophore  

SciTech Connect (OSTI)

The wild type red fluorescent protein eqFP578 (from sea anemone Entacmaea quadricolor, {lambda}{sub ex} = 552 nm, {lambda}{sub em} = 578 nm) and its bright far-red fluorescent variant Katushka ({lambda}{sub ex} = 588 nm, {lambda}{sub em} = 635 nm) are characterized by the pronounced pH dependence of their fluorescence. The crystal structures of eqFP578f (eqFP578 with two point mutations improving the protein folding) and Katushka have been determined at the resolution ranging from 1.15 to 1.85 {angstrom} at two pH values, corresponding to low and high level of fluorescence. The observed extinguishing of fluorescence upon reducing pH in eqFP578f and Katushka has been shown to be accompanied by the opposite trans-cis and cis-trans chromophore isomerization, respectively. Asn143, Ser158, His197 and Ser143, Leu174, and Arg197 have been shown to stabilize the respective trans and cis fluorescent states of the chromophores in eqFP578f and Katushka at higher pH. The cis state has been suggested as being primarily responsible for the observed far-red shift of the emission maximum of Katushka relative to that of eqFP578f.

Pletneva, Nadya V.; Pletnev, Vladimir Z.; Shemiakina, Irina I.; Chudakov, Dmitriy M.; Artemyev, Igor; Wlodawer, Alexander; Dauter, Zbigniew; Pletnev, Sergei (Russ. Acad. Sci.); (SAIC); (NCI)

2012-08-10T23:59:59.000Z

425

On red snapper caught by the Galveston, Texas headboat fishery: movement, population characteristics, and productivity  

E-Print Network [OSTI]

, and Port Isabel, Texas showed marked juvenescence in the Galveston catches. Adjustment for seasonal bias removed some, but nct all of this trenc . These findings were used to motivate a Ricker year-class yield model of the Galveston headboat fishery... of headboat catches of red snapper from Port Aransas, Texas, 1979-1981. . 11 Age-class frequency histograms of headboat catches of red snapper from Port Isabel, Texas, 1979-1981. . . . . . 46 12 Age-class f'requency histograms for summer, 1979. . . . . 54...

MacDonald, Ian R

1983-01-01T23:59:59.000Z

426

Red Hat Enterprise Virtualization - KVM-based infrastructure services at BNL  

SciTech Connect (OSTI)

Over the past 18 months, BNL has moved a large percentage of its Linux-based servers and services into a Red Hat Enterprise Virtualization (RHEV) environment. This presentation will address our approach to virtualization, critical decision points, and a discussion of our implementation. Specific topics will include an overview of hardware and software requirements, networking, and storage; discussion of the decision of Red Hat solution over competing products (VMWare, Xen, etc); details on some of the features of RHEV - both current and on their roadmap; Review of performance and reliability gains since deployment completion; path forward for RHEV at BNL and caveats and potential problems.

Cortijo, D.

2011-06-14T23:59:59.000Z

427

The universal red-giant oscillation pattern; an automated determination with CoRoT data  

E-Print Network [OSTI]

The CoRoT and Kepler satellites have provided thousands of red-giant oscillation spectra. The analysis of these spectra requires efficient methods for identifying all eigenmode parameters. The assumption of new scaling laws allows us to construct a theoretical oscillation pattern. We then obtain a highly precise determination of the large separation by correlating the observed patterns with this reference. We demonstrate that this pattern is universal and are able to unambiguously assign the eigenmode radial orders and angular degrees. This solves one of the current outstanding problems of asteroseismology hence allowing precise theoretical investigation of red-giant interiors.

Mosser, B; Goupil, M J; Michel, E; Elsworth, Y; Barban, C; Kallinger, T; Hekker, S; DeRidder, J; Samadi, R; Baudin, F; Pinheiro, F J G; Auvergne, M; Baglin, A; Catala, C

2010-01-01T23:59:59.000Z

428

A protein electrophoretic analysis of population structure in the red drum (Sciaenops ocellatus)  

E-Print Network [OSTI]

. Wright's FST values over all polymorphic loci ranged from 0. 009 to 0. 027 (mean FST = 0. 023), and estimates of the effective number of migrants (N m) per generation ranged from 9. 0 to 27. 5. Estimates of e Nei's genetic distance between pairs... Flow In The Red Drum . . . 34 FIGURE 5. UPGNA Cluster Analysis Of Nei's (1978) Genetic Distance (D) Values Of All Fourteen Red Drum Samples , 36 INTRODUCTION Th d d (~S' ll j p and commercial species in the Gulf of Mexico and the Southeastern...

Bohlmeyer, Dwight Alan

1989-01-01T23:59:59.000Z

429

A Random Walk through Star and Planet Formation  

E-Print Network [OSTI]

and its Neptune-Mass Planet 3.1 Introduction . . . . . . .of Low Mass Star Formation . . . . . 1.3 Planet FormationConstraining Theories of Planet Formation and Evolution .

Maness, Holly

2010-01-01T23:59:59.000Z

430

Zonal Flow as Pattern Formation  

E-Print Network [OSTI]

In this section, we examine the transition from statistically homogeneous turbulence to inhomogeneous turbulence with zonal flows. Statistical equations of motion can be derived from the quasilinear approximation to the Hasegawa-Mima equation. We review recent work that finds a bifurcation of these equations and shows that the emergence of zonal flows mathematically follows a standard type of pattern formation. We also show that the dispersion relation of modulational instability can be extracted from the statistical equations of motion in a certain limit. The statistical formulation can thus be thought to offer a more general perspective on growth of coherent structures, namely through instability of a full turbulent spectrum. Finally, we offer a physical perspective on the growth of large-scale structures.

Parker, Jeffrey B

2015-01-01T23:59:59.000Z

431

The dynamics of fragment formation  

SciTech Connect (OSTI)

We demonstrate that in the Quantum Molecular Dynamics model, dynamical correlations can result in the production rate for final state nucleon clusters (and hence composite fragments) being higher than would be expected if statistics and the available phase space were dominant in determining composite formation. An intranuclear cascade or a Boltzmann-Uehling-Uhlenbeck model, combined with a statistical approach in the late stage of the collision to determine composites, provides an equivalent description only under limited conditions of centrality and beam energy. We use data on participant fragment production in Au + Au collisions in the Bevalac`s BOS time projection chamber to map out the parameter space where statistical clustering provides a good description. In particular, we investigate momentum-space densities of fragments up to {sup 4}He as a function of fragment transverse momentum, azimuth relative to the reaction plane, rapidity, multiplicity and beam energy.

Keane, D. [Kent State Univ., OH (United States); EOS Collaboration

1994-09-01T23:59:59.000Z

432

Adaptive Optics in Star Formation  

E-Print Network [OSTI]

Over the past ten years, the concept of adaptive optics has evolved from early experimental stages to a standard observing tool now available at almost all major optical and near-infrared telescope facilities. Adaptive optics will also be essential in exploiting the full potential of the large optical/infrared interferometers currently under construction. Both observations with high-angular resolution and at high contrast, and with a high point source sensitivity are facilitated by adaptive optics. Among the areas which benefit most from the use of adaptive optics are studies of the circumstellar environment (envelopes, disks, outflows), substellar companions and multiple systems, and dense young stellar populations. This contribution highlights some of the recent advances in star formation studies facilitated by adaptive optics, and gives a brief tutorial on optimized observing and data reduction strategies.

Wolfgang Brandner

2003-09-29T23:59:59.000Z

433

Electrochemical formation of field emitters  

DOE Patents [OSTI]

Electrochemical formation of field emitters, particularly useful in the fabrication of flat panel displays is disclosed. The fabrication involves field emitting points in a gated field emitter structure. Metal field emitters are formed by electroplating and the shape of the formed emitter is controlled by the potential imposed on the gate as well as on a separate counter electrode. This allows sharp emitters to be formed in a more inexpensive and manufacturable process than vacuum deposition processes used at present. The fabrication process involves etching of the gate metal and the dielectric layer down to the resistor layer, and then electroplating the etched area and forming an electroplated emitter point in the etched area. 12 figs.

Bernhardt, A.F.

1999-03-16T23:59:59.000Z

434

Cobalt-iron red-ox behavior in nanostructured La{sub 0.4}Sr{sub 0.6}Co{sub 0.8}Fe{sub 0.2}O{sub 3-{delta}} cathodes  

SciTech Connect (OSTI)

Nano-sized La{sub 0.4}Sr{sub 0.6}Co{sub 0.8}Fe{sub 0.2}O{sub 3-{delta}} (LSCF) perovskite samples (prepared by a conventional acetate route and a novel acetate synthesis with HMTA additives), were tested simulating a red-ox cycle. The crystallography was studied by X-ray Powder Diffraction (XPD) and the changes in the oxidation state of the perovskite B-site were evaluated by synchrotron X-ray Absorption Near Edge Spectroscopy (XANES). After a reducing treatment, LSFC particles show the appearance of a new phase that coexists with the original one. The structural change is accompanied by a Co and Fe formal oxidation states decrease, although Fe remains always closer to 4+ and Co closer to 3+. The treatment produces a B-site valence average reduction from 3.52+ to 3.26+ and the formation of oxygen vacancies. A re-oxidation treatment under O{sub 2} rich atmosphere at 800 Degree-Sign C for 10 h shows that the change is reversible and independent of the two chemical methods used to synthesize the LSCF nano-particles. - Graphical abstract: XANES and XPD measurements in nanostructured LSCF before (black) and after (red/green) a red/ox cycle. Highlights: Black-Right-Pointing-Pointer Red-ox treatments in LSCF nano-particles cause a reversible reaction. Black-Right-Pointing-Pointer XPD analyses show that a new 'reduced' phase coexist with the oxidize one. Black-Right-Pointing-Pointer The B-site formal oxidation state decreases and the {delta} increases upon reduction. Black-Right-Pointing-Pointer Fe remains in a higher valence (closer to 4+) than Co (close to 3+). Black-Right-Pointing-Pointer The behavior seems to be independent of the synthesis method used.

Soldati, Analia L., E-mail: asoldati@cab.cnea.gov.ar [CONICET-CNEA Departamento de Caracterizacion de Materiales, Centro Atomico Bariloche, Av. Bustillo 9500, S.C. de Bariloche R8402AGP, Rio Negro (Argentina); Baque, Laura, E-mail: baque.laura@gmail.com [CONICET-CNEA Departamento de Caracterizacion de Materiales, Centro Atomico Bariloche, Av. Bustillo 9500, S.C. de Bariloche R8402AGP, Rio Negro (Argentina)] [CONICET-CNEA Departamento de Caracterizacion de Materiales, Centro Atomico Bariloche, Av. Bustillo 9500, S.C. de Bariloche R8402AGP, Rio Negro (Argentina); Napolitano, Federico, E-mail: napolitf@ib.cab.cnea.gov.ar [CONICET-CNEA Departamento de Caracterizacion de Materiales, Centro Atomico Bariloche, Av. Bustillo 9500, S.C. de Bariloche R8402AGP, Rio Negro (Argentina)] [CONICET-CNEA Departamento de Caracterizacion de Materiales, Centro Atomico Bariloche, Av. Bustillo 9500, S.C. de Bariloche R8402AGP, Rio Negro (Argentina); Serquis, Adriana, E-mail: aserquis@cab.cnea.gov.ar [CONICET-CNEA Departamento de Caracterizacion de Materiales, Centro Atomico Bariloche, Av. Bustillo 9500, S.C. de Bariloche R8402AGP, Rio Negro (Argentina)] [CONICET-CNEA Departamento de Caracterizacion de Materiales, Centro Atomico Bariloche, Av. Bustillo 9500, S.C. de Bariloche R8402AGP, Rio Negro (Argentina)

2013-02-15T23:59:59.000Z

435

Method and kit for the selective labeling of red blood cells in whole blood with TC-99M  

DOE Patents [OSTI]

Disclosed herein are a method and kit for the preparation of .sup.99m Tc labeled red blood cells using whole blood in a closed sterile system containing stannous tin in a form such that it will enter the red blood cells and be available therein for the reduction of technetium.

Srivastava, Suresh C. (Setauket, NY); Babich, John W. (Redhill, GB2); Straub, Rita (Brookhaven, NY); Richards, Powell (New Bern, NC)

1988-01-01T23:59:59.000Z

436

Method and kit for the selective labeling of red blood cells in whole blood with Tc-99m  

DOE Patents [OSTI]

Disclosed herein are a method and kit for the preparation of [sup 99m]Tc labeled red blood cells using whole blood in a closed sterile system containing stannous tin in a form such that it will enter the red blood cells and be available for the reduction of technetium. No Drawings

Srivastava, S.C.; Babich, J.W.; Straub, R.; Richards, P.

1988-07-05T23:59:59.000Z

437

Detecting Moving Objects in Airborne Forward Looking InfraRed Sequences Alexander Strehl and J. K. Aggarwal \\Lambda  

E-Print Network [OSTI]

looking infra­red (FLIR) image sequences taken from an airborne, moving platform. Ego­motion effects classification system. 1 Introduction 1.1 Motivation Forward looking infra­red (FLIR) images are frequently used static FLIR images. A comprehensive recent review by Ratches, Wal­ \\Lambda This research was supported

Strehl, Alexander

438

Detecting Moving Objects in Airborne Forward Looking Infra-Red Sequences Alexander Strehl and J. K. Aggarwal  

E-Print Network [OSTI]

-red (FLIR) image sequences taken from an airborne, moving platform. Ego-motion effects are removed through system. 1 Introduction 1.1 Motivation Forward looking infra-red (FLIR) images are frequently used static FLIR images. A comprehensive recent review by Ratches, Wal- £ This research was supported in part

Strehl, Alexander

439

Host-defense peptides isolated from the skin secretions of the Northern red-legged frog Rana aurora aurora  

E-Print Network [OSTI]

Host-defense peptides isolated from the skin secretions of the Northern red-legged frog Rana aurora aurora J. Michael Conlona,*, Agnes Sonnevendb , Carlos Davidsonc , Anni Demandtd , Thierry Jouennee-stimulated skin secretions of the Northern red-legged frog Rana aurora aurora and their primary structures

Davidson, Carlos

440

Evidence from peptidomic analysis of skin secretions that the red-legged frogs, Rana aurora draytonii and  

E-Print Network [OSTI]

Evidence from peptidomic analysis of skin secretions that the red-legged frogs, Rana aurora draytonii and Rana aurora aurora, are distinct species J. Michael Conlon a, *, Nadia Al-Ghafari a , Laurent peptides Rana aurora Rana draytonii Skin secretions a b s t r a c t The northern red-legged frog Rana

Davidson, Carlos

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


441

Red, Green and Blue Silicate Phosphor Thin Films by Pulsed Laser X. W. Sun and H. S. Kwok  

E-Print Network [OSTI]

Red, Green and Blue Silicate Phosphor Thin Films by Pulsed Laser Deposition X. W. Sun and H. S University of Science and Technology Clear Water Bay, Kowloon, Hong Kong Abstract Three kinds of silicate deposition: manganese and lead doped calcium silicate (CaSiO3:MnPb) for red color, manganese doped zinc

442

RED-BL: Energy Solution for Loading Data Centers Muhammad Saqib Ilyas  

E-Print Network [OSTI]

@lums.edu.pk Saqib Raza Cisco Systems sraza@ucdavis.edu Chao-Chih Chen UC, Davis cchchen@ucdavis.edu Zartash Afzal Uzmi SSE, LUMS zartash@lums.edu.pk Chen-Nee Chuah UC, Davis chuah@ucdavis.edu AbstractRED-BL: Energy Solution for Loading Data Centers Muhammad Saqib Ilyas SSE, LUMS saqibm

Chuah, Chen-Nee

443

SSSEALEDEALEDEALED TTTUBEUBEUBE VVVIRTUALIRTUALIRTUAL CCCATHODEATHODEATHODE OOOSCILLATORSCILLATORSCILLATOR DDDRIVENRIVENRIVEN BYBYBY AAA CCCOMPACTOMPACTOMPACT MMMARXARXARX GGGENERATORENERATORENERATOR Texas Tech Red Raiders  

E-Print Network [OSTI]

Power Processing, High Power Solid State Lasers and Power Electronics, Explosive Pulsed Power and Micro;Texas Tech Red Raiders The Center for Pulsed Power and Power Electronics The Plasma, Power Electronics, and Pulsed Power Group at Texas Tech consists of eight faculty members, with a wide range of expertise, from

Gelfond, Michael

444

Improving the photostability of bright monomeric orange and red fluorescent proteins  

E-Print Network [OSTI]

Improving the photostability of bright monomeric orange and red fluorescent proteins Nathan C illumination. Although fluorescent proteins typically bleach at a substantially slower rate than many small-molecule dyes, in many cases the lack of sufficient photostability remains an important limiting factor

Tsien, Roger Y.

445

A ``Short'' Distance to the Large Magellanic Cloud With the Hipparcos Calibrated Red Clump Stars  

E-Print Network [OSTI]

Following an approach developed by Paczy\\'nski & Stanek, we derive a distance to the Large Magellanic Cloud (LMC) by comparing red clump stars from the Hipparcos catalog with the red clump stars observed in two fields in the LMC that were selected from the ongoing photometric survey of the Magellanic Clouds to lie in low extinction regions. The use of red clump stars allows a single step determination of the distance modulus to the LMC, $\\mu_{0,LMC} = 18.065\\pm 0.031\\pm 0.09 $mag (statistical plus systematic error), and the corresponding distance, $R_{LMC}= 41.02\\pm 0.59\\pm 1.74 kpc$. This measurement is in excellent agreement with the recent determination by Udalski et al., also based on the red clump stars, but is $\\sim 0.4 $mag smaller than the generally accepted value of $\\mu_{0,LMC} = 18.50\\pm 0.15 $mag. We discuss possible reasons for this discrepancy and how it can be resolved.

K. Z. Stanek; D. Zaritsky; J. Harris

1998-03-16T23:59:59.000Z

446

Minimal RED Cell Pairs Markedly Improve Electrode Kinetics and Power Production in Microbial Reverse Electrodialysis Cells  

E-Print Network [OSTI]

Reverse Electrodialysis Cells Roland D. Cusick,,§ Marta Hatzell, Fang Zhang, and Bruce E. Logan ABSTRACT: Power production from microbial reverse electrodialysis cell (MRC) electrodes is substantially electrodes used in a microbial fuel cell (MFC) are placed on each side of a reverse electrodialysis (RED

447

Impact of the red imported fire ant on newly hatched northern bobwhite  

E-Print Network [OSTI]

The response of northern bobwhite (Colinus virginianus) to the presence of red imported fire ants (Solenopsis invicta) during the first 6 days post-hatching was examined in a 9-week-field experiment during spring and summer 1993 in southeastern...

Pedersen, Elena Kalleso

2012-06-07T23:59:59.000Z

448

RED: a Rich Epinions Dataset for Recommender Systems Simon Meyffret1,2  

E-Print Network [OSTI]

RED: a Rich Epinions Dataset for Recommender Systems Simon Meyffret1,2 , Emmanuel Guillot1}@liris.cnrs.fr ABSTRACT Recommender Systems require specific datasets to evaluate their approach. They do not require is not gathered in today datasets. In this paper, we provide a dataset containing reviews from users on items

Paris-Sud XI, Université de

449

Red Algae Respond to Waves: Morphological and Mechanical Variation in Mastocarpus papillatus Along  

E-Print Network [OSTI]

Red Algae Respond to Waves: Morphological and Mechanical Variation in Mastocarpus papillatus Along Grove, California, 93950 Abstract. Intertidal algae are exposed to the potentially severe drag forces generated by crashing waves, and several species of brown algae respond, in part, by varying the strength

Denny, Mark

450

Infra-red detector and method of making and using same  

DOE Patents [OSTI]

A low-cost infra-red detector is disclosed including a method of making and using the same. The detector employs a substrate, a filtering layer, a converting layer, and a diverter to be responsive to wavelengths up to about 1600 nm. The detector is useful for a variety of applications including spectroscopy, imaging, and defect detection.

Craig, Richard A. (Richland, WA); Griffin, Jeffrey W. (Kennewick, WA)

2007-02-20T23:59:59.000Z

451

Effect of Combining Far-Red Light with Shorter Wave Light on the Excitation of Fluorescence  

E-Print Network [OSTI]

of Fluorescence in Chlorella Recent experiments on the rate of photosyn- thesis in far-red light alone that the quantum yield of Auo- rescence in Chlorella drops when excitation is achieved by light above 680 ml* (10- teen experiments of this type are summarized in Table I. Chlorella pyrenoidosa Strain 3 were used

Govindjee

452

Intense red upconversion luminescence from Tm3Yb3 codoped transparent glass ceramic  

E-Print Network [OSTI]

choose the oxyfluoride glass ceramic as the host material in our investigations. Through thermal treatIntense red upconversion luminescence from Tm3Yb3 codoped transparent glass ceramic Wei Xu,1 (Doc. ID 158093); published January 12, 2012 Tm3Yb3 codoped transparent glass ceramic containing -PbF2

Cao, Wenwu

453

Status of the Red Knot (Calidris Canutus Rufa) in the Western Hemisphere  

E-Print Network [OSTI]

... Avian Biology Abstract The population of the rufa subspecies of the Red Knot (Calidris canutus), which breeds in the ... grounds and ensure their survival after they arrive at a time when food availability is often low. The crucial importance of Delaware ...

454

Stridulatory organ morphology, acoustics, and function in the red imported fire ant  

E-Print Network [OSTI]

occurrence, usually happening on warm days following a rain. Pest status. The red imported fire ant, Solenopsis invicta Buren, is believed to be a native of the Brazilian Pantanal, one of the largest flood plains in the world. The highly disturbed nature...

Rauth, Steven Joseph

2001-01-01T23:59:59.000Z

455

On Bitcoin and Red Balloons Moshe Babaioff, Microsoft Research, Silicon Valley  

E-Print Network [OSTI]

On Bitcoin and Red Balloons Moshe Babaioff, Microsoft Research, Silicon Valley Shahar Dobzinski balloons). We focus on another prominent example: Bitcoin, a decentralized electronic currency system. Bitcoin represents a radical new approach to monetary systems. It has been getting a large amount

Fiat, Amos

456

Red Fluorescent Protein pH Biosensor to Detect Concentrative Nucleoside Transport*S  

E-Print Network [OSTI]

Red Fluorescent Protein pH Biosensor to Detect Concentrative Nucleoside Transport*S Received concentrative nucleoside transporter, hCNT3, medi- ates Na /nucleoside and H /nucleoside co-transport. We describe a new approach to monitor H /uridine co-transport in cultured mammalian cells, using a p

Campbell, Robert E.

457

Red Sea during the Last Glacial Maximum: Implications for sea level reconstruction  

E-Print Network [OSTI]

. Gildor,1 and W. R. Peltier2 Received 13 February 2007; revised 29 July 2007; accepted 30 October 2007 based on the ICE-5G (VM2) model. Citation: Biton, E., H. Gildor, and W. R. Peltier (2008), Red Sea sea level reduction for the LGM interval range between approximately 120 m [Peltier, 2004, 2002

Peltier, W. Richard

458

Unveiling the nature of red novae cool explosions using archive plate photometry  

E-Print Network [OSTI]

Based on archive photographic photometry and recent CCD photometric data for red novae V4332 Sgr and V838 Mon, we established their stellar composition, exploded components, and the nature of explosions. Low temperature in the outburst maximum is due to quasi-adiabatic expansion of a massive stellar envelope after the central energy surge preceded the outburst.

Goranskij, Vitaly; Zharova, Alla; Shugarov, Sergei; Barsukova, Elena; Kroll, Peter

2015-01-01T23:59:59.000Z

459

MULTI-EPOCH OBSERVATIONS OF THE RED WING EXCESS IN THE SPECTRUM OF 3C 279  

SciTech Connect (OSTI)

It has been previously determined that there is a highly significant correlation between the spectral index from 10 GHz to 1350 A and the amount of excess luminosity in the red wing of quasar C IV {lambda}1549 broad emission lines (BELs). Ostensibly, the prominence of the red excess is associated with the radio jet emission mechanism and is most pronounced for lines of sight close to the jet axis. Studying the scant significant differences in the UV spectra of radio-loud and radio-quiet quasars might provide vital clues to the origin of the unknown process that creates powerful relativistic jets that appear in only about 10% of quasars. In this study, the phenomenon is explored with multi-epoch observations of the Mg II {lambda}2798 broad line in 3C 279 which has one of the largest known red wing excesses in a quasar spectrum. The amount of excess that is detected appears to be independent of all directly observed optical continuum, radio, or submillimeter properties (fluxes or polarizations). The only trend that occurs in this sparse data is: the stronger the BEL, the larger the fraction of flux that resides in the red wing. It is concluded that more monitoring is needed and spectropolarimetry with a large telescope is essential during low states to understand more.

Punsly, Brian, E-mail: brian.punsly@verizon.net, E-mail: brian.punsly@comdev-usa.com [1415 Granvia Altamira, Palos Verdes Estates, CA 90274 (United States); ICRANet, Piazza della Repubblica 10, I-65100 Pescara (Italy)

2013-01-10T23:59:59.000Z

460

Energy agencies appear to be on safe ground, avoiding California's high tide of red ink.  

E-Print Network [OSTI]

Commission. Energy is a multi-billion dollar industry. Its regulating agen- cies are funded largely to explore solar offsets.................................. 8 Commodities regulators open unusual publicEnergy agencies appear to be on safe ground, avoiding California's high tide of red ink

Kammen, Daniel M.

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


461

Radio Triggered Star Formation in Cooling Flows  

E-Print Network [OSTI]

The giant galaxies located at the centers of cluster cooling flows are frequently sites of vigorous star formation. In some instances, star formation appears to have been triggered by the galaxy's radio source. The colors and spectral indices of the young populations are generally consistent with short duration bursts or continuous star formation for durations much less than 1 Gyr, which is less than the presumed ages of cooling flows. The star formation properties are inconsistent with fueling by a continuously accreting cooling flow, although the prevalence of star formation is consistent with repeated bursts and periodic refueling. Star formation may be fueled, in some cases, by cold material stripped from neighboring cluster galaxies.

B. R. McNamara

1999-11-08T23:59:59.000Z

462

THE DEEP2 GALAXY REDSHIFT SURVEY: CLUSTERING DEPENDENCE ON GALAXY STELLAR MASS AND STAR FORMATION RATE AT z {approx} 1  

SciTech Connect (OSTI)

We present DEEP2 galaxy clustering measurements at z {approx} 1 as a function of stellar mass, star formation rate (SFR), and specific SFR (sSFR). We find a strong positive correlation between stellar mass and clustering amplitude on 1-10 h {sup -1} Mpc scales for blue, star-forming galaxies with 9.5 < log(M{sub *}/M{sub Sun }) < 11 and no dependence for red, quiescent galaxies with 10.5 < log(M{sub *}/M{sub Sun }) < 11.5. Using recently re-calibrated DEEP2 SFRs from restframe B-band magnitude and optical colors, we find that within the blue galaxy population at z {approx} 1 the clustering amplitude increases strongly with increasing SFR and decreasing sSFR. For red galaxies there is no significant correlation between clustering amplitude and either SFR or sSFR. Blue galaxies with high SFR or low sSFR are as clustered on large scales as red galaxies. We find that the clustering trend observed with SFR can be explained mostly, but not entirely, by the correlation between stellar mass and clustering amplitude for blue galaxies. We also show that galaxies above the star-forming 'main sequence' are less clustered than galaxies below the main sequence, at a given stellar mass. These results are not consistent with the high-sSFR population being dominated by major mergers. We also measure the clustering amplitude on small scales ({<=}0.3 h {sup -1} Mpc) and find an enhanced clustering signal relative to the best-fit large-scale power law for red galaxies with high stellar mass, blue galaxies with high SFR, and both red and blue galaxies with high sSFR. The increased small-scale clustering for galaxies with high sSFRs is likely linked to triggered star formation in interacting galaxies. These measurements provide strong constraints on galaxy evolution and halo occupation distribution models at z {approx} 1.

Mostek, Nick [Space Sciences Laboratory, University of California, Berkeley, CA 94720 (United States)] [Space Sciences Laboratory, University of California, Berkeley, CA 94720 (United States); Coil, Alison L. [Center for Astrophysics and Space Sciences, University of California, San Diego, La Jolla, CA 92093 (United States)] [Center for Astrophysics and Space Sciences, University of California, San Diego, La Jolla, CA 92093 (United States); Cooper, Michael [Center for Galaxy Evolution, Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States)] [Center for Galaxy Evolution, Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States); Davis, Marc [Department of Astronomy, University of California at Berkeley, Berkeley, CA 94720 (United States)] [Department of Astronomy, University of California at Berkeley, Berkeley, CA 94720 (United States); Newman, Jeffrey A. [Department of Physics and Astronomy and PITT-PACC, University of Pittsburgh, Pittsburgh, PA 15620 (United States)] [Department of Physics and Astronomy and PITT-PACC, University of Pittsburgh, Pittsburgh, PA 15620 (United States); Weiner, Benjamin J., E-mail: njmostek@lbl.gov [Steward Observatory, Department of Astronomy, University of Arizona, Tucson, AZ 85721 (United States)

2013-04-10T23:59:59.000Z

463

Hot Coal for Christmas: Dust Formation in the Swept-Up Shell Around The Peculiar Type Ib Supernova 2006jc  

E-Print Network [OSTI]

We present evidence for the formation of dust grains in an unusual Type Ib SN based on late-time spectra of SN 2006jc. The progenitor suffered a giant outburst qualitatively similar to those seen in LBVs just 2 years prior to the SN, and we speculate that the dust formation we observe is an indirect consequence of that event. The key evidence for dust formation seen in our optical spectra is (1) the appearance of a strong continuum emission source at red wavelengths, and (2) fading of the redshifted sides of narrow HeI emission lines. These two observed characteristics provide the strongest case yet for dust formation in any Type Ib/c SN. Both developments occurred simultaneously between 51 and 75 days after peak brightness, which is quick compared to other dusty SNe. The high temperature of the dust implies carbon and not silicates, and we describe how infrared photometry may test this conjecture. Geometric considerations indicate dust formation occurring in the dense gas swept-up by the forward shock, and n...

Smith, Nathan; Filippenko, Alexei V

2007-01-01T23:59:59.000Z

464

A seismic approach to testing different formation channels of subdwarf B stars  

E-Print Network [OSTI]

There are many unknowns in the formation of subdwarf B stars. Different formation channels are considered to be possible and to lead to a variety of helium-burning subdwarfs. All seismic models to date, however, assume that a subdwarf B star is a post-helium-flash-core surrounded by a thin inert layer of hydrogen. We examine an alternative formation channel, in which the subdwarf B star originates from a massive (>~2 Msun) red giant with a non-degenerate helium-core. Although these subdwarfs may evolve through the same region of the log g-Teff diagram as the canonical post-flash subdwarfs, their interior structure is rather different. We examine how this difference affects their pulsation modes and whether it can be observed. Using detailed stellar evolution calculations we construct subdwarf B models from both formation channels. The iron accumulation in the driving region due to diffusion, which causes the excitation of the modes, is approximated by a Gaussian function. The pulsation modes and frequencies are calculated with a non-adiabatic pulsation code. A detailed comparison of two subdwarf B models from different channels, but with the same log g and Teff, shows that their mode excitation is different. The excited frequencies are lower for the post-flash than for the post-non-degenerate subdwarf B star. This is mainly due to the differing chemical composition of the stellar envelope. A more general comparison between two grids of models shows that the excited frequencies of most post-non-degenerate subdwarfs cannot be well-matched with the frequencies of post-flash subdwarfs. In the rare event that an acceptable seismic match is found, additional information, such as mode identification and log g and Teff determinations, allows us to distinguish between the two formation channels.

Haili Hu; M. -A. Dupret; C. Aerts; G. Nelemans; S. D. Kawaler; A. Miglio; J. Montalban; R. Scuflaire

2008-08-22T23:59:59.000Z

465

Floating insulated conductors for heating subsurface formations  

DOE Patents [OSTI]

A heating system for a subsurface formation includes a conduit located in a first opening in the subsurface formation. Three electrical conductors are located in the conduit. A return conductor is located inside the conduit. The return conductor is electrically coupled to the ends of the electrical conductors distal from the surface of the formation. Insulation is located inside the conduit. The insulation electrically insulates the three electrical conductors, the return conductor, and the conduit from each other.

Burns, David; Goodwin, Charles R.

2014-07-29T23:59:59.000Z

466

Theoretical Investigations on the Formation and Dehydrogenation...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

of boron-nitrogen-hydrogen (BNHx) compounds that are promising materials for chemical hydrogen storage. Understanding the kinetics and reaction pathways of formation of these...

467

Heating systems for heating subsurface formations  

DOE Patents [OSTI]

Methods and systems for heating a subsurface formation are described herein. A heating system for a subsurface formation includes a sealed conduit positioned in an opening in the formation and a heat source. The sealed conduit includes a heat transfer fluid. The heat source provides heat to a portion of the sealed conduit to change phase of the heat transfer fluid from a liquid to a vapor. The vapor in the sealed conduit rises in the sealed conduit, condenses to transfer heat to the formation and returns to the conduit portion as a liquid.

Nguyen, Scott Vinh (Houston, TX); Vinegar, Harold J. (Bellaire, TX)

2011-04-26T23:59:59.000Z

468

Threshold displacement energies and defect formation energies...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

energies and defect formation energies in Y2Ti2O7. Abstract: Ab initio molecular dynamics simulations have been carried out to determine both the threshold displacement...

469

Heating tar sands formations to visbreaking temperatures  

DOE Patents [OSTI]

Methods for treating a tar sands formation are described herein. Methods may include heating at least a section of a hydrocarbon layer in the formation from a plurality of heaters located in the formation. The heat may be controlled so that at least a majority of the section reaches an average temperature of between 200.degree. C. and 240.degree. C., which results in visbreaking of at least some hydrocarbons in the section. At least some visbroken hydrocarbon fluids may be produced from the formation.

Karanikas, John Michael (Houston, TX); Colmenares, Tulio Rafael (Houston, TX); Zhang, Etuan (Houston, TX); Marino, Marian (Houston, TX); Roes, Augustinus Wilhelmus Maria (Houston, TX); Ryan, Robert Charles (Houston, TX); Beer, Gary Lee (Houston, TX); Dombrowski, Robert James (Houston, TX); Jaiswal, Namit (Houston, TX)

2009-12-22T23:59:59.000Z

470

Nonequilibrium Atmospheric Secondary Organic Aerosol Formation...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Aerosol Formation and Growth. Abstract: Airborne particles play a critical role in air quality, human health effects, visibility and climate. Secondary organic aerosols (SOA)...

471

Standard Format and Content for Emergency Plans  

Broader source: Directives, Delegations, and Requirements [Office of Management (MA)]

This volume addresses recommended emergency plan format and content for Operational Emergency Base Programs and Operational Emergency Hazardous Material Programs. Canceled by DOE G 151.1-3.

1997-08-21T23:59:59.000Z

472

Hydrogen Adsorption Induces Interlayer Carbon Bond Formation...  

Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

Hydrogen Adsorption Induces Interlayer Carbon Bond Formation in Supported Few-Layer Graphene Friday, February 28, 2014 Among the allotropes of carbon, diamond has some of the most...

473

On the Formation of Galaxy Halos: Comparing NGC 5128 and the Local Group Members  

E-Print Network [OSTI]

The metallicity distribution function (MDF) for the old red-giant stars in the halo of NGC 5128, the nearest giant elliptical galaxy, is virtually identical with the MDF for the old-disk stars in the LMC and also strongly resembles the halo MDF in M31. These galaxies all have high mean halo metallicities ( ~ -0.4$) with very small proportions of low-metallicity stars. These observations reinforce the view that metal-rich halos are quite normal for large galaxies of all types. Such systems are unlikely to have built up by accretion of pre-existing, gas-free small satellite galaxies, unless these satellites had an extremely shallow mass distribution (d log N / d log M > -1). We suggest that the halo of NGC 5128 is more likely to have assembled from hierarchical merging of gas-rich lumps in which the bulk of star formation took place during or after the merger stage.

W. E. Harris; G. L. H. Harris

2001-08-14T23:59:59.000Z

474

13 Red-Black Trees Chapter 12 showed that a binary search tree of height h can support any of the basic  

E-Print Network [OSTI]

13 Red-Black Trees Chapter 12 showed that a binary search tree of height h can support any height is large, however, the set operations may run no faster than with a linked list. Red-black trees-set operations take O.lg n/ time in the worst case. 13.1 Properties of red-black trees A red-black tree

475

Formation of $??$ atoms in $K_{?4} decay  

E-Print Network [OSTI]

We derive the decay rate of $\\pi\\mu$ atom formation in $K_{\\mu 4}$ decay. Using the obtained expressions we calculate the decay rate of atom formation and point out that considered decay can give a noticeable contribution as a background to the fundamental decay $K^+\\to \\pi^+\

S. R. Gevorkyan; A. V. Tarasov; O. O. Voskresenskaya

2009-12-01T23:59:59.000Z

476

Methods for forming wellbores in heated formations  

DOE Patents [OSTI]

A method for forming a wellbore in a heated formation includes flowing liquid cooling fluid to a bottom hole assembly in a wellbore in a heated formation. At least a portion of the liquid cooling fluid is vaporized at or near a region to be cooled. Vaporizing the liquid cooling fluid absorbs heat from the region to be cooled.

Guimerans, Rosalvina Ramona; Mansure, Arthur James

2012-09-25T23:59:59.000Z

477

DISSERTATION FORMATION OF THE HURRICANE EYE  

E-Print Network [OSTI]

DISSERTATION FORMATION OF THE HURRICANE EYE Submitted by Jonathan L. Vigh Department of Atmospheric OF THE HURRICANE EYE BE ACCEPTED AS FULFILLING IN PART REQUIREMENTS FOR THE DEGREE OF DOCTOR OF PHILOSOPHY. Schubert Department Head: Richard H. Johnson ii #12;ABSTRACT OF DISSERTATION FORMATION OF THE HURRICANE EYE

Schubert, Wayne H.

478

Shell Formation and Bone Strength Laying Hens  

E-Print Network [OSTI]

Shell Formation and Bone Strength in Laying Hens Effects of Age, Daidzein and Exogenous Estrogen Cover aquarelle: E. Spörndly-Nees #12;Shell Formation and Bone Strength in Laying Hens Effects of Age eggshells as shell quality declines with age during the laying period. This is a concern for food safety

479

Le logiciel "Tigre" en formation PLC 1 Grtice J. Vincent Le logiciel Tigre en formation PLC  

E-Print Network [OSTI]

"Tigre" en formation PLC 1 Grétice J. Vincent Le logiciel « Tigre » en formation PLC J. Vincent Le;______________________________________________________________________________________ Le logiciel "Tigre" en formation PLC 2 Grétice J. Vincent 1.1. La lecture Voici l'écran d;______________________________________________________________________________________ Le logiciel "Tigre" en formation PLC 3 Grétice J. Vincent Figure 3 1.2. La démonstration Voici l

Paris-Sud XI, Université de

480

Sequentially Triggered Star Formation in OB Associations  

E-Print Network [OSTI]

We discuss observational evidence for sequential and triggered star formation in OB associations. We first review the star formation process in the Scorpius-Centaurus OB association, the nearest OB association to the Sun, where several recent extensive studies have allowed us to reconstruct the star formation history in a rather detailed way. We then compare the observational results with those obtained for other OB associations and with recent models of rapid cloud and star formation in the turbulent interstellar medium. We conclude that the formation of whole OB subgroups (each consisting of several thousand stars) requires large-scale triggering mechanisms such as shocks from expanding wind and supernova driven superbubbles surrounding older subgroups. Other triggering mechanisms, like radiatively driven implosion of globules, also operate, but seem to be secondary processes, forming only small stellar groups rather than whole OB subgroups with thousands of stars.

Thomas Preibisch; Hans Zinnecker

2006-10-27T23:59:59.000Z

Note: This page contains sample records for the topic "red italic format" from the National Library of EnergyBeta (NLEBeta).
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they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


481

In many ways, the red blood cells of non-mammalian vertebrates are very different from those of mammals. One of  

E-Print Network [OSTI]

In many ways, the red blood cells of non-mammalian vertebrates are very different from those of mammals. One of the most obvious differences is that non-mammalian red blood cells are nucleated whereas mammalian red blood cells extrude their nuclei before entering the circulation. In addition, these nucleated

Hawai'i at Manoa, University of

482

Dynamics of TCP/RED and a Scalable Control Steven H. Low Fernando Paganini Jiantao Wang Sachin Adlakha John C. Doyle  

E-Print Network [OSTI]

1 Dynamics of TCP/RED and a Scalable Control Steven H. Low Fernando Paganini Jiantao Wang Sachin is determined predominantly by the stability of TCP/RED, not by AIMD probing nor noise traffic. We develop a gen- eral multi-link multi-source model for TCP/RED and derive a local sta- bility condition in the case

Low, Steven H.

483

Getting simultaneous red and near-infrared band data from a single digital camera for plant monitoring applications: theoretical and practical study  

E-Print Network [OSTI]

Getting simultaneous red and near-infrared band data from a single digital camera for plant Abstract. Multispectral images, including red and near-infrared bands, have proved efficient for vegetation imaging devices. A methodology is proposed to obtain simultaneously the near-infrared and red bands from

Boyer, Edmond

484

Red-sequence galaxies with young stars and dust: The cluster Abell 901/902 seen with COMBO-17  

E-Print Network [OSTI]

We report the discovery of a rich component of dusty star-forming galaxies contaminating the red-sequence in the supercluster system comprising Abell 901a, 901b and A902 at redshift ~0.17. These galaxies do not fit into the colour-density relation, because their preferred habitat is different from that of regular red-sequence galaxies, which are typically dust-poor, old and passively evolving. The dusty red galaxies prefer the medium-density outskirts of clusters while being rare in both the low-density field and the high-density cluster cores. This new result is based on the information content in the medium-band photometry of the COMBO-17 survey. The photo-z accuracy of the ~800 brightest cluster galaxies is red colour of the dusty galaxies to be a result of dust extinction combined with relatively old stellar ages. We speculate that the dusty red galaxies could either be a product of minor mergers between established old red cluster galaxies with infalling blue field galaxies, or mark a period in the internal transformation of blue field galaxies into red cluster galaxies, which is triggered by the environmental influences experienced during cluster infall.

C. Wolf; M. E. Gray; K. Meisenheimer

2005-08-06T23:59:59.000Z

485

Infra-Red Surface-Plasmon-Resonance technique for biological studies  

E-Print Network [OSTI]

We report on a Surface-Plasmon-Resonance (SPR) technique based on Fourier -Transform - Infra - Red (FTIR) spectrometer. In contrast to the conventional surface plasmon technique, operating at a fixed wavelength and a variable angle of incidence, our setup allows the wavelength and the angle of incidence to be varied simultaneously. We explored the potential of the SPR technique in the infrared for biological studies involving aqueous solutions. Using computer simulations, we found the optimal combination of parameters (incident angle, wavelength) for performing this task. Our experiments with physiologically important glucose concentrations in water and in human plasma verified our computer simulations. Importantly, we demonstrated that the sensitivity of the SPR technique in the infrared range is not lower and in fact is even higher than that for visible light. We emphasize the advantages of infra red SPR for studying glucose and other biological molecules in living cells.

V. Lirtsman; M. Golosovsky; D. Davidov

2007-11-18T23:59:59.000Z

486

Development of an automated Red Light Violation Detection System (RLVDS) for Indian vehicles  

E-Print Network [OSTI]

Integrated Traffic Management Systems (ITMS) are now implemented in different cities in India to primarily address the concerns of road-safety and security. An automated Red Light Violation Detection System (RLVDS) is an integral part of the ITMS. In our present work we have designed and developed a complete system for generating the list of all stop-line violating vehicle images automatically from video snapshots of road-side surveillance cameras. The system first generates adaptive background images for each camera view, subtracts captured images from the corresponding background images and analyses potential occlusions over the stop-line in a traffic signal. Considering round-the-clock operations in a real-life test environment, the developed system could successfully track 92% images of vehicles with violations on the stop-line in a "Red" traffic signal.

Saha, Satadal; Nasipuri, Mita; Basu, Dipak Kumar

2010-01-01T23:59:59.000Z

487

OY Car During Normal Outburst: Balmer Emission From The Red Star And The Gas Stream  

E-Print Network [OSTI]

We present observations of OY Car, obtained with the Anglo-Australian Telescope, during a normal outburst in August 1991. Two sinusoidal components are resolved in the H$\\beta$ trailed spectra and we determine the location of the narrow component to be on the secondary star with a maximum contributed flux of ~2.5 per cent to the total flux. Imaging of the line distribution reveals that the other emission component is associated with the gas stream. This follows a velocity close to the ballistic one from the red star to a distance of ~0.5 R$_{L_{1}}$ from the white dwarf. This emission penetrates the accretion disc (from 0.5--0.1 R$_{L_{1}}$), with a velocity now closer (but lower) to the keplerian velocities along the path of the gas stream. We finally discuss the implications of having observed simultaneously line emission from the gas stream and the red star during outburst.

E. T. Harlaftis; T. R. Marsh

1995-03-07T23:59:59.000Z

488

OY Car in Outburst: Balmer emission from the red star and the gas stream  

E-Print Network [OSTI]

We present observations of OY Car, obtained with the Anglo-Australian telescope, during a normal outburst in 1991. Two sinusoidal components are resolved in the Hbeta trailed spectra and we determine the location of the narrow component to be on the secondary star with a maximum contributed flux of ~2.5 per cent to the total flux. Imaging of the line distribution reveals that the other emission component is associated with the gas stream. This follows a velocity close to the ballistic one from the red star to a distance of ~0.5 R_L1 from the white dwarf. Then. its kinematics changes from 0.5-0.2 R_L1 (accretion disc) following velocities now closer to (but lower than) the keplerian velocities along the path of the gas stream. We finally dicsuss the implications of having observed simultaneously line emission from the gas stream and the red star during outburst.

E. T. Harlaftis; T. R. Marsh

1995-10-04T23:59:59.000Z

489

Diagenesis of sandstones from the Douglas Creek member of the Green River Formation (Eocene) at Red Wash field, Uintay County, Utah  

E-Print Network [OSTI]

. Another theory, regarding chemical diagenesis, is put forth by Hower et al, (1976). As the temperature increases with depth, smectite becomes unstable and may form illite, chlorite, and quartz. Kaolinite becomes unstable at temp- eratures between 120... grains. According to Perry and Hower (1970) and Hower et al (1976), the presence of partly ordered interstratified illite-smectite indicates that the maximum burial depth was no more than 9800 ft (3000 m) 18 STUDY NETHODS The study was based...

Ray, Earl Scott

1985-01-01T23:59:59.000Z

490

Sedimentary processes of the Red River between Denison Dam, TX and Alexandria, LA  

E-Print Network [OSTI]

base level. It was concluded that the suspended sediment concentration of the Red River between Index, AR and Shreveport, LA is caused by two processes: 1. ) the erosion of sediment accumulated behind the raft as the river grades to original base... Marine Regiment, Iwo Jima Col. A. F. Weirich, U. S. Army (ret. ) 1 909 - 1988 Executive Officer - Rocky Mountain Arsenal, Denver CO TABLE OF CONTENTS ABSTRACT. ACKNOWLEDGEMENTS DED ICATION . . TABLE OF CONTENTS LIST OF F IG U RES . . . . . LIST...

Weirich, Thomas Moody - Kenyon

2012-06-07T23:59:59.000Z

491

Water Balance, Salt Loading, and Salinity Control Options of Red Bluff Reservoir, Texas  

E-Print Network [OSTI]

objectives: i) to outline water balance of the reservoir, ii) to establish salt loading trends over the past several decades, and iii) to evaluate the impact of salt loading on salinity of the reservoir and its outflow. We also outlined the needs... presumably has less seepage losses. The study reported here was conducted i) for examining the reservoir water balance of Red Bluff over the past several decades, ii) for establishing salt loading trends, and iii) for evaluating the impact of salt...

Miyamoto, S.; Yuan, Fasong; Anand, Shilpa

492

Relationship of Course Woody Debris to Red-Cockaded Woodpecker Prey Diversity and Abundance  

SciTech Connect (OSTI)

The abundance of diversity of prey commonly used by the red-cockaded woodpecker were monitored in experimental plots in which course woody debris was manipulated. In one treatment, all the woody debris over four inches was removed. In the second treatment, the natural amount of mortality remained intact. The overall diversity of prey was unaffected; however, wood roaches were significantly reduced by removal of woody debris. The latter suggests that intensive utilizations or harvesting practices may reduce foraging.

Horn, G.S.

1999-09-03T23:59:59.000Z

493

Contrasting survival strategies of hatchery and wild red drum: implications for stock enhancement  

E-Print Network [OSTI]

. Marshall Kirk O. Winemiller James L. Pinckney Gregory W. Stunz Head of Department, Thomas E. Lacher May 2008 Major Subject: Wildlife and Fisheries Sciences iii ABSTRACT Contrasting Survival Strategies of Hatchery and Wild Red Drum... of the Rooker Lab. Many thanks to my committee members, Dr. Christopher Marshall, Dr. Kirk Winemiller, Dr. James Pinckney, and Dr. Gregory Stunz, for their insight and suggestions which greatly improved the content and quality of my dissertation research...

Beck, Jessica Louise

2009-05-15T23:59:59.000Z

494

NOR ANY DROP TO DRINK: An Analysis of The Jordan Red Sea Project and Reconciling  

E-Print Network [OSTI]

/yr ! Jordan River 1950s 1.3 BCM/yr FOA - UN #12;Amman Highlands AlGhor / Jordan Valley/ Wadi Araba Badia Dead as a stand-alone project" Al-Qimish 2:14-2:36 50 MCM # Amman 20 MCM # Aqaba, Wadi Araba 5 MCM # economic Valley/ Wadi Araba Badia Dead Sea (417m below sealevel) Red Sea #12;Phase 2 80 MCM # nuclear plant #12

Scott, Christopher

495

Possible causes of reddish discoloration of urine ("red water") as it involves cattle  

E-Print Network [OSTI]

produces a severe hssoglobinaaia, uhich is the result of hesolysis of circulating red blood cells by action of tosins or nitro?organisns, the free pageant srceeds the capacity of the reticulo-endothslial systaa ~ nd the henoglobfn is encreted... dilated with a bile snd the walls thickened With fibrous connective tissue. Otaat areas of hepatic tissue in all, stages of necrosis were reticulated with enlarged prominent gupffer cells containing yellow granular pigment. The spleen showed reticulo...

Lynd, Frederick Theodore

1959-01-01T23:59:59.000Z

496

AN EXTENDED GRID OF NOVA MODELS. III. VERY LUMINOUS, RED NOVAE  

SciTech Connect (OSTI)

Extremely luminous, red eruptive variables like RV in M31 are being suggested as exemplars of a new class of astrophysical objects. Our greatly extended series of nova simulations shows that classical nova models can produce very red, luminous eruptions. In a poorly studied corner of three-dimensional nova parameter space (very cold, low-mass white dwarfs, accreting at very low rates) we find bona fide classical novae that are very luminous and red because they eject very slowly moving, massive envelopes. A crucial prediction of these nova models-in contrast to the predictions of merging star ('mergeburst') models-is that a hot remnant, the underlying white dwarf, will emerge after the massive ejected envelope has expanded enough to become optically thin. This blue remnant must fade on a timescale of decades-much faster than a 'mergeburst', which must fade on timescales of millennia or longer. Furthermore, the cooling nova white dwarf and its expanding ejecta must become redder in the years after eruption, while a contracting mergeburst must become hotter and bluer. We predict that red novae will always brighten to L {approx} 1000 L{sub sun} for about one year before rising to the maximum luminosity at L {approx} 10{sup 6}-10{sup 7} L{sub sun}. The maximum luminosity attainable by a nova is likely to be L {approx} 10{sup 7} L{sub sun}, corresponding to M {approx} -12. In an accompanying paper, we describe a fading, luminous blue candidate for the remnant of M31-RV; it is observed with the Hubble Space Telescope to be compatible only with the nova model.

Shara, Michael M.; Zurek, David [Department of Astrophysics, American Museum of Natural History, Central Park West and 79th Street, New York, NY 10024-5192 (United States); Yaron, Ofer; Prialnik, Dina; Kovetz, Attay [Department of Geophysics and Planetary Sciences, Sackler Faculty of Exact Sciences, Tel Aviv University, Ramat Aviv 69978 (Israel)

2010-12-10T23:59:59.000Z

497

Characterization of freshwater as a treatment for amyloodiniosis in red drum  

E-Print Network [OSTI]

) because the number of parasites per fish is relatively small in situations where fish density is low. In September 1997, however, scientists determined that a fish kill of over one million tilapia at the Salton Sea National Wildlife Refuge in California... was the result of infestation by A. ocellatum (F WS 1997). High temperatures and salinities present in the Salton Sea at that time apparently were conducive to rapid development of lethal infestations. The red drum (Sciaenops ocellatus) is a marine, warmwater...

Harris, Courtney Elaine

1999-01-01T23:59:59.000Z

498

Red River Hot Springs Pool & Spa Low Temperature Geothermal Facility | Open  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to: navigation, search RAPIDColoradosourceRausWyoming: Energy Resources6072302°,Red

499

Identification of heat source fields from infra-red thermography: Determination of  

E-Print Network [OSTI]

-heating' in a dual-phase steel by using a dog bone sample C´edric Doudard, a,1 Sylvain Calloch a Fran¸cois Hild b;Identification of heat source fields from infra-red thermography: Determination of `self-heating' in a dual-phase steel by using a dog bone sample by C. Doudard, S. Calloch, F. Hild and S. Roux Abstract: From infra

500

The red-cockaded woodpecker on the Savannah River Site: Aspects of reproductive success.  

SciTech Connect (OSTI)

Red-cockaded woodpecker; Road to Recovery. Proceedings of the 4th Red-cockaded woodpecker Symposium. Ralph Costa and Susan J. Daniels, eds. Savannah, Georgia. January, 2003. Chapter 5. Status and Trends of Populations. Pp 224-229. Abstract: The red-cockaded woodpecker (Picoides borealis) population on the Savannah River Site has been closely monitored and studied over the last 17 years. In 1985, the USDA Forest Service Southern Research Station was given responsibility to study and manage this population in an effort to prevent its extirpation. In December 1985, there were only 4 individuals on the site: 1 pair and 2 solitary males. The population had increased to a total of 175 individuals in 42 active clusters in 2002. Although this represents a very successful recovery effort, there has been substantial annual variation in nesting survival from banding to fledging. Data were analyzed to more completely understand the factors affecting reproduction. No significant effects of age of the breeding male and female, years paired, number of helpers, habitat quality, number of nestings, and time of nest initiation were found when comparing reproductive success in 117 nesting attempts from 1999 to 2002. However, the number of neighboring groups had a direct effect on mortality rates, possibly demonstrating the importance of cluster spacing.

Johnston, Peter A.; Imm, Donald, W.; Jarvis, William L.

2004-12-31T23:59:59.000Z