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1

Tourism in the Maldives: experiencing the difference from the Maldives Ms. Bndicte AUVRAY  

E-Print Network [OSTI]

Tourism in the Maldives: experiencing the difference from the Maldives Ms. Bénédicte AUVRAY Ph Tourism Promotion Board, the country looks like a white and blue world for honeymooners, divers ­ Enclave ­ Exoticism halshs-00536400,version1-16Nov2010 Author manuscript, published in "Tourism

Paris-Sud XI, Université de

2

Maldives-NREL Cooperation | 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,ECOInformation Sharing andMaldives-NREL

3

Maldives: Energy Resources | 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 revision hasInformation Earth's Heat JumpIncMAKGalway Bay(Held &InformationWind FarmMalaysia:Maldives:

4

Maldives-Program for Scaling Up Renewable Energy in Low Income...  

Open Energy Info (EERE)

Kenya Specific Documents4 Maldives Specific Documents5 Mali Specific Documents6 Nepal Specific Documents7 Overview "The Scaling-Up Renewable Energy Program for Low Income...

5

Maldives-Supporting the Zero Emissions Strategy | 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,ECOInformation Sharing andMaldives-NREL(SREP)

6

Last resorts : a tour guide to territorial protection for the Republic of the Maldives  

E-Print Network [OSTI]

A two meter rise in sea levels projected by the end of this century threatens the sovereignty of the Maldivian nation state. While flight from the Maldives to establish a new homeland elsewhere has been proposed, the culture ...

Sleeper, Buck (Thomas Buck)

2011-01-01T23:59:59.000Z

7

MagLab - Multimedia Library  

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

Fact Sheets Arrow Multimedia Library This library offers a small collection of MagLab photos, graphics, PowerPoints and videos to which we will add over time. These are free to...

8

MagLab - Science Caf  

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

to a radio story. Munir Humayun, a professor of geochemistry at the MagLab. Sept. 3 3D Printing Watch a video of the event. David Brightbill and Mark Trombly, Making Awesome,...

9

Maldives-Program for Scaling Up Renewable Energy in Low Income Countries  

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,ECOInformation Sharing andMaldives-NREL(SREP) |

10

MagLab - Press Release Archives  

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

Have a Home at the MagLab Aug. 30 Science Caf Launches New Season with Talk on Higgs Boson Aug. 27 MagLab Gets Nearly 3 Million to Build Cool New Tools July 31 Decades-old...

11

MagLab Education - For Students  

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

and learn about power grids, environmentally responsible power systems, renewable energy and current and future power delivery systems. Coordinated by the MagLab, these...

12

MagViz Bottled Liquid Scanner at Albuquerque International Sunport  

ScienceCinema (OSTI)

The next-generation bottled liquid scanner, MagViz BLS, is demonstrated at the Albuquerque International Sunport, New Mexico

Surko, Stephen; Dennis, Steve; Espy, Michelle

2014-08-12T23:59:59.000Z

13

MagLab researchers uncover groundbreaking properties of promising...  

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

'Jason' Li Zhiqiang "Jason" Li TALLAHASSEE, Fla. - MagLab scientists working with graphene - a stronger-than steel, but feathery light material with myriad of intriguing...

14

Mag Lab Reports, Volume 16, No. 2 (Highlights Issue)  

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

for biomedical research (page 14). On the magnet science and technology front, work on cable in conduit conductors will benefit the MagLab's new Series connected Hybrid user...

15

MagLab - Electricity and Magnetism on the Web  

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

Electricity and Magnetism on the Web MagLab U logo If you have a question about physics, magnetism or electricity, you'll surely find the answer in one of the excellent Web sites...

16

MagLab Discovery Could Be Crucial Step to Quantum Computer (July...  

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

Magnetic Field Laboratory (MagLab) have observed a physical phenomenon in bilayer graphene that could usher in a new generation of quantum computers. Their results are...

17

M1 Energy | 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, Alaska:Luz IILynnM Setek Co Ltd JumpM1 Energy Jump

18

The Classification of M1-78  

E-Print Network [OSTI]

The published properties of M1-78 are discussed with the purpose to resolve the object's classification as either a planetary nebula or an ultracompact HII region. A classification as a planetary nebula is rejected primarily because of the high luminosity of the object, but because of the chemical composition and expansion velocity of the nebula, a novel classification is proposed instead: that of an ultracompact HII region with a post-main sequence central star (possibly a WN star). It must therefore follow that observable ultracompact HII regions persist beyond the main sequence lifetimes of at least some massive stars, and so cannot be transient phenomena that are seen only during pre-main sequence or early main sequence evolution.

G. T. Gussie

1994-09-15T23:59:59.000Z

19

The 2014 MagLab Science Summer Camps combined the computer technology, and robotics with World Cup Soccer  

E-Print Network [OSTI]

The 2014 MagLab Science Summer Camps combined the computer technology, and robotics with World Cup of computer programming and robotics through the Sphero robots. The final event was a Robot World Cup Match) · 25% female, and · 12% from Title I schools MagLab Summer Camps feature the Excitement of Robotic

McQuade, D. Tyler

20

Spooky Science Series. The MagLab holds a Halloween-themed event each year in October. The Spooky Science  

E-Print Network [OSTI]

Spooky Science Series. The MagLab holds a Halloween- themed event each year in October. The Spooky Science event brings families to the lab for hands-on activities and laboratory tours, planned by the MagLab staff scientists and graduate students to science education and outreach. . · The 2014 event had over

Weston, Ken

Note: This page contains sample records for the topic "maldives mag m1" 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

A Novel MagPipe Pipeline transportation system using linear motor drives  

SciTech Connect (OSTI)

A novel capsule pipeline transportation system using linear motor drives, called Magplane MagPipe, is under development with the intention to replace trucks and railways for hauling materials from the mine to the rail head, power plant, or processing plant with reduced operating cost and energy consumption. The initial demonstration of a MagPipe line in Inner Mongolia will be a 500-m-long double-pipe coal transport system with the design transportation capacity of 3 Mega-Mg per year. The pipeline consists of 6-m-long plastic pipe modules with an I-beam suspension system inside the pipe to carry sets of five coupled capsules. The pipe will also contain noncontinuous motor winding modules spaced at 50-m intervals. A set of Halbach-arrayed permanent magnets on the bottom of the capsules interact with the linear motor windings to provide propulsion. The motor is driven by variable frequency drives outside the pipe to control the speed. This paper briefly describes the overall MagPipe pipeline transportation system, including the preliminary conclusions of the linear synchronous motor analysis.

Fang, J.R.; Montgomery, D.B.; Roderick, L. [Magplane Technology Inc., Littleton, MA (United States)

2009-11-15T23:59:59.000Z

22

AFRICAN-AMERICAN STUDENTS African-American Career World, http://www.eop.com/mags-AACW.php, is the  

E-Print Network [OSTI]

AFRICAN-AMERICAN STUDENTS African-American Career World, http://www.eop.com/mags-AACW.php in the workplace. ASIAN STUDENTS Asian American: Career Center- http://goldsea.com/Text/index.php

Arnold, Jonathan

23

M/M/1 Queueing System with Delayed Controlled Vacation  

E-Print Network [OSTI]

M/M/1 Queueing System with Delayed Controlled Vacation Yonglu Deng , Zhongshan University W. John systems using a time division multiple access (TDMA) scheme (Frey and Takahashi, [7]). Researchers have that of a server's cold switch-on. The case of delayed vacation has also very recently been studied by Frey

Zhao, Yiqiang Q.

24

M1 internship account On update schedules and dynamics of  

E-Print Network [OSTI]

M1 internship account 2007-2008 On update schedules and dynamics of boolean networks Mathilde Noual Internship done at the university of Concepción under the direction of Julio Aracena hal-00688157,version1 network rely on several dierent parameters. During this internship, we have especially been looking

Paris-Sud XI, Université de

25

Part I -Mechanics J05M.1 -Rope Around a Cylinder J05M.1 -Rope Around a Cylinder  

E-Print Network [OSTI]

slipping? Explain why a small child can hold a large ocean liner in place using a device like this. µs f F with = 1016 s-1 ( 106 Ohm-1 m-1 in SI units) reflects 90% of the incident radiation. Assume the and µ

Petta, Jason

26

The E2/M1 ratio in {Delta} photoproduction  

SciTech Connect (OSTI)

New high-precision measurements of p({rvec {gamma}}, {pi}) and p({rvec {gamma}}, {gamma}) cross sections and beam asymmetries have been combined with other polarization ratios in a simultaneous analysis of both reactions. The E2/M1 mixing ratio for the n {r_arrow} {Delta} transition extracted from this analysis is EMR = {minus}3.0% {+-} 0.3 (stat+sys) {+-} 0.2 (model).

Hoblit, S. [Brookhaven National Lab., Upton, NY (United States). Physics Dept.]|[Univ. of Virginia, Charlottesville, VA (United States). Dept. of Physics; Blanpied, G. [Univ. of South Carolina, Columbia, SC (United States). Dept. of Physics; Blecher, M. [Virginia Polytechnic Inst. and State Univ., Blacksburg, VA (United States). Physics Dept.] [and others; LEGS Collaboration

1997-10-01T23:59:59.000Z

27

The E2/M1 ratio in {Delta} photoproduction  

SciTech Connect (OSTI)

The properties of the transition from the nucleon to the {Delta}(1232) serve as a benchmark for models of nucleon structure. To first order, N {r_arrow} {Delta} photo-excitation is dominated by a simple M1 quark spin-flip transition. At higher order, small L = 2 components in the N and {Delta} wavefunctions allow this excitation to proceed via an electric quadrupole transition. Since Nucleon models differ greatly on the mechanisms used to generate these L = 2 components,, the ratio of E2/M1 transitions (EMR) provides a sensitive test for structure models. Here, new high-precision measurements of p({rvec {gamma}}, {pi}) and p({rvec {gamma}}, {gamma}) cross sections and beam asymmetries have been combined with other polarization ratios in a simultaneous analysis of both reactions. Compton scattering has provided two important new constraints on the photo-pion amplitude. The E2/M1 mixing ratio for the N {r_arrow} {Delta} transition extracted from this analysis is EMR = {minus}3.0% {+-} 0.3 (stat+sys) {+-} 0.2 (model).

Sandorfi, A.M. [Brookhaven National Lab., Upton, NY (United States). Physics Dept.; Blanpied, G. [Univ. of South Carolina, Columbia, SC (United States). Dept. of Physics; Blecher, M. [Virginia Polytechnic Inst. and State Univ., Blacksburg, VA (United States). Physics Dept.] [and others; LEGS Collaboration

1997-08-01T23:59:59.000Z

28

Part I -Mechanics M05M.1 -Vibration Damping With a Piston M05M.1 -Vibration Damping With a Piston  

E-Print Network [OSTI]

Part I - Mechanics M05M.1 - Vibration Damping With a Piston M05M.1 - Vibration Damping With a Piston Problem Sometimes it is required to reduce the influence of vertical floor vibration-filled pistons (which have face area A and equilibrium volume V0). The gas pressure in the cylinder is much

Petta, Jason

29

28.99.99.M1 Student Health Services Page 1 of 1 UNIVERSITY RULE  

E-Print Network [OSTI]

The Department of Student Health Services (A.P. Beutel Health Center) is an ambulatory health care provider serving the Texas A&M University student body through the provision of primary health care services28.99.99.M1 Student Health Services Page 1 of 1 UNIVERSITY RULE 28.99.99.M1 Student Health Services

30

The development and evaluation of a sensitive minicolumn assay for the detection of aflatoxin M1 in milk  

E-Print Network [OSTI]

M1 (CSID-M1) in milk has been developed in our laboratory. In this new method, aflatoxin M1 (AfM1) is selectively adsorbed in a small glass minicolumn at the interface of a layer of packed neutral sand and a narrow band of magnesium silicate (or...

Cathey, Carol Grmela

1993-01-01T23:59:59.000Z

31

A magnetic particle time-of-flight (MagPTOF) diagnostic for measurements of shock-and compression-bang time at the NIF (invited)a)  

E-Print Network [OSTI]

Laboratory for Laser Energetics, Rochester, New York 14623, USA 3 Lawrence Livermore National Laboratory-bang time at the NIF (invited)a) H. G. Rinderknecht, H. Sio, J. A. Frenje, J. Magoon, A. Agliata, M. Shoup time-of-flight (MagPTOF) diagnostic for measurements of shock- and compression-bang time at the NIF

32

Public Relations Office 500 University Avenue Rochester, NY 14607-1484 585.276.8900 585.473.6266 fax mag.rochester.edu NEWS  

E-Print Network [OSTI]

29, 2013 Description: This exhibition, which celebrates MAG's centennial, includes both historical (March 30­April 7), free to age 18 and under if accompanied by an adult. Half-price admission Thursdays historical and con- temporary objects that explore how memory shapes both personal and cultural identities

Portman, Douglas

33

Laser hazard analysis for LASIRIS Model MAG-501L-670M-1000-45[degree]-K diode laser associated with high resolution pulsed scanner.  

SciTech Connect (OSTI)

A laser hazard analysis and safety assessment was performed for the LASIRISTM Model MAG-501L-670M-1000-45o-K diode laser associated with the High Resolution Pulse Scanner based on the ANSI Standard Z136.1-2000, American National Standard for the Safe Use of Lasers and the ANSI Standard Z136.6-2000, American National Standard for the Safe Use of Lasers Outdoors. The laser was evaluated for both indoor and outdoor use.

Augustoni, Arnold L.

2004-11-01T23:59:59.000Z

34

J.-A. FLEMING. 2014 On the characteristic curves and surfaces of incandescence lamps (Courbes caractristiques des lampes incandescence) ; Phil. Mag.,  

E-Print Network [OSTI]

80 J.-A. FLEMING. 2014 On the characteristic curves and surfaces of incandescence lamps (Courbes caractéristiques des lampes à incandescence) ; Phil. Mag., 5e série, t. XIX, p. 368; I885. L'auteur étudie les résistance correspondant à la force électromotrice vo à laquelle l'incandescence commence à se produire, et r

Paris-Sud XI, Université de

35

M1 Master Mathematiques de Metz Mod`eles probabilistes en finance  

E-Print Network [OSTI]

M1 ­ Master Math´ematiques de Metz Mod`eles probabilistes en finance 2007/2008 R. Lamberton, B. Lapeyre: Introduction au calcul stochastique appliqu´e `a la finance. Ellipses, 1997 (b) S. E. Shreve: Stochastic calculus for finance. I: The binomial asset pricing model. Springer Finance, 2004 (c

Thalmaier, Anton

36

New probe of M1 and E1 strengths in GDR regions  

SciTech Connect (OSTI)

The M1 strengths (or level density of 1{sup +} states) are of importance for estimation of interaction strengths between neutrinos and nuclei for the study of the supernova neutrino-process. In 1957, Agodi predicted theoretically angular distribution of neutrons emitted from states excited via dipole transitions with linearly polarized gamma-ray beam at the polar angle of ?=90 should be followed by a simple function, a + b cos(2?), where ?, is azimuthal angel. However, this theoretical prediction has not been verified over the wide mass region except for light nuclei as deuteron. We have measured neutron angular distributions with (polarized gamma, n) reactions on Au, Nal, and Cu. We have verified the Agodi's prediction for the first time over the wide mass region. This suggests that (polarized gamma, n) reactions may be useful tools to study M1 strengths in giant resonance regions.

Hayakawa, T. [Japan Atomic Energy Agency and National Astronomical Observatory in Japan (Japan); Ogata, K. [RCNP, Osaka University (Japan); Miyamoto, S.; Mochizuki, T.; Horikawa, K.; Amano, S. [University of Hyogo (Japan); Imazaki, K.; Li, D.; Izawa, Y. [Institute for Laser Technology (Japan); Chiba, S. [Tokyo Institute of Technology (Japan)

2014-05-02T23:59:59.000Z

37

GFMC calculations of electromagnetic moments and M1 transitions in A {<=} 9 nuclei  

SciTech Connect (OSTI)

We present recent Green?s function Monte Carlo calculations of magnetic moments and M1 transitions in A{<=}#20;9 nuclei, which include corrections arising from two-body meson-exchange electromagnetic currents. Two-body effects provide significant corrections to the calculated observables, bringing them in excellent agreement with the experimental data. In particular, we find that two body corrections are especially large in the A = 9, T = 3/2 systems, in which they account for up to ~#24; 20% (~#24; 40%) of the total predicted value for the {sup 9}Li ({sup 9}C) magnetic moment.

Pastore, Saori [Department of Physics and Astronomy, University of South Carolina, Columbia, SC; Pieper, Steven C. [Argonne National Laboratory; Schiavilla, Rocco [JLAB, Old Dominion U.; Wiringa, Robert Bruce [Physics Division, Argonne National Laboratory, Argonne, Illinois

2013-08-01T23:59:59.000Z

38

25.07.03.M1.01 Vendor Protest Procedures Page 1 of 2 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

25.07.03.M1.01 Vendor Protest Procedures Page 1 of 2 STANDARD ADMINISTRATIVE PROCEDURE 25.07.03.M1.01 Vendor Protest Procedures Approved July 18, 1997 Revised January 7, 2002 Revised May 22, 2007 Revised This Standard Administrative Procedure (SAP) details the steps necessary for a vendor to challenge a purchase

39

29.01.03.M1.22 Information Resources Vendor Access Page 1 of 4 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

29.01.03.M1.22 Information Resources ­ Vendor Access Page 1 of 4 STANDARD ADMINISTRATIVE PROCEDURE 29.01.03.M1.22 Information Resources ­ Vendor Access Approved July 18, 2005 Revised December 4, 2009 that will mitigate information security risks associated with vendor access. Reason for SAP Vendors play an important

40

29.01.03.M1.01 Network Scanning and Vulnerability Assessments Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

29.01.03.M1.01 Network Scanning and Vulnerability Assessments Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE 29.01.03.M1.01 Network Scanning and Vulnerability Assessments Approved October 1, 2002 Revised review: August 14, 2016 Statement and Reason for Standard Administrative Procedure The purpose

Note: This page contains sample records for the topic "maldives mag m1" 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.


41

Nucleotide sequence of the 2 matrix protein genes (M1 and M2) of hirame rhabdovirus (HRV),  

E-Print Network [OSTI]

Nucleotide sequence of the 2 matrix protein genes (M1 and M2) of hirame rhabdovirus (HRV), a fish of hirame rhabdovirus (HRV). The M1 protein gene was 684 nucleotides long, encoding 227 amino acids.8% at the nucleotide level and 81.1 and 44.8% at the amino acid level. The M2 protein gene was 582 nucleotides long

Boyer, Edmond

42

Tricalcium silicate Ca3SiO5 superstructure analysis: a route towards the structure of the M1 polymorph  

E-Print Network [OSTI]

Tricalcium silicate Ca3SiO5 superstructure analysis: a route towards the structure of the M1 a structural model for the M1 polymorph of tricalcium silicate Ca3SiO5 from Powder X-Ray Diffraction (XRD) data of a synthetic rock named clinker, which contains at least four major phases: two calcium silicates called alite

Boyer, Edmond

43

29.01.03. M1.11 Information Resources Intrusion Detection Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

includes, but is not limited to, all information resources management personnel, owners, and system29.01.03. M1.11 Information Resources ­ Intrusion Detection Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE 29.01.03.M1.11 Information Resources ­ Intrusion Detection Approved July 18, 2005 Revised April 27

44

A magnetic particle time-of-flight (MagPTOF) diagnostic for measurements of shock- and compression-bang time at the NIF (invited)  

SciTech Connect (OSTI)

A magnetic particle time-of-flight (MagPTOF) diagnostic has been designed to measure shock- and compression-bang time using D{sup 3}He-fusion protons and DD-fusion neutrons, respectively, at the National Ignition Facility (NIF). This capability, in combination with shock-burn weighted areal density measurements, will significantly constrain the modeling of the implosion dynamics. This design is an upgrade to the existing particle time-of-flight (pTOF) diagnostic, which records bang times using DD or DT neutrons with an accuracy better than 70 ps [H. G. Rinderknecht et al., Rev. Sci. Instrum. 83, 10D902 (2012)]. The inclusion of a deflecting magnet will increase D{sup 3}He-proton signal-to-background by a factor of 1000, allowing for the first time simultaneous measurements of shock- and compression-bang times in D{sup 3}He-filled surrogate implosions at the NIF.

Rinderknecht, H. G., E-mail: hgr@mit.edu; Sio, H.; Frenje, J. A.; Gatu Johnson, M.; Zylstra, A. B.; Sinenian, N.; Rosenberg, M. J.; Li, C. K.; Sguin, F. H.; Petrasso, R. D. [Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 (United States); Magoon, J.; Agliata, A.; Shoup, M.; Glebov, V. U.; Hohenberger, M.; Stoeckl, C.; Sangster, T. C. [Laboratory for Laser Energetics, Rochester, New York 14623 (United States); Ayers, S.; Bailey, C. G.; Rygg, J. R. [Lawrence Livermore National Laboratory, Livermore, California 94550 (United States); and others

2014-11-15T23:59:59.000Z

45

Determination of gamma from Charmless B --> M1 M2 Decays Using U-Spin  

E-Print Network [OSTI]

In our previous paper we applied U-spin symmetry to charmless hadronic B+- --> M0 M+- decays for the purpose of precise extraction of the unitarity angle gamma. In this paper we extend our approach to neutral B0 and Bs --> M1 M2 decays. A very important feature of this method is that no assumptions regarding relative sizes of topological decay amplitudes need to be made. As a result, this method avoids an uncontrollable theoretical uncertainty that is often related to the neglect of some topological diagrams (e.g., exchange and annihilation graphs) in quark-diagrammatic approaches. In charged B+- decays, each of the four data sets, P0 P+-, P0 V+-, V0 P+- and V0 V+-, with P=pseudoscalar and V=vector, can be used to obtain a value of gamma. Among neutral decays, only experimental data in the B0, Bs --> P- P+ subsector is sufficient for a U-spin fit. Application of the U-spin approach to the current charged and neutral B decay data yields: gamma=(80^{+6}_{-8}) degrees. In this method, which is completely data dr...

Soni, A; Soni, Amarjit; Suprun, Denis A.

2007-01-01T23:59:59.000Z

46

Determination of gamma from Charmless B --> M1 M2 Decays Using U-Spin  

E-Print Network [OSTI]

In our previous paper we applied U-spin symmetry to charmless hadronic B+- --> M0 M+- decays for the purpose of precise extraction of the unitarity angle gamma. In this paper we extend our approach to neutral B0 and Bs --> M1 M2 decays. A very important feature of this method is that no assumptions regarding relative sizes of topological decay amplitudes need to be made. As a result, this method avoids an uncontrollable theoretical uncertainty that is often related to the neglect of some topological diagrams (e.g., exchange and annihilation graphs) in quark-diagrammatic approaches. In charged B+- decays, each of the four data sets, P0 P+-, P0 V+-, V0 P+- and V0 V+-, with P=pseudoscalar and V=vector, can be used to obtain a value of gamma. Among neutral decays, only experimental data in the B0, Bs --> P- P+ subsector is sufficient for a U-spin fit. Application of the U-spin approach to the current charged and neutral B decay data yields: gamma=(80^{+6}_{-8}) degrees. In this method, which is completely data driven, in a few years we should be able to obtain a model independent determination of gamma with an accuracy of O(few degrees).

Amarjit Soni; Denis A. Suprun

2006-09-08T23:59:59.000Z

47

Large low-energy $M1$ strength for $^{56,57}$Fe within the nuclear shell model  

E-Print Network [OSTI]

A strong enhancement at low $\\gamma$-ray energies has recently been discovered in the $\\gamma$-ray strength function of $^{56,57}$Fe. In this work, we have for the first time obtained theoretical $\\gamma$ decay spectra for states up to $\\approx 8$ MeV in excitation for $^{56,57}$Fe. We find large $B(M1)$ values for low $\\gamma$-ray energies that provide an explanation for the experimental observations. The role of mixed $E2$ transitions for the low-energy enhancement is addressed theoretically for the first time, and it is found that they contribute a rather small fraction. Our calculations clearly show that the high-$\\ell$ ($=f$) diagonal terms are most important for the strong low-energy $M1$ transitions. As such types of $0\\hbar\\omega$ transitions are expected for all nuclei, our results indicate that a low-energy $M1$ enhancement should be present throughout the nuclear chart. This could have far-reaching consequences for our understanding of the $M1$ strength function at high excitation energies, with profound implications for astrophysical reaction rates.

B. Alex Brown; A. C. Larsen

2014-09-11T23:59:59.000Z

48

29.01.03.M1.15 Information Resources Physical Access Page 1 of 4 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

the processes to grant, control, monitor and remove physical access to information resource facilities of their function at the university. 2.1.2 All physical security systems shall comply with applicable regulations PROCEDURE 29.01.03.M1.15 Information Resources Physical Security Approved July 18, 2005 Revised February

49

29.01.03.M1.12 Information Resources Network Access Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

29.01.03.M1.12 Information Resources Network Access Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE Administrative Procedure Statement The information resources network infrastructure in Bryan/College Station for SAP The purpose of this Texas A&M University network access standard administrative procedure

50

29.01.03.M1.13 Information Resources Network Configuration Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

29.01.03.M1.13 Information Resources Network Configuration Page 1 of 3 STANDARD ADMINISTRATIVE to this infrastructure. 2. APPLICABILITY This Standard Administrative Procedure (SAP) applies to all University network.27 Exclusions from Required Risk Mitigation Measures. The intended audience is all network system administrators

51

MODEL ANALYSES AND GUIDANCE (MAG) APPLICATION MAG User's Manual  

E-Print Network [OSTI]

the National Weather Service's (NWS) Numerical Weather Prediction computer models. The website offers Guidance: Provides a path to view products created from the National Weather Service's (NWS) numerical Weather Service's Tropical Cyclone models. These products are only available when tropical cyclones

52

MagLab - MagLab Dictionary: Hybrid Magnet (Transcript)  

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

Hybrid Magnet As explained by Scott Hannahs, DC Facilities & Instrumentation director. Hybrid magnet The lab's world-record 45 tesla hybrid magnet. The premier magnet system at the...

53

MagLab - Microanalysis Laboratory  

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

Microanalysis Laboratory BSCCO Sample of the superconducting material bismuth strontium calcium copper oxide (BSCCO). Section pictured measures 120 microns wide. Click on photo for...

54

MagLab - Interactive Tutorials  

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

laws, tools and historical milestones associated with electricity and magnetism. Our virtual demonstrations allow you to manipulate variables at your own speed and visualize...

55

MagLab - Rheostat Tutorial  

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

tutorial, try downloading the latest version of Java. In the mid 1820s, Georg Ohm, a German professor of mathematics, began investigating electrical resistance. Through...

56

MagLab - Microwaves Tutorial  

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

All these water molecules moving around and bumping into each other generate friction, which produces heat and warms the food. The greater the density of water molecules,...

57

MagLab - Faraday Cage  

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

we benefit from these waves in the form of microwavable popcorn, tunes over the car radio, and the very light that allows us to see. Electromagnetic Spectrum Some scientists,...

58

Implications for Damage Recognition during Dpo4-Mediated Mutagenic Bypass of m1G and m3C Lesions  

SciTech Connect (OSTI)

DNA is susceptible to alkylation damage by a number of environmental agents that modify the Watson-Crick edge of the bases. Such lesions, if not repaired, may be bypassed by Y-family DNA polymerases. The bypass polymerase Dpo4 is strongly inhibited by 1-methylguanine (m1G) and 3-methylcytosine (m3C), with nucleotide incorporation opposite these lesions being predominantly mutagenic. Further, extension after insertion of both correct and incorrect bases, introduces additional base substitution and deletion errors. Crystal structures of the Dpo4 ternary extension complexes with correct and mismatched 3'-terminal primer bases opposite the lesions reveal that both m1G and m3C remain positioned within the DNA template/primer helix. However, both correct and incorrect pairing partners exhibit pronounced primer terminal nucleotide distortion, being primarily evicted from the DNA helix when opposite m1G or misaligned when pairing with m3C. Our studies provide insights into mechanisms related to hindered and mutagenic bypass of methylated lesions and models associated with damage recognition by repair demethylases.

Rechkoblit, Olga; Delaney, James C.; Essigmann, John M.; Patel, Dinshaw J. (MIT); (MSKCC)

2012-05-08T23:59:59.000Z

59

The E2/M1 mixing ratio in the excitation of the {Delta} from polarized photo-reactions  

SciTech Connect (OSTI)

In constituent quark models, a tensor interaction, mixing quark spins with their relative motion, is introduced to reproduce the observed baryon spectrum. This has a consequence completely analogous to the nuclear tensor force between the n and p in deuterium. A D state component is mixed into what would otherwise be a purely S-wave object. The D-wave component breaks spherical symmetry, resulting in a non-vanishing matrix element for the nucleon and a static quadrupole moment and deformation for its first excited state, the {Delta} resonance, at {approximately}325 MeV. The magnitude and sign of this D-state component are quite sensitive to the internal structure of the proton and have been of great interest in recent years. The intrinsic deformation of the spin 1/2 nucleon cannot be observed directly; it must be inferred from transition amplitudes such as N {yields} {Delta}. In a spherical bag model, the {Delta} is viewed as a pure quark-spin-flip transition proceeding only through M1 excitation. If there are D-state admixtures in the ground state of the nucleon and/or {Delta}, quadrupole excitation, in addition to spin-flip M1, is also allowed. The problem is to evaluate the relative magnitude of this E2 excitation in the presence of the dominant M1 transition. A variety of models predict this mixing ratio to be quite small, anywhere from {minus}0.9% to {minus}6%, so that a high degree of precision is demanded of experiment.

The LEGS Collaboration

1993-12-01T23:59:59.000Z

60

07.03.01.M1: Political Campaign Events and Partisan Political Activities on Texas A&M University Property Page 1 of 2 UNIVERSITY RULE  

E-Print Network [OSTI]

07.03.01.M1: Political Campaign Events and Partisan Political Activities on Texas A&M University Property Page 1 of 2 UNIVERSITY RULE 07.03.01.M1 Political Campaign Events and Partisan Political partisan political activity. Texas A&M Universitycannot endorse, support or promote any political candidate

Note: This page contains sample records for the topic "maldives mag m1" 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

29.01.03.M1.26 Information Resources Security Risks Assessment Reviews Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

29.01.03.M1.26 Information Resources ­ Security Risks Assessment Reviews Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE 29.01.03.M1.26 Information Resources ­ Information Security Risk Assessment Reviews security risk assessments are vital procedures for maintaining the security of information resources

62

29.01.03.M1.16 Information Resources-Portable Devices: Information Security Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

information resources. This includes, but is not limited to: laptops, Personal Digital Assistants (PDAs29.01.03.M1.16 Information Resources- Portable Devices: Information Security Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE 29.01.03.M1.16 Information Resources ­ Portable Devices: Information Security Approved

63

M-1C.  

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

DEPARTlIENT OF ENERGY EERE PROJECT MANAGEMENT CENTER NEPA DETERlIINATION RECIPI ENT:City of Boston PROJECT TITLE: EECBG City Of Boston (S) Page 1 01'2 STATE:MA Funding...

64

Search for 14.4 keV solar axions from M1 transition of Fe-57 with CUORE crystals  

E-Print Network [OSTI]

We report the results of a search for axions from the 14.4 keV M1 transition from Fe-57 in the core of the sun using the axio-electric e?ect in TeO2 bolometers. The detectors are 5x5x5 cm3 crystals operated at about 10 mK in a facility used to test bolometers for the CUORE experiment at the Laboratori Nazionali del Gran Sasso in Italy. An analysis of 43.65 kg d of data was made using a newly developed low energy trigger which was optimized to reduce the detectors energy threshold. An upper limit of 0.63 c kg-1 d-1 was established at 95% C.L.. From this value, a lower bound at 95% C.L. was placed on the Peccei-Quinn energy scale of fa >= 0.76 10**6 GeV for a value of S=0.55 for the flavor-singlet axial vector matrix element. Bounds are given for the interval 0.15 < S < 0.55.

The Cuore Collaboration; F. Alessandria; R. Ardito; D. R. Artusa; F. T. Avignone III; O. Azzolini; M. Balata; T. I. Banks; G. Bari; J. Beeman; F. Bellini; A. Bersani; M. Biassoni; T. Bloxham; C. Brofferio; C. Bucci; X. Z. Cai; L. Canonica; S. Capelli; L. Carbone; L. Cardani; M. Carrettoni; N. Casali; N. Chott; M. Clemenza; C. Cosmelli; O. Cremonesi; R. J. Creswick; I. Dafinei; A. Dally; V. Datskov; A. De Biasi; M. P. Decowski; M. M. Deninno; S. Di Domizio; M. L. di Vacri; L. Ejzak; R. Faccini; D. Q. Fang; H. A. Farach; E. Ferri; F. Ferroni; E. Fiorini; M. A. Franceschi; S. J. Freedman; B. K. Fujikawa; A. Giachero; L. Gironi; A. Giuliani; J. Goett; P. Gorla; C. Gotti; E. Guardincerri; T. D. Gutierrez; E. E. Haller; K. Han; K. M. Heeger; H. Z. Huang; R. Kadel; K. Kazkaz; G. Keppel; L. Kogler; Yu. G. Kolomensky; D. Lenz; Y. L. Li; C. Ligi; X. Liu; Y. G. Ma; C. Maiano; M. Maino; M. Martinez; R. H. Maruyama; N. Moggi; S. Morganti; T. Napolitano; S. Newman; S. Nisi; C. Nones; E. B. Norman; A. Nucciotti; F. Orio; D. Orlandi; J. L. Ouellet; M. Pallavicini; V. Palmieri; L. Pattavina; M. Pavan; M. Pedretti; G. Pessina; S. Pirro; E. Previtali; V. Rampazzo; F. Rimondi; C. Rosenfeld; C. Rusconi; S. Sangiorgio; N. D. Scielzo; M. Sisti; A. R. Smith; L. Taffarello; M. Tenconi; W. D. Tian; C. Tomei; S. Trentalange; G. Ventura; M. Vignati; B. S. Wang; H. W. Wang; C. A. Whitten Jr.; T. Wise; A. Woodcraft; L. Zanotti; C. Zarra; B. X. Zhu; S. Zucchelli

2013-04-26T23:59:59.000Z

65

Temperature-dependent Raman and ultraviolet photoelectron spectroscopy studies on phase transition behavior of VO{sub 2} films with M1 and M2 phases  

SciTech Connect (OSTI)

Structural and electronic phase transitions behavior of two polycrystalline VO{sub 2} films, one with pure M1 phase and the other with pure M2 phase at room temperature, were investigated by temperature-controlled Raman spectroscopy and ultraviolet photoelectron spectroscopy (UPS). We observed characteristic transient dynamics in which the Raman modes at 195?cm{sup ?1} (V-V vibration) and 616?cm{sup ?1} (V-O vibration) showed remarkable hardening along the temperature in M1 phase film, indicating the rearrangements of V-V pairs and VO{sub 6} octahedra. It was also shown that the M1 Raman mode frequency approached those of invariant M2 peaks before entering rutile phase. In UPS spectra with high energy resolution of 0.03?eV for the M2 phase film, narrower V{sub 3d} band was observed together with smaller gap compared to those of M1 phase film, supporting the nature of Mott insulator of M2 phase even in the polycrystalline film. Cooperative behavior of lattice rearrangements and electronic phase transition was suggested for M1 phase film.

Okimura, Kunio, E-mail: okifn@keyaki.cc.u-tokai.ac.jp; Hanis Azhan, Nurul [Graduate School of Engineering, Tokai University, Hiratsuka 259-1292 (Japan); Hajiri, Tetsuya [UVSOR Facility, Institute for Molecular Science, Okazaki 444-8585 (Japan); Graduate School of Engineering, Nagoya University, Nagoya 464-8603 (Japan); Kimura, Shin-ichi [UVSOR Facility, Institute for Molecular Science, Okazaki 444-8585 (Japan); Graduate School of Frontier Biosciences, Osaka University, Suita 565-0871 (Japan); Zaghrioui, Mustapha; Sakai, Joe [GREMAN, UMR 7347 CNRS, Universit Franois Rabelais de Tours, Parc de Grandmont, 37200 Tours (France)

2014-04-21T23:59:59.000Z

66

CHROMOSPHERIC EVAPORATION IN AN M1.8 FLARE OBSERVED BY THE EXTREME-ULTRAVIOLET IMAGING SPECTROMETER ON HINODE  

SciTech Connect (OSTI)

We discuss observations of chromospheric evaporation for a complex flare that occurred on 2012 March 9 near 03:30 UT obtained from the Extreme-ultraviolet Imaging Spectrometer (EIS) on board the Hinode spacecraft. This was a multiple event with a strong energy input that reached the M1.8 class when observed by EIS. EIS was in raster mode and fortunately the slit was almost at the exact location of a significant energy input. Also, EIS obtained a full-CCD spectrum of the flare, i.e., the entire CCD was readout so that data were obtained for about the 500 lines identified in the EIS wavelength ranges. Chromospheric evaporation characterized by 150-200 km s{sup -1} upflows was observed in multiple locations in multi-million degree spectral lines of flare ions such as Fe XXII, Fe XXIII, and Fe XXIV, with simultaneous 20-60 km s{sup -1} upflows in million degree coronal lines from ions such as Fe XII-Fe XVI. The behavior of cooler, transition region ions such as O VI, Fe VIII, He II, and Fe X is more complex, but upflows were also observed in Fe VIII and Fe X lines. At a point close to strong energy input in space and time, the flare ions Fe XXII, Fe XXIII, and Fe XXIV reveal an isothermal source with a temperature close to 14 MK and no strong blueshifted components. At this location there is a strong downflow in cooler active region lines from ions such as Fe XIII and Fe XIV, on the order of 200 km s{sup -1}. We speculate that this downflow may be evidence of the downward shock produced by reconnection in the current sheet seen in MHD simulations. A sunquake also occurred near this location. Electron densities were obtained from density sensitive lines ratios from Fe XIII and Fe XIV. Atmospheric Imaging Assembly (AIA) observations from the Solar Dynamics Observatory are used with JHelioviewer to obtain a qualitative overview of the flare. However, AIA data are not presented in this paper. In summary, spectroscopic data from EIS are presented that can be used for predictive tests of models of chromospheric evaporation as envisaged in the Standard Flare Model.

Doschek, G. A.; Warren, H. P. [Space Science Division, Naval Research Laboratory, Washington, DC 20375 (United States)] [Space Science Division, Naval Research Laboratory, Washington, DC 20375 (United States); Young, P. R. [College of Science, George Mason University, 4400 University Drive, Fairfax, VA 22030 (United States)] [College of Science, George Mason University, 4400 University Drive, Fairfax, VA 22030 (United States)

2013-04-10T23:59:59.000Z

67

08.01.01.M1.02 Investigation and Resolution of Complaints Against Faculty Members for Illegal Discrimination, Sexual Harassment, or Related Retaliation Charges Page 1 of 5  

E-Print Network [OSTI]

a discrimination, sexual harassment or related retaliation complaint as provided by University Rule 08.01.01.M1. 1

Behmer, Spencer T.

68

BENDIX SYSTEMS DIVISION ANN A R8 oR, M1CH NO. REV.NO. Solar Wind Programming for  

E-Print Network [OSTI]

experiment program decommutates its own data, organizes it, processes it, and prepares it for output. Specifically, for Solar Wind, there is provision (using sense switches) for allowing or inhibiting the outputBENDIX SYSTEMS DIVISION ANN A R8 oR, M1CH NO. REV.NO. Solar Wind Programming for I I DPS 2000

Rathbun, Julie A.

69

Econometrics (26:223:554:01) Spring 2012 Thursdays, 10:00 AM-12:50 P.M., 1 Washington Park 512, Newark Campus  

E-Print Network [OSTI]

Econometrics (26:223:554:01) Spring 2012 Thursdays, 10:00 AM-12:50 P.M., 1 Washington Park 512://www.rci.rutgers.edu/~rpatrick/hp.html This is the first of two required econometrics courses for Ph.D. students in Finance and Economics. The purpose of this course is to develop basic econometric estimation and hypothesis testing tools necessary to analyze

Lin, Xiaodong

70

Econometrics (26:223:554:01) Spring 2013 Thursdays, 10:00 AM-12:50 P.M., 1 Washington Park 512, Newark Campus  

E-Print Network [OSTI]

Econometrics (26:223:554:01) Spring 2013 Thursdays, 10:00 AM-12:50 P.M., 1 Washington Park 512://www.rci.rutgers.edu/~rpatrick/hp.html This is the first of two required econometrics courses for Ph.D. students in Finance and Economics. The purpose of this course is to develop basic econometric estimation and hypothesis testing tools necessary to analyze

71

Econometrics (26:223:554:01) Spring 2011 Thursdays, 10:00 AM-12:50 P.M., 1 Washington Park 512, Newark  

E-Print Network [OSTI]

Econometrics (26:223:554:01) Spring 2011 Thursdays, 10:00 AM-12:50 P.M., 1 Washington Park 512://www.rci.rutgers.edu/~rpatrick/hp.html This is the first of two required econometrics courses for Ph.D. students in Finance and Economics. The purpose of this course is to develop basic econometric estimation and hypothesis testing tools necessary to analyze

Lin, Xiaodong

72

MagLab - Science Highlights Archive  

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

PDF file (summaries from 2008 on) or PowerPoint file (summaries prior to 2008). 2013 Science & Engineering Research Summaries Date Research Area Title Site Program Contact Aug....

73

MagLab - Science Show and Tell  

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

Arrow Meet the Magnets Arrow Q & A Arrow World Records Arrow By the Numbers Arrow Science Show & Tell Arrow Audio Slideshows Arrow History & Timeline Arrow Look Whos at the...

74

MagLab: NMR - MRI Publications  

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

J. Mol. Biol., 426 (2), 436-46 (2014) read online 17 Kaner, P.; Ruiz-Orta, C.; Boz, E.; Wagener, K.B.; Tasaki, M.; Tashiro, K. and Alamo, R.G., Kinetic Control of Chlorine...

75

MagLab - Barkhausen Effect Tutorial  

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

Effect During experiments carried out in 1919 involving magnetism and acoustics, German scientist Heinrich Barkhausen provided convincing evidence that iron and other...

76

MagLab - Magnets and Materials  

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

needed for everything from magnets for fusion, high energy physics, MRI, to electric power transmission lines and transformers. ASC and MS&T have particularly strong...

77

MagLab: Science in Tallahassee  

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

Tract also offers hiking and camping opportunities as well as the audio enhanced Living Forest trail where the trees tell their own stories. View Web site View Map Birdsong...

78

MagLab - Magic Angle Spinning Probe  

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

how far apart the atoms are and how they fit together. When the atoms respond to specific radio waves transmitted inside the magnet, they convey data about themselves that is...

79

Mag Lab Reports, Volume 15, Issue 1  

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

again. But the President capped all non-defense spending and Congress opted to meet this demand by (among other cuts) pulling roughly 1 billion from the anticipated level of 2008...

80

MagStar Technologies | 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 Auger11.Spain: Energy Resources Jump

Note: This page contains sample records for the topic "maldives mag m1" 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.


81

a. Lngsamt & adiabatiskt reversibel, dvs en isentropisk process V1 = nRT1 / p1 = (m/M) RT1/p1 , massa m = 1 kg  

E-Print Network [OSTI]

Svar 1303: a. Långsamt & adiabatiskt reversibel, dvs en isentropisk process V1 = n·R·T1 / p1 = (m/M) ·R·T1/p1 , massa m = 1 kg H2 : M = 0.002 kg/mol; CO : M = 0.028 kg/mol; CO2 : M = 0.044 kg/mol p1 = z bar V1 = (R/M) · (300 + 50·a) / z m3 . t.ex. 30066 : p = 3 bar, gas = CO, T1 = 450 K V1 = 0.445 m3

Zevenhoven, Ron

82

Sandia National Laboratories: M-1  

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 Spoerke SSLS ExhibitIowaLos Alamos National LaboratoryEngineers

83

Propane ammoxidation over the Mo-V-Te-Nb-O M1 phase: Reactivity of surface cations in hydrogen abstraction steps  

SciTech Connect (OSTI)

Density functional theory calculations (GGA-PBE) have been performed to investigate the adsorption of C3 (propane, isopropyl, propene, and allyl) and H species on the proposed active center present in the surface ab planes of the bulk Mo-V-Te-Nb-O M1 phase in order to better understand the roles of the different surface cations in propane ammoxidation. Modified cluster models were employed to isolate the closely spaced V=O and Te=O from each other and to vary the oxidation state of the V cation. While propane and propene adsorb with nearly zero adsorption energy, the isopropyl and allyl radicals bind strongly to V=O and Te=O with adsorption energies, {Delta}E, being {le} -1.75 eV, but appreciably more weakly on other sites, such as Mo=O, bridging oxygen (Mo-O-V and Mo-O-Mo), and empty metal apical sites ({Delta}E > -1 eV). Atomic H binds more strongly to Te = O ({Delta}E {le} -3 eV) than to all the other sites, including V = O ({Delta}E = -2.59 eV). The reduction of surface oxo groups by dissociated H and their removal as water are thermodynamically favorable except when both H atoms are bonded to the same Te=O. Consistent with the strong binding of H, Te=O is markedly more active at abstracting the methylene H from propane (E{sub a} {le} 1.01 eV) than V = O (E{sub a} = 1.70 eV on V{sup 5+} = O and 2.13 eV on V{sup 4+} = O). The higher-than-observed activity and the loose binding of Te = O moieties to the mixed metal oxide lattice of M1 raise the question of whether active Te = O groups are in fact present in the surface ab planes of the M1 phase under propane ammoxidation conditions.

Muthukumar, Kaliappan [University of Cincinnati; Yu, Junjun [University of Cincinnati; Xu, Ye [ORNL; Guliants, Vadim V. [University of Cincinnati

2011-01-01T23:59:59.000Z

84

A class of infinite-dimensional representations of the Lie superalgebra osp(2m+1|2n) and the parastatistics Fock space  

E-Print Network [OSTI]

An orthogonal basis of weight vectors for a class of infinite-dimensional representations of the orthosymplectic Lie superalgebra osp(2m+1|2n) is introduced. These representations are particular lowest weight representations V(p), with a lowest weight of the form [-p/2,...,-p/2|p/2,...,p/2], p being a positive integer. Explicit expressions for the transformation of the basis under the action of algebra generators are found. Since the relations of algebra generators correspond to the defining relations of m pairs of parafermion operators and n pairs of paraboson operators with relative parafermion relations, the parastatistics Fock space of order p is also explicitly constructed. Furthermore, the representations V(p) are shown to have interesting characters in terms of supersymmetric Schur functions, and a simple character formula is also obtained.

Stoilova, N I

2015-01-01T23:59:59.000Z

85

STEM HAADF Image Simulation of the Orthorhombic M1 Phase in the Mo-V-Nb-Te-O Propane Oxidation Catalyst  

SciTech Connect (OSTI)

A full frozen phonon multislice simulation of high angle annular dark field scanning transmission electron microscopy (HAADF STEM) images from the M1 phase of the Mo-V-Nb-Te-O propane oxidation catalyst has been performed by using the latest structural model obtained using the Rietveld method. Simulated contrast results are compared with experimental HAADF images. Good agreement is observed at ring sites, however significant thickness dependence is noticed at the linking sites. The remaining discrepancies between the model based on Rietveld refinement and image simulations indicate that the sampling of a small volume element in HAADF STEM and averaging elemental contributions of a disordered site in a crystal slab by using the virtual crystal approximation might be problematic, especially if there is preferential Mo/V ordering near the (001) surface.

D Blom; X Li; S Mitra; T Vogt; D Buttrey

2011-12-31T23:59:59.000Z

86

MagLab News: MagLab to Celebrate Significant Milestone in Large...  

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

as they prepare to ship a critical section of a new record-breaking magnet to Germany. The magnet's cold mass is lifted by a crane. The 7.2 ton cold-mass of the series...

87

Adsorption of propane, isopropyl, and hydrogen on cluster models of the M1 phase of Mo-V-Te-Nb-O mixed metal oxide catalyst  

SciTech Connect (OSTI)

The Mo-V-Te-Nb-O mixed metal oxide catalyst possessing the M1 phase structure is uniquely capable of directly converting propane into acrylonitrile. However, the mechanism of this complex eight-electron transformation, which includes a series of oxidative H-abstraction and N-insertion steps, remains poorly understood. We have conducted a density functional theory study of cluster models of the proposed active and selective site for propane ammoxidation, including the adsorption of propane, isopropyl (CH{sub 3}CHCH{sub 3}), and H which are involved in the first step of this transformation, that is, the methylene C-H bond scission in propane, on these active site models. Among the surface oxygen species, the telluryl oxo (Te=O) is found to be the most nucleophilic. Whereas the adsorption of propane is weak regardless of the MO{sub x} species involved, isopropyl and H adsorption exhibits strong preference in the order of Te=O > V=O > bridging oxygens > empty Mo apical site, suggesting the importance of TeO{sub x} species for H abstraction. The adsorption energies of isopropyl and H and consequently the reaction energy of the initial dehydrogenation of propane are strongly dependent on the number of ab planes included in the cluster, which points to the need to employ multilayer cluster models to correctly capture the energetics of surface chemistry on this mixed metal oxide catalyst.

Govindasamy, Agalya [University of Cincinnati; Muthukumar, Kaliappan [University of Cincinnati; Yu, Junjun [University of Cincinnati; Xu, Ye [ORNL; Guliants, Vadim V. [University of Cincinnati

2010-01-01T23:59:59.000Z

88

CMS Videos & Magnet M1 Website  

E-Print Network [OSTI]

Doing 8 weeks internship in CERN gave me the opportunity to learn new skills and experiences. CERN is an organization where they operate the world's largest particle physics laboratory. Working on projects as a student is important to prepare for the work after the graduation. In this report, I will discuss the projects that I was assigned to, which are website upgrading, sketching drawings, and video editing, and present the results and compare them with the old ones.

Almakhrazi, Majed Ahmed

2014-01-01T23:59:59.000Z

89

jp501776m 1..11  

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

Strain Effects on the Water-Graphene Interfacial and Confinement Behavior Ariel A. Chialvo,* , Lukas Vlcek, , and Peter T. Cummings Chemical Sciences Division...

90

Cours de Sismologie M1 R. Madariaga  

E-Print Network [OSTI]

stations: jij ttr ,obsiobs,,obs -= 11 ---= k kjk k kikij xx c xx c r 2 0 2 0,calc )( 1 )( 1 On localise

Madariaga, Raúl

91

MagLab - Pioneers in Electricity and Magnetism: Lev Davidovich...  

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

Lev Davidovich Landau (1908-1968) Lev Davidovich Landau While growing up in the Soviet Union, Lev Landau was so far ahead of his classmates that he was ready to begin college at...

92

Fine coal cleaning via the micro-mag process  

DOE Patents [OSTI]

A method of cleaning particulate coal which is fed with a dense medium slurry as an inlet feed to a cyclone separator. The coal particle size distribution is in the range of from about 37 microns to about 600 microns. The dense medium comprises water and ferromagnetic particles that have a relative density in the range of from about 4.0 to about 7.0. The ferromagnetic particles of the dense medium have particle sizes of less than about 15 microns and at least a majority of the particle sizes are less than about 5 microns. In the cyclone, the particulate coal and dense-medium slurry is separated into a low gravity product stream and a high gravity produce stream wherein the differential in relative density between the two streams is not greater than about 0.2. The low gravity and high gravity streams are treated to recover the ferromagnetic particles therefrom.

Klima, Mark S. (Finleyville, PA); Maronde, Carl P. (McMurray, PA); Killmeyer, Richard P. (Pittsburgh, PA)

1991-01-01T23:59:59.000Z

93

Mag Lab Reports - Volume 17 No. 3.indd  

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

indentifi ed by negative ESI at >1% relative abundance in either phase of the pine pellet pyrolysis product. Biomass pyrolysis products are dominated by O x species, whereas the...

94

MagLab - Science in Literature: Chapter Books  

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

Books Chapter books for intermediate grades and middle school provide a rich source of science-related material. Students will make their own connections to classroom science and...

95

MagLab - Science in Literature: Science Fiction  

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

Science Fiction Here are some titles for readers not afraid to venture beyond the realm of the known and comfortable. Science fiction gives writers and their audience the chance to...

96

MagLab - Science in Literature: Non-Fiction  

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

and other sciences to poignant stories chronicling the transformative effects of science on people's lives. Awakenings Awakenings Author: Oliver Sacks Ages: Adults and young...

97

MagLab - Science in Literature: Science Education  

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

Books on Science Education Science and the art of teaching are forever evolving. These books help educators stay ahead of the curve with new ideas, strategies and activities to...

98

MagLab - Pioneers in Electricity and Magnetism: William Gilbert  

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

William Gilbert (1544-1603) William Gilbert William Gilbert was an English physician and natural philosopher who wrote a six-volume treatise that compiled all the information...

99

MagLab - Pioneers in Electricity and Magnetism  

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

list chronologically View list alphabetically William Gilbert William Gilbert (1544-1603) - William Gilbert was an English physician and natural philosopher who wrote a...

100

New MagViz Airport Liquid Analysis System Undergoes Testing  

ScienceCinema (OSTI)

LOS ALAMOS, New Mexico, December 16, 2008?An innovative application of a technology first used for medical imaging may enhance airport security if Los Alamos National Laboratory scientists are successful. Los Alamos technologists have adapted Magnetic Res

None

2010-01-08T23:59:59.000Z

Note: This page contains sample records for the topic "maldives mag m1" 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

CAMEL: Concept Annotated iMagE Libraries  

E-Print Network [OSTI]

Haar wavelet signature for each sliding window, and then clustering all window signatures in order to identify regions with homogeneous wavelet signatures. For a detailed description of the WALRUS system and its components see.12 The new functionality... Sliding window generator Wavelet signature clustering Dynamic Haar wavelet Region feature extraction module WALRUS system CAMEL system Figure 3. Architecture of the CAMEL system The last piece of new functionality includes the Concept Interpreter...

Natsev, Apostol; Chadha, Atul; Soetarman, Basuki; Vitter, Jeffrey Scott

2001-01-01T23:59:59.000Z

102

MagLab - Pioneers in Electricity and Magnetism: Carl Friedrich...  

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

Gauss to develop various surveying improvements. Most notably, he invented the heliotrope (a device that used a mirror to magnify the rays of the sun in order to send signals...

103

Mag.Dr. Bernhard Kron, Privatdoz. Wienerwaldgymnasium BG/BRG  

E-Print Network [OSTI]

wie GAM und Google SketchUp) · Alleinverantwortlicher Lehrer f¨ur das schulautonome Unterrichtsfach

Fulmek, Markus

104

Mag-Foot: a steel bridge inspection robot  

E-Print Network [OSTI]

A legged robot that moves across a steel structure is developed for steel bridge inspection. Powerful permanent magnets imbedded in each foot allow the robot to hang from a steel ceiling powerlessly. Although the magnets ...

Asada, Harry

105

MagLab - Timeline of Electricity and Magnetism: 1940 - 1959  

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

and Calculator (ENIAC) was designed to speed the calculation and improve the accuracy of firing and bombing tables. Fueled by new technologies, computers ever since have become...

106

Mag Lab Safety Policy: Magnet Cell Safety Procedures  

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

experiments. Two people make fewer mistakes, solve problems quicker, do experimental procedures quicker, and generally make more efficient use of magnet time. This becomes...

107

MagLab - Pioneers in Electricity and Magnetism: Heinrich Hertz  

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

Heinrich Hertz (1857-1894) Heinrich Hertz German physicist Heinrich Hertz discovered radio waves, a milestone widely seen as confirmation of James Clerk Maxwells electromagnetic...

108

MagLab - Timeline of Electricity and Magnetism: 1890 - 1899  

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

- 1939 1940 - 1959 1960 - 1979 1980 - 2003 During experiments with cathode ray tubes, German physicist Wilhelm Roentgen discovered a previously unknown form of electromagnetic...

109

MagLab - Pioneers in Electricity and Magnetism: Walther Meissner  

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

Walther Meissner (1882-1974) Walther Meissner Fritz Walther Meissner was born on December 16, 1882, in Berlin, Germany. He studied mechanical engineering at the Technische...

110

MagLab - Timeline of Electricity and Magnetism: 1775 - 1799  

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

were not fully understood, many ideas we consider strange today continued to thrive. German physician Anton Mesmer claimed he could cure a broad range of ailments with a type of...

111

MagLab - Timeline of Electricity and Magnetism: 1840 - 1849  

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

Maxwell. Other scientists applying their intellect to theoretical questions included German physicist Wilhelm Weber, who attempted (unsuccessfully) to bring together all existing...

112

MagLab - Timeline of Electricity and Magnetism: 1900 - 1909  

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

classical mechanics. The field of quantum mechanics was born. Audion Triode In 1900, German physicist Max Planck published a theory suggesting that atoms did not release their...

113

MagLab - Pioneers in Electricity and Magnetism: Heinrich Friedrich...  

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

magnetism, but they knew almost nothing about the relationship between the two. Baltic German physicist Heinrich Lenz took the first step toward filling this gap with his...

114

MagLab - Pioneers in Electricity and Magnetism: Werner Siemens  

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

Werner von Siemens (1816-1892) Werner von Siemens Werner Siemens, the fourth of 14 children born to a tenant farmer and his wife, entered the world on December 13, 1816, in Lenthe,...

115

MagLab - Pioneers in Electricity and Magnetism: Siegmund Loewe  

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

Siegmund Loewe (1885-1962) Siegmund Loewe Siegmund Loewe was a German engineer and businessman who developed vacuum tube forerunners of the modern integrated circuit. He pioneered...

116

MagLab - Timeline of Electricity and Magnetism: 1850 - 1869  

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

Alliance Company was founded in Paris and began manufacturing machines for generating electric current that evolved over the years. In 1858, the glow of the first electrified...

117

MagLab - Timeline of Electricity and Magnetism: 1910 - 1929  

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

the world, station KDKA in Pittsburgh, Pennsylvania, is launched by the Westinghouse Electric and Manufacturing Company. 1922 Neon tube lighting becomes available commercially and...

118

MagLab - Kids Web Resources on Electricity and Magnetism  

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

Web Resources for Kids This is your launch pad to dozens of adventures, games and interactive activities, offered on science sites designed just for kids. With lots of content on...

119

MagLab - Science in Literature: Picture Books  

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

global warming. Plainly and frankly, it touches on topics such as deforestation, greenhouse effect, rising sea levels, the threat to animals and weather extremes. But the book is...

120

MagLab - Pioneers in Electricity and Magnetism: Svante Arrhenius  

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

to many prominent chemists around the world. One of these chemists, Wilhelm Ostwald of Germany, was so intrigued by the paper that he traveled to Uppsala to meet Arrhenius and...

Note: This page contains sample records for the topic "maldives mag m1" 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

MagLab - Pioneers in Electricity and Magnetism: Gerd Binning  

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

Gerd Binnig (1947-Present) Gerd Binnig A native of Germany, the physicist Gerd Binning co-developed the scanning tunneling microscope (STM) with Heinrich Rohrer while the pair...

122

MagLab - RET Blog 2013: Erin Smidt  

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

never heard about either. ITER (pronounced eater) is an acronym for International Thermonuclear Experimental Reactor. ITER is an international fusion project that sounds...

123

Climate Mag_27JUN2013_ms07022013.indd  

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

development of validated parameterizations of new carbon- climate feedbacks for Earth System Models. LANL is also working with Chevron and DOE Fossil Energy on measuring CH 4...

124

EA-306 MAG Energy Solutions, Inc. | 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 in Review: TopEnergy DOEDealingVehicle1 Closing American Electric Power80AC3-AB WPSB3-A

125

EA-306-A MAG Energy Solutions, Inc. | 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 in Review: TopEnergy DOEDealingVehicle1 Closing American Electric Power80AC3-AB WPSB3-A-A

126

Climate Mag_27JUN2013_ms07022013.indd  

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 User Group and Userof aChristinaCliff joins EMSL

127

MagLab - Meet the Magnets: 45 Tesla Hybrid  

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

Features > Meet the Magnets Meet the Magnets Choose a Magnet 45 Tesla Hybrid 900 MHz NMR Magnet 25 Tesla Split Magnet 14.5 Tesla ICR Magnet 100 Tesla Multi-shot Magnet 600 MHz...

128

MagLab: 45 Tesla Hybrid Magnet - Publications  

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

Magnets & Facilities > Hybrid Magnet Arrow Publications Featuring Data from the 45 Tesla Hybrid Magnet The hybrid magnet was commissioned in December 1999. Nature, Nature Physics,...

129

MagLab - Travel Information to Los Alamos  

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

Shipping address: Los Alamos National Laboratory Attn: RECIPIENT NAME NHMFL, MS E536 Bikini Atoll Road, SM-30 TA-35127O1U Los Alamos, NM 87545 For more information please...

130

Radiative rates for E1, E2, M1, and M2 transitions in the Br-like ions Sr IV, Y V, Zr VI, Nb VII, and Mo VIII  

E-Print Network [OSTI]

Energies and lifetimes are reported for the lowest 375 levels of five Br-like ions, namely Sr~IV, Y~V, Zr~VI, Nb~VII, and Mo~VIII, mostly belonging to the 4s$^2$4p$^5$, 4s$^2$4p$^4$4$\\ell$, 4s4p$^6$, 4s$^2$4p$^4$5$\\ell$, 4s$^2$4p$^3$4d$^2$, 4s4p$^5$4$\\ell$, and 4s4p$^5$5$\\ell$ configurations. Extensive configuration interaction has been included and the general-purpose relativistic atomic structure package ({\\sc grasp}) has been adopted for the calculations. Additionally, radiative rates are listed among these levels for all E1, E2, M1, and M2 transitions. From a comparison with the measurements, the majority of our energy levels are assessed to be accurate to better than 2\\%, although discrepancies between theory and experiment for a few are up to 6\\%. An accuracy assessment of the calculated radiative rates (and lifetimes) is more difficult, because no prior results exist for these ions.

Aggarwal, K M

2015-01-01T23:59:59.000Z

131

Motif list Expression data Motif combination (M1)  

E-Print Network [OSTI]

pm #12;K T k k PI score PID(M) PID(R ) PI score = log (PID(M)/PID(R)) PID(M) PID(R ) k k k 0.2-0.3 0

132

THfE UNIIVEIITY M1athematics Research  

E-Print Network [OSTI]

ANALYSIS Karl Nickel This document has been approved for public release and sale; its distribution) by the following interval Newton method: -2- #1136 #12;X(0) · ·(0) "appropriate" ;Ev' := n ,fxvXV (4) x(v+l) E ·(v

Kreinovich, Vladik

133

SAMPLING METHODS: A LIST OF SOURCES M.1 Introduction  

E-Print Network [OSTI]

for sampling methods are available through online literature databases; Federal, State, and university libraries; the internet; and other sources. M.2 List of Sources Department of Energy (DOE). 1987, Safety, and Health, Office of Environmental Audit, Washington, D.C. ! General Description of Document

134

Molecular analysis of Streptococcus pyogenes M1 protein  

E-Print Network [OSTI]

Bakers dimercurial uranyl nitrate hexahydrate potassiumIII) nitrate potassium hexachloroplatinate uranyl acetate

McNamara, Case W.

2006-01-01T23:59:59.000Z

135

Energy (cm-1 MolarExtinctionCoefficient(M-1  

E-Print Network [OSTI]

Chloroform Dichloromethane Acetonitrile -3 -2 -1 0 1 2 3 4 5 -1 Time (ps) OD(mOD) -0.8 -0.6 -0.4 -0.2 0 0.2 0 in acetonitrile following photoexcitation at 266 nm. Measured at probe frequencies ranging from1820 cm-1 to 1920- stretch fundamental transition of ClNO dis- solved in acetonitrile following 266-nm pho- tolysis

Reid, Philip J.

136

ARM - VAP Product - visstpx04m1rv1minnis  

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 Depth (AOD)Productssondeadjustsondeadjust Documentation Data Managementg15v4minnis Documentation visst :

137

ARM - VAP Product - visstpx04m1rv3minnis  

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 Depth (AOD)Productssondeadjustsondeadjust Documentation Data Managementg15v4minnis Documentation visst :rv3minnis

138

ARM - VAP Product - visstpx04m1rv4minnis  

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 Depth (AOD)Productssondeadjustsondeadjust Documentation Data Managementg15v4minnis Documentation visst

139

ARM - VAP Product - visstpx08m1rv4minnis  

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 Depth (AOD)Productssondeadjustsondeadjust Documentation Data Managementg15v4minnis Documentation

140

Group M1 Response to the Snowmass 2001 Charge Working Group M1: Muon-Based Accelerators  

E-Print Network [OSTI]

; cost-effective longitudinal manipulation and ionization cooling techniques for reducing transverse emittance; and rapid and efficient acceleration techniques that accommodate large longitudinal, but requirements are more severe. Emittance reduction must include longitudinal cooling ("emittance exchange

Note: This page contains sample records for the topic "maldives mag m1" 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

MagLab - Science in Literature: Fiction for Grown-Ups  

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

Fiction for Grown-Ups Skillful authors weave real science into plots featuring swashbuckling heroes, famed physicists and a Dorothy clone lost not in the Land of Oz, but of Quarks....

142

PPG and MAG Team Up for Turbine Blade Research | Department of...  

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

and researchers with the opportunity to develop less expensive, better-performing carbon fiber materials and manufacturing processes. Pictured here is the carbon fiber...

143

20 Trains MAY 2008 www.TrainsMag.com 21 By DAVID LUSTIG  

E-Print Network [OSTI]

's Topeka, Kan., shops. The two say the fuel cell locomotive has the po- tential to reduce air pollution the oxygen used by a fuel cell comes from the air, while the hydrogen must be provided. Electricity needed been used in mining.

Barkan, Christopher P.L.

144

MagLab - Pioneers in Electricity and Magnetism: Sir Humphry Davy  

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

Humphry Davy (1778-1829) Humphry Davy Humphry Davy was a pioneer in the field of electrochemistry who used electrolysis to isolate many elements from the compounds in which they...

145

Total number of Mag Lab employees 360 Percentage of employees with PhDs 36  

E-Print Network [OSTI]

Capacity, in megawatts, of the motor generator powering the pulsed magnets at the lab's Los Alamos National,400,000 Magnetic field, in tesla2 , of the lab's hybrid magnet, which creates the most powerful sustained magnetic, at which chilled water is run through resistive magnets to keep them cold 45 Magnetic field, in tesla

Weston, Ken

146

MagLab Education: FREEDM Systems Center Pre-college Education...  

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

participants knowledge of electrical power production, with a focus on renewable energy resources. The goals are to: Develop and assess long-term partnerships with middle and...

147

MagLab Reports, Volume 19, No. 2 (Summer 2012): The 2011 Highlights...  

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

19 No. 2 Table of ConTenTs 48 4 53 featuRes ReseaRch stORIes Condensed matter sCienCe Graphene, Kondoheavy fermion systems, magnetism & magnetic materials, molecular conductors,...

148

Proof-of-Concept Simulations of The Magnetic Null (MagNul) Thruster  

E-Print Network [OSTI]

. Choueiri Electric Propulsion and Plasma Dynamics Laboratory, Princeton, New Jersey, 08544, USA Plasma of the simula- tions upheld the concept's presumed ability to accelerate plasma in a desired direction intrinsic advantages that deserve further study. The design is inherently steady state and electrodeless

Choueiri, Edgar

149

DROPLET FEATURES EXTRACTION WITH A DYNAMIC ACTIVE CONTOUR FOR MIG/MAG  

E-Print Network [OSTI]

velocity. All these measurements are sampled synchronously with a high speed video system operating of the im- ages. However our images are too complex to expect local, low level operations to generate are well detected. This approach enables the estimation of the relevant variables in the establishment

Paris-Sud XI, Université de

150

A review of the MAg internship on the Southworth Ranch, Seneca, Oregon  

E-Print Network [OSTI]

ALLOTMENIS ANNUAL OPERATING PLAN ~10 MANAGEMENT OF LIVESTOCK GRAZING SYSTEM The Allotment Management Plan for your Allotments contains a grazing system that has been developed to fit the particular needs of your operation and your allotment. With minor... variations, this schedule needs to be followed over the long term if the system is to be effective in managing the resources. Included with this annual plan is a schedule for this years pasture moves and the utilization standards for each pasture...

Nydam, Trace S.

1990-01-01T23:59:59.000Z

151

MagLab - Pioneers in Electricity and Magnetism: Georg Simon Ohm  

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

roots and struggled financially most of his life. Despite those disadvantages, the German physicist is well known today for his formulation of a law, termed Ohms law,...

152

MagLab - Pioneers in Electricity and Magnetism: Charles-Augustin...  

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

on topics ranging from mathematical solutions of engineering problems to studies of friction, elasticity, electricity and magnetism. In 1777 Coulomb was awarded part of the...

153

Volume 19, No. 1 of MagLab Reports (Spring 2012)  

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

for a tunnel diode oscillator (TDO) cir- cuit, where changes in sample resistance are observed by a shift in the resonant circuit frequency. Magnetic fi eld was pro- vided by a 16...

154

Af projektleder, mag.scient., ph.d. Bernhard Bierlich, Center for Afrikastudier, Kbenhavns Universitet  

E-Print Network [OSTI]

-projektet i 2006-2007 var nyskabende og benyt- tede en virkningsfuld analytisk blanding af antropologiske og. Diverse kontakter kom i stand, især med leder af Extension Service, Kwame Boateng. Forskningen på øerne

155

Mineralogy and diagenesis of Gulf Coast Tertiary shales Ann-Mag Field, Brooks County, Texas  

E-Print Network [OSTI]

composition with increasing depth of burial provides evidence of systematic diagenetic conversions (Boles and Franks, 1979; Hower et al. , 1976; Perry and Hower, 1972; Weaver and Beck, 1971; Dunoyer De Segonzac, 1970; Burst, 1969; Powers, 1967). When... not be neglected, many workers have shown that significant mineral ogic changes do occur due to diagenesi s of clay minerals from the same source (Boles and Franks, 1979; Hower, et al. , 1976; Perry and Hower, 1972; Dunoyer De Segonzac, 1970; Burst, 1969). Also...

Bott, Winston Frederick

1985-01-01T23:59:59.000Z

156

MagLab - The largest and highest powered magnet lab in the world  

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 Jun Jul(Summary)morphinanInformation InInformation InExplosion Monitoring:Home|Physics Research High-Energy- Density

157

Application to Export Electric Energy OE Docket No. EA-306-A MAG 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 EnergyEnergy Cooperation |South42.2 (April 2012)Tie Ltd | Department

158

Application to Export Electric Energy OE Docket No. EA-306-A MAG 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 EnergyEnergy Cooperation |South42.2 (April 2012)Tie Ltd | DepartmentSolutions: Federal Register Notice

159

MagLab - Cell 15: 45.1 Tesla / 32 mm Hybrid Magnet  

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

Magnets & Facilities Arrow Cell 15: 45.1 Tesla 32 mm Hybrid Magnet The labs flagship magnet, the 45 T Hybrid, is composed of a 33.5 T resistive magnet nested in an 11.5 T...

160

MagLab - Series Connected Hybrid for the Helmholtz Centre Berlin  

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

based on the Magnet Labs Series-Connected Hybrid concept, will be housed at the Berlin Neutron Scattering Center. The magnet will produce a magnetic field between 25 tesla and...

Note: This page contains sample records for the topic "maldives mag m1" 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

Neutron Scattering at 25 Teslas: MagLab Completes Conical Bore...  

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

central field with a unique conical warm bore with 30 degree opening angles suitable for neutron scattering experiments. Development and fabrication of this Conical Bore Resistive...

162

INSTALLATION MAG~NiX.ILRI DIVI8ION, CAN.fAN,CONN.  

Office of Legacy Management (LM)

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) "ofEarlyEnergyDepartment ofDepartment ofof EnergyYou$ EGcG ENERGYELIkNATIONHEALXH: l ._I * .z-y:c*f -:;

163

ECS Journal of Solid State Science and Technology, 1 (1) M1-M5 (2012) M1 2162-8769/2012/1(1)/M1/5/$28.00 The Electrochemical Society  

E-Print Network [OSTI]

, Lamar University, Beaumont, Texas 77710, USA bDepartment of Chemistry and Biochemistry, Lamar University

Guo, John Zhanhu

164

International reserves management and the current account  

E-Print Network [OSTI]

Guyana Indonesia Jordan Kazakhstan Kyrgyz Republic Laoof Iraq Jamaica Jordan Kazakhstan Macedonia, FYR MaldivesJamaica Japan Jordan Kazakhstan Kenya Korea Kuwait Kyrgyz

Aizenman, Joshua

2007-01-01T23:59:59.000Z

165

Honduras-Program for Scaling Up Renewable Energy in Low Income...  

Open Energy Info (EERE)

Kenya Specific Documents4 Maldives Specific Documents5 Mali Specific Documents6 Nepal Specific Documents7 Overview "The Scaling-Up Renewable Energy Program for Low Income...

166

Kenya-Program for Scaling Up Renewable Energy in Low Income Countries...  

Open Energy Info (EERE)

Kenya Specific Documents4 Maldives Specific Documents5 Mali Specific Documents6 Nepal Specific Documents7 Overview "The Scaling-Up Renewable Energy Program for Low Income...

167

South Asia Regional Initiative for Energy Cooperation and Development...  

Open Energy Info (EERE)

ourwork Country Afghanistan, Pakistan, Bhutan, India, Sri Lanka, Bangladesh, Nepal, Maldives Southern Asia, Southern Asia, Southern Asia, Southern Asia, Southern Asia,...

168

Mali-Program for Scaling Up Renewable Energy in Low Income Countries...  

Open Energy Info (EERE)

Kenya Specific Documents4 Maldives Specific Documents5 Mali Specific Documents6 Nepal Specific Documents7 Overview "The Scaling-Up Renewable Energy Program for Low Income...

169

E-Print Network 3.0 - arab jamahiriya malaysia Sample Search...  

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

d... Dominica 180 Malaysia 165 Dominican Republic 157 Maldives 178 Ecuador 137 Mali 225 Egypt 177 Marshall... Uganda 184 Sierra Leone 141 Ukraine 280 Singapore 335 United Arab...

170

E-Print Network 3.0 - argentina brazil chile Sample Search Results  

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

Malaysia Maldives Mali Malta Chad Chile China Colombia Comoros Tajikistan Tanzania Thailand Togo Mauritania Source: Alechina, Natasha - School of Computer Science,...

171

Part I--Mechanics J04M.1--Bead on a Wire (J06M.3) J04M.1--Bead on a Wire (J06M.3)  

E-Print Network [OSTI]

axis with constant angular velocity . Earth's gravity causes acceler- ation g in the negative z Law Central Force (J06M.2) Problem A particle of mass m moves in an attractive, power-law central force, F r-n . Define constant k so that the potential energy is U(r) = - k rn-1 . The particle is set

Petta, Jason

172

Geol. Mag. 149 (4), 2012, pp. 743749. c Cambridge University Press 2012 743 doi:10.1017/S0016756812000131  

E-Print Network [OSTI]

of oxygen in deep water strongly questions current thinking about anoxia throughout the Archaean, making0016756812000131 RAPID COMMUNICATION A deep subaqueous fan depositional model for the Palaeoarchaean (3.46 Ga, France §ChemCam team, Mars Science Laboratory project ¶Earthbyte Group, School of Geosciences

Boyer, Edmond

173

IEEE TRANSACTIONS ON MAGNETICS, VOL. MAG-23, NO. 2, MARCH 1987 Transport Propertiesof a Superconductor-Semiconductor Ohmic Contact  

E-Print Network [OSTI]

a Superconductor-Semiconductor Ohmic Contact A. Davidson, M.J. Brady, D.J. Frank, J. M. Woodall, and A. Kleinsasser of the proposed superconducting-base, semiconductor-isolated transistor (SUBSIT), lackingonly the emitter tunnel named SUBSIT (for Superconducting-Base Semiconductor-Isolated Transistor). Experimentally, Silver could

Woodall, Jerry M.

174

Tasks for tests and A-levels using CAS Heidi Metzger-Schuhker, Mag. Commercial Highschool HORN, Austria  

E-Print Network [OSTI]

, Austria ACDCA (Austrian Center for Didactics of Computer Algebra) heidi.metzger@hakhorn.ac.at Abstract://www.acdca.ac.at (Website of the Austrian Center for Didactics of Computer Algebra) 1. Initial situation If mathematics (Austrian Center for Didactics of Computer Algebra). For the vocational school system ­ especially

Spagnolo, Filippo

175

Calculations of helical twisting powers from intermolecular torques David J. Earla)  

E-Print Network [OSTI]

helical twisting power HTP M Pcwr 1 , 1 where P is the helical pitch of the phase induced by the dopant in designing molecules with high HTP values 100 m 1 .4 In this case, a small quantity of chiral dopant can that each individual conformation of a flexible dopant can have a different mag- nitude for its HTP

Wilson, Mark R.

176

Water/Wastewater Engineering Report (Storm Sewer/Infiltration Sanitary Sewage Separation-M1 Model)  

E-Print Network [OSTI]

Consumption Due to Rain......................... 21 Table 10. Annual and OSD Period Electricity Savings.................................................... 22 Table 11. Calculation of Growth Factor from 1999 to 2007.../2010. .................................. 22 Table 12. Electricity Savings in 2007 and 2010 Using Base Year 1999.......................... 22 Table 13. Calculation of Growth Factor from 2002 to 2007/2010. .................................. 22 Table 14. Electricity Savings in 2007 and 2010...

Liu, Z.; Brumbelow, K.; Haberl, J. S.

2006-10-30T23:59:59.000Z

177

08.01.01.M1 Civil Rights Compliance Page 1 of 3 UNIVERSITY RULE  

E-Print Network [OSTI]

: Discrimination, sexual harassment, or related retaliation complaint procedures are initiated by filing for the receipt, investigation, and resolution of discrimination, sexual harassment, or related retaliation complaints as required by System Regulation 08.01.01 Sections 1.1 and 1.2. Rule and Responsibilities 1

Behmer, Spencer T.

178

TP 1 M1 Informatique Apprentissage Automatique Premi`eres classifications : apprentissage et evaluation  

E-Print Network [OSTI]

de crit`eres observ´es sur 3 esp`eces diff´erentes d'iris de Gasp´esie (Setosa, Versicolor, Verginica suivant : def plot_2D(data, target, target_names): colors = cycle('rgbcmykw') # cycle de couleurs target_ids = range(len(target_names)) pl.figure() for i, c, label in zip(target_ids, colors, target_names): Universit

Denis, François

179

TP 1 M1 Informatique Apprentissage Automatique Premi`eres classifications : apprentissage et evaluation  

E-Print Network [OSTI]

de crit`eres observ´es sur 3 esp`eces diff´erentes d'iris de Gasp´esie (Setosa, Versicolor, Verginica suivant : def plot_2D(data, target, target_names): colors = cycle('rgbcmykw') # cycle de couleurs target_ids = range(len(target_names)) pl.figure() for i, c, label in zip(target_ids, colors, target_names): pl

Denis, François

180

A.E. K.Ris Ris -M -1 ^ 5 Title and author(s)  

E-Print Network [OSTI]

Department or group Metallurgy Group's own registration number(s) A 180 Copies to Library (100) A.R. Mackintosh N.V. Holm C F . Jacobsen F. Juul Metallurgy (40) #12;ISBN nr - B7-!>50-023&-6 - 2 - 1

Note: This page contains sample records for the topic "maldives mag m1" 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

M1G / M2G Rotation Summaries Thursday, August 15th  

E-Print Network [OSTI]

in Japan, and two years of part time study at Western Michigan University's Department of Paper Science State football game Medical Scientist Training Program The University of Iowa 2206 MERF, Iowa City, IA on Faculty" video 5:00 pm Photo Expedition and Ice Breaker 6:30 pm Dinner at Moonrakers 126 E. Washington St

Engelhardt, John F.

182

Du, X., Kockelman, K. M. 1 1 TRACKING TRANSPORTATION AND INDUSTRIAL PRODUCTION ACROSS A  

E-Print Network [OSTI]

commodities highlight the importance of food 35 and petroleum manufacturing sectors, in terms of production expansions) and exogenous economic shocks (e.g., increases in14 export demands).15 Other spatial IO commodity flows and transportation network flows to17 evaluate the indirect impacts of an unexpected event

Kockelman, Kara M.

183

E-Print Network 3.0 - aflatoxin m1 contamination Sample Search...  

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

& Department of Wildlife and Fisheries Sciences, Texas A&M University Collection: Environmental Sciences and Ecology 5 Displacement ofAflatoxin-Producing Fungi from Cottonseed,...

184

M1L11OR04020102 IASCC initial Assessment Results Rev2  

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

of Initial Test Conditions for Experiments to Assess Irradiation Assisted Stress Corrosion Cracking Mechanisms December 2010 Prepared by J.T. Busby and M.N. Gussev Oak Ridge...

185

SECTION M EVALUATION FACTORS FOR AWARD TABLE OF CONTENTS M-1 EVALUATION OF PROPOSALS .....................................................................................2  

National Nuclear Security Administration (NNSA)

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) "ofEarlyEnergyDepartmentNationalRestart of the Review ofElectronicNORTH LASSOLICITATION, OFFER AND

186

SECTION M EVALUATION FACTORS FOR AWARD TABLE OF CONTENTS M-1 EVALUATION OF PROPOSALS .....................................................................................2  

National Nuclear Security Administration (NNSA)

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) "ofEarlyEnergyDepartmentNationalRestart of the Review ofElectronicNORTH LASSOLICITATION, OFFER ANDM

187

SI}M!1ARY REPORT ON SITE nnTESTIGATION AND REMOVAL ACTIVITIES  

E-Print Network [OSTI]

PREPARED POR: u~s~ Environmental Protection Agency Region V1:I1 Waste Management Division E·uilding.s~. ~ ~ '" .. ~ ~ '" 10 Site Utilit.ies ~ '" 10 Dx'a·in Syst.em 10 Water Sampling , 10 Soil S'a.mpling ~ '" ., 11 Drl1l1l Protection Agency - Emergency Response Branch (EPA) tasked the Ecology & Environment, Inc" f 'Tec

188

C:\MYDOCS\FBSS-M~1\HATTIE\LAYOUT94.TXT  

U.S. Energy Information Administration (EIA) 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:1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National and Regional Data; Row: NAICS98,,,1999,0,0,1e+15,1469,6,01179,"WAT","HY"Tables andA 6 J (MillionCubic357 Energy1993 Federal

189

STANDARD ADMINISTRATIVE PROCEDURE 25.99.08.M1.01 Communication Allowances  

E-Print Network [OSTI]

job responsibilities may be enhanced by the provision of personal communication devices. Departments and operation of personal communication devices under the provisions of this Procedure. Communication Allowances salary supplements for service plans. 1.2 A personal communication device acquired by provisions

190

Search for Resonant Absorption of Solar Axions Emitted in M1 Transition in $^{57}$Fe Nuclei  

E-Print Network [OSTI]

A search for resonant absorbtion of 14.4 keV solar axions by $^{57}$Fe target was performed. The Si(Li) detector placed inside the low-background setup was used to detect the $\\gamma$-quanta appearing in the deexcitation of 14.4 keV nuclear level: $A+\\rm{^{57}Fe} \\to \\rm{^{57}Fe^{*}} \\to \\rm{^{57}Fe} + \\gamma$. The new upper limit for the hadronic axion mass have been obtained: $m_{A} \\leq 151$ eV (90% C.L.) ($S$=0.5, $z$=0.56).

A. V. Derbin; A. I. Egorov; I. A. Mitropol'sky; V. N. Muratova; D. A. Semenov; E. V. Unzhakov

2009-06-01T23:59:59.000Z

191

One source of uncertainty in fishery assessments based on tag release and  

E-Print Network [OSTI]

tagging experi- ment in which 504 skipjack tuna, Kat- suwonus pelamis, were double tagged, by using pelamis, off the Maldives M. Shiham Adam Renewable Resources Assessment Group T. H. Huxley School

192

Population dynamics and movements of skipjack tuna (Katsuwonus pelamis) in the Maldivian fishery: analysis of tagging data from an  

E-Print Network [OSTI]

Population dynamics and movements of skipjack tuna (Katsuwonus pelamis) in the Maldivian fishery du listao (Katsuwonus pelamis) dans la pêcherie des Maldives : analyse des données de marquage au

Hawai'i at Manoa, University of

193

The Right to Life with Dignity: Economic and Social Rights Respect in the World  

E-Print Network [OSTI]

Rep. Costa Rica Cote dIvoire Croatia Cuba Cyprus Czech Rep.Japan Spain Switzerland Poland Croatia Maldives TurkmenistanSeychelles China Costa Rica Croatia Grenada Ireland Italy

Kolp, Felicity Ann

2010-01-01T23:59:59.000Z

194

Total Synthesis of (+)-Spectinabilin, Taiwaniaquinoids, Synthetic Progress toward Aspergillin PZ, and Synthesis of a Photoswitchable Agonist of Glutamate Receptor-dMAG  

E-Print Network [OSTI]

Fortunately, a simple switch to PDC afforded the carboxylicPresumably the neutral PDC oxidant prevented racemizationdiluted with DMF (15 ml) and PDC (4.24 g, 10.1 mmol) was

Xu, Yue

2010-01-01T23:59:59.000Z

195

J. BUCHANAN. 2014 On the thermo-electric position of carbon (Position du carbone dans la srie thermo-lectrique); Phil. Mag., 5e srie, t. XX,  

E-Print Network [OSTI]

baguette de charbon de 12mm de diamtre, semblable celles que l'on emploie dans les lampes arc et une'il doit y avoir dveloppement de chaleur (phnomne de Peltier) l'ex- trmit ngative du filament d-lectrique et par 6 la temprature absolue de l'une des soudures, l'efl'et de Peltier a pour expression k, et It

Paris-Sud XI, Universit de

196

61.01.02.M0.M1: Public Information Page 1 of 4 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

to resubmit the request to the PIO. 2.2 Public Information Liaison Coordinator (PILC) 2.2.1 University Colleges, Divisions, and Executive Offices shall appoint a primary and secondary PILC to perform public information related functions. 2.2.2 These individuals are formally assigned the role of PILC by the President

197

BENDIX SYSTEMS DIVISION ANN ARa0 R, M1C H NO. Description of SIDE/ CCGE Exper-  

E-Print Network [OSTI]

the raw and thermalized solar wind particles at the surface of the moon. It will also provide some interface with ALSEP and a single mounting interface, common power and programming electronics, and a common Manager ~ohn Meyers - Project Engineer (Student) Kit Webster - Programming and data reduction (Student

Rathbun, Julie A.

198

29.01.03.M1.09 Information Resources Incident Management Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

likelihood that security incidents could be propagated to other systems beyond departmental control, system, process, store, retrieve, display, and transmit information or data. SIRS Security Incident Reporting follow System Regulation 10.02.01, Control of Fraud, Waste and Abuse. 2.6 If there is a substantial

199

Myeloid-Specific Rictor Deletion Induces M1 Macrophage Polarization and Potentiates In Vivo Pro-Inflammatory  

E-Print Network [OSTI]

(PI3K)/protein kinase B (Akt) axis plays a central role in attenuating inflammation upon macrophage a mouse model lacking Rictor, an essential mTORC2 component, in myeloid cells. Primary macrophages similarly affected inflammation in vivo, mice were either fed a high fat diet, a situation promoting chronic

Sabatini, David M.

200

OPEN 4:30p.m. 1:00a.m. daily (except University holidays)  

E-Print Network [OSTI]

: Italian, Ranch, Blue Cheese, Balsamic, Caesar Extra Dressing $ .59 6- piece Sushi $5.39 Fresh Fruit $ . 72-Broccoli Tomato Basil Veggie White Chicken Bacon Ranch Your choice of White or Whole Wheat Crust Hot Sandwiches.69 Chicken Caesar Salad $5.89 Chef Salad $5.89 All salads come with one dressing packet. Choice of Dressings

McConnell, Terry

Note: This page contains sample records for the topic "maldives mag m1" 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

29.01.03.M1.06 Information Resources Backup and Recovery Page 1 of 3 STANDARD ADMINISTRATIVE PROCEDURE  

E-Print Network [OSTI]

for off-site storage, shall be documented and reviewed periodically. Additionally, mission critical data shall be backed up on a scheduled basis and stored off-site in a secure, environmentally safe facility decisions by the data owner. 3.3 Physical access controls implemented at off-site backup storage locations

202

21.99.04.M1, Lost, Found, Stolen, or Abandoned Property Page 1 of 3 UNIVERSITY RULE  

E-Print Network [OSTI]

. The System has provided guidance for the disposition of personal property through regulation 21 ­ Personal property that is outside the possession or control of owner and the owners identity is not readily) will be deposited in the MSC Student Programs Account and managed by MSC Hospitality. Proceeds will be used

203

New limit on the mass of 9.4-keV solar axions emitted in an M1 transition in $^{83}$Kr nuclei  

E-Print Network [OSTI]

A search for resonant absorption of the solar axion by $^{83}\\rm{Kr}$ nuclei was performed using the proportional counter installed inside the low-background setup at the Baksan Neutrino Observatory. The obtained model independent upper limit on the combination of isoscalar and isovector axion-nucleon couplings $|g_3-g_0|\\leq 1.69\\times 10^{-6}$ allowed us to set the new upper limit on the hadronic axion mass of $m_{A}\\leq 130$ eV (95\\% C.L.) with the generally accepted values $S$=0.5 and $z$=0.56.

Derbin, A V; Gavrilyuk, Yu M; Kazalov, V V; Kim, H J; Kim, Y D; Kobychev, V V; Kuzminov, V V; Ali, Luqman; Muratova, V N; Panasenko, S I; Ratkevich, S S; Semenov, D A; Tekueva, D A; Yakimenko, S P; Unzhakov, E V

2015-01-01T23:59:59.000Z

204

08.01.01.M1.01 Investigation and Resolution of Complaints Against Non-faculty Employees and Unrelated Third Parties for Illegal Discrimination,  

E-Print Network [OSTI]

are initiated by filing a discrimination, sexual harassment, or related retaliation complaint as described

205

Effects of elevated CH4 and CO2 on the mobility of metals in near-surface sediments Hingst, M. 1  

E-Print Network [OSTI]

, and injecting it into deep, geologic reservoirs for enhanced hydrocarbon recovery and storage. One concern pathways such as fractures and/or improperly plugged and abandoned wells. We hypothesize that CO2 migration the surface and oxidizes to CO2 (34%) in the vadose zone near a plugged and abandoned well. Four sediment

Texas at Austin, University of

206

MSU Recycling recycle.msu.edu 517-355-1723 MARCH 15, 2014 9:00A.M.1:00P.M.  

E-Print Network [OSTI]

ELECTRONICS Computers (All Parts) Mice Keyboards Laptops All Types of External Drives CRT Monitors LCD Makers Fryers Toaster Ovens Electric Knives Electric Razors/Trimmers Hair Dryers Electric Toothbrushes

Liu, Taosheng

207

OhioSeaGrantC o l l e g e P r o g r a m 1 March 2005 -31 March 2006 Annual Report  

E-Print Network [OSTI]

and universities (Bowling Green State University, Kent State University, Ohio State University, and the University of Toledo) during year one and four new projects at Bowling Green and Ohio State. The total research budget,167,000 in year one. In year two, we propose to continue funding on five projects at Bowling Green and Ohio State

Jones, Michelle

208

Macrophage imbalance (M1 vs. M2) and upregulation of mast cells in wall of ruptured human cerebral aneurysms: preliminary results  

E-Print Network [OSTI]

Cite this article as: Hasan et al. : Macrophage imbalance (JOURNAL OF NEUROINFLAMMATION Hasan et al. Journal ofpreliminary results David Hasan 1,4* , Nohra Chalouhi 2 ,

Hasan, David; Chalouhi, Nohra; Jabbour, Pascal; Hashimoto, Tomoki

2012-01-01T23:59:59.000Z

209

A series of layered intergrowth phases grown by molecular beam epitaxy: Sr{sub m}TiO{sub 2+m}(m=1-5)  

SciTech Connect (OSTI)

Sr{sub m}TiO{sub 2+m} phases having one TiO{sub 2} layer sandwiched between m SrO layers were grown using molecular beam epitaxy. The out-of-plane (in-plane) lattice parameters determined by x-ray diffraction were c(a)=9.14 A (3.78 A), 23.55 A (3.75 A), and 14.60 A (3.75 A) for Sr{sub 3}TiO{sub 5}, Sr{sub 4}TiO{sub 6}, and Sr{sub 5}TiO{sub 7}, respectively. Both lattice parameters change abruptly on going from the m=2 Ruddlesden-Popper phase to m=3 phase, indicating a significant change in the bond lengths (or strain states) on transitioning from the known members to the higher order members of this structural family. Electron microscopy confirmed the artificially layered structures.

Fisher, P.; Wang, S.; Skowronski, M.; Salvador, P. A.; Snyder, M.; Maksimov, O. [Department of Materials Science and Engineering, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213 (United States); Electro-Optics Center, Pennsylvania State University, Freeport, Pennsylvania 16229 (United States)

2007-12-17T23:59:59.000Z

210

Calcium release triggered by activation of the acetycholine receptor in M1-CNiFERs brings the yellow and blue "arms" of TN-XXL closer  

E-Print Network [OSTI]

& Education e-Advances Stories of Discovery Science Snippets Health Information Science Education Resource system to monitor different types of receptors and chemical signals in the brain. Their cell-based neurotransmitter fluorescent engineered reporters (CNiFERs) consist of cultured cells that have been engineered

Kleinfeld, David

211

file:///C:/Documents%20and%20Settings/anderk5/My%20Documents/M... 1 of 1 7/28/2008 3:51 PM  

E-Print Network [OSTI]

Power Transmission and Gearing Conference (PTG) ( Call for Papers pdf) Description The ASME International Power Transmission and Gearing Conference (PTG) is an integral part of the 2007 ASME International results, new developments, and novel concepts in the ASME Power Transmission and Gearing Conference (PTG

Anderson, Kurt S.

212

ECOLOGY LECTURE (BI 40601) & LABORATORY (BI40711) Lecture Fischer 316, TTH 10:0011:35; Lab Fischer 224, M 1:004:00  

E-Print Network [OSTI]

ECOLOGY LECTURE (BI 40601) & LABORATORY (BI40711) FALL 2005 Lecture Fischer 316, TTH 10 EMAILpacker@susqu.edu OFFICE HOURS MW 9:0010:00, W 1:302:30 WHAT IS ECOLOGY? Ecology is the study of interrelationships between organisms and their biotic and abiotic environments. As a basic science, ecology informs

Packer, Alissa A.

213

file:///C:/Documents%20and%20Settings/anderk5/My%20Documents/M... 1 of 2 8/22/2008 4:27 PM  

E-Print Network [OSTI]

Symposium on International Design and Design Education (DEC) ( Call for Papers pdf) Description The 6th Symposium on International Design and Design Education (DEC) is an integral part of the 2009 ASME-oriented implementation is a must. Therefore, the 5th Symposium on International Design and Design Education

Anderson, Kurt S.

214

A p r i l 9 2 0 1 4 R o o m 1 6 0 P B B 1 2 : 2 0 P M Introduction  

E-Print Network [OSTI]

species Regulatory and Stewardship responsibilities ¡ Endangered Species Act ¡ Migratory Bird Treaty Act

Gray, Matthew

215

Michael MargaliotList of Publications May 2014 [M1] Margaliot, M. and Langholz, G. New Approaches to Fuzzy Modeling and  

E-Print Network [OSTI]

Approaches to Fuzzy Modeling and Control - Design and Analysis, World Scientific, 2000. [M2] Kolman, E. and Margaliot, M. Knowledge-Based Neurocomputing: A Fuzzy Logic Approach, Springer-Verlag, 2009. [M3] Laschov, D1] Margaliot, M. and Langholz, G. "Fuzzy Lyapunov based approach to the design of fuzzy controllers

Margaliot, Michael

216

Michael MargaliotList of Publications July 2013 [M1] Margaliot, M. and Langholz, G. New Approaches to Fuzzy Modeling and  

E-Print Network [OSTI]

Approaches to Fuzzy Modeling and Control - Design and Analysis, World Scientific, 2000. [M2] Kolman, E. and Margaliot, M. Knowledge-Based Neurocomputing: A Fuzzy Logic Approach, Springer-Verlag, 2009. Journal Papers [J1] Margaliot, M. and Langholz, G. "Fuzzy Lyapunov based approach to the design of fuzzy controllers

Margaliot, Michael

217

Design and first experiments on MagPieR, the magnetic microrobot Soukeyna Bouchebout1, Aude Bolopion2, Mohamed Kharboutly2, Ioan Alexandru Ivan2,3, Joel Agnus2  

E-Print Network [OSTI]

and copper is sputtered to ensure the conductivity for the electrodeposition of the nickel and the mechanical)). It is composed of two different layers: a 24m thick layer of nickel, which is a ferromagnetic material coherence. The nickel layer is then electroplated. The microrobots are obtained by saw dicing the whole

Paris-Sud XI, Universit de

218

commercial peat-based media (Pro-Mix BX), maintained on overhead watering as needed, eventually moved to daily subirrigation including Peters 15-5-15 Cal-Mag (Scotts) fertilizer at  

E-Print Network [OSTI]

Jet 8006VS twinfan nozzle operating at 30 psi. Plants were sprayed to wet, treatments replicated six times effective than when combined with the wetting agent; there were generally no meaningful differences due and fruit quality for 35 red and white vinifera winegrape varieties. The 2013 season started with a cool

Danforth, Bryan Nicholas

219

abstracting instructions extent: Topics by E-print Network  

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

solar maximum (by 0.4 mag); and at high airmass (0.25 mag brighter at airmass 1.5). Light pollution (line + continuum) contributes < 0.03 mag in U, ? 0.02 mag in B, ? 0.10 mag in...

220

Fishery Bulletin Index Volume 99(14), 2001  

E-Print Network [OSTI]

chinook salmon (Oncorhynchus tshawytscha): an analysis using microsatel lite DNA markers, by R. John dus in two fishing zones on the Great Barrier Reef, Austra lia, by Jill St John, Garry R. Russ, Ian W the Maldives, by M. S. Adam and Geof frey P. Kirkwood 197 The effect of sea state on estimates of abundance

Note: This page contains sample records for the topic "maldives mag m1" 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

Climatic Research Unit University of East Anglia  

E-Print Network [OSTI]

studies:the Maldives, Australia and the Mediterranean. Climate Change andTourism www January, 2000, University of Surrey). These publications review the impacts of climate change for a wide range of international holiday destinations visited by UK tourists. The impacts of climate change

Feigon, Brooke

222

Contact Us! The Center for South Asian Studies  

E-Print Network [OSTI]

emerging in India, Pakistan, Afghanistan, Bangladesh, Ne- pal, Bhutan, the Maldives, and Sri Lanka. Sponsored by the Duke Center for South Asian Studies, the Certificate will provide you with resources countries like India and Bangladesh have become key locations for international businesses looking to export

Zhou, Pei

223

Application to Export Electric Energy OE Docket No. EA-306-A...  

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

Solutions, Inc. Application to Export Electric Energy OE Docket No. EA-306-A MAG Energy Solutions, Inc. Application from MAG Energy Solutions, Inc. to export electric energy to...

224

8cm DIPOLE MDC No. 097 Rev. C COLD TESTING Sheet 1 of 7  

E-Print Network [OSTI]

NO Warm bore tube heaters OFF: (6) RHIC-MAG-R-7751- 220 5 Activate lead heaters. Check water flow. RHIC-down. RHIC-MAG-R-7751- 240 5 Start Cool-Down. RHIC-MAG-R-7751- 250 5 Verifiy operation of lead heaters & water flow by cryogenics operator. RHIC-MAG-R-7751- 260 5 Cryogenics operator to notify control room

Ohta, Shigemi

225

SPITZER 24 {mu}m EXCESSES FOR BRIGHT GALACTIC STARS IN BOOeTES AND FIRST LOOK SURVEY FIELDS  

SciTech Connect (OSTI)

Optically bright Galactic stars (V {approx}< 13 mag) having f {sub {nu}}(24 {mu}m) > 1 mJy are identified in Spitzer mid-infrared surveys within 8.2 deg{sup 2} for the Booetes field of the NOAO Deep Wide-Field Survey and within 5.5 deg{sup 2} for the First Look Survey (FLS). One hundred and twenty-eight stars are identified in Booetes and 140 in the FLS, and their photometry is given. (K - [24]) colors are determined using K magnitudes from the Two Micron All Sky Survey for all stars in order to search for excess 24 {mu}m luminosity compared to that arising from the stellar photosphere. Of the combined sample of 268 stars, 141 are of spectral types F, G, or K, and 17 of these 141 stars have 24 {mu}m excesses with (K - [24]) > 0.2 mag. Using limits on absolute magnitude derived from proper motions, at least eight of the FGK stars with excesses are main-sequence stars, and estimates derived from the distribution of apparent magnitudes indicate that all 17 are main-sequence stars. These estimates lead to the conclusion that between 9% and 17% of the main-sequence FGK field stars in these samples have 24 {mu}m infrared excesses. This result is statistically similar to the fraction of stars with debris disks found among previous Spitzer targeted observations of much brighter, main-sequence field stars.

Hovhannisyan, L. R.; Mickaelian, A. M. [Byurakan Astrophysical Observatory and Isaac Newton Institute of Chile Armenian Branch, 378433, Byurakan, Aragatzotn Province (Armenia); Weedman, D. W.; Houck, J. R. [Astronomy Department, Cornell University, Ithaca, NY 14853 (United States); Le Floc'h, E. [Steward Observatory, University of Arizona, Tucson, AZ, 85721 (United States); Soifer, B. T. [Spitzer Science Center, California Institute of Technology, 220-6, Pasadena, CA 91125 (United States); Brand, K. [Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218 (United States); Dey, A.; Jannuzi, B. T. [National Optical Astronomy Observatory, 950 N. Cherry Ave., Tucson, AZ 85719 (United States)], E-mail: lilithov11@yahoo.com, E-mail: dweedman@isc.astro.cornell.edu

2009-07-15T23:59:59.000Z

226

Los Angeles Times: Ahmed M. Abdel-Ghaffar, 60; USC engineering... http://www.latimes.com/news/obituaries/la-me-abdelghaffar4-2008m... 1 of 2 5/4/08 12:26 AM  

E-Print Network [OSTI]

the Golden Gate Bridge and collected data for a study on vibrations. "He really loved bridges; he thought advanced bridge design and monitoring By Jocelyn Y. Stewart Los Angeles Times Staff Writer May 4, 2008 and monitoring of bridges led to the development of more efficient and reliable ways to build them, has died. He

Southern California, University of

227

Interactive Investor Trading Limited, trading as "Interactive Investor", is authorised and regulated by the Financial Services Authority. Registered Office: Dashwood House, 69 Old Broad Street, London EC2M 1QS, telephone . Registered in England with Compa  

E-Print Network [OSTI]

and regulated by the Financial Services Authority. Registered Office: Dashwood House, 69 Old Broad Street the bid of the southern French town of Cadarache. ITER aims to be a test bed for clean, safe, inexhaustible energy, emulating the sun's nuclear fusion. It is not expected to generate electricity before 2050

228

Lambda network having 2.sup.m-1 nodes in each of m stages with each node coupled to four other nodes for bidirectional routing of data packets between nodes  

DOE Patents [OSTI]

The Lambda network is a single stage, packet-switched interprocessor communication network for a distributed memory, parallel processor computer. Its design arises from the desired network characteristics of minimizing mean and maximum packet transfer time, local routing, expandability, deadlock avoidance, and fault tolerance. The network is based on fixed degree nodes and has mean and maximum packet transfer distances where n is the number of processors. The routing method is detailed, as are methods for expandability, deadlock avoidance, and fault tolerance.

Napolitano, Jr., Leonard M. (825 El Quanito Dr., Danville, CA 94526)

1995-01-01T23:59:59.000Z

229

Sbartai, A.; Namour, P.; Errachid, A.; Krejci, J.; Sejnohov, R.; Renaud, L.; Larbi Hamlaoui, M.;1 Loir, A.-S.; Garrelie, F.; Donnet, C.; Soder, H.; Audouard, E.; Granier, J.; Jaffrezic-Renault N., (2012)2  

E-Print Network [OSTI]

toxic compounds must be banned, such as "heavy16 metals", in particular mercury impregnation or films (DPASV) determinations, at the nanomolar level, of the four heavy metal ions of the European5 Water. It was shown that the four heavy metals could be detected simultaneously in the10 concentration ratio usually

Paris-Sud XI, Université de

230

A1 = (b1 + m1y1)y1 = (2 + 2 1)(1) = 4 m2 A2 = (b2 + m2y2)y2 = (2.5 + 2 1)(1) = 4.5 m2  

E-Print Network [OSTI]

and the flow is subcritical . 55 © 2006 Pearson Education, Inc., Upper Saddle River, NJ. All rights reserved use of adopters of the book Water-Resources Engineering, Second Edition, by David A. Chin. ISBN 0.5 ? 3) (9.81)(4 ? 3 + 1.5 ? 32)3 = 0.19 hence Fr = 0.45 and the flow is subcritical . 3.27. From

Bowen, James D.

231

Engi 9614: Special Topics in Environmental Engineering: Renewable Energy and Resource Conservation Midterm Exam, 17 October 2012, Wednesday, 11:45 a.m. 1:00 p.m., Instructor: Dr. C. A. Coles  

E-Print Network [OSTI]

Engi 9614: Special Topics in Environmental Engineering: Renewable Energy and Resource Conservation, so this is a beneficial method. Raising the standard of living and harnessing more sources of energy the demographic transition that the more prosperous countries have gone through. Abortion is a method that has

Coles, Cynthia

232

MOOCs and More: The Changing Landscape of Online Education Tuesday, January 15, 2013 (MOOCs: Massive Open Online Courses) Featured speakers: Martha E. 11:30 a.m. 1:00 p.m.  

E-Print Network [OSTI]

Building, 1st Floor and Tom Ivacko, Program Manager, Center for Local, State, and Urban Policy (CLOSUP), UM Ball, UM School of Education Personal Property Tax What Effects the Impending Changes Might Ultimately Have Featured speakers: Panel with Dr. Debra Horner, Project Manager; Tom Ivacko, Program Manager

Kamat, Vineet R.

233

Multisensor Geophysical Fusion for Improved Sub-surface Imaging at Historic Camptown Cemetery, Brenham, Texas  

E-Print Network [OSTI]

in the mapping of Camptown Cemetery: magnetics (MAG), electromagnetic induction (EMI), and ground penetrating radar (GPR). The approach is to combine, or fuse, the MAG, EMI, and GPR information, rendering a joint interpretation in which the confidence...

Meehan, Tate

2013-09-30T23:59:59.000Z

235

THE EFFECTS OF TEACHER VS STUDENT CENTERED INSTRUCTIONAL STRATEGIES ON THE VOCABULARY LEARNING OF SIXTH GRADE THAI STUDENTS  

E-Print Network [OSTI]

: Function/ Use of vocabulary 118 Appendix B: Students Posttest : Spelling 120 Appendix B2: Students Posttest : Meaning 121 Appendix B3: Students Posttest : : Function/ Use of vocabulary 122 viii Appendix C: Students Vocabulary List 124.... The Expanding Circle e.g. Bhutan (1,1614) Brunet (260) China (1,208,841) Fiji (771) Hong Kong (5,838) Indonesia (194,615) Japan (124,815) Maldives (246) Mayanmar (45,555) Nepal (21,350) Thailand (58,183) South Korea (44,563) The Outer Circle...

Khuvasanond, Kirati

2013-05-31T23:59:59.000Z

236

The inferred redshift distribution of the faint blue excess  

E-Print Network [OSTI]

We infer the redshift distribution of the faint blue galaxy excess (FBE) at B=23.5 by subtracting the predicted distribution of giant/normal galaxies from the observed N(z) distribution for all types. This is possible because of the recent deep {\\it Hubble Space Telescope} (HST) WFPC2 morphological number counts which have convincingly demonstrated that little evolution of the giant population is seen to B=26.0. The mean redshift of the FBE at B=23.5 is found to be _{FBE}=0.40 +/- 0.07 with upper and lower quartiles defined by z_{0.75}=0.58 +/- 0.05 and z_{0.25}=0.28 +/- 0.05, respectively. We compare this inferred FBE N(z) distribution to the predictions from three generic faint galaxy models: dwarf dominated (no evolution), pure luminosity evolution, and evolving dwarfs. The inferred FBE N(z) distribution strongly supports a hybrid evolving dwarf--rich model wherein a large population of dwarfs present at z=0.5 has subsequently faded to obscurity. The total integrated number density of dwarfs (down to M_{B}=-11) is estimated to be a factor of 20 times greater than that of E---Sc galaxies and the estimated fading to be 1.0 < \\Delta m < 1.4 mags. Thus, the dwarf population is estimated to be responsible for ~30% of the luminosity density locally, rising to ~57% at z=0.5.

Simon P. Driver; Warrick J. Couch; Steven Phillipps; Rogier A. Windhorst

1996-05-10T23:59:59.000Z

237

The Utility of Zebrafish in Stress ResearchHart, P.1,2, Bergner, C.2, Egan, R.2, Cachat, J.1, Canavello, P.1, Bartels, B.1, Beeson, E.1, Elkhayat, S.1, Elegante, M.1, Mohnot, S.1, Tien, D.1, Tien, A.1 , Kalueff, A.1,2 1 Pharmacology Dept., Tulane Universi  

E-Print Network [OSTI]

significantly more Methods Novel Tank Exposure Test: Observers record endpoints and sessions are also video taped for automated analysis (CleverSys Inc.). Ethanol withdrawal: Groups of zebrafish were chronically evidence from cortisol assays, we were able to demonstrate the consistency and reliability of this species

Kalueff, Allan V.

238

A mini-survey for variability in early L dwarfs  

E-Print Network [OSTI]

We report differential I-band photometry of four early L-dwarfs obtained to study variability. We detect variability on the timescale of hours in two objects, 2M0746425+200032 (at a level of 0.007 mag -- 6.5 sigma) and 2M1108307+683017 (0.012 mag -- 5 sigma). We also place upper limits of 0.02 mag (1 sigma) on the variability of two others.

F. J. Clarke; B. R. Oppenheimer; C. G. Tinney

2002-05-27T23:59:59.000Z

239

Infrared Maximally Abelian Gauge  

E-Print Network [OSTI]

The confinement scenario in Maximally Abelian gauge (MAG) is based on the concepts of Abelian dominance and of dual superconductivity. Recently, several groups pointed out the possible existence in MAG of ghost and gluon condensates with mass dimension 2, which in turn should influence the infrared behavior of ghost and gluon propagators. We present preliminary results for the first lattice numerical study of the ghost propagator and of ghost condensation for pure SU(2) theory in the MAG.

Tereza Mendes; Attilio Cucchieri; Antonio Mihara

2006-11-01T23:59:59.000Z

240

E-Print Network 3.0 - analysis estudo das Sample Search Results  

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

mag- netica e com as novas etapas de estudo. Alem disso, os dados... an- cia magnetica e a sua aplicacao a reconstrucao em imageamento paralelo. Ele ......

Note: This page contains sample records for the topic "maldives mag m1" 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

MMOIRES ORIGINAUX Loi de superposition et expriences nouvelles  

E-Print Network [OSTI]

. Zeitschr., 6 (1905) 8ij. 5. Le Radium, 6 (190J 219. 6. l'Itil. Mag., 1.8 (1909) 252. 7. Journ. Soc. Physico

Paris-Sud XI, Université de

242

E-Print Network 3.0 - auroral field lines Sample Search Results  

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

RETRIEVAL OF AURORAL IMAGES --THOUSANDS OF IRREGULAR SHAPES Summary: of the solar wind interaction with the Earth's mag- netic field. On the other hand, the auroral image data...

243

E-Print Network 3.0 - ablation assisted resonance Sample Search...  

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

enhancement (LGE) mag- netic resonance imaging (MRI) immediately post-ablation (IPA... enhancement MRI magnetic resonance imaging NE nonenhancing RF radiofrequency RFA...

244

(12) United States Patent Jalali et al.  

E-Print Network [OSTI]

.V. Bennet, E.P. Scott and B.H. Kolner, "Temporal Mag ni?cation and Reversal of 100Gb/s Optical Data

Jalali. Bahram

245

Microsoft Word - 25A2284 Continued  

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

to this need, ITN Energy Systems, in collaboration with MAG Industrial Automation Systems, the Electric Power Research Institute, Southern California Edison, and the Colorado...

246

Materials  

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

2 MAG LAB REPORTS Volume 18 No. 1 CONDENSED MATTER SCIENCE Technique development, graphene, magnetism & magnetic materials, topological insulators, quantum fl uids & solids,...

247

E-Print Network 3.0 - agricultural protection zone Sample Search...  

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

in MAgPIE, and in step 4 agricultural production and resource... . In the coming decades, world agricultural systems will face serious transitions. Population growth, income... for...

248

Cable Measuring Engine Operation Procedures  

E-Print Network [OSTI]

MEASURING ENGINE OPERATION PROCEDURES LBNL-40565 SC-MAG-597MEASURING ENGINE OPERATION PROCEDURES INDEX IN T ROD U C TCALIBRATION PROCEDURE . .

Authors, Various

2011-01-01T23:59:59.000Z

249

This material is supported in part by the National Science Foundation under awards CNS-1042537 and CNS-1042543 (PRObE). http://www.nmc-probe.org/  

E-Print Network [OSTI]

#center#in#Los#Alamos,#NM# Environmentally friendly !Energy%efficient%320%ton%Mul4Stack% chillers%with%free$cooling$units%and% Mag

Maccabe, Barney

250

ENERGY U.S. DEPARTMENT OF Office  

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

method, one that uses permanent mag- nets and specialized alloys. The result would be refrigerators, air conditioners and giant warehouse freezers that are greener, quieter and...

251

E-Print Network 3.0 - andri riid ennu Sample Search Results  

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

en ongeveer 160 bladzijden mag ik eindelijk mijn dank uitspreken aan Summary: , Wim Kruizinga, Auke Meetsma en Andries Bruins voor het uitvoeren van analyses of hulp daarbij....

252

Application to Export Electric Energy OE Docket No. EA-306-A...  

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

Solutions to esport electric energy to Canada. Federal Register Notice. Application to Export Electric Energy OE Docket No. EA-3060-A MAG Energy Solutions, Federal Register Notice...

253

E-Print Network 3.0 - agriculture development mead Sample Search...  

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

Parangal sa Mag... Oceanography 2:35-47. Wilson G. Mendoza, Ralph N. Mead, Larry E. Brand, ... Source: Miami, University of - Rosenstiel School of Marine and Atmospheric...

254

Maricopa Assn. of Governments- PV and Solar Domestic Water Heating Permitting Standards  

Broader source: Energy.gov [DOE]

In an effort to promote uniformity, the Maricopa Association of Governments (MAG) approved standard procedures for securing necessary electrical/building permits for residential (single-family) and...

255

UNIVERSIT D'ORLANS COLE DOCTORALE COLE DOCTORALE SCIENCES ET  

E-Print Network [OSTI]

. Principales utilisations nergtiques du gaz de synthse 13 IV.1 Gnralits 13 IV.2 Moteur gaz (MAG) 13 IV.3 Turbine g

Paris-Sud XI, Universit de

256

antilles island arc: Topics by E-print Network  

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

The morphology of the underthrust oceanic crust controls the mag matic activity of the island arc, and particularly the development, in space and time, of "arc compartments." Denis...

257

Land Use and the Chinatown Problem  

E-Print Network [OSTI]

Ralph Henn, Chinatown in Hunters Point, S. F. Mag. (1970).had simply said that Hunters Point or any remote area was

Chou, Christopher

2014-01-01T23:59:59.000Z

258

National High Magnetic Field Laboratory: Cryogenics  

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

Facilities The Mag Lab's Cryogenics Laboratory is a fully developed facility for conducting low temperature experimental research and development. The laboratory, which...

259

Page 1 of 13 Paper published on J. Micromech. Microeng. 20 (2010) 045029 (9pp)  

E-Print Network [OSTI]

plagued computer architects. An exciting new storage tech- nology based on microelectromechanical systems remains 2 orders of mag- nitude higher than disk storage (Figure 1). Microelectromechanical systems (MEMS

2010-01-01T23:59:59.000Z

260

E-Print Network 3.0 - acoustically-induced geomagnetic perturbations...  

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

geomagnetically perturbed days cor- responding to the decreasing phase... -speed solar wind, mag- netic field disturbances in the interplanetary space and in the geomagnetic...

Note: This page contains sample records for the topic "maldives mag m1" 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

Dynamics Studies of a Malachite Green-RNA Complex Revealing the Origin of the Red-Shift and Energetic Contributions of Stacking Interactions  

E-Print Network [OSTI]

Dynamics Studies of a Malachite Green-RNA Complex Revealing the Origin of the Red characterization of the dynamics of a malachite green (MAG)-RNA aptamer complex revealed surprisingly asymmetric shift. The work presented here examines the dynamical nature of the MAG molecule inside the RNA ligand

Nguyen, Dat H.

262

TB235 Rev.B 0602 1United States & Canada 800-207-0144 Germany 0800 6931 000  

E-Print Network [OSTI]

...................................................................... 10 GST· Bind buffer preparation 10 Column chromatography 10 Small scale purification - batch method................................................................................. 12 GST· Bind buffer preparation 12 GST· Mag Agarose Beads purification 13 Processing the Sample after 50 ml 70541-3 70541-4 BugBuster ® GST· Bind Purification Kit 70794-3 GST· MagTM Agarose Beads 2 ml 10

Lebendiker, Mario

263

Essays on International Finance and Trade  

E-Print Network [OSTI]

1973M 1-20 09M7 Real oil prices TOT 1973M 1-20 09M7 1973M 1-1973M 1-20 09M7 REER Real oil prices 1973M 1-20 09M7 1973M1975M 1-20 09M7 Real oil prices TOT 1975M 1-20 09M7 1975M 1-

Zeng, Li

2009-01-01T23:59:59.000Z

264

MatLab Reports Volume 21 Issue 1 (2014)  

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

Superconductor Spaghetti PAGE 10 Volume 21 No. 1 * Spring 2014 The Berlin Magnet: Extraordinary Challenges and Solutions PAGE 24 Future of High Fields MagSci Report & Users Talk...

265

Astroparticle Physics Jrg R. Hrandel  

E-Print Network [OSTI]

;t eL~ L Itil]IAH OIEAH. -~P£tY. 1,9° o c~. ~, \\ \\ · ~SCM P~~ , ,,,. /,6o ~,~ 50UTH. ~.,m MAG/Y. IAT

Hörandel, Jörg R.

266

SDSS Data Management and Photometric Quality Assessment  

E-Print Network [OSTI]

We summarize the Sloan Digital Sky Survey data acquisition and processing steps, and describe runQA, a pipeline designed for automated data quality assessment. In particular, we show how the position of the stellar locus in color-color diagrams can be used to estimate the accuracy of photometric zeropoint calibration to better than 0.01 mag in 0.03 deg2 patches. Using this method, we estimate that typical photometric zeropoint calibration errors for SDSS imaging data are not larger than ~0.01 mag in the g, r, and i bands, 0.02 mag in the z band, and 0.03 mag in the u band (root-mean-scatter for zeropoint offsets).

Z. Ivezic; R. H. Lupton; D. Schlegel; B. Boroski; J. Adelman-McCarthy; B. Yanny; S. Kent; C. Stoughton; D. Finkbeiner; N. Padmanabhan; C. M. Rockosi; J. E. Gunn; G. R. Knapp; M. A. Strauss; G. T. Richards; D. Eisenstein; T. Nicinski; S. J. Kleinman; J. Krzesinski; P. R. Newman; S. Snedden; A. R. Thakar; A. Szalay; J. A. Munn; J. A. Smith; D. Tucker; B. C. Lee

2004-10-07T23:59:59.000Z

267

IEEE TRANSACTIONS ON BIOMEDICAL ENGINEERING, VOL. 51, NO. 12, DECEMBER 2004 2129 Influence of Head Tissue Conductivity in Forward  

E-Print Network [OSTI]

IEEE TRANSACTIONS ON BIOMEDICAL ENGINEERING, VOL. 51, NO. 12, DECEMBER 2004 2129 Influence of Head Tissue Conductivity in Forward and Inverse Magnetoencephalographic Simulations Using Realistic Head Abstract--The influence of head tissue conductivity on mag- netoencephalography (MEG) was investigated

Utah, University of

268

Performance Comparison of Nb3Sn Magnets at LBNL  

E-Print Network [OSTI]

2LCOI SC-MAG#722 LBNL-49917 Performance Comparison ofNb 3 Sn Magnets at LBNL L. Chiesa, S. Caspi, M . Coccoli,the Superconducting Magnet Group at LBNL has been developing

Chiesa, L.

2011-01-01T23:59:59.000Z

269

Status and Highlights of Educational Programming Gregory S. Boebinger, National High Magnetic Field Laboratory  

E-Print Network [OSTI]

in Higher Education REU = 18 students at all three MagLab sites (44% female, 39% African American, 28 in international journals including: The Journal of Women and Minorities in Science and Engineering, the Journal

Weston, Ken

270

Performance characterization of the Caltech corn act torus injector P. K. Loewenhardt,a) M. R. Browqb) J. Yee, and P. M. Bellan  

E-Print Network [OSTI]

A compact torus (CT), or spheromak, is a toroidal mag- netofluid configuration in which plasma is cot tokamak by the Caltech Spheromak Ijec- tion experiment to study helicity injection and refueling,3

Brown, Michael R.

271

Subscriber access provided by HARVARD UNIV ACS Nano is published by the American Chemical Society. 1155 Sixteenth Street  

E-Print Network [OSTI]

electrical,3 and mag- netic4 properties that differ from bulk materials. To harness these properties into the sculpted sur- face and thus has the potential to affect the optical and electronic properties

Prentiss, Mara

272

TEAMWORK--Jeffrey Spaleta, Kevin Sterne and Nathaniel Frissell of Virginia Tech and  

E-Print Network [OSTI]

with the installation of 40 antennas, two radar systems and a control building on 15 acres of Adak land leased from convection patterns in the ionosphere, where the interaction of the solar wind with Earth's mag- netic field

Herrick, Robert R.

273

International Sunport  

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

Security, the MagViz system is a new, ultra-low-field MRI approach first designed for brain imaging, but with a unique variation. Given a container of something that shouldn't be...

274

Expense Account Data Dictionary Acct OMNI Acct Descr Account Use Description  

E-Print Network [OSTI]

Nuclear Mag Resonance Charges for high resolution nuclear magnetic resonance (NMR), in vivo spectroscopy and volunteers as authorized by law; includes athletic awards, engraved plaques and trophies, certificates, etc

Weston, Ken

275

NMR STUDIES OF LIQUID CRYSTALS AND MOLECULES DISSOLVED IN LIQUID CRYSTAL SOLVENTS  

E-Print Network [OSTI]

84) Drobny G. , Pines A. , Sinton S. , Weitekamp D. , andMag. Res. 37, 93 (1980) 88) Sinton S. , PhD Thesis, Dept. ofDrobny G. , Pines A. , Sinton S. , Weitekamp D. , Ramis-79

Drobny, G.P.

2010-01-01T23:59:59.000Z

276

E-Print Network 3.0 - auto zoom function Sample Search Results  

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

of Engineering Science, Robotics Research Group, Active Vision Group Collection: Engineering 55 CHI '95 MOSAIC OF CREATIVITY s May 7-11 1995 Videos The DragMag Image...

277

InsideIllinoisDec. 6, 2007 Vol. 27, No. 11  

E-Print Network [OSTI]

student John Tobin (now at the University of Michigan) and graduate student Woojin Kwon. The Spitzer Space a pirouet- ting ice skater pulling in her arms. The force of the growing mag- netic field ejects some

Lewis, Jennifer

278

Astronomical studies of solar system bodies 2060 Chiron and 1 Ceres  

E-Print Network [OSTI]

In this thesis two separate projects are investigated, a stellar occultation by 2060 Chiron and rotationally resolved spectra of 1 Ceres. On 29 November 2011 UT, 2060 Chiron occulted a 14-mag star; data were successfully ...

Ruprecht, Jessica Dawn

2013-01-01T23:59:59.000Z

279

E-Print Network 3.0 - argentine andes constraints Sample Search...  

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

only barrier to atmospheric circulation... that have been made for the Central and Colombian Andes and (2) an examination of the source and mag- nitude... of error for each...

280

Superconducting magnets for muon capture and phase rotation  

E-Print Network [OSTI]

of Various Cases for Superconducti ng Magnets Inside andTransactions on Applied Superconductivity 7, No 2. P 642 (LBNL-43998 SC-MAG-683 SUPERCONDUCTING MAGNETS FOR MUON

Green, M.A.

2011-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "maldives mag m1" 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

Mechanical design of a high field common coil magnet  

E-Print Network [OSTI]

This paper presents the mechanical design for a 14 tesla 2-The design addresses mechanical issues particular to theLBNL #43481 SC MAG #668 MECHANICAL DESIGN OF A mGH FIELD

Caspi, S.

2011-01-01T23:59:59.000Z

282

untied as long as the magnetization remains smooth and finite. Skyrmions are therefore  

E-Print Network [OSTI]

neutron-scattering experiments and related theoretical work that established that lattices of skyrmions of a weak mag- netic field4,5 . But because neutron scattering can detect only periodic structures

Blaustein, Andrew R.

283

Facilities: NHMFL 14.5 Tesla Fourier Transform Ion Cyclotron Resonance Mass Spectrometer Citation: A Pseudoatomic Model of the COPII Cage Obtained from Cryo-Electron Microscopy and Mass Spectrometry,  

E-Print Network [OSTI]

Facilities: NHMFL 14.5 Tesla Fourier Transform Ion Cyclotron Resonance Mass Spectrometer Citation ultrahigh-resolution 14.5 tesla Fourier transform ion cyclotron resonance mass spectrometry. The Mag

Weston, Ken

284

The Stabilisation Potential of Individual and Mixed Assemblages of Natural Bacteria and Microalgae  

E-Print Network [OSTI]

The Stabilisation Potential of Individual and Mixed Assemblages of Natural Bacteria and Microalgae components (heterotrophic bacteria and autotrophic microalgae) in terms of their individual contribution benthic assemblages (prokaryotic, eukaryotic and mixed cultures) of bacteria and microalgae. Mag

Paris-Sud XI, Universit de

285

antennae galaxies arp: Topics by E-print Network  

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

(PAH) emission stemming from a deeply embedded (AV24mag) region of less than 120pc in size. There is also a con... Alonso-Herrero, A; Esquej, P; Gonzalez-Martin, O;...

286

Novel Electrolytes and Additives  

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

7 Point of Reference - Electrode and Electrolyte Chemistries Gen 2 electrolyte EC:EMC (3:7 by wt.) + 1.2M LiPF 6 Cu (-) Al (+) Mag-10 graphite Particle size 5 m Celgard...

287

Solution for Practice Exam III  

E-Print Network [OSTI]

1. (20pts) Given a sphere of radius 2 centered at the origin, ?nd the equation for ... mag) 21') . (rage-1 Y'SRQ) -Y\\ circle. o l mr. = gmgl i {vz- zrjlrcls 1' m "'5. O.

288

1118 OPTICS LETTERS / Vol. 24, No. 16 / August 15, 1999 Selecting optical patterns with spatial phase modulation  

E-Print Network [OSTI]

parallel to the crystal a axis to take advantage of the r13 electro- optic coefficient-crystal light valve. The effective mag- nitude of the spatial wave vector of the phase modu- lation

Saffman, Mark

289

Superconducting magnets for muon capture and phase rotation  

E-Print Network [OSTI]

LBNL-43998 SC-MAG-683 SUPERCONDUCTING MAGNETS FOR MUONDE-AC03-76SF00098. Green SUPERCONDUCTING MAGNETS FOR MUONet ai, "The Use of Superconducting Solenoids in a Muon

Green, M.A.

2011-01-01T23:59:59.000Z

290

National High Magnetic Field Laboratory - Series Connected Hybrid  

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

Magnet Lab Series Connected Hybrid for Magnet Lab Figure 1. Vertical Section of the Series Connected Hybrid Magnet for the Mag Lab. The Magnet Lab has embarked on innovative...

291

Microsoft Word - Transmittal of Final Audit Report A-13-02, SRS...  

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

DSM:MAG:13-1490:UFC 2300.00 Department of Energy Carlsbad Field Office P.O. Box 3090 Carlsbad, New Mexico 88221 August 6, 2013 Mr. John E. Kieling, Chief Hazardous Waste Bureau New...

292

Abstract-This paper investigates four different short circuit fault conditions which can occur for an inverter-fed perma-  

E-Print Network [OSTI]

for an inverter-fed perma- nent magnet synchronous motor (PMSM) with buried mag- nets. The fault conditions Condition #... Inverter PM machine (at steady state) N Short circuit fault conditions of a buried PMSM

Jantsch, Axel

293

A late, infrared flash from the afterglow of GRB 050319  

E-Print Network [OSTI]

We report the detection of a bright, near-infrared flash from the afterglow of GRB 050319, 6.15 hours after the burst. The IR flash faded rapidly from J=13.12 mag. to J > 15.5 mag. in about 4 minutes. There are no reported simultaneous observations at other wavelengths making it an unique event. We study the implications of its late timing in the context of current theoretical models for GRB afterglows.

Koshy George; Dipankar P. K. Banerjee; Thyagarajan Chandrasekahar; Nagarhalli M. Ashok

2006-02-17T23:59:59.000Z

294

Magnetic mesoporous materials for removal of environmental wastes  

SciTech Connect (OSTI)

We have synthesized two different magnetic mesoporous materials that can be easily separated from aqueous solutions by applying a magnetic field. Synthesized magnetic mesoporous materials, Mag-SBA-15 (magnetic ordered mesoporous silica) and Mag-OMC (magnetic ordered mesoporous carbon), have a high loading capacity of contaminants due to high surface area of the supports and high magnetic activity due to the embedded iron oxide particles. Application of surface-modified Mag-SBA-15 was investigated for the collection of mercury from water. The mercury adsorption using Mag-SBA-15 was rapid during the initial contact time and reached a steady-state condition, with an uptake of approximately 97% after 7 hours. Application of Mag-OMC for collection of organics from water, using fluorescein as an easily trackable model analyte, was explored. The fluorescein was absorbed into Mag-OMC within minutes and the fluorescent intensity of solution was completely disappeared after an hour. In another application, Mag-SBA-15 was used as a host of tyrosinase, and employed as recyclable catalytic scaffolds for tyrosinase-catalyzed biodegradation of catechol. Tyrosinase aggregates in Mag-SBA-15, prepared in a two step process of tyrosinase adsorption and crosslinking, could be used repeatedly for catechol degradation with no serious loss of enzyme activity. Considering these results of cleaning up water from toxic inorganic, organic and biochemical contaminants, magnetic mesoporous materials have a great potential to be employed for the removal of environmental contaminants and potentially for the application in large-scale wastewater treatment plants.

Kim, Byoung Chan; Lee, Jinwoo; Um, Wooyong; Kim, Jaeyun; Joo, Jin; Lee, Jin Hyung; Kwak, Ja Hun; Kim, Jae Hyun; Lee, Changha; Lee, Hongshin; Addleman, Raymond S.; Hyeon, Taeghwan; Gu, Man Bock; Kim, Jungbae

2011-09-15T23:59:59.000Z

295

TENDENCIAS Y CONTRATENDENCIAS EN LA GESTION DE LAS GOBERNACIONES VENEZOLANAS: EL CASO DEL ESTADO LARA  

E-Print Network [OSTI]

@yahoo.com, haydeeochoa@gmail.com Resumen El proceso de descentralización y privatización en Venezuela surgió como una descentralización política territorial iniciado en Venezuela desde 1989. En este trabajo nos proponemos explorar la, descentralización, privatización, modelo de desarrollo, Venezuela. 1 Magíster en Ciencia Política y Magíster en

Boyer, Edmond

296

Control of flowering time and spike development in cereals: the earliness per se Eps-1 region in wheat, rice, and Brachypodium  

E-Print Network [OSTI]

spring growth habit) carrying the Eps-A m 1 allele for latewinter growth habit) carrying the Eps-A m 1 allele for earlyPCR) markers flanking the Eps-A m 1 region (Table 1), and

Faricelli, Maria E.; Valrik, Miroslav; Dubcovsky, Jorge

2010-01-01T23:59:59.000Z

297

E-Print Network 3.0 - accelerator workshop snowmass Sample Search...  

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

Collection: Plasma Physics and Fusion 2 Snowmass 2001 M1 Working Group: MuonBased Accelerators Snowmass'01 M1 Working Group Summary: Snowmass 2001 M1 Working Group: Muon-Based...

298

CfA4: LIGHT CURVES FOR 94 TYPE Ia SUPERNOVAE  

SciTech Connect (OSTI)

We present multi-band optical photometry of 94 spectroscopically confirmed Type Ia supernovae (SNe Ia) in the redshift range 0.0055-0.073, obtained between 2006 and 2011. There are a total of 5522 light-curve points. We show that our natural-system SN photometry has a precision of {approx}< 0.03 mag in BVr'i', {approx}< 0.06 mag in u', and {approx}< 0.07 mag in U for points brighter than 17.5 mag and estimate that it has a systematic uncertainty of 0.014, 0.010, 0.012, 0.014, 0.046, and 0.073 mag in BVr'i'u'U, respectively. Comparisons of our standard-system photometry with published SN Ia light curves and comparison stars reveal mean agreement across samples in the range of {approx}0.00-0.03 mag. We discuss the recent measurements of our telescope-plus-detector throughput by direct monochromatic illumination by Cramer et al. This technique measures the whole optical path through the telescope, auxiliary optics, filters, and detector under the same conditions used to make SN measurements. Extremely well characterized natural-system passbands (both in wavelength and over time) are crucial for the next generation of SN Ia photometry to reach the 0.01 mag accuracy level. The current sample of low-z SNe Ia is now sufficiently large to remove most of the statistical sampling error from the dark-energy error budget. But pursuing the dark-energy systematic errors by determining highly accurate detector passbands, combining optical and near-infrared (NIR) photometry and spectra, using the nearby sample to illuminate the population properties of SNe Ia, and measuring the local departures from the Hubble flow will benefit from larger, carefully measured nearby samples.

Hicken, Malcolm; Challis, Peter; Kirshner, Robert P.; Bakos, Gaspar; Berlind, Perry; Brown, Warren R.; Caldwell, Nelson; Calkins, Mike; Falco, Emilio; Fernandez, Jose; Friedman, Andrew S.; Groner, Ted; Hartman, Joel [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Rest, Armin [Space Telescope Science Institute, Baltimore, MD 21218 (United States); Cramer, Claire E. [NIST (National Institute of Standards and Technology), Gaithersburg, MD 20899 (United States); Wood-Vasey, W. Michael [Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260 (United States); Currie, Thayne [NASA, Goddard Space Flight Center, Greenbelt, MD 20771 (United States); De Kleer, Kathy [Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States); Esquerdo, Gil; Everett, Mark, E-mail: mhicken@cfa.harvard.edu [Planetary Science Institute, 1700 East Fort Lowell Road, Tucson, AZ 85719 (United States); and others

2012-06-01T23:59:59.000Z

299

Re-calibration of SDF/SXDS Photometric Catalogs of Suprime-Cam with SDSS Data Release 8  

E-Print Network [OSTI]

We present photometric recalibration of the Subaru Deep Field (SDF) and Subaru/XMM-Newton Deep Survey (SXDS). Recently, Yamanoi et al. (2012) suggested the existence of a discrepancy between the SDF and SXDS catalogs. We have used the Sloan Digital Sky Survey (SDSS) Data Release 8 (DR8) catalog and compared stars in common between SDF/SXDS and SDSS. We confirmed that there exists a 0.12 mag offset in B-band between the SDF and SXDS catalogs. Moreover, we found that significant zero point offsets in i-band (~ 0.10 mag) and z-band (~ 0.14 mag) need to be introduced to the SDF/SXDS catalogs to make it consistent with the SDSS catalog. We report the measured zero point offsets of five filter bands of SDF/SXDS catalogs. We studied the potential cause of these offsets, but the origins are yet to be understood.

Yagi, Masafumi; Yamanoi, Hitomi; Furusawa, Hisanori; Nakata, Fumiaki; Komiyama, Yutaka

2012-01-01T23:59:59.000Z

300

On the CCD Calibration of Zwicky galaxy magnitudes & The Properties of Nearby Field Galaxies  

E-Print Network [OSTI]

We present CCD photometry for galaxies around 204 bright (m_Z = -0.35 \\pm 0.15 mag. The scatter around this fit is about 0.4 mag. Correcting the Zwicky magnitude system with the best fit model results in a 60% lower normalization and 0.35 mag brighter M_* in the luminosity function. This brings the CfA2 luminosity function closer to the other low redshift estimations (eg Stromlo-APM or LCRS). We find a significant positive angular correlation of magnitudes and position in the sky at scales smaller than about 5 armin, which corresponds to a mean separation of 120 Kpc/h. We also present colours, sizes and ellipticities for galaxies in our fields which provides a good local reference for the studies of galaxy evolution.

E. Gaztanaga; G. B. Dalton

1999-10-11T23:59:59.000Z

Note: This page contains sample records for the topic "maldives mag m1" 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 NEW CEPHEID DISTANCE TO THE GIANT SPIRAL M101 BASED ON IMAGE SUBTRACTION OF HUBBLE SPACE TELESCOPE/ADVANCED CAMERA FOR SURVEYS OBSERVATIONS  

SciTech Connect (OSTI)

We accurately determine a new Cepheid distance to M101 (NGC 5457) using archival Hubble Space Telescope (HST)/Advanced Camera for Surveys V and I time series photometry of two fields within the galaxy. We make a slight modification to the ISIS image subtraction package to obtain optimal differential light curves from HST data. We discovered 827 Cepheids with periods between 3 and 80 days, the largest extragalactic sample of Cepheids observed with HST by a factor of two. With this large Cepheid sample, we find that the relative distance of M101 from the Large Magellanic Cloud is {Delta}{mu}{sub LMC} = 10.63 {+-} 0.04 (random) {+-} 0.06 (systematic) mag. If we use the geometrically determined maser distance to NGC 4258 as our distance anchor, the distance modulus of M101 is {mu}{sub 0} = 29.04 {+-} 0.05 (random) {+-} 0.18 (systematic) mag or D = 6.4 {+-} 0.2 (random) {+-} 0.5 (systematic) Mpc. The uncertainty is dominated by the maser distance estimate ({+-}0.15 mag), which should improve over the next few years. We determine a steep metallicity dependence, {gamma}, for our Cepheid sample through two methods, yielding {gamma} = -0.80 {+-} 0.21 (random) {+-} 0.06 (systematic) mag dex{sup -1} and {gamma} = -0.72{sup +0.22}{sub -0.25} (random) {+-} 0.06 (systematic) mag dex{sup -1}. We see marginal evidence for variations in the Wesenheit period-luminosity relation slope as a function of deprojected galactocentric radius. We also use the tip of the red giant branch method to independently determine the distance modulus to M101 of {mu}{sub 0} = 29.05 {+-} 0.06 (random) {+-} 0.12 (systematic) mag.

Shappee, Benjamin J.; Stanek, K. Z., E-mail: shappee@astronomy.ohio-state.edu, E-mail: kstanek@astronomy.ohio-state.edu [Department of Astronomy, Ohio State University, Columbus, OH 43210 (United States)

2011-06-01T23:59:59.000Z

302

On Primitivity and the Unital Full Free Product of Finite Dimensional C*-algebras  

E-Print Network [OSTI]

= kp1 and k2 = kp2 Assume B is {isomorphic to Ll j=1Mnj . To prove the result it is enough to show there are positive integers (m(1); : : :m(l)) such that n1m(1) + + nlm(l) = k: Let (B1; B) = [m1(1); : : : ;m1(l)]; (B2; u Bu) = [m2...(1); : : : ;m2(l)]: Since (MN ; B1) (B1; B) = (MN ; B2) (B2; u Bu) we deduce thatm1m1(j) = m2m2(j) for all 1 j l. Multiplying by k and using N = m1k1 = m2k2 we conclude N p1 m1(j) = km1m1(j) = km2m2(j) = N p2 m2(j); so p2m1(j) = p1m2(j). Since gcd...

Torres Ayala, Francisco

2012-07-16T23:59:59.000Z

303

VOLUME 80, NUMBER 9 P H Y S I C A L R E V I E W L E T T E R S 2 MARCH 1998 Giant Spin Relaxation of an Ultracold Cesium Gas  

E-Print Network [OSTI]

of attention. The atomic sample is spin polarized and confined in a mag- netic trap. The condensation of an Ultracold Cesium Gas J. Söding, D. Guéry-Odelin, P. Desbiolles, G. Ferrari,* and J. Dalibard Laboratoire of magnitude larger than predicted, ruling out a Bose-Einstein condensation of Cs in this internal state. [S

Guéry-Odelin, David

304

E. L. BRADY AND M. DEUTSCH yields very definite information concerning the parities  

E-Print Network [OSTI]

of Physics and Chemistry Department, Massachusetts Institute of Technology, Cambridge, MassachusettsGect. Unfortunately, it seems at present entirely unfeasible to separate the nuclear magnetic substates by application been proposed to change the relative populations of the several mag- netic substates of an excited

Browder, Tom

305

High Energy Solar Physics: Anticipating HESSI ASP Conference Series, Vol. xxx, 2000  

E-Print Network [OSTI]

High Energy Solar Physics: Anticipating HESSI ASP Conference Series, Vol. xxx, 2000 R. Ramaty and N. Mandzhavidze, eds. Solar Flare Theory and the Status of Flare Understanding E.R. Priest Department current understanding of the mag­ netohydrodynamics of solar flares. The theory of reconnection in 2D

Priest, Eric

306

Home Grounds and Gardens Soil Report  

E-Print Network [OSTI]

Conventional Fertilizer Recommendations We recommend that you uniformly broadcast 4.6 lbs per 1,000 sq. ft of Potash include 14 lbs of sul-po-mag (0-0-22). Composted manure is an excellent source of all three 1 lb of Nitrogen for every 800 lbs of manure applied per 1000 sq. ft. Manures and composts

New Hampshire, University of

307

Investigation of the profit rate problem of machining economics using geometric programming  

E-Print Network [OSTI]

the objective function of stage 1. Since this constraint is tight, it mag also be written as an equation. Table 13 contains the resulting stage 2 program. Table 13. MPMCP Posgnomlal Stage 2 Primal Program Minimize go=Co~ tm+Co2tmT subject to 0l...

Lundeen, Calvin Douglas

1986-01-01T23:59:59.000Z

308

A 2.15 hr ORBITAL PERIOD FOR THE LOW-MASS X-RAY BINARY XB 1832-330 IN THE GLOBULAR CLUSTER NGC 6652  

SciTech Connect (OSTI)

We present a candidate orbital period for the low-mass X-ray binary (LMXB) XB 1832-330 in the globular cluster NGC 6652 using a 6.5 hr Gemini South observation of the optical counterpart of the system. Light curves in g' and r' for two LMXBs in the cluster, sources A and B in previous literature, were extracted and analyzed for periodicity using the ISIS image subtraction package. A clear sinusoidal modulation is evident in both of A's curves, of amplitude {approx}0.11 mag in g' and {approx}0.065 mag in r', while B's curves exhibit rapid flickering, of amplitude {approx}1 mag in g' and {approx}0.5 mag in r'. A Lomb-Scargle test revealed a 2.15 hr periodic variation in the magnitude of A with a false alarm probability less than 10{sup -11}, and no significant periodicity in the light curve for B. Though it is possible that saturated stars in the vicinity of our sources partially contaminated our signal, the identification of A's binary period is nonetheless robust.

Engel, M. C.; Heinke, C. O.; Sivakoff, G. R.; Elshamouty, K. G. [Physics Department, 4-183 CCIS, University of Alberta, Edmonton, AB T6G 2E1 (Canada); Edmonds, P. D., E-mail: mcengel@ualberta.ca, E-mail: heinke@ualberta.ca [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2012-03-10T23:59:59.000Z

309

LEIOCEPHALIDAE 1989 Leiocephalinae Frost and Etheridge, Misc. Publ. Mus. Nat. Hist. Univ.  

E-Print Network [OSTI]

, Hispaniola, Navassa, and Martinique. Recently extinct species were found on Barbuda and Antigua, Anguilla, Guadeloupe, Hispaniola, Puerto Rico, and Jamaica. Leiocephalus Gray 1827 Leiocephalus Gray, Philos. Mag, 84: 1. Range: Cuba and nearby islands, the Cayman Islands, the Bahama Islands, Hispaniola

310

Electrochemical Properties of Nanostructured Al1-xCux Alloys as Anode Materials for Rechargeable Lithium-Ion Batteries  

E-Print Network [OSTI]

controlling these two properties is the mag- nitude of interaction between the active and the inactiveElectrochemical Properties of Nanostructured Al1-xCux Alloys as Anode Materials for Rechargeable Lithium-Ion Batteries C. Y. Wang,a, * Y. S. Meng,b, * G. Ceder,c, *,z and Y. Lia,d,z a Advanced Materials

Ceder, Gerbrand

311

editor's note Welcome to the seventh issue of Flux, a magazine designed to explore the staggering  

E-Print Network [OSTI]

of burnt tree waste? See "Fueling the Future," on page 8, for more about the Mag Lab's clean- energy and watched plenty of stories about the energy crunch facing our country and our world. Each time you gas up resources, we've showcased the story "Fueling the Future," which explains some of the critical clean-energy

Weston, Ken

312

24 JOM May 1998 The lightest of all metals, lithium is used  

E-Print Network [OSTI]

of applications, including the production of organolithium compounds, as an alloying addition to aluminum and mag and aluminum, the dominant structuralmetals,andwiththoseofmag- nesium and titanium, both considered too pricey that its market distribution may be radically al- tered by rapid growth in one applica- tion: automotive

Sadoway, Donald Robert

313

Jack Dongarra A Historical Overview and  

E-Print Network [OSTI]

a performance advantage of at least one order of magnitude over conventional systems of that time. Raw mean the rate of execution for floating-point operations. Here we chart Kilo-flop (thousands the complete lifespan of modern computing-- we see an increase in performance averaging two orders of mag

Dongarra, Jack

314

Of the estimated 5 million barrels of crude oil released into the Gulf of Mexico from the Deepwater Horizon oil spill, a  

E-Print Network [OSTI]

Of the estimated 5 million barrels of crude oil released into the Gulf of Mexico from the Deepwater Horizon oil spill, a fraction washed ashore onto sandy beaches from Louisiana to the Florida panhandle. Researchers at the MagLab compare the detailed molecular analysis of hydrocarbons in oiled sands from

Weston, Ken

315

a1d l-type ca: Topics by E-print Network  

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

We also obtained spectra of the well-known J15.4-16.1 mag late M-type cluster members PPl 1, Teide 1, and Calar 3. We find that the former six objects have early- to mid-L...

316

Editorial responsibility: T. Koyaguchi David S. Stevenson (Y)  

E-Print Network [OSTI]

convection, the conduit radius to the fourth power, and inversely proportional to the degassed mag- ma is proportional to the flow rate of the over- turning magmas (proportional to the density difference driving convection 7 Volcano monitoring Introduction Persistent volcanism involves prolonged high thermal

317

STATO NOME SEDE Promotori Posti disponibili  

E-Print Network [OSTI]

* requisiti linguistici * ARGENTINA UNIVERSIDAD DE BUENOS AIRES - FADU UBA Davide Fassi 5 LM http Zurlo 5 LM LM http://www.pri.unc.edu.ar/ 20-mag 30-nov agosto marzo conoscenza lingua spagnola AUSTRALIA Giovanni Conti 5 LM LM LM LM LM LM http://www.studyabroad.qut.edu.au/apply/entryrequire/englishr equi

318

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

319

First results from CSSWE CubeSat: Characteristics of relativistic electrons in the near-Earth environment during the October 2012  

E-Print Network [OSTI]

yearly window-averaged sunspot num- bers and weekly window-averaged solar wind speed (km/s) in the topSat mission, which was launched into a highly inclined (65) low Earth orbit, are analyzed along Spectrometer (MagEIS) instruments aboard the Van Allen Probes, which are in a low inclination (10) geo

Li, Xinlin

320

Nucleic Acids Research doi:10.1093/nar/gkn305  

E-Print Network [OSTI]

server for rapidly generating accurate 3D protein structures using only assigned nuclear magnetic no NOE and/or J-coupling data to perform its calculations. CS23D accepts chemical shift files in either. Tests conducted on more than 100 proteins from the BioMagResBank indicate that CS23D converges (i

Lin, Guohui

Note: This page contains sample records for the topic "maldives mag m1" 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

Inferring the scale height of the lunar nightside double layer  

E-Print Network [OSTI]

compared to the solar wind plasma, due to the ambipolar potential drop across the wake boundary identified that across the wake boundary. [3] The MAG/ER instrument uses vector magnetic field data and measurements angle on field lines with higher tip angles encounter a smaller average potential before reflecting (the

California at Berkeley, University of

322

Space Sci Rev (2011) 165:5991 DOI 10.1007/s11214-011-9777-9  

E-Print Network [OSTI]

· Particle acceleration · Turbulence · Wake · Lunar surface · Lunar core · Dust · Electric fields · Crustal in the Earth's mag- netosphere, at the bow shock, and in the solar wind; and the formation and structure, USA #12;60 D.G. Sibeck et al. lunar wake. Planetary topics include the lunar exosphere and its

California at Berkeley, University of

323

Tiny camera could aid in robotics, night vision Monday, January 17, 2011  

E-Print Network [OSTI]

Tiny camera could aid in robotics, night vision Monday, January 17, 2011 Researchers from night-vision surveillance, robotic vision, endoscopic imaging, and consumer electronics. "We were on this article! 0 COMMENTS Page 1 of 1Tiny camera could aid in robotics, night vision | R&D Mag 1/19/2011http

Rogers, John A.

324

Noise Driven Short-Time Phase Spectrum Compensation Procedure for Speech Enhancement  

E-Print Network [OSTI]

Noise Driven Short-Time Phase Spectrum Compensation Procedure for Speech Enhancement Anthony P.lyons, k.paliwal}@griffith.edu.au Abstract Typical speech enhancement algorithms operate on the short- time approach to speech enhancement has been proposed where the noisy mag- nitude spectrum is recombined

325

38 IEEE TRANSACTIONS ON POWER ELECTRONICS, VOL. 23, NO. 1, JANUARY 2008 Dual Interleaved Active-Clamp Forward With  

E-Print Network [OSTI]

ZVS by utilizing the energy stored in the mag- netizing inductor. The voltage stress on the primary-voltage MOSFETs are needed for the primary switches. Also, the two interleaved parts utilize auxiliary windings the magnetizing inductors and the equivalent capacitors of the switches during the transition time, switching loss

Lehman, Brad

326

arXiv:0904.0799v1[physics.flu-dyn]5Apr2009 Bistability and hysteresis of dipolar dynamos generated by turbu-  

E-Print Network [OSTI]

and it is believed to be responsible for the mag- netic fields of cosmic objects including the sun and most planets distribution TS = T0 - d2 r2 /2 and a gravity field in the form g = -dr, where rd is the length of the posi- tion vector with respect to the center of the sphere. This form of temperature profile alludes

Schmidt, Matthias

327

96-well Format DNA Extraction Protocol for Freeze-dried Maize Seedling Leaves  

E-Print Network [OSTI]

Cat# T100-30). Add ~ 1 cM of glass beads* or three 3 mm metal beads (3 mm Tungsten Carbide Beads of the youngest leaf. * Note that glass beads are not compatible all extraction methods. Metal beads are necessary for MagAttract. If tissue may be used for other methods, use metal beads. b. Cover tubes with air pore

Wurtele, Eve Syrkin

328

2014 Society of Economic Geologists, Inc. Economic Geology, v. 109, pp. 16431666  

E-Print Network [OSTI]

by or genetically related to carbon- atites and agpaitic to hyperagpaitic intrusions. As a result, the causes to be magmatic (Castor, 2008); others, like Bayan Obo, are interpreted to be hydrothermal, albeit involving and Nechalacho, are interpreted to have formed by a combination of both mag- matic and hydrothermal processes

329

Structure of magnetic fields in NOAA active regions 0486 and 0501 and in the associated interplanetary ejecta  

E-Print Network [OSTI]

field occurs at the day side mag- netopause and this reconnection transports energy from the solar wind interplanetary ejecta Vasyl Yurchyshyn Big Bear Solar Observatory, 40386 North Shore Lane, Big Bear City, CA Bear Solar Observatory, 40386 North Shore Lane, Big Bear City, CA 92314, USA Crimean Astrophysical

Yurchyshyn, Vasyl

330

Magellan Instant Camera testbed  

E-Print Network [OSTI]

The Magellan Instant Camera (MagIC) is an optical CCD camera that was built at MIT and is currently used at Las Campanas Observatory (LCO) in La Serena, Chile. It is designed to be both simple and efficient with minimal ...

McEwen, Heather K. (Heather Kristine), 1982-

2004-01-01T23:59:59.000Z

331

Acta Mechanica Sinica (2013) 29(1):7384 DOI 10.1007/s10409-013-0056-8  

E-Print Network [OSTI]

, electric and mag- netic ones), and thus they have potential applications, say, in energy harvest, among, and elastic elds, MEE materials can convert energies from one form to the other (among the mechanical and actuators with applications in hi-tech ar- eas such as ultrasonic and microwave elds [2, 3]. Besides, MEE

Pan, Ernie

2013-01-01T23:59:59.000Z

332

Introduction The Dark Energy Survey (DES) requires a photometric precision of  

E-Print Network [OSTI]

Introduction The Dark Energy Survey (DES) requires a photometric precision of 0.02 mag for a wide scattering, aerosol and dust scattering, water vapor absorption, etc. We can derive the atmospheric to monitor the water, aerosol, Rayleigh scattering, and ozone components of the atmosphere. These filters had

333

ATLANTIC THREAD HERRING (OPISTHONEMA OGLINUM) -  

E-Print Network [OSTI]

there on a secondary magnet. Using the average recovery efficiencies, 1 earlier at all of the plants for recovery of steel tags placed in menhaden. Primary magnets are lo- cated over these magnets the same day fish are processed. Secondary mag- nets were located at other positions

334

ISSN1834-3937 Sydney FeStival  

E-Print Network [OSTI]

swims design Where art & Science meet: vivian chan ShaW & anne SchoField SYDNEY ALUMNI MAgAzINE NOVEMb 668 812 John Malkovich in The Giacomo Variations Concert Hall, Sydney Opera House, January 20 Sutter City Recital Hall Angel Place, January 18 Leadership Partner #12;SAM NOV 2010 1 editor Diana

Viglas, Anastasios

335

VOLUME 75, NUMBER 2 P H Y S I C A L R E V I E W L E T T E R S 10 JULY 1995 Phonon and Magnetic Neutron Scattering at 41 meV in YBa2Cu3O7  

E-Print Network [OSTI]

Neutron Scattering at 41 meV in YBa2Cu3O7 Hung Fai Fong, B. Keimer, and P. W. Anderson Department is the generalized magnetic susceptibility whose imaginary part x00 q, v is measur- able by neutron scattering. Below to be of mag- netic origin in polarized neutron scattering experiments by Mook et al. [2]. (We quote the in

Aksay, Ilhan A.

336

Optimal PMU Placement Evaluation for Power System Dynamic State Estimation  

E-Print Network [OSTI]

flow along the transmission lines or transformers. · Bus power injection measurements: the real of dis- tribution systems, the line current magnitude measurements (along the transmission lines. · Current phasor measurements: the phase angles and mag- nitudes of current phasors along transmission lines

Bishop, Gary

337

Observability and Estimation Uncertainty Analysis for PMU Placement Alternatives  

E-Print Network [OSTI]

measurements: the real and reactive power flow along the transmission lines or transformers. · Bus power-3175 USA e-mail: {jing2009, welch, gb}@cs.unc.edu along the transmission lines or transformers: the phase angles and mag- nitudes of current phasors along transmission lines or transformers. Recent

Bishop, Gary

338

Part 8, Authors: K To Kyzer  

E-Print Network [OSTI]

de Namur. Namur. Agronoomia.?Agronoomia. Polluas janduse ja Loomatervishoim Ajakiri. Tartu. All-Pets Mag.?All-Pets Magazine. Chicago. Al?g. Deutsch. Gefl?gel-Ztg.?Allgemeine Deutsche Gefl?gel-Zeitung. Leipzig. [Not available] Allg. Forst- u. Jagd...

Segal, Dorothy B.; Ray, Doris H.; Carson, Gertrude B.; Hassall, Albert; Doss, Mildred A.

1946-01-01T23:59:59.000Z

339

OXYGEN GAS-PHASE ABUNDANCE REVISITED M. K. Andre,1,2  

E-Print Network [OSTI]

OXYGEN GAS-PHASE ABUNDANCE REVISITED M. K. Andre´,1,2 C. M. Oliveira,2 J. C. Howk,2 R. Ferlet,1 J gas-phase oxygen abundance along the sight lines toward 19 early-type Galactic stars at an average mag?1 with a standard deviation of 15% is consistent with previous surveys. The mean oxygen abundance

Howk, Jay Christopher

340

Electron-inertia effects on driven magnetic field reconnection N. Al-Salti and B. K. Shivamoggi  

E-Print Network [OSTI]

University of Central Florida, Orlando, Florida 32816-1364 Received 26 March 2003; accepted 8 August 2003 reconnection has been found not to take place. © 2003 American Institute of Physics. DOI: 10.1063/1.1615242 I others . Colli- sionless reconnection appears to be the origin of strong mag- netic activity in solar

Davidson, Fordyce A.

Note: This page contains sample records for the topic "maldives mag m1" 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

The Astrophysical Journal, 708:314333, 2010 January 1 doi:10.1088/0004-637X/708/1/314 C 2010. The American Astronomical Society. All rights reserved. Printed in the U.S.A.  

E-Print Network [OSTI]

. The American Astronomical Society. All rights reserved. Printed in the U.S.A. FORMATION OF TORUS-UNSTABLE FLUX the tether-cutting reconnection. During the eruption, the central part of the sigmoid brightens due 1. INTRODUCTION 1.1. Solar Eruptions Coronal mass ejections (CMEs) are large clouds of mag- netized

Demoulin, Pascal

342

hal-00258511,version1-22Feb2008 FFLO state in thin superconducting films  

E-Print Network [OSTI]

hal-00258511,version1-22Feb2008 FFLO state in thin superconducting films A. Buzdin1 , Y. Matsuda2 in thin superconducting films in the parallel magnetic field. For the tetragonal crystal symmetry superconducting state the critical field should be isotropic. The mag- netic field pins also the direction

Paris-Sud XI, Université de

343

Annales Geophysicae, 23, 29832987, 2005 SRef-ID: 1432-0576/ag/2005-23-2983  

E-Print Network [OSTI]

No. 4 satellite (835 km, 98 inclination) is equipped with particle trackers based on silicon strip rays) ­ Mag- netospheric physics (Energetic particles, trapped) ­ Solar physics, astrophysics of angular distribution (Armstrong et al. (1990); Badhwar and Konradi (1990)) in different solar activity

Paris-Sud XI, Université de

344

Magnetotransport behavior of Co nanowires coupled to Ni80Fe20 films S. Goolaup, A. O. Adeyeye, and N. Singh  

E-Print Network [OSTI]

of patterned array of 60-nm-thick Co nanowires NWs with Cu spacer layer. The hybrid structures display unique lateral dimensions of the materials have a drastic effect on the fundamental mag- netic properties separated by a Cu spacer layer. The properties of the underlying Co NWs are strongly influ- enced

Adeyeye, Adekunle

345

Astronomische Nachrichten Astronomical Notes  

E-Print Network [OSTI]

of the centrifugal force on tearing instability must be present in the specific geometry of the MRI. Magnetic the change of global topology, con- verts magnetic energy into particle energy such as heat and acceleration al. 2004), coupled velocity and magnetic field fluctuations are observed above critical applied mag

Tatsuno, Tomoya

346

IEEE TRANSACTIONS ON MAGNETICS, VOL. 43, NO. 2, FEBRUARY 2007 693 Fabrication, Microstructure, Magnetic, and Recording  

E-Print Network [OSTI]

the method we used to fabricate the media as well as an energetic rationale for the driving force to produce is progressing on patterned media [1] as well as heat assisted mag- netic recording (HAMR) [2], [3]. Both grains are percolated and hence magnetically coupled and have strong perpendicular magnetic anisotropy

Laughlin, David E.

347

Our best juniors still struggle with Gauss's Law: Characterizing their difficulties  

E-Print Network [OSTI]

. Pepper, Stephanie V. Chasteen, Steven J. Pollock and Katherine K. Perkins Science Education Initiative difficulties with Gauss's law observed in an upper-division Electricity and Mag- netism (E&M) course symmetry it is impossible (rather than "difficult") to calculate the electric field using Gauss's law. One

Colorado at Boulder, University of

348

Pacific Southwest Forest & Range  

E-Print Network [OSTI]

. Rotation of the cups and vanes is detected by means of permanent mag- nets and magnetic reed switches. The magnets are imbedded in an aluminum rotor attached to the anemometer shaft (fig. 2). Four magnets are used , ( C) cup, (D) wea the r shi eld, (E) stainless steel ball bearings, (F) magnet holder with magnets

Standiford, Richard B.

349

Passive Sensing and Active Sensing of A Biomimetic Whisker DaeEun Kim1 and Ralf Moller2  

E-Print Network [OSTI]

the whisker carrying a permanent magnet is surrounded by mag- netic sensors, and these sensors can measure reported that a biomimetic whisker with steel shaft and magnetic sensors can measure the vibration. In the biological whisker sys- tem, mechanoreceptors surrounding the whisker shaft in the follicle structure measure

Moeller, Ralf

350

A planar ion trap chip with integrated structures for an adjustable magnetic field gradient  

E-Print Network [OSTI]

field necessary for magnetic-gradient- induced coupling between ionic effective spins. We dem- onstrate] magnetic field gradient, however, such coupling is induced. Also, coupling between spin states of different-gradient- induced coupling (MAGIC). A static gradient can be generated by permanent mag- nets [15, 16] or by current

Wunderlich, Christof

351

(This is a sample cover image for this issue. The actual cover is not yet available at this time.) This article appeared in a journal published by Elsevier. The attached  

E-Print Network [OSTI]

- gated and used as permanent magnets because of their high mag- netization (Ms), Curie temperature (Tc on the structural and magnetic properties of high coercivity (Hc) SrFe10Al2O19 hexaferrite have been investigated are ferromagnetically aligned but the coupling between Fe moments at the different crystallographic positions may

Liu, J. Ping

352

Softhard exchange-coupled layered structures with modulated exchange coupling  

E-Print Network [OSTI]

, Tuscaloosa, Alabama 35487-0209 Received 8 April 2003; accepted 28 June 2003 Magnetically soft/hard exchange-coupled for high performance permanent magnets in the past decades and much progress has been made in improving permanent mag- netic properties. A figure of merit of permanent magnetic materials is the maximum magnetic

Garmestani, Hamid

353

Industrial & Enterprise Systems Engineering Industrial Engineering Undergraduate Curriculum  

E-Print Network [OSTI]

Each student must satisfy the liberal education requirements of the College of Engineering, including of these courses and should be taken instead of CS 101. 4 Engineering Science Elective ­ 3 hours required. Choose Side of Engineering MATH 241--Calculus III PHYS 212--Univ Physics, Elec & Mag TAM 211--Statics Liberal

Illinois at Urbana-Champaign, University of

354

Jammed vortex matter Hajime Yoshino1  

E-Print Network [OSTI]

. Abstract: Irrationally frustrated Josephson junction array (JJA), namely JJA with irrational number density point. Figure 1: Josephson junction array (JJA) on a square lattice. The vertexes and bonds represent- not develop usual periodic vortex lattices. 1 Introduction Josephson junction array under mag- netic field

Katsumoto, Shingo

355

Intermediate-band Surface Photometry of the Edge-on Galaxy NGC 4565  

E-Print Network [OSTI]

We present a deep, 42.79 hr image of the nearby, edge-on galaxy NGC 4565 in the Beijing-Arizona-Taipei-Connecticut (BATC) 6660A band using the large-format CCD system on the 0.6m Schmidt telescope at the Xinglong Station of the National Astronomical Observatories of China (NAOC). we obtain a final image that is calibrated to an accuracy of 0.02 mag in zero point, and for which we can measure galaxy surface brightness to an accuracy of 0.25 mag at a surface brightness at 27.5 mag arcsec^-2 at 6660A, corresponding to a distance of 22 kpc from the center of the disk. The integrated magnitude of NGC4565 in our filter is m6660=8.99 (R magnitude of 9.1) to a surface brightness of 28 mag arcsec-2. We analyze the faint outer parts of this galaxy using a two-dimensional model comprised of three components: an exponential thin disk, an exponential thick disk, and a power-law halo. A total of 12 parameters are included in our model. We determine the best values of our model parameters via 10,000 random initial values, 3...

Wu, H; Deng, Z; Wu, Hong; Burstein, Dave; Deng, Zugan

2002-01-01T23:59:59.000Z

356

Deep Intermediate-Band Surface Photometry of NGC 5907  

E-Print Network [OSTI]

We obtained very deep exposures of NGC 5907 with a Schmidt telescope, large-format CCD, and intermediate-band filters centered at 6660A and 8020A. These two filters, part of a 15-filter set, are custom-designed to avoid the brightest (and most variable) night sky lines, with the result that our images go deeper, with lower sky noise, than those taken with broad-band filters. Our errors of observation reach 1 mag/arcsec^2 at 29.00 mag/arcsec-2 in the 6660A image (= 28.7 in R-band), and 27.4 mag/arcsec^ in the 8020A image (same zero point as I-band). Fainter than R = 27 mag arcsec^, the surface brightness around NGC 5907 is strongly asymmetric, being mostly brighter the NW side of the galaxy midplane. This asymmetry rules out a halo for the origin of the faint surface brightness we see. Rather, this asymmetry is likely an artifact due to a combination of light from a faint ring around this galaxy (as described in Shang et al. 1998, ApJL 504, 23) and residual surface brightness at faint levels from stars that ou...

Zheng, Z Y; Su, H J; Burstein, D; Chen, J S

1999-01-01T23:59:59.000Z

357

To better understand the processes that connect the Earth environment to the Sun,  

E-Print Network [OSTI]

: The solar wind is heated and accelerated within 5 RS, and the supersonic solar wind decouples from the Sun year by a panel of senior scientists. These tar- gets are then publicized, and individual researchers (AU)). It is inflated by the solar wind and threaded by mag- netic fields that affect the electrical

Yurchyshyn, Vasyl

358

Deep Photometry of the Globular Cluster M5: Distance Estimates from White Dwarf and Main Sequence Stars  

E-Print Network [OSTI]

We present deep VI photometry of stars in the globular cluster M5 (NGC 5904) based on images taken with the Hubble Space Telescope. The resulting color-magnitude diagram reaches below V ~ 27 mag, revealing the upper 2-3 magnitudes of the white dwarf cooling sequence, and main sequence stars eight magnitudes and more below the turn-off. We fit the main sequence to subdwarfs of known parallax to obtain a true distance modulus of (m-M)_0 = 14.45 +/- 0.11 mag. A second distance estimate based on fitting the cluster white dwarf sequence to field white dwarfs with known parallax yielded (m-M)_0 = 14.67 +/- 0.18 mag. We couple our distance estimates with extensive photometry of the cluster's RR Lyrae variables to provide a calibration of the RR Lyrae absolute magnitude yielding M_V(RR) = 0.42 +/- 0.10 mag at [Fe/H] = -1.11 dex. We provide another luminosity calibration in the form of reddening-free Wasenheit functions. Comparison of our calibrations with predictions based on recent models combining stellar evolution and pulsation theories shows encouraging agreement. (Abridged)

Andrew C. Layden; Ata Sarajedini; Ted von Hippel; Adrienne M. Cool

2005-07-14T23:59:59.000Z

359

High coercivity CoCrPt films achieved by post-deposition rapid thermal annealing  

E-Print Network [OSTI]

layer, a CoCrPt mag- netic layer, a capping Mn diffusion layer, and a final CrTi oxidation protection conditions were stud- ied. II. EXPERIMENT All layers were deposited onto glass substrates by rf di- ode, and CrTi oxida- tion protection layer were all 200 ? thick. Post-deposition annealing was performed

Laughlin, David E.

360

Structure of the low-latitude magnetopause: MAGION-4 observations Z. Nemecek1  

E-Print Network [OSTI]

, each lasting from 1­10 min, are common just upstream of the bow shock. Such pulses are often quasi and at the quasi-parallel bow shock have been suggested (Sibeck et al., 1989 a,b). They must be considered. Such an increase corresponds to an enhancement in both magnetosheath thermal and mag- netic pressures which in turn

Paris-Sud XI, Université de

Note: This page contains sample records for the topic "maldives mag m1" 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

Annales Geophysicae, 24, 339354, 2006 SRef-ID: 1432-0576/ag/2006-24-339  

E-Print Network [OSTI]

wind flow which slows across the bow shock and deflects around the Earth's geomagnetic field-Earth line). The solar wind mag- netic field lines, deflected initially away from the Earth's bow viscosity and thermal conduc- tivity). The magnetic field is convected with the flow through

Paris-Sud XI, Université de

362

Fuzzy Systems in Instrumentation: Fuzzy Control Emil M. Petriu and Graham Eatherley  

E-Print Network [OSTI]

and trailer is finally presented. I. INTRODUCTION The basic idea of "fuzzy logic control" (FLC) was suggested,namely, the realm of fuzzy-logic-based process control," [L.A. Zadeh, "Fuzzy logic," ZEEE Computer Mag., pp. 83 and trailer is finallypresented. 11. FUZZY CONTROL Fig. 1 shows the general structure of a fuzzy logic control

Petriu, Emil M.

363

The Relationship between the Optical Depth of the 9.7 micron Silicate Absorption Feature and Infrared Differential Extinction in Dense Clouds  

E-Print Network [OSTI]

We have examined the relationship between the optical depth of the 9.7 micron silicate absorption feature (tau_9.7) and the near-infrared color excess, E(J-Ks) in the Serpens, Taurus, IC 5146, Chameleon I, Barnard 59, and Barnard 68 dense clouds/cores. Our data set, based largely on Spitzer IRS spectra, spans E(J-Ks)=0.3 to 10 mag (corresponding to visual extinction between about 2 and 60 mag.). All lines of sight show the 9.7 micron silicate feature. Unlike in the diffuse ISM where a tight linear correlation between the 9.7 micron silicate feature optical depth and the extinction (Av) is observed, we find that the silicate feature in dense clouds does not show a monotonic increase with extinction. Thus, in dense clouds, tau_9.7 is not a good measure of total dust column density. With few exceptions, the measured tau_9.7 values fall well below the diffuse ISM correlation line for E(J-Ks) > 2 mag (Av >12 mag). Grain growth via coagulation is a likely cause of this effect.

J. E. Chiar; K. Ennico; Y. J. Pendleton; A. C. A. Boogert; T. Greene; C. Knez; C. Lada; T. Roellig; A. G. G. M. Tielens; M. Werner; D. C. B. Whittet

2007-07-24T23:59:59.000Z

364

VOLUME 74, NUMBER 26 P H Y S I C A L R E V I E W L E T T E R S 26 JUNE 1995 Evaporative Cooling of Sodium Atoms  

E-Print Network [OSTI]

which allow the cooling of atoms to temperatures below the recoil limit. Optical techniques and trap loss due to ex- cited state collisions [5]. The technique of forced evapora- tive cooling relies of different cooling and trapping techniques involving lasers and mag- netic fields we were able to obtain

365

A numeric solution for metric-affine gravity and Einstein's gravitational theory with Proca matter  

E-Print Network [OSTI]

A special case of metric-affine gauge theory of gravity (MAG) is equivalent to general relativity with Proca matter as source. We study in detail a corresponding numeric solution of the Reissner-Nordstr"om type. It is static, spherically symmetric, and of electric type. In particular, this solution has no horizon, so it has a naked singularity as its origin.

Marc Toussaint

1999-10-12T23:59:59.000Z

366

Production of Energetic Electrons during Magnetic Reconnection J. F. Drake, M. A. Shay, and W. Thongthai  

E-Print Network [OSTI]

islands where locally unmagnetized particles could be both trapped and accel- erated. Hoshino et al) The production of energetic electrons during magnetic reconnection is explored with full particle simulations are not expected to efficiently accelerate electrons. In the early studies of particle acceleration during mag

Shay, Michael

367

11. D. E. Smith et al., Science 284, 1495 (1999). 12. M. H. Carr, The Surface of Mars (Yale Univ. Press, New  

E-Print Network [OSTI]

11. D. E. Smith et al., Science 284, 1495 (1999). 12. M. H. Carr, The Surface of Mars (Yale Univ. Solomon, J. W. Head, C. H. Thurber, J. Geophys. Res. 90, 3049 (1985); M. T. Zuber, D. E. Smith, F. G, Rock Mag- netism (Cambridge Univ. Press, Cambridge, 1997)]. 28. D. E. Smith et al., Science 279, 1686

Li, Zhanqing

368

DDM DM LDAO FOS12 C12 DDM DM LDAO FOS12 C12  

E-Print Network [OSTI]

Sepharose Ni are magnetic beads designed for rapid small-scale purification and screening of histidine Purification (IMAC) Collect supernatants and add His Mag Sepharose Ni into each detergent solubilized membrane(s) GE Healthcare Data file 28-9833-26 AA Membrane protein purification Membrane Protein Purification Kit

Lebendiker, Mario

369

NATURE NANOTECHNOLOGY | VOL 6 | AUGUST 2011 | www.nature.com/naturenanotechnology 465 news & views  

E-Print Network [OSTI]

, T., Hsu, A. & Wang, H. IEEE Commun. Mag. 48, 122­128 (June 2010). 4. Lin, Y-M. et al. Science 332. IEEE International Microwave Symposium (Baltimore, 5­10 June 2011). 11. Xia, F., Mueller, T., Lin, Y-M., Valdes-Garcia, A. & Avouris, P. Nature Nanotech. 4, 839­843 (2009). 12.

Bruck, Jehoshua (Shuki)

370

THE HST EXTREME DEEP FIELD (XDF): COMBINING ALL ACS AND WFC3/IR DATA ON THE HUDF REGION INTO THE DEEPEST FIELD EVER  

SciTech Connect (OSTI)

The eXtreme Deep Field (XDF) combines data from 10 years of observations with the Hubble Space Telescope Advanced Camera for Surveys (ACS) and the Wide-Field Camera 3 Infra-Red (WFC3/IR) into the deepest image of the sky ever in the optical/near-IR. Since the initial observations of the Hubble Ultra-Deep Field (HUDF) in 2003, numerous surveys and programs, including supernovae follow-up, HUDF09, CANDELS, and HUDF12, have contributed additional imaging data across this region. However, these images have never been combined and made available as one complete ultra-deep image dataset. We combine them now with the XDF program. Our new and improved processing techniques provide higher quality reductions of the total dataset. All WFC3/IR and optical ACS data sets have been fully combined and accurately matched, resulting in the deepest imaging ever taken at these wavelengths, ranging from 29.1 to 30.3 AB mag (5? in a 0.''35 diameter aperture) in 9 filters. The combined image therefore reaches to 31.2 AB mag 5? (32.9 at 1?) for a flat f {sub ?} source. The gains in the optical for the four filters done in the original ACS HUDF correspond to a typical improvement of 0.15 mag, with gains of 0.25 mag in the deepest areas. Such gains are equivalent to adding ?130 to ?240 orbits of ACS data to the HUDF. Improved processing alone results in a typical gain of ?0.1 mag. Our 5? (optical+near-IR) SExtractor catalogs reveal about 14,140 sources in the full field and about 7121 galaxies in the deepest part of the XDF.

Illingworth, G. D.; Magee, D.; Oesch, P. A. [UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States); Bouwens, R. J.; Labb, I.; Franx, M. [Leiden Observatory, Leiden University, NL-2300 RA Leiden (Netherlands); Stiavelli, M. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Van Dokkum, P. G. [Department of Astronomy, Yale University, New Haven, CT 06520 (United States); Trenti, M. [Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA (United Kingdom); Carollo, C. M. [Institute for Astronomy, ETH Zurich, 8092 Zurich (Switzerland); Gonzalez, V., E-mail: gdi@ucolick.org [University of California, Riverside, 900 University Avenue, Riverside, CA 92507 (United States)

2013-11-01T23:59:59.000Z

371

The ARAUCARIA project: Deep near-infrared survey of nearby galaxies. I. The distance to the Large Magellanic Cloud from K-band photometry of red clump stars  

E-Print Network [OSTI]

We have obtained deep imaging in the near-infrared J and K bands for 2 nearby fields in the bar of the LMC with the ESO NTT telescope, under exquisite seeing conditions. The K, J-K color-magnitude diagrams constructed from these data are of outstanding photometric quality and reveal the presence of several hundreds of red clump stars. Using the calibration of Alves for the K-band absolute magnitude of Hipparcos-observed red clump stars in the solar neigbourhood we derive a distance modulus to our observed LMC fields of 18.487 mag. Applying a correction for the tilt of the LMC bar with respect to the line of sight according to the geometrical model of van der Marel et al., the corresponding LMC barycenter distance is 18.501 mag. If we adopt a K-band population correction of -0.03 mag, as done by Alves et al. 2002, to account for the difference in age and metallicity between the solar neighborhood and LMC red clump star populations, we obtain an LMC barycenter distance modulus of 18.471 mag from our data. This is in excellent agreement with the result of Alves et al., and of another very recent study of Sarajedini et al. (2002) obtained from K-band photometry. However, we emphasize that current model predictions about the uncertainties of population corrections seem to indicate that errors up to about 0.12 mag may be possible, probably in any photometric band. Therefore, work must continue to tighten the constraints on these corrections. We also determine the mean red clump star magnitude in our LMC fields in the J band, which could be a useful alternative to the K band should future work reveal that population effect corrections for red clump stars in the J band are smaller, or more reliably determined than those for the K band.

G. Pietrzynski; W. Gieren

2002-08-07T23:59:59.000Z

372

DuCxyBu;Axx +=+=&Consider the system: Given x(0) and u(t) for t 0. The solution is  

E-Print Network [OSTI]

, the solution is: Du[k]Bu[m]CAx[0]CAy[k] Bu[m]Ax[0]Ax[k] 1k 0m 1mkk 1k 0m 1mkk ++= += - = -- - = -- The main

Hu, Tingshu

373

A New Efficient Spectral Galerkin Method for Singular Perturbation ...  

E-Print Network [OSTI]

[1]), up-wind finite difference method (cf. [9]), the boundary layer resolving ..... Then by (3.10) and integration by part, ?i,m(y) = (1 ? y2)mL(m?1) i+m+1(y) + ? y.

374

Demand Side Dispatching, Part 2: An Industrial Application  

E-Print Network [OSTI]

DEMAND SIDE DISPATCHING, Part 2: AN INDUSTRIAL APPUCATION Ravi Nath Donald A. Cerget Edward T. Henderson Sr. Consultant Sr. Account Executive Sr. Engineer Linnhoff March, Inc. Detroit Edison Detroit Edison Houston, TX Detroit, M1 Detroit, M1...

Nath, R.; Cerget, D. A.; Henderson, E. T.

375

Paper Presented at International Instrumentation Symposium PNNL-SA-35920 Embedded Health Monitoring Workshop, May 2002  

E-Print Network [OSTI]

for the gas turbine engine used on the M1 Abrams tank. Research was performed on methods for real time Monitoring (PHM) system for the gas turbine engine used on the M1 Abrams tank. The purpose of this paper

376

NIMROD: A computational laboratory for studying nonlinear fusion magnetohydrodynamicsa...  

E-Print Network [OSTI]

amplification in spheromaks to be very closely related to the m 1 dynamo modes and magnetic reversal in reversed

Held, Eric

377

Promoting system-level learning from project-level lessons  

SciTech Connect (OSTI)

A growing number of low and middle income nations (LMCs) have adopted some sort of system for environmental impact assessment (EIA). However, generally many of these EIA systems are characterised by a low performance in terms of timely information dissemination, monitoring and enforcement after licencing. Donor actors (such as the World Bank) have attempted to contribute to a higher performance of EIA systems in LMCs by intervening at two levels: the project level (e.g. by providing scoping advice or EIS quality review) and the system level (e.g. by advising on EIA legislation or by capacity building). The aims of these interventions are environmental protection in concrete cases and enforcing the institutionalisation of environmental protection, respectively. Learning by actors involved is an important condition for realising these aims. A relatively underexplored form of learning concerns learning at EIA system-level via project level donor interventions. This 'indirect' learning potentially results in system changes that better fit the specific context(s) and hence contribute to higher performances. Our exploratory research in Ghana and the Maldives shows that thus far, 'indirect' learning only occurs incidentally and that donors play a modest role in promoting it. Barriers to indirect learning are related to the institutional context rather than to individual characteristics. Moreover, 'indirect' learning seems to flourish best in large projects where donors achieved a position of influence that they can use to evoke reflection upon system malfunctions. In order to enhance learning at all levels donors should thereby present the outcomes of the intervention elaborately (i.e. discuss the outcomes with a large audience), include practical suggestions about post-EIS activities such as monitoring procedures and enforcement options and stimulate the use of their advisory reports to generate organisational memory and ensure a better information dissemination.

Jong, Amos A. de, E-mail: amosdejong@gmail.com [Innovation Management, Utrecht (Netherlands); Runhaar, Hens A.C., E-mail: h.a.c.runhaar@uu.nl [Section of Environmental Governance, Utrecht University, Utrecht (Netherlands); Runhaar, Piety R., E-mail: piety.runhaar@wur.nl [Organisational Psychology and Human Resource Development, University of Twente, Enschede (Netherlands); Kolhoff, Arend J., E-mail: Akolhoff@eia.nl [The Netherlands Commission for Environmental Assessment, Utrecht (Netherlands); Driessen, Peter P.J., E-mail: p.driessen@geo.uu.nl [Department of Innovation and Environment Sciences, Utrecht University, Utrecht (Netherlands)

2012-02-15T23:59:59.000Z

378

Math. Proc. Camb. Phil. Soc. (2001), 130, 365 Printed in the United Kingdom c 2001 Cambridge Philosophical Society  

E-Print Network [OSTI]

in this direction were obtained by Westcott [21, 22], who considered the one-sided case and gave conditions that implied rr((x, )) m1/x, where m1 = m1(µ) xµ(dx) denotes the first moment associated with µ. Westcott also

Grübel, Rudolf

379

Synthesis and applications of quinazoline-based fluorescent nucleoside analogues  

E-Print Network [OSTI]

then 200 L of 0.45M 1H-tetrazole was pushed into the otherthen 200 L of 0.45M 1H-tetrazole was pushed into the otherthen 200 L of 0.45M 1H-tetrazole was pushed into the other

Xie, Yun

2010-01-01T23:59:59.000Z

380

maple and xmaple  

E-Print Network [OSTI]

m := matrix( [ [8,2,3] , [3,2,1] , [6,6,7] ] ); m1 := mulrow( m , 1, 1/8 ); m2 := addrow( m1, 1, 2, -3 ); m3 .... You are now ready to move on to the next section, matlab...

Note: This page contains sample records for the topic "maldives mag m1" 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

Seismic attenuation studies using frequency domain synthetic seismograms  

E-Print Network [OSTI]

of Model 6. Reflection coefficient is z. 0137 in each case. 0 1s varied to show the resulting effect on the notches in the ratio, , 37. Downgo1ng time domain ratios for the first permuta- tion of 11odel 6. (} 1s 30 in each case. Reflection coefficient... 1 = n t, i=n m 1 E = 11 a)~ n, m-1 m-1 ~n, m-1 & Fi i=n n m-1 (A)n, m an, m-1 21 an qm-1 12 22 m-1 11 i=n al 11 12 a21 a22 1 1 z;F; r; 1=n z. F. 2r. I 1 1 1 From the basic matrix equations (6), (7), (8), and (9), the responses Ri...

Butler, Theresa Meade

2012-06-07T23:59:59.000Z

382

PHOTOMETRY OF VARIABLE STARS FROM DOME A, ANTARCTICA: RESULTS FROM THE 2010 OBSERVING SEASON  

SciTech Connect (OSTI)

We present results from a season of observations with the Chinese Small Telescope ARray, obtained over 183 days of the 2010 Antarctic winter. We carried out high-cadence time-series aperture photometry of 9125 stars with i ?< 15.3 mag located in a 23 deg{sup 2} region centered on the south celestial pole. We identified 188 variable stars, including 67 new objects relative to our 2008 observations, thanks to broader synoptic coverage, a deeper magnitude limit, and a larger field of view. We used the photometric data set to derive site statistics from Dome A. Based on two years of observations, we find that extinction due to clouds at this site is less than 0.1 and 0.4 mag during 45% and 75% of the dark time, respectively.

Wang, Lingzhi; Zhu, Zonghong [Department of Astronomy, Beijing Normal University, Beijing 100875 (China); Macri, Lucas M.; Wang, Lifan [Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A and M University, College Station, TX 77843 (United States); Ashley, Michael C. B.; Lawrence, Jon S.; Luong-Van, Daniel; Storey, John W. V. [School of Physics, University of New South Wales, NSW 2052 (Australia); Cui, Xiangqun; Feng, Long-Long; Gong, Xuefei; Liu, Qiang; Shang, Zhaohui; Yang, Huigen; Yang, Ji; Yuan, Xiangyan; Zhou, Xu; Zhu, Zhenxi [Chinese Center for Antarctic Astronomy, Nanjing 210008 (China); Pennypacker, Carl R. [Center for Astrophysics, Lawrence Berkeley National Laboratory, Berkeley, CA (United States); York, Donald G., E-mail: wanglingzhi@bao.ac.cn [Department of Astronomy and Astrophysics and Enrico Fermi Institute, University of Chicago, Chicago, IL 60637 (United States)

2013-12-01T23:59:59.000Z

383

Efficient One-Step Electrolytic Recycling of Low-Grade and Post-Consumer Magnesium Scrap  

SciTech Connect (OSTI)

Metal Oxygen Separation Technologies, Inc. (abbreviated MOxST, pronounced most) and Boston University (BU) have developed a new low-cost process for recycling post-consumer co-mingled and heavily-oxidized magnesium scrap, and discovered a new chemical mechanism for magnesium separations in the process. The new process, designated MagReGenTM, is very effective in laboratory experiments, and on scale-up promises to be the lowest-cost lowest-energy lowest-impact method for separating magnesium metal from aluminum while recovering oxidized magnesium. MagReGenTM uses as little as one-eighth as much energy as today's methods for recycling magnesium metal from comingled scrap. As such, this technology could play a vital role in recycling automotive non-ferrous metals, particularly as motor vehicle magnesium/aluminum ratios increase in order to reduce vehicle weight and increase efficiency.

Adam C. Powell, IV

2012-07-19T23:59:59.000Z

384

Microlensing in the double quasar SBS1520+530  

E-Print Network [OSTI]

We present the results of a monitoring campaign of the double quasar SBS1520+530 at Maidanak observatory from April 2003 to August 2004. We obtained light curves in V and R filters that show small-amplitude \\Delta m~0.1 mag intrinsic variations of the quasar on time scales of about 100 days. The data set is consistent with the previously determined time delay of \\Delta t=(130+-3) days by Burud et al. (2002). We find that the time delay corrected magnitude difference between the quasar images is now larger by (0.14+-0.03) mag than during the observations by Burud et al. (2002). This confirms the presence of gravitational microlensing variations in this system.

E. R. Gaynullina; R. W. Schmidt; T. Akhunov; O. Burkhonov; S. Gottloeber; K. Mirtadjieva; S. N. Nuritdinov; I. Tadjibaev; J. Wambsganss; L. Wisotzki

2005-05-24T23:59:59.000Z

385

The Carnegie Hubble Program: The Distance and Structure of the SMC as Revealed by Mid-infrared Observations of Cepheids  

E-Print Network [OSTI]

Using Spitzer observations of classical Cepheids we have measured the true average distance modulus of the SMC to be $18.96 \\pm 0.01_{stat} \\pm 0.03_{sys}$ mag (corresponding to $62 \\pm 0.3$ kpc), which is $0.48 \\pm 0.01$ mag more distant than the LMC. This is in agreement with previous results from Cepheid observations, as well as with measurements from other indicators such as RR Lyrae stars and the tip of the red giant branch. Utilizing the properties of the mid--infrared Leavitt Law we measured precise distances to individual Cepheids in the SMC, and have confirmed that the galaxy is tilted and elongated such that its eastern side is up to 20 kpc closer than its western side. This is in agreement with the results from red clump stars and dynamical simulations of the Magellanic Clouds and Stream.

Scowcroft, Victoria; Madore, Barry F; Monson, Andy; Persson, S E; Rich, Jeff; Seibert, Mark; Rigby, Jane R

2015-01-01T23:59:59.000Z

386

A semi-analytic model of magnetized liner inertial fusion  

E-Print Network [OSTI]

Presented is a semi-analytic model of magnetized liner inertial fusion (MagLIF). This model accounts for several key aspects of MagLIF, including: (1) preheat of the fuel (optionally via laser absorption); (2) pulsed-power-driven liner implosion; (3) liner compressibility with an analytic equation of state, artificial viscosity, internal magnetic pressure, and ohmic heating; (4) adiabatic compression and heating of the fuel; (5) radiative losses and fuel opacity; (6) magnetic flux compression with Nernst thermoelectric losses; (7) magnetized electron and ion thermal conduction losses; (8) end losses; (9) enhanced losses due to prescribed dopant concentrations and contaminant mix; (10) deuterium-deuterium and deuterium-tritium primary fusion reactions for arbitrary deuterium to tritium fuel ratios; and (11) magnetized alpha-particle fuel heating. We show that this simplified model, with its transparent and accessible physics, can be used to reproduce the general 1D behavior presented throughout the original Ma...

McBride, Ryan D

2015-01-01T23:59:59.000Z

387

PSN J07285387+3349106 in NGC 2388: extremely rapidly declining luminous supernova  

E-Print Network [OSTI]

We present CCD BVRI photometry for PSN J07285387+3349106 in NGC 2388 collected from 2015 February 17 until March 17. Decaying by 3.6 mag in the R band in the first 20 days post-maximum, this object is among the fastest supernovae observed to date. The peak absolute R magnitude exceeds -18.7 and may be as high as -20.1.

Tsvetkov, D Yu; Pavlyuk, N N

2015-01-01T23:59:59.000Z

388

A NEW DISTANCE TO M33 USING BLUE SUPERGIANTS AND THE FGLR METHOD  

SciTech Connect (OSTI)

The quantitative spectral analysis of medium resolution optical spectra of A and B supergiants obtained with DEIMOS and ESI at the Keck Telescopes is used to determine a distance modulus of 24.93 +- 0.11 mag (968 +- 50 kpc) for the Triangulum Galaxy M33. The analysis yields stellar effective temperatures, gravities, interstellar reddening, and extinction, the combination of which provides a distance estimate via the flux-weighted gravity-luminosity relationship (FGLR). This result is based on an FGLR calibration that is continually being polished. An average reddening of (E(B - V)) approx 0.08 mag is found, with a large variation ranging from 0.01 to 0.16 mag, however, demonstrating the importance of accurate individual reddening measurements for stellar distance indicators in galaxies with evident signatures of interstellar absorption. The large-distance modulus found is in good agreement with recent work on eclipsing binaries, planetary nebulae, long-period variables, RR Lyrae stars, and also with Hubble Space Telescope (HST) observations of Cepheids, if reasonable reddening assumptions are made for the Cepheids. Since distances based on the tip of the red giant branch (TRGB) method found in the literature give conflicting results, we have used HST Advanced Camera for Surveys V- and I-band images of outer regions of M33 to determine a TRGB distance of 24.84 +- 0.10 mag, in basic agreement with the FGLR result. We have also determined stellar metallicities and discussed the metallicity gradient in the disk of M33. We find metallicity of Z {sub sun} at the center and 0.3 Z {sub sun} in the outskirts at a distance of one isophotal radius. The average logarithmic metallicity gradient is -0.07 +- 0.01 dex kpc{sup -1}. However, there is a large scatter around this average value, very similar to what has been found for the H II regions in M33.

U, Vivian; Urbaneja, Miguel A.; Kudritzki, Rolf-Peter; Jacobs, Bradley A.; Bresolin, Fabio [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Przybilla, Norbert, E-mail: vivian@ifa.hawaii.ed, E-mail: urbaneja@ifa.hawaii.ed, E-mail: kud@ifa.hawaii.ed, E-mail: bjacobs@ifa.hawaii.ed, E-mail: bresolin@ifa.hawaii.ed, E-mail: przybilla@sternwarte.uni-erlangen.d [Dr. Remeis-Sternwarte Bamberg, Sternwartstrasse 7, D-96049 Bamberg (Germany)

2009-10-20T23:59:59.000Z

389

PROGRAMA FISICA II. INTRODUCCI O  

E-Print Network [OSTI]

PROGRAMA F´ISICA II. INTRODUCCI ´O I ELECTRICITAT I.1 Camp electrost`atic I.2 Potencial i energia I.4 `Optica #12;BIBLIOGRAFIA B`asica 1. Tipler, P.A. F´isica. Vol. II, ed. Revert´e, 1992. 2. Purcell Blum, R. F´isica: Electricidad, Mag- netismo y Luz. Vol. II, ed. Revert´e, 1986. Complement`aria 1

Batiste, Oriol

390

Modelling of Infrared emission from Cyg X3 and the UKIRT IRCAM3 point spread function  

E-Print Network [OSTI]

in order to test for any extended emission around the X­ray binary Cyg X­3. We found that the point spread ranging from 12 magnitude (Cyg X­3) to 18th mag for some of the faintest stars. The positions of the stars instrument. 2 #12; 2.1 k­band image The k­band image, figure 2 or the finder chart provided by Fender (Fender

Ogley, Richard

391

Los Alamos Team Demonstrates Bottle Scanner Technology  

ScienceCinema (OSTI)

Los Alamos scientists are demonstrating a Nuclear Magnetic Resonance Imaging (NMR) technology that may provide a breakthrough for screening liquids at airport security. By adding low-power X-ray data to the NMR mix, scientists believe they have unlocked a new detection technology. Funded in part by the Department of Homeland Security's Science and Technology Directorate, the new technology is called MagRay.

Espy, Michelle; Schultz, Larry

2014-06-02T23:59:59.000Z

392

Phase-Diagram of Ultrathin Ferromagnetic-Films with Perpendicular Anisotropy  

E-Print Network [OSTI]

of numerous ultrathin ferromagnetic films that show (l) a planar mag- netization for temperature T above the spin reorientation transition temperature Tz, (2) a perpendicular magneti- zation at low temperatures, and (3) an intermediate tem- perature... regime having a perpendicular magnetization with an up-and-down stripe-domain structure. It is based upon the usual ferromagnetic exchange Hamiltoni- an, including the magnetostatic dipolar interaction, sup- plemented by an easy-axis spin anisotropy...

Abanov, Artem; KALATSKY, V.; Pokrovsky, Valery L.; SASLOW, WM.

1995-01-01T23:59:59.000Z

393

Design study of magnetic environments for XYZ polarization analysis using 3He for the new thermal time of flight spectrometer TOPAS  

E-Print Network [OSTI]

We present a finite element calculation of the magnetic field (MagNet software) taken with the newly proposed PASTIS Coil, which uses a wide-angle banana shaped 3He Neuton Spin Filter cell (NSF) to cover a large range of scattering angle. The goal of this insert is to enable XYZ polarization analysis to be installed on the future thermal time-of flight spectrometer TOPAS.

Zahir Salhi; Earl Babcock; Alexander Ioffe

2012-01-25T23:59:59.000Z

394

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

395

Los Alamos Team Demonstrates Bottle Scanner Technology  

SciTech Connect (OSTI)

Los Alamos scientists are demonstrating a Nuclear Magnetic Resonance Imaging (NMR) technology that may provide a breakthrough for screening liquids at airport security. By adding low-power X-ray data to the NMR mix, scientists believe they have unlocked a new detection technology. Funded in part by the Department of Homeland Security's Science and Technology Directorate, the new technology is called MagRay.

Espy, Michelle; Schultz, Larry

2014-05-06T23:59:59.000Z

396

Archival search for recurrent activity at the position the gamma-ray burst GRB 970228 optical counterpart  

E-Print Network [OSTI]

We have examined 8004 plates at the Harvard College Observatory Plate Collection searching for optical transient emission from the gamma-ray burst GRB 970228. This is the first archival search carried out so far for a gamma-ray burst with known transient optical emission. The total exposure time amounts to ~1.1 yr. No convincing optical activity was found above 12.5 mag at the expected position of the GRB 970228 optical counterpart.

Javier Gorosabel; Alberto J. Castro-Tirado

1998-02-18T23:59:59.000Z

397

OPTICAL AND INFRARED PHOTOMETRY OF THE TYPE Ia SUPERNOVAE 1991T, 1991bg, 1999ek, 2001bt, 2001cn, 2001cz, AND 2002bo  

E-Print Network [OSTI]

Vladimir D. Ivanov,10 Wojtek Krzemin´ski,1 Craig Kulesa,11 Patrick McCarthy,12 Amaya Moro-Marti´n,11 Ce´sar the time of B-band maximum. The use of Ám15(B) is now one of many methods used to calibrate absolute mag multicolor technique using a continuous set of multi- color templates with the important additions of a self-calibrated

Moro-Martin, Amaya

398

Normal-state transport in electron-doped La2-xCexCuO4 thin films in magnetic fields up to 40 Tesla  

E-Print Network [OSTI]

Normal-state transport in electron-doped La2-xCexCuO4 thin films in magnetic fields up to 40 Tesla.17 are studied in magnetic fields up to 40 Tesla. For the whole doping region investigated, the negative, the upper critical mag- netic field Bc2 order of 100 Tesla 8 is too high to be achieved. The n-type HTSCs

Moshchalkov, Victor V.

399

hal-00133055,version1-29Mar2007 Nuclear spin interferences in bulk water at room temperature.  

E-Print Network [OSTI]

hal-00133055,version1-29Mar2007 Nuclear spin interferences in bulk water at room temperature. J in NMR pacs 03.67.-a: Quantum information pacs 67.57.Lm: Spin dynamics Abstract Nuclear spin interference in a static mag- netic field B0 4.7 T. For a homogeneity of B0 of the order of B0/B0 = 2 10-8 , the nuclear

Boyer, Edmond

400

NEAR-INFRARED IMAGING OF A z = 6.42 QUASAR HOST GALAXY WITH THE HUBBLE SPACE TELESCOPE WIDE FIELD CAMERA 3  

SciTech Connect (OSTI)

We report on deep near-infrared F125W (J) and F160W (H) Hubble Space Telescope Wide Field Camera 3 images of the z = 6.42 quasar J1148+5251 to attempt to detect rest-frame near-ultraviolet emission from the host galaxy. These observations included contemporaneous observations of a nearby star of similar near-infrared colors to measure temporal variations in the telescope and instrument point-spread function (PSF). We subtract the quasar point source using both this direct PSF and a model PSF. Using direct subtraction, we measure an upper limit for the quasar host galaxy of m{sub J} > 22.8 and m{sub H} > 23.0 AB mag (2 {sigma}). After subtracting our best model PSF, we measure a limiting surface brightness from 0.''3 to 0.''5 radius of {mu}{sub J} > 23.5 and {mu}{sub H} > 23.7 AB mag arcsec{sup -2} (2 {sigma}). We test the ability of the model subtraction method to recover the host galaxy flux by simulating host galaxies with varying integrated magnitude, effective radius, and Sersic index, and conducting the same analysis. These models indicate that the surface brightness limit ({mu}{sub J} > 23.5 AB mag arcsec{sup -2}) corresponds to an integrated upper limit of m{sub J} > 22-23 AB mag, consistent with the direct subtraction method. Combined with existing far-infrared observations, this gives an infrared excess log (IRX) > 1.0 and corresponding ultraviolet spectral slope {beta} > -1.2 {+-} 0.2. These values match those of most local luminous infrared galaxies, but are redder than those of almost all local star-forming galaxies and z {approx_equal} 6 Lyman break galaxies.

Mechtley, M.; Windhorst, R. A.; Cohen, S. H.; Jansen, R. A.; Scannapieco, E. [School of Earth and Space Exploration, Arizona State University, P.O. Box 871404, Tempe, AZ 85287 (United States); Ryan, R. E.; Koekemoer, A. M. [Space Telescope Science Institute, Baltimore, MD 21218 (United States); Schneider, G.; Fan, X. [Steward Observatory, University of Arizona, Tucson, AZ 85721 (United States); Hathi, N. P. [Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Keel, W. C. [Department of Physics and Astronomy, University of Alabama, Box 870324, Tuscaloosa, AL 35487 (United States); Roettgering, H. [Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA, Leiden (Netherlands); Schneider, D. P. [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States); Strauss, M. A. [Princeton University Observatory, Princeton, NJ 08544 (United States); Yan, H. J. [Department of Physics and Astronomy, The University of Missouri, 701 South College Ave, Columbia, MO 65211 (United States)

2012-09-10T23:59:59.000Z

Note: This page contains sample records for the topic "maldives mag m1" 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

Development of Advanced Electrolytes and Electrolyte Additives  

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

2.5 3.0 3.5 4.0 Voltage (V) 1 st cycle 500 th cycle 1000 th cycle I 240 mA.g -1 TMSEMC 1M LiTFSI EMS 1M LiTFSI EMS 1.0M LiPF 6 EMSEMC 55 1.0M LiPF 6 EMSEMC 55 9 1M...

402

Decommissioning and PIE of the MEGAPIE spallation target  

SciTech Connect (OSTI)

A key experiment in the Accelerated Driven Systems roadmap, the MEGAwatt PIlot Experiment (MEGAPIE) (1 MW) was initiated in 1999 in order to design and build a liquid lead-bismuth spallation target, then to operate it into the Swiss spallation neutron facility SINQ at Paul Scherrer Institute. The target has been designed, manufactured, and tested during integral tests, before irradiation carried out end of 2006. During irradiation, neutron and thermo hydraulic measurements were performed allowing deep interpretation of the experiment and validation of the models used during design phase. The decommissioning, Post Irradiation Examinations and waste management phases were defined properly. The phases dedicated to cutting, sampling, cleaning, waste management, samples preparation and shipping to various laboratories were performed by PSI teams: all these phases constitute a huge work, which allows now to perform post-irradiation examination (PIE) of structural material, irradiated in relevant conditions. Preliminary results are presented in the paper, they concern chemical characterization. The following radio-nuclides have been identified by ?-spectrometry: {sup 60}Co, {sup 101}Rh, {sup 102}Rh, {sup 108m}Ag, {sup 110m}Ag, {sup 133}Ba, {sup 172}Hf/Lu, {sup 173}Lu, {sup 194}Hg/Au, {sup 195}Au, {sup 207}Bi. For some of these nuclides the activities can be easily evaluated from ?-spectrometry results ({sup 207}Bi, {sup 194}Hg/Au), while other nuclides can only be determined after chemical separations ({sup 108m}Ag, {sup 110m}Ag, {sup 195}Au, {sup 129}I, {sup 36}Cl and ?-emitting {sup 208-210}Po). The concentration of {sup 129}I is lower than expected. The chemical analysis already performed on spallation and corrosion products in the lead-bismuth eutectic (LBE) are very relevant for further applications of LBE as a spallation media and more generally as a coolant.

Latge, C.; Henry, J. [CEA-Cadarache, DEN-DTN, 13108 Saint-Paul-les-Durance (France); Wohlmuther, M.; Dai, Y.; Gavillet, D.; Hammer, B.; Heinitz, S.; Neuhausen, J.; Schumann, D.; Thomsen, K.; Tuerler, A.; Wagner, W. [PSI, Villigen (Switzerland); Gessi, A. [ENEA, Brasimone (Italy); Guertin, A. [CNRS, Subatech, Nantes (France); Konstantinovic, M. [SCK-CEN, Mol (Belgium); Lindau, R. [KIT, Karlsruhe (Germany); Maloy, S. [DOE-LANL, Los Alamos (United States); Saito, S. [JAEA, Tokai (Japan)

2013-07-01T23:59:59.000Z

403

A search for ultra-compact dwarf galaxies in the Centaurus galaxy cluster  

E-Print Network [OSTI]

Aim: To extend the investigations of ultra-compact dwarf galaxies (UCDs) beyond the well studied Fornax and Virgo clusters. Methods: We measured spectroscopic redshifts of about 400 compact object candidates with 19.2 < V < 22.4 mag in the central region of the Centaurus galaxy cluster (d=43Mpc), using VIMOS@VLT. The luminosity range of the candidates covers that of bright globular clusters (GCs) and of UCDs in Fornax and Virgo. Results: We confirm the cluster membership of 27 compact objects, covering an absolute magnitude range -12.2 < M_V < -10.9 mag. We do not find counterparts to the two very large and bright UCDs in Fornax and Virgo with M_V=-13.5 mag, possibly due to survey incompleteness. The compact objects' distribution in magnitude and space is consistent with that of the GC population. Their kinematics and spatial distribution associate them to the central galaxies rather than to the overall cluster potential. The compact objects have a mean metallicity consistent with that of the metal-rich globular cluster sub-population. Compact objects with high S/N spectra exhibit solar [alpha/Fe] abundances, consistent with typical dwarf elliptical galaxy values and unlike galactic bulge globular clusters. HST based size estimates for a sub-sample of eight compact objects reveal the existence of one very large object with half-light radius r_h around 30 pc, having M_V=-11.6 mag (~10^7 M_sun). This source shows super-solar [alpha/Fe] abundances. Seven further sources are only marginally larger than typical GCs with r_h in the range 4 to 10 pc. Conclusions: We consider the largest compact object found to be the only bona-fide UCD detected in our study. In order to improve our understanding of UCDs in Centaurus, a significant increase of our survey completeness is necessary.

S. Mieske; M. Hilker; A. Jordan; L. Infante; M. Kissler-Patig

2007-06-19T23:59:59.000Z

404

Spectroscopic metallicities for Fornax UCDs, GCs and dE,Ns  

E-Print Network [OSTI]

Various formation channels for the puzzling ultra-compact dwarf galaxies (UCDs) have been proposed in the last few years. To better judge on some of the competing scenarios, we present spectroscopic [Fe/H] estimates for a sample of 26 compact objects in the central region of the Fornax cluster, covering the magnitude range of UCDs and bright globular clusters. We find a break in the metallicity distribution of compact objects at M_V ~ -11 mag (~3*10^6 M_sun): for M_V-11 mag. This metallicity break is accompanied by a change in the size-luminosity relation for compact objects, as deduced from HST-imaging: for M_V-11 mag, r_h is almost luminosity-independent. We therefore assume a limiting absolute magnitude of M_V=-11 mag between UCDs and globular clusters. The mean metallicity of five Fornax dE,N nuclei included in our study is about 0.8 dex lower than that of the UCDs, at 4.5 sigma significance. Because of this large metallicity discrepancy we disfavor the hypothesis that most of the Fornax UCDs are the remnant nuclei of tidally stripped dE,Ns. Our metallicity estimates for UCDs are closer to but slightly below those derived for young massive clusters (YMCs) of comparable masses. We therefore favor a scenario where most UCDs in Fornax are successors of merged YMCs produced in the course of violent galaxy-galaxy mergers. It is noted that in contrast to that, the properties of Virgo UCDs are more consistent with the stripping scenario, suggesting that different UCD formation channels may dominate in either cluster.

S. Mieske; M. Hilker; L. Infante; A. Jordan

2005-12-20T23:59:59.000Z

405

The Tully-Fisher Relation and Its Residuals for a Broadly Selected Sample of Galaxies  

E-Print Network [OSTI]

We measure the relation between galaxy luminosity and disk circular velocity (the Tully-Fisher [TF] relation), in the g, r, i, and z-bands, for a broadly selected sample of galaxies from the Sloan Digital Sky Survey, with the goal of providing well defined observational constraints for theoretical models of galaxy formation. The input sample of 234 galaxies has a roughly flat distribution of absolute magnitudes in the range -18.5 > Mr > -22, and our only morphological selection is an axis-ratio cut b/a < 0.6 to allow accurate inclination corrections. Long-slit spectroscopy yields usable H-alpha rotation curves for 162 galaxies. Observational errors, including distance errors due to peculiar velocities, are small compared to the intrinsic scatter of the TF relation. The slope of the forward TF relation steepens from -5.5 +/- 0.2 mag/log(km/s) in the g-band to -6.6 +/- 0.2 mag/log(km/s) in the z-band. The intrinsic scatter is approximately 0.4 mag in all bands. The scatter is not dominated by rare outliers or by any particular class of galaxies, though it drops slightly, to 0.36 mag, if we restrict the sample to nearly bulgeless systems. Correlations of TF residuals with other galaxy properties are weak: bluer galaxies are significantly brighter than average in the g-band but only marginally brighter in the i-band; more concentrated galaxies are slightly fainter than average; and the TF residual is virtually independent of half-light radius, contrary to the trend expected for gravitationally dominant disks. The observed residual correlations do not account for most of the intrinsic scatter, implying that this scatter is instead driven largely by variations in the ratio of dark to luminous matter within the disk galaxy population.

James Pizagno; Francisco Prada; David H. Weinberg; Hans-Walter Rix; Richard W. Pogge; Eva K. Grebel; Daniel Harbeck; Michael Blanton; J. Brinkmann; James E. Gunn

2007-07-12T23:59:59.000Z

406

High Power Hg Target Conceptual Design Review  

E-Print Network [OSTI]

to Hg Hg Temp Rise Input Energy (hp) Losses Lost Energy (hp) Output Energy (hp) BTU/min BTU/min BTU/min BTU/ min KW HP BTU/min F/sec Elect Motor 60 60 hp * 5% inefficiency 3 57 127 127 2 3 Mag Coupling 5 Energy (hp) BTU/min BTU/min BTU/min BTU/ min KW HP BTU/min F/sec Elect Motor 60 60 hp * 5% inef

McDonald, Kirk

407

A Unified Energy-Reservoir Model Containing Contributions from $^{56}$Ni and Neutron Stars and Its Implication to Luminous Type Ic Supernovae  

E-Print Network [OSTI]

Most type-Ic core-collapse supernovae (CCSNe) produce $^{56}$Ni and neutron stars (NSs) or black holes (BHs). The dipole radiation of nascent NSs has usually been neglected in explaining supernovae (SNe) with peak absolute magnitude $M_{\\rm peak}$ in any band are $\\gtrsim -19.5$~mag, while the $^{56}$Ni can be neglected in fitting most type-Ic superluminous supernovae (SLSNe Ic) whose $M_{\\rm peak}$ in any band are $\\lesssim -21$~mag, since the luminosity from a magnetar (highly magnetized NS) can outshine that from a moderate amount of $^{56}$Ni. For luminous SNe Ic with $-21 \\lesssim M_{\\rm peak}\\lesssim -19.5$~mag, however, both contributions from $^{56}$Ni and NSs cannot be neglected without serious modeling, since they are not SLSNe and the $^{56}$Ni mass could be up to $\\sim 0.5 M_{\\odot}$. In this paper we propose a unified model that contain contributions from both $^{56}$Ni and a nascent NS. We select three luminous SNe Ic-BL, SN~2010ay, SN~2006nx, and SN~14475, and show that, if these SNe are powere...

Wang, S Q; Dai, Z G; Wu, X F

2015-01-01T23:59:59.000Z

408

Frequency of Solar-Like Systems and of Ice and Gas Giants Beyond the Snow Line from High-Magnification Microlensing Events in 2005-2008  

E-Print Network [OSTI]

We present the first measurement of planet frequency beyond the "snow line" for planet/star mass-ratios[-4.5200) microlensing events during 2005-8. The sample host stars have typical mass M_host 0.5 Msun, and detection is sensitive to planets over a range of projected separations (R_E/s_max,R_E*s_max), where R_E 3.5 AU sqrt(M_host/Msun) is the Einstein radius and s_max (q/5e-5)^{2/3}, corresponding to deprojected separations ~3 times the "snow line". Though frenetic, the observations constitute a "controlled experiment", which permits measurement of absolute planet frequency. High-mag events are rare, but the high-mag channel is efficient: half of high-mag events were successfully monitored and half of these yielded planet detections. The planet frequency derived from microlensing is a factor 7 larger than from RV studies at factor ~25 smaller separations [2

Gould, A; Gaudi, B S; Udalski, A; Bond, I A; Greenhill, J; Street, R A; Dominik, M; Sumi, T; Szymanski, M K; Han, C

2014-01-01T23:59:59.000Z

409

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

410

Post common envelope binaries from SDSS. IV: SDSSJ121258.25-012310.1, a new eclipsing system  

E-Print Network [OSTI]

From optical photometry we show that SDSSJ121258.25-012310.1 is a new eclipsing, post common-envelope binary with an orbital period of 8.06 hours and an eclipse length of 23 minutes. We observed the object over 11 nights in different bands and determined the ephemeris of the eclipse to HJD_mid = 2454104. 7086(2) + 0.3358706(5) x E, where numbers in parenthesis indicate the uncertainties in the last digit. The depth of the eclipse is 2.85 +/- 0.17 mag in the V band, 1.82 +/- 0.08 mag in the R band and 0.52 +/- 0.02 mag in the I band. From spectroscopic observations we measured the semi-amplitude of the radial velocity K_2 = 181 +/- 3 km/s for the secondary star. The stellar and binary parameters of the system were constrained from a) fitting the SDSS composite spectrum of the binary, b) using a K-band luminosty-mass relation for the secondary star, and c) from detailed analyses of the eclipse light curve. The white dwarf has an effective temperature of 17700 +/- 300 K, and its surface gravity is logg =7.53 +/-...

Gmez-Morn, A Nebot; Schreiber, M R; Gnsicke, B T; Pyrzas, S; Schwarz, R; Southworth, J; Kohnert, J; Vogel, J; Krumpe, M; Rodrguez-Gil, P

2009-01-01T23:59:59.000Z

411

An Investigation of the Effect of Graphite Degradation on the Irreversible Capacity in Lithium-ion Cells  

SciTech Connect (OSTI)

The effect of surface structural damage on graphitic anodes, commonly observed in tested Li-ion cells, was investigated. Similar surface structural disorder was artificially induced in Mag-10 synthetic graphite anodes using argon-ion sputtering. Raman microscopy, scanning electron microscopy (SEM) and Brunauer Emmett Teller (BET) measurements confirmed that Ar-ion sputtered Mag-10 electrodes display similar degree of surface degradation as the anodes from tested Li-ion cells. Artificially modified Mag-10 anodes showed double the irreversible charge capacity during the first formation cycle, compared to fresh un-altered anodes. Impedance spectroscopy and Fourier transform infrared (FTIR) spectroscopy on surface modified graphite anodes indicated the formation of a thicker and slightly more resistive SEI layer. Gas chromatography/mass spectroscopy (GC/MS) analysis of solvent extracts from the electrodes detected the presence of new compounds with M{sub w} on the order of 1600 g mol{sup -1} for the surface modified electrode with no evidence of elevated M{sub w} species for the unmodified electrode. The structural disorder induced in the graphite during long-term cycling maybe responsible for the slow and continuous SEI layer reformation, and consequently, the loss of reversible capacity due to the shift of lithium inventory in cycled Li-ion cells.

Stevenson, Cynthia; Hardwick, Laurence J.; Marcinek, Marek; Beer, Leanne; Kerr, John B.; Kostecki, Robert

2008-03-03T23:59:59.000Z

412

Awakening of The High Redshift Blazar CGRaBS J0809+5341  

E-Print Network [OSTI]

CGRaBS J0809+5341, a high redshift blazar at z = 2.144, underwent a giant optical outburst on 2014 April 19 when it brightened by $\\sim$5 mag and reached an unfiltered apparent magnitude of 15.7 mag. This implies an absolute magnitude of -30.5 mag, making it one of the brightest quasars in the Universe. This optical flaring triggered us to carry out observations during the decaying part of the flare covering a wide energy range using the {\\it Nuclear Spectroscopic Telescope Array}, {\\it Swift}, and ground based optical facilities. For the first time, the source is detected in $\\gamma$-rays by the Large Area Telescope onboard the {\\it Fermi Gamma-Ray Space Telescope}. A high optical polarization of $\\sim$10\\% is also observed. Using the Sloan Digital Sky Survey spectrum, accretion disk luminosity and black hole mass are estimated as $1.5 \\times 10^{45}$ erg s$^{-1}$ and $10^{8.4}~M_{\\odot}$ respectively. Using a single zone leptonic emission model, we reproduce the spectral energy distribution of the source du...

Paliya, Vaidehi S; Stalin, C S; Fabian, A C; Ramya, S; Covino, S; Tagliaferri, G; Sahayanathan, S; Ravikumar, C D

2015-01-01T23:59:59.000Z

413

OGLE-IV: Fourth Phase of the Optical Gravitational Lensing Experiment  

E-Print Network [OSTI]

We present both the technical overview and main science drivers of the fourth phase of the Optical Gravitational Lensing Experiment (hereafter OGLE-IV). OGLE-IV is currently one of the largest sky variability surveys worldwide, targeting the densest stellar regions of the sky. The survey covers over 3000 square degrees in the sky and monitors regularly over a billion sources. The main targets include the inner Galactic Bulge and the Magellanic System. Their photometry spans the range of $12mag and $13mag, respectively. Supplementary shallower Galaxy Variability Survey covers the extended Galactic bulge and 2/3 of the whole Galactic disk within the magnitude range of $10mag. All OGLE-IV surveys provide photometry with milli-magnitude accuracy at the bright end. The cadence of observations varies from 19-60 minutes in the inner Galactic bulge to 1-3 days in the remaining Galactic bulge fields, Magellanic System and the Galactic disk. OGLE-IV provides the astronomical com...

Udalski, A; Szyma?ski, G

2015-01-01T23:59:59.000Z

414

A Time Delay for the Largest Gravitationally Lensed Quasar: SDSS J1004+4112  

E-Print Network [OSTI]

We present 426 epochs of optical monitoring data spanning 1000 days from December 2003 to June 2006 for the gravitationally lensed quasar SDSS J1004+4112. The time delay between the A and B images is 38.4+/-2.0 days in the expected sense that B leads A and the overall time ordering is C-B-A-D-E. The measured delay invalidates all published models. The models failed because they neglected the perturbations from cluster member galaxies. Models including the galaxies can fit the data well, but strong conclusions about the cluster mass distribution should await the measurement of the longer, and less substructure sensitive, delays of the C and D images. For these images, a CB delay of 681+/-15 days is plausible but requires confirmation, while CB and AD delays of >560 days and > 800 days are required. We clearly detect microlensing of the A/B images, with the delay-corrected flux ratios changing from B-A=0.44+/-0.01 mag in the first season to 0.29+/-0.01 mag in the second season and 0.32+/-0.01 mag in the third season.

J. Fohlmeister; C. S. Kochanek; E. E. Falco; J. Wambsganss; N. Morgan; C. W. Morgan; E. O. Ofek; D. Maoz; C. R. Keeton; J. C. Barentine; G. Dalton; J. Dembicky; W. Ketzeback; R. McMillan; C. S. Peters

2006-07-21T23:59:59.000Z

415

The young low-mass star ISO-Oph-50: Extreme variability induced by a clumpy, evolving circumstellar disk  

E-Print Network [OSTI]

ISO-Oph-50 is a young low-mass object in the ~Myr old Ophiuchus star forming region undergoing dramatic changes in its optical/near/mid-infrared brightness by 2-4 mag. We present new multi-band photometry and near-infrared spectra, combined with a synopsis of the existing literature data. Based on the spectroscopy, the source is confirmed as a mid M dwarf, with evidence for ongoing accretion. The near-infrared lightcurves show large-scale variations, with 2-4 mag amplitude in the bands IJHK, with the object generally being bluer when faint. Near its brightest state, the object shows colour changes consistent with variable extinction of dAV~7 mag. High-cadence monitoring at 3.6mu reveals quasi-periodic variations with a typical timescale of 1-2 weeks. The best explanation for these characteristics is a low-mass star seen through circumstellar matter, whose complex variability is caused by changing inhomogeneities in the inner parts of the disk. When faint, the direct stellar emission is blocked; the near-infra...

Scholz, Aleks; Geers, Vincent

2015-01-01T23:59:59.000Z

416

MOVING OBJECTS IN THE HUBBLE ULTRA DEEP FIELD  

SciTech Connect (OSTI)

We identify proper motion objects in the Hubble Ultra Deep Field (UDF) using the optical data from the original UDF program in 2004 and the near-infrared data from the 128 orbit UDF 2012 campaign. There are 12 sources brighter than I = 27 mag that display >3{sigma} significant proper motions. We do not find any proper motion objects fainter than this magnitude limit. Combining optical and near-infrared photometry, we model the spectral energy distribution of each point-source using stellar templates and state-of-the-art white dwarf models. For I {<=} 27 mag, we identify 23 stars with K0-M6 spectral types and two faint blue objects that are clearly old, thick disk white dwarfs. We measure a thick disk white dwarf space density of 0.1-1.7 Multiplication-Sign 10{sup -3} pc{sup -3} from these two objects. There are no halo white dwarfs in the UDF down to I = 27 mag. Combining the Hubble Deep Field North, South, and the UDF data, we do not see any evidence for dark matter in the form of faint halo white dwarfs, and the observed population of white dwarfs can be explained with the standard Galactic models.

Kilic, Mukremin; Gianninas, Alexandros [Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, 440 W. Brooks St., Norman, OK 73019 (United States); Von Hippel, Ted, E-mail: kilic@ou.edu, E-mail: alexg@nhn.ou.edu, E-mail: ted.vonhippel@erau.edu [Embry-Riddle Aeronautical University, 600 S. Clyde Morris Blvd., Daytona Beach, FL 32114 (United States)

2013-09-01T23:59:59.000Z

417

Time-Resolved Near-Infrared Photometry of Extreme Kuiper Belt Object Haumea  

E-Print Network [OSTI]

We present time-resolved near-infrared (J and H) photometry of the extreme Kuiper belt object (136108) Haumea (formerly 2003 EL61) taken to further investigate rotational variability of this object. The new data show that the near-infrared peak-to-peak photometric range is similar to the value at visible wavelengths, \\Delta m_R = 0.30+/-0.02 mag. Detailed analysis of the new and previous data reveals subtle visible/near-infrared color variations across the surface of Haumea. The color variations are spatially correlated with a previously identified surface region, redder in B-R and darker than the mean surface. Our photometry indicates that the J-H colors of Haumea (J-H=-0.057+/-0.016 mag) and its brightest satellite Hi'iaka (J-H=-0.399+/-0.034 mag) are significantly (>9 sigma) different. The satellite Hi'iaka is unusually blue in J-H, consistent with strong 1.5 micron water-ice absorption. The phase coefficient of Haumea in the J-band is found to increase monotonically with wavelength in the range 0.4

Pedro Lacerda

2008-11-23T23:59:59.000Z

418

A Test of Tully-Fisher Distance Estimates Using Cepheids and Type Ia Supernovae  

E-Print Network [OSTI]

We update and extend the results of Shanks (1997, MNRAS, 290, L77) by making a direct test of Tully-Fisher distance estimates to thirteen spiral galaxies with HST Cepheid distances and to ten spiral galaxies with Type Ia supernova (SNIa) distances. The results show that the Tully-Fisher distance moduli are too short with respect to the Cepheid distances by 0.46+-0.11mag and too short with respect to the SNIa distances by 0.49+-0.18mag. Combining the HST Cepheid and the best SNIa data suggests that, overall, previous Tully-Fisher distances at v~1000 kms-1 were too short by 0.43+-0.09mag, a result which is significant at the 4.6 sigma level. These data therefore indicate that previous Tully-Fisher distances should be revised upwards by 22+-5% implying, for example, a Virgo distance of 19.0+-1.8Mpc. The value of Ho from Tully-Fisher estimates is correspondingly revised downwards from Ho=84+-10kms-1Mpc-1 to Ho=69+-8kms-1Mpc-1. There is evidence that the Tully-Fisher relation at large distances is affected by Malmquist bias. In this case, we argue that Ho<50kms-1Mpc-1 cannot be ruled out by Tully-Fisher considerations.

T. Shanks

1999-01-24T23:59:59.000Z

419

The Tully-Fisher Relation and Its Residuals for a Broadly Selected Sample of Galaxies  

E-Print Network [OSTI]

We measure the relation between galaxy luminosity and disk circular velocity (the Tully-Fisher [TF] relation), in the g, r, i, and z-bands, for a broadly selected sample of galaxies from the Sloan Digital Sky Survey, with the goal of providing well defined observational constraints for theoretical models of galaxy formation. The input sample of 234 galaxies has a roughly flat distribution of absolute magnitudes in the range -18.5 > Mr > -22, and our only morphological selection is an axis-ratio cut b/a < 0.6 to allow accurate inclination corrections. Long-slit spectroscopy yields usable H-alpha rotation curves for 170 galaxies. Observational errors, including distance errors due to peculiar velocities, are small compared to the intrinsic scatter of the TF relation. The slope of the forward TF relation steepens from -5.4 +/- 0.2 mag/log(km/s) in the g-band to -6.4 +/- 0.2 mag/log(km/s) in the z-band. The intrinsic scatter is approximately 0.4 mag in all bands. The scatter is not dominated by rare outliers o...

Pizagno, J; Weinberg, D H; Rix, H W; Pogge, R W; Grebel, E K; Harbeck, D; Blanton, M; Brinkmann, J; Gunn, J E; Pizagno, James; Prada, Francisco; Weinberg, David H.; Rix, Hans-Walter; Pogge, Richard W.; Grebel, Eva K.; Harbeck, Daniel; Blanton, Michael; Gunn, James E.

2006-01-01T23:59:59.000Z

420

A Test of the Calibration of the Tully-Fisher Relation Using Cepheid and SNIa Distances  

E-Print Network [OSTI]

We make a direct test of Tully-Fisher distance estimates to eleven spiral galaxies with HST Cepheid distances and to twelve spiral galaxies with SNIa distances. The HST Cepheid distances come from the work of Freedman (1997), Sandage et al (1996) and Tanvir et al (1995). The SNIa distances come from Pierce (1994), calibrated using the Cepheid results of Sandage et al (1996). The Tully-Fisher distances mostly come from the work of Pierce (1994). The results show that the Tully-Fisher distance moduli are too short with respect to the Cepheid distances by 0.46+-0.14mag and too short with respect to the SNIa distances by 0.46+-0.19mag. Combining the HST Cepheid and SNIa data suggests that, overall, previous Tully-Fisher distances were too short by 0.46+-0.11mag, a result which is significant at the 4sigma level. These data therefore indicate that previous Tully-Fisher distances should be revised upwards by 24+-6% implying, for example, a Virgo distance of 19.3+-1.9Mpc. The value of Ho from Tully-Fisher estimates is correspondingly revised downwards from Ho=84+-10 to Ho=68+-8.

T. Shanks

1997-02-18T23:59:59.000Z

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
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421

Design, implementation, and on-sky performance of an advanced apochromatic triplet atmospheric dispersion corrector for the Magellan adaptive optics system and VisAO camera  

E-Print Network [OSTI]

We present the novel design, laboratory verification, and on-sky performance of our advanced triplet atmospheric dispersion corrector (ADC), an important component of the Magellan Adaptive Optics system (MagAO), which recently achieved first light in December 2012. High-precision broadband (0.5-1.0 microns) atmospheric dispersion correction at visible wavelengths is essential both for wavefront sensing (WFS) on fainter guide stars, and for performing visible AO science using our VisAO science camera. At 2 airmasses (60 degrees from zenith) and over the waveband 500-1000 nm, our triplet design produces a 57% improvement in geometric rms spot size, a 33% improvement in encircled energy at 20 arcsec radius, and a 62% improvement in Strehl ratio when compared to a conventional doublet design. This triplet design has been fabricated, tested in the lab, and integrated into the MagAO WFS and the VisAO science camera. We present on-sky results of the ADC in operation with the MagAO system. We also present a zero-beam...

Kopon, Derek; Males, Jared R; Gasho, Victor

2013-01-01T23:59:59.000Z

422

SDSS J160043.6+074802.9: a very rapid sdO pulsator  

E-Print Network [OSTI]

We report the serendipitous discovery of the Sloan Digital Sky Survey star, SDSS J160043.6+074802.9 to be a very rapid pulsator. The variation is dominated by a frequency near 8380 microHz (period = 119.33 s) with a large amplitude (0.04 mag) and its first harmonic at 16760 microHz (59.66 s; 0.005 mag). In between these frequencies, we find at least another 8 variations with periods between 62 and 118 seconds and amplitudes between about 0.007 and 0.003 mag; weaker oscillations might also be present. Preliminary spectrograms from the performance verification phase of the Southern African Large Telescope indicate that SDSS J160043.6+074802.9 is a spectroscopic binary consisting of an sdO star and a late-type main-sequence companion. This makes it the first unambiguous detection of such an sdO star to pulsate, and certainly the first found to exhibit multi-frequency variations.

Woudt, P A; Zietsman, E; Warner, B; Loaring, N S; Copley, C; Kniazev, A; Visnen, P; Still, M; Stobie, R S; Burgh, E B; Nordsieck, K H; Percival, J W; O'Donoghue, D; Buckley, D A H

2006-01-01T23:59:59.000Z

423

A mathematical treatment of the stability problem  

E-Print Network [OSTI]

These column operations do not change the determinant, thus 21 1 0 0 D ~ det (xl 1 G~ Q2 0 (X 2n-4 F(h) h ~ 9 n-2 (-1) h (-1) Hence, first by column expansion, then by row expansion 0 0 D (-1) F (h) det H n-2 (-1) F(h)det H n 2 6 2n-4 (-1) F(h... t F ). Now define the 2mxn matrix K 2m ~ ' 0 a1 a 2 1 3 a 2m-1 and the (2m+1)x(m+1) matrix 2m+1 0 0 1 0 -a 1 1 a2 1 a2 a 2m Then 0 H K 2lll 2m m 27 and 0 "2 +1"2m+1 = E m+1 Define the 2mxm matrix Q ~ ~ a ~ P Q ~ ~ s p R 2m Q...

Kelly, Claude Leslie

2012-06-07T23:59:59.000Z

424

AN r-PROCESS KILONOVA ASSOCIATED WITH THE SHORT-HARD GRB 130603B  

SciTech Connect (OSTI)

We present ground-based optical and Hubble Space Telescope (HST) optical and near-IR observations of the short-hard GRB 130603B at z = 0.356, which demonstrate the presence of excess near-IR emission matching the expected brightness and color of an r-process powered transient (a {sup k}ilonova{sup )}. The early afterglow fades rapidly with {alpha} {approx}< -2.6 at t Almost-Equal-To 8-32 hr post-burst and has a spectral index of {beta} Almost-Equal-To -1.5 (F{sub {nu}}{proportional_to}t {sup {alpha}}{nu}{sup {beta}}), leading to an expected near-IR brightness at the time of the first HST observation of m{sub F160W}(t = 9.4 days) {approx}> 29.3 AB mag. Instead, the detected source has m{sub F160W} = 25.8 {+-} 0.2 AB mag, corresponding to a rest-frame absolute magnitude of M{sub J} Almost-Equal-To -15.2 mag. The upper limit in the HST optical observations is m{sub F606W} {approx}> 27.7 AB mag (3{sigma}), indicating an unusually red color of V - H {approx}> 1.9 mag. Comparing the observed near-IR luminosity to theoretical models of kilonovae produced by ejecta from the merger of an NS-NS or NS-BH binary, we infer an ejecta mass of M{sub ej} Almost-Equal-To 0.03-0.08 M{sub Sun} for v{sub ej} Almost-Equal-To 0.1-0.3c. The inferred mass matches the expectations from numerical merger simulations. The presence of a kilonova provides the strongest evidence to date that short GRBs are produced by compact object mergers, and provides initial insight on the ejected mass and the primary role that compact object merger may play in the r-process. Equally important, it demonstrates that gravitational wave sources detected by Advanced LIGO/Virgo will be accompanied by optical/near-IR counterparts with unusually red colors, detectable by existing and upcoming large wide-field facilities (e.g., Pan-STARRS, DECam, Subaru, LSST)

Berger, E.; Fong, W.; Chornock, R. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2013-09-10T23:59:59.000Z

425

Full Abstraction for Nominal General References  

E-Print Network [OSTI]

}. For each m (MA \\ IA): iA A m1 A · · · A mi A m Initial moves are P-Answers,and whenever m1 A m2, m1, m2 The -calculus is a functional calculus with nominal references. TY A, B ::= ½ | ? | [A] | A B | A B TE M, N ::= x | x.M | M N -term | skip return | n | pred M | succ N arithmetic | if0 M then N1 else N2

426

E=1/2Mv2 Pf Pb(Pf>Pb)  

E-Print Network [OSTI]

/2Mv2 , ( 3.1). 3.1 UF6 , Pf Pb(Pf>Pb) . i J2 = V1P1f V2P2f = M2 M1 1/2 x (1-x) . = y/(1-y) x/(1-x) = (M2/M1)1/2 UF6 = (M2/M1)1/2 =(238 UF6/235 UF6)1/2 = (352/349)1/2 = 1.00429 1 . 5% 900

Hong, Deog Ki

427

J. Math. Anal. Appl. 421 (2015) 747753 Contents lists available at ScienceDirect  

E-Print Network [OSTI]

subspaces of X, PMi is the best approximation operator to the linear subspace Mi, and M := M1 + · · · + Mr to x X from M := M1 + · · · + Mr in the space X based on the knowledge of these PMi . E-mail address, i.e., mi = PMi (x - m1 - · · · - mi-1). Now consider lim s Es x. Note that Es x = x - ys for some ys

Pinkus, Allan

2015-01-01T23:59:59.000Z

428

Review article Induced seismicity and hydraulic fracturing for the recovery of  

E-Print Network [OSTI]

of gas and oil from low-permeability sedimentary rocks (M 1.0e3.8). Reactivation of faults and resultant seismicity linked to the hydraulic fracturing of low-permeability sedimentary rocks such as `tight' sandston and magnitudes are (a) mining (M 1.6e5.6); (b) oil and gas field depletion (M 1.0e7.3); (c) water injection

Foulger, G. R.

429

ACADEMIC CALENDAR Medical School  

E-Print Network [OSTI]

CLASSES RESUME M-1, M-2 W SEPTEMBER 18 CONVOCATION/PRESIDENT'S RECEPTION ALL CLASSES 4:30 P.M. TH OCTOBER CLERKSHIPS RESUME M-3 M JANUARY 6 CLASSES RESUME M-1, M-2 M JANUARY 20 MARTIN LUTHER KING, JR. DAY.M. M MARCH 24 CLASSES RESUME M-1, M-2 F MAY 9 CLASSES END M-2 TH MAY 15 CLINICAL ROTATIONS END SENIOR

430

application cryogenic monitoring: Topics by E-print Network  

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

... Only one 10-digit reference number should be allotted to any one applicant and only one M1 monitoring@admin.ox.ac.uk...

431

ON CONSISTENCY OF CELL-VERTEX FINITE-VOLUME FORMULATIONS FOR VISCOELASTIC FLOW  

E-Print Network [OSTI]

, given F(u), we 2 #12;can obtain the original discrete function f(x) by inverse DFT: f(x) = M-1 u=0 F

Grant, P. W.

432

E-Print Network 3.0 - arabidopsis transcriptome profiling1woa...  

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

Universiteit - Department of Plant Systems Biology, Bioinformatics and Evolutionary Genomics Division Collection: Biology and Medicine 2 PROPOSITION DE STAGE M1M2 Analysis of...

433

EIGENVALUE ASYMPTOTICS FOR SCHRDINGER OPERATORS ON SPARSE GRAPHS  

E-Print Network [OSTI]

, BKW, D2, DK, F, M1, M2, K1, KL2, Woj1]. In certain more spe- cific geometric situations the bottom

Recanati, Catherine

434

ESSENTIAL SPECTRUM AND WEYL ASYMPTOTICS FOR DISCRETE LAPLACIANS  

E-Print Network [OSTI]

is given through Cheeger/isoperimetrical inequalities, e.g., [BHJ, BKW, D1, D2, DK, Fuj, M1, M2, KL2, Woj

Paris-Sud XI, Université de

435

a new weight  

E-Print Network [OSTI]

by the National Science Foundation of China (NSFC 11101413). 1136 ..... Step 1. According to the energy estimate (2.30), the sequence {hm}? m=1 is bounded...

2012-05-15T23:59:59.000Z

436

Max-Planck-Institut fur Mathematik  

E-Print Network [OSTI]

- 1)/2, D2 = d2(d2 - 1)/2, and Cmn = |mn. Here, |mn := (Lm Ln)| , with Lm, m = 1, ..., D1, Ln, n = 1

437

Guiding the osteogenic fate of mouse and human mesenchymal stem cells through feedback system control  

E-Print Network [OSTI]

3, S3238 (2009). 37. Diefenderfer, D. L. , Osyczka, A. M. ,1, 38. Osyczka, A. M. , Diefenderfer, D. L. , Bhargave, G. &

Honda, Y; Ding, X; Mussano, F; Wiberg, A; Ho, C-M; Nishimura, I

2013-01-01T23:59:59.000Z

438

Bivariate B-splines and its Applications in Spatial Data Analysis  

E-Print Network [OSTI]

(m)ijk (w) := w1c (m 1) i+1;j;k + w2c (m 1) i;j+1;k + w3c (m 1) i;j;k+1; form = 1; :::; d: (2.23) Then, Dmw s(v) = d! (d m)! X i+j+k=d m c(m)ijk (w)Bd m;ijk(v): (2.24) Proof. When m = 1, we need to show that Dws(v) = d X i+j+k=d 1 c(1)ijk...

Pan, Huijun 1987-

2011-08-09T23:59:59.000Z

439

Universitt Tbingen Mathematisches Institut  

E-Print Network [OSTI]

Approximation S() := m-1 i=0 [(1 - )Wti + Wti+1 ](Wti+1 - Wti ) des Integrals t 0 WsdWs. Zeigen Sie lim ||||0 S

Tübingen, Universität

440

E-Print Network 3.0 - applying bayesian neural Sample Search...  

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

Centre de mathmatiques Collection: Mathematics 90 Predicting EMG Activity from Neural Firing in M1 with Bayesian Backfitting Summary: Predicting EMG Activity from Neural Firing...

Note: This page contains sample records for the topic "maldives mag m1" 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

Talk With Baby: A Guide for Parents.  

E-Print Network [OSTI]

. Distributed in furtherance of the Acts of Congress of May 8, 1914, as amended, and June 30, 1914. 3M-1-84, Revision FLE 3 ...

Anonymous

1984-01-01T23:59:59.000Z

442

Summary Statistics Table 1. Crude Oil Prices  

Annual Energy Outlook 2013 [U.S. Energy Information Administration (EIA)]

Energy Information Administration, Form FEA-P110-M-1, "Refiners' Monthly Cost Allocation Report," January 1978 through June 1978; Form ERA-49, "Domestic Crude Oil Entitlements...

443

PROGRAM OVERVIEW The Naval Postgraduate School (NPS) has a strong sponsored pro-  

E-Print Network [OSTI]

RESEARCH FISCAL YEAR ANNUAL REPORT 2011 BY SPONSOR ARMY $8.1m 4% AIR FORCE $9.9m 5% CRADA $1.5m 1% OTHER

444

Chloride improves fruit yield and quality of strawberry (Fragaria ananassa Duch.)  

E-Print Network [OSTI]

1988; 88: 194-199 Martnez Barroso MC, Alvarez CE, Toxicityof 2 dS m -1 (Martnez Barroso and Alvarez 1997). Hypotheses

Bellof, Svenja; Schubert, Sven

2009-01-01T23:59:59.000Z

445

The 7 Ways Small Cells are Forever Changing Wireless  

E-Print Network [OSTI]

support. 2. Picocells Small, short-range (~100m), 1-2W, low-cost ($5-40K CapEx, small OpEx), deployed

Andrews, Jeffrey G.

446

ACADEMIC CALENDAR Medical School  

E-Print Network [OSTI]

/CLASSES BEGIN M-2 9:00 A.M./ 1:00 P.M. M SEPTEMBER 3 LABOR DAY HOLIDAY M-1, M-2 TU SEPTEMBER 4 CLASSES RESUME M/CLERKSHIPS RESUME M-1, M-2, M-3 AS ASSIGNED M JANUARY 21 MARTIN LUTHER KING, JR. DAY CELEBRATION ALL CLASSES 4:30 P.M. SA-SU MARCH 9-17 SPRING BREAK M-1, M-2 F MARCH 15 MATCH DAY M-4 11:00 A.M. M MARCH 18 CLASSES RESUME

447

http://frwebgate.access.gpo.gov/cgi-bin/getdoc.cgi?dbname=106...  

National Nuclear Security Administration (NNSA)

capability combat vehicles that are significantly superior to the existing M1 series of tanks in terms of capability for combat, survival, support, and deployment, including but...

448

MOUVEMENTS DE MARKOV POUR DES TRESSES QUASIPOSITIVES  

E-Print Network [OSTI]

1, . . . , m-1 et r´elations [j, k] = 1 pour |k - j| > 1 et jkj = kjk pour |k - j| = 1. Une tresse b

Orevkov, Stepan

449

On the Alspach conjecture P.N. Balister  

E-Print Network [OSTI]

odd) or Kn minus a 1-factor (n even) with cycles of lengths m1, . . . , mt. In this paper we show that if the cycle lengths mi are bounded by some linear function of n and n is sufficiently large (n odd) or Kn minus a 1-factor I (n even) with cycles of lengths m1, . . . , mt. If we just require

Balister, Paul

450

Very low-mass spectroscopic companion around the  

E-Print Network [OSTI]

.04 AU PPl 15: 1st BD binary (Basri & Martin 1999) SB2, M2/M1=0.85 M1=0.07Msol M2=0.06 MSol P=6 days a=0 BD eclipsing SB2 (Stassun et al. 2006) P=10 days q = 0.6 PPl 15: 1st BD binary (Basri & Martin 1999

Joergens, Viki

451

Google:[Leonid Zakharov] http://w3.pppl.gov/~zakharov How far is magnetic fusion from being  

E-Print Network [OSTI]

.2) Monetary value of electricity Cel kg = 6.29 3 Ccost of electricity 0.04 CDT electricity 0.33 · 106 [$ ] $2M, (1.3) and the cost of tritium (2003) CT kg $30M. (1.4) Consumption of 1 kg of T per m2

Zakharov, Leonid E.

452

Ph.D. QUALIFYING EXAMINATION DEPARTMENT OF PHYSICS AND ASTRONOMY  

E-Print Network [OSTI]

, m = (j + m)(j - m + 1) |j, m - 1 . #12;2. (10 points): Calculate the efficiency of the Diesel cycle is the electric field inside the block? (6 pts.) (b) What is the electric charge density in the volume

Baskaran, Mark

453

Dtermination des formes modulaires par les valeurs de  

E-Print Network [OSTI]

(resp. d'ordre 3) de . ? titre d'exemple, on a #23; 2 0 (m) #1; = 8 pjm #2; 1 + 1 p #1;#3; sinon et #23; 3 0 (m) #1; = 8 pjm #2; 1 + 3 p #1;#3; sinon. [Miy89, theorem 4.2.7] Ce

Royer, Emmanuel

454

CARACTRISATION DES FORMES MODULAIRES PAR DES VALEURS DE FONCTIONS L  

E-Print Network [OSTI]

d'ordre 2 (resp. d'ordre 3) de . ? titre d'exemple, on a #23; 2 0 (m) #1; = 8 pjm #2; 1 + 1 p #1;#3; sinon et #23; 3 0 (m) #1; = 8 pjm #2; 1 + 3 p #1;#3; sinon. [Miy

Royer, Emmanuel

455

Primes Solutions Of Linear Diophantine Equations  

E-Print Network [OSTI]

Let k => 1, m => 1 be small fixed integers, gcd(k, m) = 1. This note develops some techniques for proving the existence of infinitely many primes solutions x = p, and y = q of the linear Diophantine equation y = mx + k.

N. A. Carella

2014-04-03T23:59:59.000Z

456

Wireless LAN E001 Fujitsu  

E-Print Network [OSTI]

PC Code Image Brand Model 1 / 5 #12; CPU System Memory HDD Display Size Weight OS Accessory LAN Wireless LAN Remarks PC PC Code Image Brand Model E008 EPSON Endeavor NT331 Celeron M1.40GHz LAN Wireless LAN Remarks PC PC Code Image Brand Model E019 EPSON Endeavor NT331 Celeron M1.40GHz

Katsumoto, Shingo

457

49 (2012-5) Investigation of phonon transport in alloyed crystals by perturbation approach  

E-Print Network [OSTI]

?6?6, 20 K TA1 TA2 LA mi/m=0.2 mi/m=0.5 mi/m=0.8 mi/m=1.2 mi/m=1.8 mi/m=2.0 mi/m=3.0 mi/m=5.0 2% mi/m=1 concentration at 20 K. 1 10 ­4 10 ­3 10 ­2 10 ­1 ms(THz) Frequency (THz) 6?6?6, 20 K TA1 TA2 LA mi/m=0.2 mi/m=0.5 mi/m=0.8 mi/m=1.5 mi/m=1.8 mi/m=2.0 mi/m=3.0 mi/m=5.0 2% 4 4 Fig. 3 Phonon scattering rates due

Maruyama, Shigeo

458

RADIATIVE TRANSFER SIMULATIONS OF NEUTRON STAR MERGER EJECTA  

SciTech Connect (OSTI)

Mergers of binary neutron stars (NSs) are among the most promising gravitational wave (GW) sources. Next generation GW detectors are expected to detect signals from NS mergers within about 200 Mpc. The detection of electromagnetic wave (EM) counterparts is crucial to understanding the nature of GW sources. Among the possible EM emission from the NS merger, emission powered by radioactive r-process nuclei is one of the best targets for follow-up observations. However, predictions so far have not taken into account detailed r-process element abundances in the ejecta. We perform for the first time radiative transfer simulations of the NS merger ejecta including all the r-process elements from Ga to U. We show that the opacity of the NS merger ejecta is about ? = 10 cm{sup 2} g{sup 1}, which is higher than that of Fe-rich Type Ia supernova ejecta by a factor of ?100. As a result, the emission is fainter and lasts longer than previously expected. The spectra are almost featureless due to the high expansion velocity and bound-bound transitions of many different r-process elements. We demonstrate that the emission is brighter for a higher mass ratio of the two NSs and a softer equation of state adopted in the merger simulations. Because of the red color of the emission, follow-up observations in red optical and near-infrared (NIR) wavelengths will be the most efficient. At 200 Mpc, the expected brightness of the emission is i = 22-25 AB mag, z = 21-23 AB mag, and 21-24 AB mag in the NIR JHK bands. Thus, observations with wide-field 4 m- and 8 m-class optical telescopes and wide-field NIR space telescopes are necessary. We also argue that the emission powered by radioactive energy can be detected in the afterglow of nearby short gamma-ray bursts.

Tanaka, Masaomi [National Astronomical Observatory of Japan, Mitaka, Tokyo (Japan); Hotokezaka, Kenta, E-mail: masaomi.tanaka@nao.ac.jp, E-mail: hotoke@tap.scphys.kyoto-u.ac.jp [Department of Physics, Kyoto University, Kyoto (Japan)

2013-10-01T23:59:59.000Z

459

Robust Machine Learning Applied to Astronomical Datasets III: Probabilistic Photometric Redshifts for Galaxies and Quasars in the SDSS and GALEX  

E-Print Network [OSTI]

We apply machine learning in the form of a nearest neighbor instance-based algorithm (NN) to generate full photometric redshift probability density functions (PDFs) for objects in the Fifth Data Release of the Sloan Digital Sky Survey (SDSS DR5). We use a conceptually simple but novel application of NN to generate the PDFs - perturbing the object colors by their measurement error - and using the resulting instances of nearest neighbor distributions to generate numerous individual redshifts. When the redshifts are compared to existing SDSS spectroscopic data, we find that the mean value of each PDF has a dispersion between the photometric and spectroscopic redshift consistent with other machine learning techniques, being sigma = 0.0207 +/- 0.0001 for main sample galaxies to r < 17.77 mag, sigma = 0.0243 +/- 0.0002 for luminous red galaxies to r < ~19.2 mag, and sigma = 0.343 +/- 0.005 for quasars to i < 20.3 mag. The PDFs allow the selection of subsets with improved statistics. For quasars, the improvement is dramatic: for those with a single peak in their probability distribution, the dispersion is reduced from 0.343 to sigma = 0.117 +/- 0.010, and the photometric redshift is within 0.3 of the spectroscopic redshift for 99.3 +/- 0.1% of the objects. Thus, for this optical quasar sample, we can virtually eliminate 'catastrophic' photometric redshift estimates. In addition to the SDSS sample, we incorporate ultraviolet photometry from the Third Data Release of the Galaxy Evolution Explorer All-Sky Imaging Survey (GALEX AIS GR3) to create PDFs for objects seen in both surveys. For quasars, the increased coverage of the observed frame UV of the SED results in significant improvement over the full SDSS sample, with sigma = 0.234 +/- 0.010. We demonstrate that this improvement is genuine. [Abridged

Nicholas M. Ball; Robert J. Brunner; Adam D. Myers; Natalie E. Strand; Stacey L. Alberts; David Tcheng

2008-04-21T23:59:59.000Z

460

THE ACS NEARBY GALAXY SURVEY TREASURY  

SciTech Connect (OSTI)

The ACS Nearby Galaxy Survey Treasury (ANGST) is a systematic survey to establish a legacy of uniform multi-color photometry of resolved stars for a volume-limited sample of nearby galaxies (D < 4 Mpc). The survey volume encompasses 69 galaxies in diverse environments, including close pairs, small and large groups, filaments, and truly isolated regions. The galaxies include a nearly complete range of morphological types spanning a factor of {approx}10{sup 4} in luminosity and star formation rate. The survey data consist of images taken with the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope (HST), supplemented with archival data and new Wide Field Planetary Camera 2 (WFPC2) imaging taken after the failure of ACS. Survey images include wide field tilings covering the full radial extent of each galaxy, and single deep pointings in uncrowded regions of the most massive galaxies in the volume. The new wide field imaging in ANGST reaches median 50% completenesses of m {sub F475W} = 28.0 mag, m {sub F606W} = 27.3 mag, and m {sub F814W} = 27.3 mag, several magnitudes below the tip of the red giant branch (TRGB). The deep fields reach magnitudes sufficient to fully resolve the structure in the red clump. The resulting photometric catalogs are publicly accessible and contain over 34 million photometric measurements of >14 million stars. In this paper we present the details of the sample selection, imaging, data reduction, and the resulting photometric catalogs, along with an analysis of the photometric uncertainties (systematic and random), for both ACS and WFPC2 imaging. We also present uniformly derived relative distances measured from the apparent magnitude of the TRGB.

Dalcanton, Julianne J.; Williams, Benjamin F.; Rosema, Keith; Gogarten, Stephanie M.; Christensen, Charlotte; Gilbert, Karoline; Hodge, Paul [Department of Astronomy, Box 351580, University of Washington, Seattle, WA 98195 (United States); Seth, Anil C. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Dolphin, Andrew [Raytheon, 1151 E. Hermans Road, Tucson, AZ 85756 (United States); Holtzman, Jon [Department of Astronomy, New Mexico State University, Box 30001, 1320 Frenger St., Las Cruces, NM 88003 (United States); Skillman, Evan D.; Weisz, Daniel [Department of Astronomy, University of Minnesota, 116 Church St. SE, Minneapolis, MN 55455 (United States); Cole, Andrew [School of Mathematics and Physics, University of Tasmania, Hobart, Tasmania (Australia); Girardi, Leo [Osservatorio Astronomico di Padova - INAF, Vicolo dell'Osservatorio 5, I-35122 Padova (Italy); Karachentsev, Igor D. [Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnji Arkhyz, Karachai-Circessia Republic 369167 (Russian Federation); Olsen, Knut [NOAO, National Optical Astronomy Observatory 950 N. Cherry Ave., Tucson, AZ 85719 (United States); Freeman, Ken [Mount Stromlo Observatory, Research School of Astronomy and Astrophysics, The Australian National Univ., ACT 0200 (Australia); Gallart, Carme [Inst. de AstrofIsica de Canarias, VIa Lactea, s/n, 38200 La Laguna, Tenerife (Spain); Harris, Jason [Steward Observatory, Univ. of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); De Jong, Roelof S. [Space Telescope Science Inst., 3700 San Martin Dr., Baltimore, MD 21218 (United States)], E-mail: jd@astro.washington.edu, E-mail: ben@astro.washington.edu, E-mail: krosema@astro.washington.edu, E-mail: stephanie@astro.washington.edu, E-mail: christensen@astro.washington.edu, E-mail: fabio@astro.washington.edu, E-mail: trq@astro.washington.edu, E-mail: aseth@cfa.harvard.edu (and others)

2009-07-15T23:59:59.000Z

Note: This page contains sample records for the topic "maldives mag m1" 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

2MASS wide field extinction maps - I. The Pipe nebula  

E-Print Network [OSTI]

We present a 8 deg x 6 deg, high resolution extinction map of the Pipe nebula using 4.5 million stars from the Two Micron All Sky Survey (2MASS) point source catalog. The use of NICER, a robust and optimal technique to map the dust column density, allows us to detect a Av = 0.5 mag extinction at a 3-sigma level with a 1 arcmin resolution. We find for the Pipe nebula a normal reddening law, E(J-H) = (1.85 +/- 0.15) E(H-K). We measure the cloud distance using Hipparchos and Tycho parallaxes, and obtain ~130 pc. This, together with the total estimated mass, 10^4 Msun, makes the Pipe the closest massive cloud complex to Earth. We compare the NICER extinction map to the NANTEN 12CO observations and derive with unprecedented accuracy the relationship between the near-infrared extinction and the 12CO column density and hence (indirectly) the 12CO X-factor, that we estimate to be 2.91 10^20 cm^-2 K^-1 km^-1 s in the range Av Pipe field. This represents a significant increase of the known numbers of such stars in the Galaxy. Our analysis confirms the power and simplicity of the color excess technique to study molecular clouds. The comparison with the NANTEN 12CO data corroborates the insensitivity of CO observations to low column densities (up to approximately 2 mag in Av), and shows also an irreducible uncertainty in the dust-CO correlation of about 1 mag of visual extinction.

Marco Lombardi; Joao Alves; Charles J. Lada

2006-06-27T23:59:59.000Z

462

The Near-Infrared Photometric Properties of Bright Giants in the Central Regions of the Galactic Bulge  

E-Print Network [OSTI]

Images recorded through broad (J, H, K), and narrow (CO, and 2.2micron continuum) band filters are used to investigate the photometric properties of bright (K < 13.5) stars in a 6 x 6 arcmin field centered on the SgrA complex. The giant branch ridgelines in the (K, J-K) and (K, H-K) color-magnitude diagrams are well matched by the Baade's Window (BW) M giant sequence if the mean extinction is A_K ~ 2.8 mag. Extinction measurements for individual stars are estimated using the M_K versus infrared color relations defined by M giants in BW, and the majority of stars have A_K between 2.0 and 3.5 mag. The extinction is locally high in the SgrA complex, where A_K ~ 3.1 mag. Reddening-corrected CO indices, CO_o, are derived for over 1300 stars with J, H, and K brightnesses, and over 5300 stars with H and K brightnesses. The distribution of CO_o values for stars with K_o between 11.25 and 7.25 can be reproduced using the M_K versus CO_o relation defined by M giants in BW. The data thus suggest that the most metal-rich giants in the central regions of the bulge and in BW have similar photometric properties and 2.3micron CO strengths. Hence, it appears that the central region of the bulge does not contain a population of stars that are significantly more metal-rich than what is seen in BW.

T. J. Davidge

1998-03-24T23:59:59.000Z

463

TOWARD IDENTIFYING THE UNASSOCIATED GAMMA-RAY SOURCE 1FGL J1311.7-3429 WITH X-RAY AND OPTICAL OBSERVATIONS  

SciTech Connect (OSTI)

We present deep optical and X-ray follow-up observations of the bright unassociated Fermi-LAT gamma-ray source 1FGL J1311.7-3429. The source was already known as an unidentified EGRET source (3EG J1314-3431, EGR J1314-3417), hence its nature has remained uncertain for the past two decades. For the putative counterpart, we detected a quasi-sinusoidal optical modulation of {Delta}m {approx} 2 mag with a period of {approx_equal}1.5 hr in the Rc, r', and g' bands. Moreover, we found that the amplitude of the modulation and peak intensity changed by {approx}>1 mag and {approx}0.5 mag, respectively, over our total six nights of observations from 2012 March to May. Combined with Swift UVOT data, the optical-UV spectrum is consistent with a blackbody temperature, kT {approx_equal} 1 eV and the emission volume radius R{sub bb} {approx_equal} 1.5 Multiplication-Sign 10{sup 4} d{sub kpc} km (d{sub kpc} is the distance to the source in units of 1 kpc). In contrast, deep Suzaku observations conducted in 2009 and 2011 revealed strong X-ray flares with a light curve characterized with a power spectrum density of P(f) {proportional_to} f {sup -2.0{+-}0.4}, but the folded X-ray light curves suggest an orbital modulation also in X-rays. Together with the non-detection of a radio counterpart, and significant curved spectrum and non-detection of variability in gamma-rays, the source may be the second 'radio-quiet' gamma-ray emitting millisecond pulsar candidate after 1FGL J2339.7-0531, although the origin of flaring X-ray and optical variability remains an open question.

Kataoka, J.; Takahashi, Y.; Maeda, K. [Research Institute for Science and Engineering, Waseda University, 3-4-1, Okubo, Shinjuku, Tokyo 169-8555 (Japan); Yatsu, Y.; Kawai, N. [Tokyo Institute of Technology, 2-12-1, Ohokayama, Meguro, Tokyo 152-8551 (Japan); Urata, Y.; Tsai, A. [Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan (China); Cheung, C. C. [National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001 (United States); Totani, T.; Makiya, R. [Department of Astronomy, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502 (Japan); Hanayama, H.; Miyaji, T., E-mail: kataoka.jun@waseda.jp [Ishigakijima Astronomical Observatory, National Astronomical Observatory of Japan, 1024-1 Arakawa, Ishigaki, Okinawa, 907-0024 (Japan)

2012-10-01T23:59:59.000Z

464

ON THE DETECTABILITY OF A PREDICTED MESOLENSING EVENT ASSOCIATED WITH THE HIGH PROPER MOTION STAR VB 10  

SciTech Connect (OSTI)

Extrapolation of the astrometric motion of the nearby low-mass star VB 10 indicates that sometime in late 2011 December or during the first 2-3 months of 2012, the star will make a close approach to a background point source. Based on astrometric uncertainties, we estimate a 1 in 2 chance that the distance of closest approach {rho}{sub min} will be less than 100 mas, a 1 in 5 chance that {rho}{sub min} < 50 mas, and a 1 in 10 chance that {rho}{sub min} < 20 mas. The last would result in a microlensing event with a 6% magnification in the light from the background source and an astrometric shift of 3.3 mas. The lensing signal will however be significantly diluted by the light from VB 10, which is 1.5 mag brighter than the background source in B band, 5 mag brighter in I band, and 10 mag brighter in K band, making the event undetectable in all but the bluer optical bands. However, we show that if VB 10 happens to harbor a {approx}1 M{sub J} planet on a moderately wide ( Almost-Equal-To 0.18 AU-0.84 AU) orbit, there is a chance (1% to more than 10%, depending on the distance of closest approach and orbital period and inclination) that a passage of the planet closer to the background source will result in a secondary event of higher magnification. The detection of secondary events could be made possible with a several-times-per-night multi-site monitoring campaign.

Lepine, Sebastien [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States); DiStefano, Rosanne, E-mail: lepine@amnh.org, E-mail: rd@cfa.harvard.edu [Harvard Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2012-04-10T23:59:59.000Z

465

Prospects for x-ray polarimetry measurements of magnetic fields in magnetized liner inertial fusion plasmas  

SciTech Connect (OSTI)

Magnetized Liner Inertial Fusion (MagLIF) experiments, where a metal liner is imploded to compress a magnetized seed plasma may generate peak magnetic fields ?10{sup 4} T (100 Megagauss) over small volumes (?10{sup ?10}m{sup 3}) at high plasma densities (?10{sup 28}m{sup ?3}) on 100 ns time scales. Such conditions are extremely challenging to diagnose. We discuss the possibility of, and issues involved in, using polarimetry techniques at x-ray wavelengths to measure magnetic fields under these extreme conditions.

Lynn, Alan G., E-mail: lynn@ece.unm.edu; Gilmore, Mark [Department of Electrical and Computer Engineering, University of New Mexico, Albuquerque, New Mexico 87131 (United States)

2014-11-15T23:59:59.000Z

466

The Harlequin Cabbage-bug.  

E-Print Network [OSTI]

to the insects during the spring, from the time the bugs leare their hibernating quarters until the egg-laying period is over. When the bugs become verp abundant upon the trap crop they should be destroyed either by spraying with pure kerosene, burning... to use this material is in the flestruction of the insects on the trap crops and upon crop rem- nants. Kerosene emulsion of 15 per cent. strength mag be used to ki!l the young or immature hugs. Djre~tion~s for making this are appende J . This insect...

Paddock, F.B. (Floyd B.)

1915-01-01T23:59:59.000Z

467

Statics and Dynamics of Spin and Electric Dipoles in 3-Dimension, 4-Dimension, and Other Dimensions  

E-Print Network [OSTI]

-dimensional spaces where polar vec- tors have n components, spin has n (n ?1)/2 components. Moreover, although a rotation can make an arbitrary polar vector have only one noniero component, the same is not true for spin (and mag- netic field). In particular, for n... com- ponent we have derived the equation of motion for spin in n dimensions, and for n =4 we apply it to free Larmor precession, where we find two modes [at y(H~2+H34)]. Simple ferromagnets and spin glasses are also discussed for n=4. Since no true...

SASLOW, WM; Fulling, Stephen A.; Hu, Chia-Ren.

1985-01-01T23:59:59.000Z

468

Character of states near the Fermi level in (Ga,Mn)As: Impurity to valence band crossover RID E-6453-2010  

E-Print Network [OSTI]

doping region. In GaAs:Mn, the most remarkable among these is the onset of carrier mediated ferromagnetism. The understanding of mag- netic properties of these doped semiconductors which are close to the metal-insulator transition can, therefore, only... theory community7,15,18?22 and provides a qualitative, and often a semiquantitative, description of micromagnetic and magne- totransport characteristics of bulk and microstructured #1;Ga,Mn#2;As ferromagnets.6,7,15 Our paper, which we believe further...

Jungwirth, T.; Sinova, Jairo; MacDonald, A. H.; Gallagher, B. L.; Novak, V.; Edmonds, K. W.; Rushforth, A. W.; Campion, R. P.; Foxon, C. T.; Eaves, L.; Olejnik, E.; Masek, J.; Yang, S-R Eric; Wunderlich, J.; Gould, C.; Molenkamp, L. W.; Dietl, T.; Ohno, H.

2007-01-01T23:59:59.000Z

469

"!#$%'&()$021436587 9A@BC5D9EBGFH@7I@P$Q1SRTUV WYX`$a'14RTbcRTde1SfGgihqprs%412tvuuw xyy Hd$yefygyTxheiHd$yecjqkl#mn$xhopyqn  

E-Print Network [OSTI]

Ggihqprs%412tvuuw xyy Hd$yefygyTxheiHd$yecjqkl#mn$xhopyqn ersqrtTuTvw)w)xTy{z|tuf}r~rSxTw)xTyv yvC'nvYD8Sv chromospheric conditions is plotted in Fig. 1. "!Tvw : # E$%$YC'CcA}{8|'YSi ( & 2 ' ( For instance, in regions of sufficiently strong vertical mag- netic field, a series of shocks may lift

Kosovichev, Alexander G.

470

Symmetries of migration related segments of all [001] coincidence site lattice tilt boundaries in (001) projections for all holohedral cubic materials  

SciTech Connect (OSTI)

Utilizing bicrystallography in two dimensions (2D), the symmetries of migration related segments of Coincidence Site Lattice (CSL) boundaries are derived for projections along their [001] tilt axis in grain boundaries of crystalline materials that possess the holohedral point symmetry of the cubic system (i.e. m3m). These kinds of edge-on projections are typical for atomic resolution imaging of such tilt boundaries with Transmission Electron Microscopes (TEM). This fact facilitates the visual confirmation of our predictions by recently published Zcontrast scanning TEM investigations [H. Yang et al., Phil. Mag. 93 (2013) 1219] and many other TEM studies.

Moeck, Peter; York, Bryant W.; Browning, Nigel D.

2014-09-11T23:59:59.000Z

471

In-situ magnetoresistance measurements during patterning of spin valve devices  

E-Print Network [OSTI]

. This dissertation does not exceed the limit of length. Some of the work in this thesis has been published as listed below. Publications Control of the switching properties of magnetic thin films and spin valve devices by patterning, D.Morecroft, C... .W. Leung, N.A. Stelmashenko, J.L. Prieto, D.B. Jardine and M.G. Blamire. IEEE Trans. Mag. 37 Issue: 4 Part: 1 (2001) pp. 2079 2081. In-situ magnetoresistance measurements during patterning of thin films and spin valve devices, D.Morecroft, C...

Morecroft, Deborah

472

Microwave Absorption and Radiation from Large-area Multilayer CVD Graphene  

E-Print Network [OSTI]

2009;9(1):4226. [32] Schwierz F. Graphene transistors. Nat Nano 2010;5(7):48796. [33] Dragoman M, Neculoiu D, Dragoman D, Deligeorgis G, Konstantinidis G, Cismaru A, et al. Graphene for microwaves. IEEE Microw Mag 2010;11(7):816. [34] Fallahi A... graphene were mea- sured at 457 nm (2.71 eV), 532 nm (2.33 eV) and 633 nm (1.96 eV) (see Fig. S1ad). The DC resistivity was measured using a four-point probe contact stylus. The Keithley Model 2100/120 Digital Multimeter with a four-point probe...

Wu, Bian; Tuncer, Hatice M.; Katsounaros, Anestis; Wu, Weiping; Cole, Matthew T.; Ying, Kai; Zhang, Lianhong; Milne, William I.; Hao, Yang

473

Analysis of sub-surface towing of tendons and comparison of results using WINPOST and ORCAFLEX  

E-Print Network [OSTI]

dmpm or ~m Reheard tn Sbdh ~ Canvergenae: Mas Mht Msg. Or Mag. Of Neragarm Taienece Damphtg SRL Error SRL Change 30 0. 0001 1800 2000 tLOTO Speed (nua) Dhecthm (deg) 0. 00 0. 00 Stags DunNon Number (a) 0 9. 000 1 208dtO Tbne Slaps (s) hear... Outer 0. 00028 08100 Une Target Damping (% arhhmt): Axle( Sending Tomhn O. MOO 0. 0000 0. 0000 Nea Our(sac 2 (m): 0. 000 Water Densgy Varhdhrc Water Densh)r. Constant Density (isbn"3) 1. 02$ Seabed Type Flat Seabed Origin (m) Dhecgon Slaps...

Mendon, Perdoor Mukthi

2002-01-01T23:59:59.000Z

474

Gamma-Ray Bursts Trace UV Metrics of Star Formation over 3 < z < 5  

E-Print Network [OSTI]

We present the first uniform treatment of long duration gamma-ray burst (GRB) host galaxy detections and upper limits over the redshift range 3-15.6 mag, and with extrapolations of the assumed Schechter-type LF well beyond this range. We review proposed astrophysical and observational biases for our sample, and find they are for the most part minimal. We therefore conclude, as the simplest interpretation of our results, that GRBs successfully trace UV metrics of cosmic star formation over the range 3

Greiner, Jochen; Schady, Patricia; Krhler, Thomas; Trenti, Michele; Cikota, Aleksandar; Bolmer, Jan; Elliott, Jonathan; Delvaux, Corentin; Perna, Rosalba; Afonso, Paulo; Kann, D Alexander; Klose, Sylvio; Savaglio, Sandra; Schmidl, Sebastian; Schweyer, Tassilo; Tanga, Mohit; Varela, Karla

2015-01-01T23:59:59.000Z

475

Relationship of shale dewatering and smectite dehydration to undercompaction occurrence. Final report, October 1995--September 1996  

SciTech Connect (OSTI)

The cause(s) of abnormal fluid pressures in sedimentary basins are not clearly understood. One step in determining the mechanism(s) of abnormal pressure generation in sedimentary basins is to develop and understanding of the relationship among undercompacted shale, abnormal pressure, and temperature. The research focused on understanding undercompaction and how it related to smectite-illite conversion. A series of carefully designed experiments were used to help clarify and evaluate the relationship of smectite-illite transformation to undercompaction. Work was performed at the East Flour Bluff oil field, Nueces County, TX and the Ann Mag oil field, south TX.

Leftwich, J.T. Jr.

1996-12-01T23:59:59.000Z

476

VARIABLE STARS IN THE ULTRA-FAINT DWARF SPHEROIDAL GALAXY URSA MAJOR I  

SciTech Connect (OSTI)

We have performed the first study of the variable star population of Ursa Major I (UMa I), an ultra-faint dwarf satellite recently discovered around the Milky Way (MW) by the Sloan Digital Sky Survey. Combining time series observations in the B and V bands from four different telescopes, we have identified seven RR Lyrae stars in UMa I, of which five are fundamental-mode (RRab) and two are first-overtone pulsators (RRc). Our V, B - V color-magnitude diagram of UMa I reaches V {approx} 23 mag (at a signal-to-noise ratio of {approx}6) and shows features typical of a single old stellar population. The mean pulsation period of the RRab stars (P{sub ab}) = 0.628, {sigma} = 0.071 days (or (P{sub ab}) = 0.599, {sigma} = 0.032 days, if V4, the longest period and brightest variable, is discarded) and the position on the period-amplitude diagram suggest an Oosterhoff-intermediate classification for the galaxy. The RR Lyrae stars trace the galaxy horizontal branch (HB) at an average apparent magnitude of (V(RR)) = 20.43 {+-} 0.02 mag (average on six stars and discarding V4), giving in turn a distance modulus for UMa I of (m - M){sub 0} = 19.94 {+-} 0.13 mag, distance d = 97.3{sup +6.0}{sub -5.7} kpc, in the scale where the distance modulus of the Large Magellanic Cloud is 18.5 {+-} 0.1 mag. Isodensity contours of UMa I red giants and HB stars (including the RR Lyrae stars identified in this study) show that the galaxy has an S-shaped structure, which is likely caused by the tidal interaction with the MW. Photometric metallicities were derived for six of the UMa I RR Lyrae stars from the parameters of the Fourier decomposition of the V-band light curves, leading to an average metal abundance of [Fe/H] = -2.29 dex ({sigma} = 0.06 dex, average on six stars) on the Carretta et al. metallicity scale.

Garofalo, Alessia; Moretti, Maria Ida [Dipartimento di Astronomia, Universita di Bologna, Via Ranzani 1, I-40127 Bologna (Italy)] [Dipartimento di Astronomia, Universita di Bologna, Via Ranzani 1, I-40127 Bologna (Italy); Cusano, Felice; Clementini, Gisella [INAF-Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127 Bologna (Italy)] [INAF-Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127 Bologna (Italy); Ripepi, Vincenzo; Dall'Ora, Massimo; Coppola, Giuseppina; Musella, Ilaria; Marconi, Marcella, E-mail: alessia.garofalo@studio.unibo.it, E-mail: fcusano@na.astro.it, E-mail: gisella.clementini@oabo.inaf.it, E-mail: ripepi@na.astro.it, E-mail: dallora@na.astro.it, E-mail: imoretti@na.astro.it, E-mail: coppola@na.astro.it, E-mail: ilaria@na.astro.it, E-mail: marcella@na.astro.it [INAF-Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, I-80131 Napoli (Italy)] [INAF-Osservatorio Astronomico di Capodimonte, Salita Moiariello 16, I-80131 Napoli (Italy)

2013-04-10T23:59:59.000Z

477

SEVEN-YEAR MULTI-COLOR OPTICAL MONITORING OF BL LACERTAE OBJECT S5 0716+714  

SciTech Connect (OSTI)

We have monitored the BL Lacertae object S5 0716+714 in five intermediate optical wavebands from 2004 September to 2011 April. Here, we present data that include 8661 measurements representing one of the largest databases obtained for an object in the optical domain. A simple analysis of the data indicates that the object was active most of the time, and intraday variability was frequently observed. In total, the object varied by 2.614 mag in the i band. Strong bluer-when-brighter chromatism was observed on long, intermediate, and short timescales.

Dai Yan; Wu Jianghua; Zhu Zonghong; Wang Lingzhi [Department of Astronomy, Beijing Normal University, Beijing 100875 (China); Zhou Xu; Ma Jun [Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Beijing 100012 (China); Yuan Qirong, E-mail: zhuzh@bnu.edu.cn [Department of Physics and Institute of Theoretical Physics, Nanjing Normal University, Nanjing 210046 (China)

2013-02-15T23:59:59.000Z

478

15 colour photometry of Landolt SA95 standard star field  

E-Print Network [OSTI]

In this paper, we present a set of photometric observations in 15 colors of stars in the Landolt covered by the system range from 300 nm to 1000 nm. Visual magnitudes of the stars being studied in the field are from 10th to 20th mag. The observational methodology and the data reduction procedures are described. The relationships between the BATC intermediate-band system and the Landolt UBVRI broad band system are obtained. A catalogue of the photometry has been produced which contains the SEDs of 3613 stars. The electronic form of this catalogue can be accessed at the CDS via anonymous ftp to cdsarc.u-strasbg.fr.

Zhou, X; Ma, J; Xue, S; Wu, H; Chen, J; Zhu, J; Sun, W; Windhorst, R A; Zhou, Xu; Jiang, Zhaoji; Ma, Jun; Xue, Suijian; Wu, Hong; Chen, Jiansheng; Zhu, Jin; Sun, Weihsin; Windhorst, Rogier A.

2003-01-01T23:59:59.000Z

479

The distance modulus of the Large Magellanic Cloud: Constraints from RR Lyrae pulsation properties  

E-Print Network [OSTI]

It has recently been suggested that the discrepancy between the "long" and "short" distance moduli of the Large Magellanic Cloud (LMC), as inferred from the properties of the Cepheid and RR Lyrae variables, respectively, might be due to the action of "third parameters" between the Galaxy and the LMC, which would make the RR Lyraes in the old LMC globular clusters brighter than their Galactic counterparts by $\\simeq 0.3 {mag}$. Through analysis of the RR Lyrae pulsation properties, we show that this idea is not supported by the available data. A satisfactory explanation of the problem has yet to be found.

M. Catelan

1996-01-05T23:59:59.000Z

480

THE BROWN DWARF KINEMATICS PROJECT (BDKP). III. PARALLAXES FOR 70 ULTRACOOL DWARFS  

SciTech Connect (OSTI)

We report parallax measurements for 70 ultracool dwarfs (UCDs) including 11 late-M, 32 L, and 27 T dwarfs. In this sample, 14 M and L dwarfs exhibit low surface gravity features, 6 are close binary systems, and 2 are metal-poor subdwarfs. We combined our new measurements with 114 previously published UCD parallaxes and optical-mid-IR photometry to examine trends in spectral-type/absolute magnitude, and color-color diagrams. We report new polynomial relations between spectral type and M{sub JHK}. Including resolved L/T transition binaries in the relations, we find no reason to differentiate between a 'bright' (unresolved binary) and a 'faint' (single source) sample across the L/T boundary. Isolating early T dwarfs, we find that the brightening of T0-T4 sources is prominent in M{sub J} where there is a [1.2-1.4] mag difference. A similar yet dampened brightening of [0.3-0.5] mag happens at M{sub H} and a plateau or dimming of [-0.2 to -0.3] mag is seen in M{sub K} . Comparison with evolutionary models that vary gravity, metallicity, and cloud thickness verifies that for L into T dwarfs, decreasing cloud thickness reproduces brown dwarf near-IR color-magnitude diagrams. However we find that a near constant temperature of 1200 {+-}100 K along a narrow spectral subtype of T0-T4 is required to account for the brightening and color-magnitude diagram of the L-dwarf/T-dwarf transition. There is a significant population of both L and T dwarfs which are red or potentially 'ultra-cloudy' compared to the models, many of which are known to be young indicating a correlation between enhanced photospheric dust and youth. For the low surface gravity or young companion L dwarfs we find that 8 out of 10 are at least [0.2-1.0] mag underluminous in M{sub JH} and/or M{sub K} compared to equivalent spectral type objects. We speculate that this is a consequence of increased dust opacity and conclude that low surface gravity L dwarfs require a completely new spectral-type/absolute magnitude polynomial for analysis.

Faherty, Jacqueline K.; Shara, Michael M.; Cruz, Kelle L. [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10034 (United States); Burgasser, Adam J. [Center of Astrophysics and Space Sciences, Department of Physics, University of California, San Diego, CA 92093 (United States); Walter, Frederick M. [Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800 (United States); Van der Bliek, Nicole [CTIO/National Optical Astronomy Observatory (Chile); West, Andrew A. [Department of Astronomy, Boston University, 725 Commonwealth Ave Boston, MA 02215 (United States); Vrba, Frederick J. [US Naval Observatory, Flagstaff Station, P.O. Box 1149, Flagstaff, AZ 86002 (United States); Anglada-Escude, Guillem, E-mail: jfaherty@amnh.org [Department of Terrestrial Magnetism, Carnegie Institution of Washington 5241 Broad Branch Road, NW, Washington, DC 20015 (United States)

2012-06-10T23:59:59.000Z

Note: This page contains sample records for the topic "maldives mag m1" 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.


481

A robot manipulator calibration procedure with experimental verification  

E-Print Network [OSTI]

satisfy the following mag- nitude condition. U, . '+V, '+ V, . ' = I (2 g) If the X and Y components are chosen as the rotation parameters (ir and (u then U; = (n, Vis ? t', n (2. 9) Similarly if the X and Z components are chosen then U;?= ~1..., dz)] 0 1 0 dy dz 0 0 0 1 [Rot(6z, 6y, 6z)] 1 ? 6z by 0 6z 1 ? bz 0 -by bz 1 0 0 0 0 1 where dz, dy and dz are differences in the position components between the two poses along X, Y and Z axes in the nominal model end-effector kame. Similarly...

Padavala, Satya Srinivas

2012-06-07T23:59:59.000Z

482

The Secondary Star of the HgMn Binary Phi Her  

E-Print Network [OSTI]

The binary nature of the bright (V = 4.2 mag) Mercury-Manganese star Phi Her has been known since 1976 and it was considered a low-amplitude single-lined SB. In a recent study we found evidence for lines of the secondary star. Other recent results from interferometry provide a good measure of the light ratio. It is very plausible that the secondary is a late main-sequence A star. We find the rotational velocity of the secondary to be ~42 +/- 5 km/s.

M. M. Dworetsky; Rosemary Willatt

2006-12-15T23:59:59.000Z

483

An Overview of Operational Characteristics of Selected Irrigation Districts in the Texas Lower Rio Grande Valley: Harlingen Irrigation District Cameron County No. 1  

E-Print Network [OSTI]

the pumping facility, approximately 200 yards from the river. As indicated in Table 3, an insertion mag meter is used with each pump. The District?s records for these meters and totalizer information are submitted to the Watermaster who periodically... on Environmental Quality 2004). The Watermaster program is funded through flat rate and variable fees charged to water right holders within the Watermaster?s program area. The current annual flat rate (i.e., base) fee is $50.00 per water rights holder, plus...

Wolfe, Clint D.; Stubbs, Megan J.; Rister, M. Edward; Sturdivant, Allen W.; Lacewell, Ronald D.; Pennington, Ellen L.; Rogers, Callie S.

484

A priori Enclosures for ODEs: An Alternative to Fixed Point Iterations  

E-Print Network [OSTI]

of Recurrence Relation I. Required: i mi i + 2, Bi 0 so that |bij| Bi P(j - mi, mi)rj for all j > mi. II n-1 i=0 mi j=0 rn-i+j P ( - j, i) |bij| P (, n) + B-1 rn+m-1 P ( - m-1, m-1 + n) +n-1 max =0 |a r | + n-1 i=0 Bi rn+mi-i P (, n) (-1)i+1 i! P (mi - 2 - i, i + 1) P ( - mi + 1 + i, mi - 1 - i) + i-1 =0

485

Information et Codage Leon IV. Codage entropique  

E-Print Network [OSTI]

mot de code ci , et la distribution des longueurs du code VLC est donc {l1,...,lM }. 1. Minimiser leM . page 1 #12;1. Montrer que nécessairement l1 l2 ··· lM . Commenter. Indication : Raisonner par l remplacer lM par lM -1. 3. Déduire du raisonnement de la question précédente que lM-1 = lM , et qu'on peut

Rioul, Olivier

486

A Wnt1 Regulated Frizzled-1/beta-Catenin Signaling Pathway as a Candidate Regulatory Circuit Controlling Mesencephalic Dopaminergic Neuron-Astrocyte Crosstalk : Therapeutical Relevance for Neuron Survival and Neuroprotection  

E-Print Network [OSTI]

M) of the DA-specific neurotoxins, 6-hydroxydopamine (6-OHDA), or the active metabolite of MPTP, 1-methyl-4-phenyl-1,2,3,6- tetrahydropyridine (MPP+). For antagonism studies, we used Dickkopf-1 (Dkk-1, R&D Systems, MN, USA 100 ng/ml). Dkk-1 is a high... designed a duplicate assay and b-actin was used exclusively as the housekeeping gene. The assay IDs were: Fzd-1, Mm00445405_s1; Fzd-2, Mm012504981_s1; Fzd-3, Mm00445423_m1; Fzd-4, Mm00433382_m1; Fzd- 5, Mm03053323_s1; Fzd-6, Mm00433383_M1; Fzd-7, Mm01255614...

L'Episcopo, Francesca; Serapide, Maria F; Tirolo, Cataldo; Testa, Nunzio; Caniglia, Salvatore; Morale, Maria C; Pluchino, Stefano; Marchetti, Bianca

2011-07-13T23:59:59.000Z

487

Tunable quantum beam splitters for coherent manipulation of a solid-state tripartite qubit system  

E-Print Network [OSTI]

are lines of constant characteristic sweeping rates, ? 1 and ? 2 , defi ned in the text. The white circles mark the hot spots , where the interference fringes generated by M 2 tend to fade out and the interference fringes generated by M 1 dominate... disappear (the fringes tend to fade out) and the interference fringes generated by M 1 dominate, displayed as a chain of hot spots marked by the circles in Figure 2a . When both M 1 and M 2 can be treated as beam splitters, all three paths (1...

Sun, Guozhu; Wen, Xueda; Mao, Bo; Chen, Jian; Yu, Yang; Wu, Peiheng; Han, Siyuan

2010-08-10T23:59:59.000Z

488

Diversity in extinction laws of Type Ia supernovae measured between $0.2$ and $2\\,\\mu\\mathrm{m}$  

E-Print Network [OSTI]

We present ultraviolet (UV) observations of six nearby Type~Ia supernovae (SNe~Ia) obtained with the Hubble Space Telescope, three of which were also observed in the near-IR (NIR) with Wide-Field Camera~3. UV observations with the Swift satellite, as well as ground-based optical and near-infrared data provide complementary information. The combined data-set covers the wavelength range $0.2$--$2~\\mu$m. By also including archival data of SN 2014J, we analyse a sample spanning observed colour excesses up to $E(B-V)=1.4~$mag. We study the wavelength dependent extinction of each individual SN and find a diversity of reddening laws when characterised by the total-to-selective extinction $R_V$. In particular, we note that for the two SNe with $E(B-V)\\gtrsim1~$mag, for which the colour excess is dominated by dust extinction, we find $R_V=1.4\\pm0.1$ and $R_V=2.8\\pm0.1$. Adding UV photometry reduces the uncertainty of fitted $R_V$ by $\\sim50\\,$% allowing us to also measure $R_V$ of individual low-extinction objects whi...

Amanullah, R; Goobar, A; Ferretti, R; Papadogiannakis, S; Petrushevska, T; Brown, P J; Cao, Y; Contreras, C; Dahle, H; Elias-Rosa, N; Fynbo, J P U; Gorosabel, J; Guaita, L; Hangard, L; Howell, D A; Hsiao, E Y; Kankare, E; Kasliwal, M; Leloudas, G; Lundqvist, P; Mattila, S; Nugent, P; Phillips, M M; Sandberg, A; Stanishev, V; Sullivan, M; Taddia, F; stlin, G; Asadi, S; Herrero-Illana, R; Jensen, J J; Karhunen, K; Lazarevi, S; Varenius, E; Santos, P; Sridhar, S Seethapuram; Wallstrm, S H J; Wiegert, J

2015-01-01T23:59:59.000Z

489

THE METALLICITY DEPENDENCE OF THE CEPHEID P L RELATION IN M101  

SciTech Connect (OSTI)

The impact of metallicity on the Cepheid period-luminosity (P L) relation is investigated using Hubble Space Telescope Advanced Camera for Surveys V and I images of M101. Variations in the reddening-free Wesenheit parameter (W), which is employed as a proxy for luminosity, are examined as a function of the radial distance from the center of M101 (and thus metallicity). We determine that there is no dependence of the slope on metallicity. However, the intercept is found to depend on metallicity by ?{sub VI} = 0.33 0.12 mag dex{sup 1} and ?{sub VI} = 0.71 0.17 mag dex{sup 1} using 2? and 3? rejection criteria, respectively. Sigma-clipping impacts the derived metallicity dependence, and the 2? criterion applied likely mitigates blending, particularly in the crowded inner regions of M101. A metallicity-corrected distance for M101 is obtained from 619 Cepheids (? = 28.96 0.11), a result that agrees with the recently determined SN Ia distance. The metallicity effects described can be bypassed by working at near and mid-infrared wavelengths (e.g., the Carnegie Hubble Program)

Mager, Violet A.; Madore, Barry F.; Freedman, Wendy L., E-mail: mager@susqu.edu, E-mail: barry@obs.carnegiescience.edu, E-mail: wendy@obs.carnegiescience.edu [Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)

2013-11-01T23:59:59.000Z

490

The magnification of SN 1997ff, the farthest known supernova  

SciTech Connect (OSTI)

With a redshift of z {approx} 1.7, SN 1997ff is the most distant type Ia supernova discovered so far. This SN is close to several bright, z = 0.6-0.9 galaxies, and we consider the effects of lensing by those objects on the magnitude of SN 1997ff. We estimate their velocity dispersions using the Tully-Fisher and Faber-Jackson relations corrected for evolution effects, and calculate, applying the multiple-plane lensing formalism, that SN 1997ff is magnified by 0.34{+-}0.12 mag. Due to the spatial configuration of the foreground galaxies, the shear from individual lenses partially cancels out,and the total distortion induced on the host galaxy is considerably smaller than that produced by a single lens having the same magnification. After correction for lensing, the revised distance to SN 1997ff is m-M = 45.49 {+-} 0.34 mag, which improves the agreement with the {Omega}{sub M} = 0.35, {Omega}{Lambda} = 0.65 cosmology expected from lower-redshift SNe Ia, and is inconsistent at the {approx} 3 sigma confidence level with a uniform gray dust model or a simple evolution model.

Benitez, Narciso; Riess, Adam; Nugent, Peter; Dickinson, Mark; Chornock, Ryan; Filippenko, Alexei V.

2002-09-03T23:59:59.000Z

491

A constellation of CubeSats with synthetic tracking cameras to search for 90% of potentially hazardous near-Earth objects  

E-Print Network [OSTI]

Congress mandated NASA to find 90% of near-Earth objects (NEO) with sizes over 140m that are potentially hazardous to the Earth by the year 2020. After an in-depth look at a number of alternative approaches, the National Research Council (NRC) concluded in 2010 that this goal was nearly impossible to reach by 2020. In this paper, we present a new space mission concept that is capable of addressing the challenges of this Congressional mandate. The proposed mission concept relies on two emerging technologies: the technique of synthetic tracking to detect NEOs and the new generation of small and capable interplanetary spacecraft. Synthetic tracking is a technique that de-streaks asteroid images by taking multiple fast exposures. With synthetic tracking, a 600 sec observation with a 10cm telescope, which can fit in a CubeSat, can detect a 20.5 mag moving object without losing sensitivity from streaking. Our primary science objective is to detect, track, catalogue, and characterize 90% of NEAs of H=22 mag (diamete...

Shao, Michael; Spangelo, Sara; Werne, Thomas

2015-01-01T23:59:59.000Z

492

A Deep, Wide-Field Study of Holmberg II with Suprime-Cam: Evidence for Ram Pressure Stripping  

E-Print Network [OSTI]

We present a deep, wide-field optical study of the M81 group dwarf galaxy Holmberg II (HoII) based on Subaru/Suprime-Cam imaging. Individual stars are resolved down to I~25.2, i.e. about 1.5 mag below the tip of the red giant branch (RGB). We use resolved star counts in the outskirts of the galaxy to measure the radial surface brightness profile down to \\mu_V~32 mag arcsec^-2, from which we determine a projected exponential scalelength of 0.70'+-0.01' (i.e. 0.69+-0.01 kpc). The composite profile, ranging from the cored centre out to R=7', is best fit by an EFF profile which gives a half-light radius of 1.41'+-0.04' (i.e. 1.39+-0.04 kpc), and an absolute magnitude M_V=-16.3. The low surface-brightness stellar component of HoII is regular and symmetric and has an extent much smaller than the vast HI cloud in which it is embedded. We compare the spatial distribution of the young, intermediate age, and old stellar populations, and find that the old RGB stars are significantly more centrally concentrated than the ...

Bernard, Edouard J; Barker, Michael K; Irwin, Michael J; Jablonka, Pascale; Arimoto, Nobuo

2012-01-01T23:59:59.000Z

493

Stellar Populations in the Central 0.5 pc of the Galaxy I: A New Method for Constructing Luminosity Functions and Surface-Density Profiles  

E-Print Network [OSTI]

We present new high angular resolution near-infrared spectroscopic observations of the nuclear star cluster surrounding the Milky Way's central supermassive black hole. Using the integral-field spectrograph OSIRIS on Keck II behind the laser-guide-star adaptive optics system, this spectroscopic survey enables us to separate early-type (young, 4-6 Myr) and late-type (old, >1 Gyr) stars with a completeness of 50% down to K' = 15.5 mag, which corresponds to ~10 \\msun for the early-type stars. This work increases the radial extent of reported OSIRIS/Keck measurements by more than a factor of 3 from 4" to 14" (0.16 pc to 0.56 pc), along the projected disk of young stars. For our analysis, we implement a new method of completeness correction using a combination of star-planting simulations and Bayesian inference. We assign probabilities for the spectral type of every source detected in deep imaging down to K' = 15.5 mag using information from spectra, simulations, number counts, and the distribution of stars. The i...

Do, Tuan; Ghez, Andrea M; Morris, Mark R; Yelda, Sylvana; Martinez, Gregory D; Wright, Shelley A; Matthews, Keith

2013-01-01T23:59:59.000Z

494

X-ray Flashes or soft Gamma-ray Bursts? The case of the likely distant XRF 040912  

E-Print Network [OSTI]

In this work, we present a multi-wavelength study of XRF 040912, aimed at measuring its distance scale and the intrinsic burst properties. We performed a detailed spectral and temporal analysis of both the prompt and the afterglow emission and we estimated the distance scale of the likely host galaxy. We then used the currently available sample of XRFs with known distance to discuss the connection between XRFs and classical Gamma-ray Bursts (GRBs). We found that the prompt emission properties unambiguously identify this burst as an XRF, with an observed peak energy of E_p=17+/-13 keV and a burst fluence ratio S(2-30keV)/S(30-400keV)>1. A non-fading optical source with R~24 mag and with an apparently extended morphology is spatially consistent with the X-ray afterglow, likely the host galaxy. XRF 040912 is a very dark burst since no afterglow optical counterpart is detected down to R>25 mag (3 sigma limiting magnitude) at 13.6 hours after the burst. The host galaxy spectrum detected from 3800A to 10000A, shows...

Stratta, G; Butler, N; Atteia, J L; Gendre, B; Pelangeon, A; Malacrino, F; Mellier, Y; Kann, D A; Klose, S; Zeh, A; Masetti, N; Palazzi, E; Gorosabel, J; Castro-Tirado, A J; De Postigo, A U; Jelinek, M; Cepa, J; Castaneda, H; Martnez-Delgado, D; Bor, M; Braga, J; Crew, G; Donaghy, T Q; Dezalay, J P; Doty, J; Fenimore, E E; Galassi, M; Graziani, C; Jernigan, J G; Kawai, N; Lamb, D Q; Levine, A; Manchanda, J; Martel, F; Matsuoka, M; Nakagawa, Y; Olive, J F; Pizzichini, G; Prigozhin, G Y; Ricker, G; Sakamoto, T; Shirasaki, Y; Sugita, S; Suzuki, M; Takagishi, K; Tamagawa, T; Vanderspek, R; Villasenor, J; Woosley, S E; Yamauchi, M; Yoshida, A

2006-01-01T23:59:59.000Z

495

Variable stars in the newly discovered Milky Way satellite in Bootes  

E-Print Network [OSTI]

We present $V,I$ light curves for 12 variable stars identified in the newly discovered satellite of the Milky Way in the Bootes constellation (Belokurov et al. 2006).Our sample includes 11 RR Lyrae stars (5 first overtone, 5 fundamental mode and 1 double mode pulsator),and one long period variable close to the galaxy red giant branch tip. The RR Lyrae stars trace very well the average $V$ luminosity of the galaxy horizontal branch, leading to a true distance modulus for the galaxy of $\\mu_0$=19.11 $\\pm$ 0.08 mag for an assumed metal abundance of [Fe/H]=-2.5 (Monoz et al. 2006), and for $E(B-V)$=0.02 mag. Average periods are =0.69 d and =0.37 d for {\\it ab-} and {\\it c-} type RR Lyrae stars, respectively, making of Bootes the second pure Oosterhoff type II (OoII) dSph after Ursa Minor. The location of the double mode RR Lyrae (RRd) in the Petersen diagram is consistent with RRd stars in OoII clusters, and corresponds to an intrinsic luminosity of $log L/logL\\odot$=1.72 (for Z=10$^{-4}$ and M=0.80 M$\\odot$) according to Bono et al. (1996) pulsation models.

M. Dall'Ora; G. Clementini; K. Kinemuchi; V. Ripepi; M. Marconi; L. Di Fabrizio; C. Greco; C. T. Rodgers; C. Kuehn; H. A. Smith

2006-11-09T23:59:59.000Z

496

Near-infrared low-resolution spectroscopy of Pleiades L-type brown dwarfs  

E-Print Network [OSTI]

The fundamental properties of brown dwarfs evolve with age. Models describing the evolution of luminosities and effective temperatures, among other physical parameters, can be empirically constrained using brown dwarfs of various masses in star clusters of well determined age and metallicity. We aim to carry out a spectroscopic and photometric characterization of low-mass brown dwarfs of the ~120 Myr old Pleiades open cluster. We obtained low-resolution near-infrared spectra of the J=17.4-18.8 mag candidate L-type brown dwarfs PLIZ 28 and 35, BRB 17, 21, 23, and 29, which are Pleiades members by photometry and proper motion. We also obtained spectra of the well-known J=15.4-16.1 mag late M-type cluster members PPl 1, Teide 1, and Calar 3. We find that the former six objects have early- to mid-L spectral types and confirm previously reported M-types for the other three objects. The spectra of the L0-type BRB 17 and PLIZ 28 present a triangular H-band continuum shape and remarkable VO absorption, indicating tha...

Bihain, G; Osorio, M R Zapatero; Bjar, V J S; Caballero, J A

2010-01-01T23:59:59.000Z

497

Lick Northern Proper Motion Program. III. Lick NPM2 Catalog  

E-Print Network [OSTI]

The Lick Northern Proper Motion (NPM) program, a two-epoch (1947-1988) photographic survey of the northern two-thirds of the sky (Dec. > -23 deg), has measured absolute proper motions, on an inertial system defined by distant galaxies, for 380,000 stars from 8 14) anonymous stars for astrometry and galactic studies, 92,000 bright (B NPM2 proper motions are on the ICRS system, via Tycho-2 stars, to an accuracy of 0.5 mas/yr in each field. RMS proper motion precision is 6 mas/yr. Positional errors average 80 mas at the mean plate epoch 1968, and 200 mas at the NPM2 catalog epoch 2000. NPM2 photographic photometry errors average 0.18 mag in B, and 0.20 mag in B-V. The NPM2 Catalog and the updated (to J2000) NPM1 Catalog are available at the CDS Strasbourg data center and on the NPM WWW site (http://www.ucolick.org/~npm). The NPM2 Catalog completes the Lick Northern Proper Motion program after a half-century of w...

Hanson, R B; Jones, B F; Monet, D G; Hanson, Robert B.; Klemola, Arnold R.; Jones, Burton F.; Monet, David G.

2004-01-01T23:59:59.000Z

498

A LIKELY CLOSE-IN LOW-MASS STELLAR COMPANION TO THE TRANSITIONAL DISK STAR HD 142527  

SciTech Connect (OSTI)

With the uniquely high contrast within 0.''1 ({Delta}mag(L') = 5-6.5 mag) available using Sparse Aperture Masking with NACO at Very Large Telescope, we detected asymmetry in the flux from the Herbig Fe star HD 142527 with a barycenter emission situated at a projected separation of 88 {+-} 5 mas (12.8 {+-} 1.5 AU at 145 pc) and flux ratios in H, K, and L' of 0.016 {+-} 0.007, 0.012 {+-} 0.008, and 0.0086 {+-} 0.0011, respectively (3{sigma} errors), relative to the primary star and disk. After extensive closure-phase modeling, we interpret this detection as a close-in, low-mass stellar companion with an estimated mass of {approx}0.1-0.4 M{sub Sun }. HD 142527 has a complex disk structure, with an inner gap imaged in both the near and mid-IR as well as a spiral feature in the outer disk in the near-IR. This newly detected low-mass stellar companion may provide a critical explanation of the observed disk structure.

Biller, Beth; Benisty, Myriam; Chauvin, Gael; Olofsson, Johan; Pott, Joerg-Uwe; Mueller, Andre; Bonnefoy, Mickaeel; Henning, Thomas [Max-Planck-Institut fuer Astronomie, Koenigstuhl 17, 69117 Heidelberg (Germany); Lacour, Sylvestre; Thebault, Philippe [LESIA, CNRS/UMR-8109, Observatoire de Paris, UPMC, Universite Paris Diderot, 5 place Jules Janssen, 92195 Meudon (France); Juhasz, Attila [Leiden Observatory, Leiden University, P.O. Box 9513, 2300 RA Leiden (Netherlands); Sicilia-Aguilar, Aurora [Departamento de Fisica Teorica, Facultad de Ciencias, Universidad Autonoma de Madrid, 28049 Cantoblanco, Madrid (Spain); Tuthill, Peter [School of Physics, University of Sydney, NSW 2006 (Australia); Crida, Aurelien, E-mail: biller@mpia.de [Universite de Nice - Sophia antipolis/C.N.R.S./Observatoire de la Cote d'Azur, Laboratoire Lagrange (UMR 7293), Boulevard de l'Observatoire, B.P. 4229 06304 NICE cedex 04 (France)

2012-07-10T23:59:59.000Z

499

Near-Infrared Detection and Characterization of the Exoplanet HD 95086 b with the Gemini Planet Imager  

E-Print Network [OSTI]

HD 95086 is an intermediate-mass debris-disk-bearing star. VLT/NaCo $3.8 \\mu m$ observations revealed it hosts a $5\\pm2 \\mathrm{M}_{Jup}$ companion (HD 95086 b) at $\\simeq 56$ AU. Follow-up observations at 1.66 and 2.18 $\\mu m$ yielded a null detection, suggesting extremely red colors for the planet and the need for deeper direct-imaging data. In this Letter, we report H- ($1.7 \\mu m$) and $\\mathrm{K}_1$- ($2.05 \\mu m$) band detections of HD 95086 b from Gemini Planet Imager (GPI) commissioning observations taken by the GPI team. The planet position in both spectral channels is consistent with the NaCo measurements and we confirm it to be comoving. Our photometry yields colors of H-L'= $3.6\\pm 1.0$ mag and K$_1$-L'=$2.4\\pm 0.7$ mag, consistent with previously reported 5-$\\sigma$ upper limits in H and Ks. The photometry of HD 95086 b best matches that of 2M 1207 b and HR 8799 cde. Comparing its spectral energy distribution with the BT-SETTL and LESIA planet atmospheric models yields T$_{\\mathrm{eff}}\\sim$600-1...

Galicher, Raphael; Bonnefoy, Mickael; Baudino, Jean-Loup; Currie, Thayne; Boccaletti, Anthony; Chauvin, Gael; Lagrange, Anne-Marie; Marois, Christian

2014-01-01T23:59:59.000Z

500

DETAILED INTERSTELLAR POLARIMETRIC PROPERTIES OF THE PIPE NEBULA AT CORE SCALES  

SciTech Connect (OSTI)

We use R-band CCD linear polarimetry collected for about 12,000 background field stars in 46 fields of view toward the Pipe nebula to investigate the properties of the polarization across this dark cloud. Based on archival Two Micron All Sky Survey data, we estimate that the surveyed areas present total visual extinctions in the range 0.6 mag {<=} A{sub V} {<=} 4.6 mag. While the observed polarizations show a well-ordered large-scale pattern, with polarization vectors almost perpendicularly aligned to the cloud's long axis, at core scales one sees details that are characteristics of each core. Although many observed stars present degrees of polarization that are unusual for the common interstellar medium (ISM), our analysis suggests that the dust grains constituting the diffuse parts of the Pipe nebula seem to have the same properties as the normal Galactic ISM. Estimates of the second-order structure function of the polarization angles suggest that most of the Pipe nebula is magnetically dominated and that turbulence is sub-Alvenic. The Pipe nebula is certainly an interesting region to investigate the processes that prevailed during the initial phases of low-mass stellar formation.

Franco, G. A. P. [Departamento de Fisica-ICEx-UFMG, Caixa Postal 702, 30.123-970 Belo Horizonte (Brazil); Alves, F. O.; Girart, J. M., E-mail: franco@fisica.ufmg.b [Institut de Ciencies de l'Espai (CSIC-IEEC), Campus UAB-Facultat de Ciencies, Torre C5-Parell 2a, 08193 Bellaterra, Catalunya (Spain)

2010-11-01T23:59:59.000Z