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they are not comprehensive nor are they the most current set.
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1

Recollection 1965-1971: The Groningen High Latitude Survey  

E-Print Network [OSTI]

Recollection 1965-1971: The Groningen High Latitude Survey Istv├ín Fejes F├?MI Satellite Geodetic to Groningen #12;The new WSN 1970 #12;Wesselius and Fejes, 1970 #12;GHLS: The first colored contour map Low

Peletier, Reynier

2

Conjugate High Latitude Measurements along the 40 Magnetic Meridian  

E-Print Network [OSTI]

Conjugate High Latitude Measurements along the 40┬║ Magnetic Meridian: Autonomous Adaptive Low the 2014 season marked as red squares. #12;Autonomous Adaptive Low-Power Instrument #12;Conjugate observations of Travelling Convection Vorticies produced by solar wind pressure

Michigan, University of

3

High-latitude ionospheric response to co-rotating interaction region- and coronal mass ejection-driven geomagnetic storms revealed by GPS tomography and ionosondes  

Science Journals Connector (OSTI)

...New Brunswick, Canada E3B 5A3 2 Department...ionosonde data with solar wind measurements...Arctic region of Canada. 2. Geomagnetic...et al. (2007). Solar wind parameters including...Research Council of Canada. The UK authors...for providing the solar wind data and geomagnetic...

2010-01-01T23:59:59.000Z

4

High-Latitude Ocean and Sea Ice Surface Fluxes: Requirements and Challenges for Climate Mark Bourassa1  

E-Print Network [OSTI]

temperatures, seasonal sea ice, and the remoteness of the regions all conspire to make observations difficult latitudes - the vertical exchanges of heat, momentum and material between the ocean, atmosphere and ice1 High-Latitude Ocean and Sea Ice Surface Fluxes: Requirements and Challenges for Climate Research

Gille, Sarah T.

5

Latitude Based Model for Tilt Angle Optimization for Solar Collectors in the Mediterranean Region  

Science Journals Connector (OSTI)

Abstract This paper inspects the different parameters that intervene in the determination of the optimal tilt angle for maximum solar energy collection. It proposes a method for calculating the optimal tilt angle based upon the values of the daily global solar radiation on a horizontal surface. A computer program using the mathematical model to calculate the solar radiation incident on an inclined surface as a function of the tilt angle is implemented. Four years data of daily global solar radiation on a horizontal surface in 35 sites in different countries of the Mediterranean region is used. The program assumes a due south orientation of the collectors and it determines the optimal tilt angle for maximum solar radiation collection for sites in the Mediterranean region. A regression analysis using the results of the computer simulation is conducted to develop a latitude based tilt angle optimization mathematical model for maximum solar radiation collection for the sites. We tested both a linear and a quadratic model (of the form ax2+bx) for representing the relationship between the annual optimal tilt angle and the site's latitude. The quadratic model is better; it provides very high prediction accuracy. 99.87% of the variation in the annual optimal tilt angle is explained by the variability in site's latitude with an average residual angle of only 0.96░ for all 35 sites studied. It also gives an average percentage decrease in the annual solar radiation of only 0.016% when compared with actual optimal tilt angles.

Hassane Darhmaoui; Driss Lahjouji

2013-01-01T23:59:59.000Z

6

PoGOLite: Neutron Background Studies for High Latitudes  

E-Print Network [OSTI]

PoGOLite: Neutron Background Studies for High Latitudes Maria Fernanda Mu├▒oz Salinas SH2006. The measurements showed a neutron background ten times higher than expected. Because of this, new simulations of the PoGOLite flight which will take place in the summer of 2012. The neutron background was simulated

Haviland, David

7

Latitude Distribution of Interplanetary Magnetic Field Lines Rooted in Active Regions  

Science Journals Connector (OSTI)

Electrons, accelerated in solar active regions to ? 10 keV, escape along open magnetic field lines and generate plasma radiation (Type III bursts ... Here we describe the latitude distribution of the field lines ...

G. A. Dulk; J. L. Steinberg; S. Hoangů

1986-01-01T23:59:59.000Z

8

E-Print Network 3.0 - amplify high-latitude warming Sample Search...  

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

high latitudes, more than low albedo, helped main- tain the warm... of equilibrium, the loss of heat in high latitudes--mainly where cold continental air masses flow over the...

9

SIMULATED FARADAY ROTATION MEASURES TOWARD HIGH GALACTIC LATITUDES  

SciTech Connect (OSTI)

We study the Faraday rotation measure (RM) due to the Galactic magnetic field (GMF) toward high Galactic latitudes. The RM arises from the global, regular component as well as from the turbulent, random component of the GMF. We model the former based on observations and the latter using the data of magnetohydrodynamic turbulence simulations. For a large number of different GMF models, we produce mock RM maps around the Galactic poles and calculate various statistical quantities with the RM maps. We find that the observed medians of RMs toward the north and south Galactic poles, {approx}0.0 {+-} 0.5 rad m{sup -2} and {approx} + 6.3 {+-} 0.5 rad m{sup -2}, are difficult to explain with any of our many alternate GMF models. The standard deviation of observed RMs, {approx}9 rad m{sup -2}, is clearly larger than that of simulated RMs. The second-order structure function of observed RMs is substantially larger than that of simulated RMs, especially at small angular scales. We discuss other possible contributions to RM toward high Galactic latitudes. Besides observational errors and the intrinsic RM of background radio sources against which RM is observed, we suggest that the RM due to the intergalactic magnetic field may account for a substantial fraction of the observed RM. Finally, we note that reproducing the observed medians may require additional components or/and structures of the GMF that are not present in our models.

Akahori, Takuya; Kim, Jongsoo [Korea Astronomy and Space Science Institute, Daedeokdaero 776, Yuseong-Gu, Daejeon 305-348 (Korea, Republic of); Ryu, Dongsu [Department of Astronomy and Space Science, Chungnam National University, Daejeon 305-764 (Korea, Republic of); Gaensler, B. M., E-mail: jskim@kasi.re.kr, E-mail: akahori@physics.usyd.edu.au, E-mail: bryan.gaensler@sydney.edu.au, E-mail: ryu@canopus.cnu.ac.kr [Sydney Institute for Astronomy, School of Physics, University of Sydney, NSW 2006 (Australia)

2013-04-20T23:59:59.000Z

10

MEASUREMENTS OF THE SUN'S HIGH-LATITUDE MERIDIONAL CIRCULATION  

SciTech Connect (OSTI)

The meridional circulation at high latitudes is crucial to the buildup and reversal of the Sun's polar magnetic fields. Here, we characterize the axisymmetric flows by applying a magnetic feature cross-correlation procedure to high-resolution magnetograms obtained by the Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Observatory. We focus on Carrington rotations 2096-2107 (2010 April to 2011 March)-the overlap interval between HMI and the Michelson Doppler Imager (MDI). HMI magnetograms averaged over 720 s are first mapped into heliographic coordinates. Strips from these maps are then cross-correlated to determine the distances in latitude and longitude that the magnetic element pattern has moved, thus providing meridional flow and differential rotation velocities for each rotation of the Sun. Flow velocities were averaged for the overlap interval and compared to results obtained from MDI data. This comparison indicates that these HMI images are rotated counterclockwise by 0.{sup 0}075 with respect to the Sun's rotation axis. The profiles indicate that HMI data can be used to reliably measure these axisymmetric flow velocities to at least within 5 Degree-Sign of the poles. Unlike the noisier MDI measurements, no evidence of a meridional flow counter-cell is seen in either hemisphere with the HMI measurements: poleward flow continues all the way to the poles. Slight north-south asymmetries are observed in the meridional flow. These asymmetries should contribute to the observed asymmetries in the polar fields and the timing of their reversals.

Rightmire-Upton, Lisa [Department of Physics, University of Alabama in Huntsville, Huntsville, AL 35899 (United States); Hathaway, David H. [NASA Marshall Space Flight Center, Huntsville, AL 35812 (United States); Kosak, Katie, E-mail: lar0009@uah.edu, E-mail: david.hathaway@nasa.gov, E-mail: mkosak2011@my.fit.edu [Florida Institute of Technology, Melbourne, FL 32901 (United States)

2012-12-10T23:59:59.000Z

11

Energetic particles and coronal mass ejections in the high latitude heliosphere: Ulysses-LET observations  

SciTech Connect (OSTI)

We have investigated energetic ions of non-corotating nature in the high latitude heliosphere. Major particle events were observed by Ulysses up to latitudes of 60 deg. S. All were associated with passage of coronal mass ejections (CMEs) over the spacecraft. The relationship of these events with solar activity was investigated using Yohkoh soft X-ray images.

Bothmer, V.; Marsden, R. G.; Sanderson, T. R.; Trattner, K. J.; Wenzel, K.-P.; Balogh, A.; Forsyth, R. J.; Goldstein, B. E.; Uchida, Y.; Hudson, H. S. [Space Science Department of ESA, ESTEC, Noordwijk (Netherlands); Blackett Laboratory, Imperial College, London (United Kingdom); Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California (United States); Physics Department, Science University, Tokyo (Japan); Institute for Astronomy, University of Hawaii, Honolulu, Hawaii (United States)

1996-07-20T23:59:59.000Z

12

The Masses Of The B-Stars In The High Galactic Latitude Eclipsing Binary IT Lib  

E-Print Network [OSTI]

A number of blue stars which appear to be similar to Population I B-stars in the star forming regions of the galactic disk are found more than 1 kpc from the galactic plane. Uncertainties about the true distances and masses of these high latitude B-stars has fueled a debate as to their origin and evolutionary status. The eclipsing binary IT Lib is composed of two B-stars, is approximately one kiloparsec above the galactic plane, and is moving back toward the plane. Observations of the light and velocity curves presented here lead to the conclusion that the B-stars in this system are massive young main-sequence stars. While there are several possible explanations, it appears most plausible that the IT Lib system formed in the disk about 30 million years ago and was ejected on a trajectory taking it to its present position.

John C. Martin

2002-10-28T23:59:59.000Z

13

High-latitude eruptions cast shadow over the African monsoon and the flow of the Nile  

E-Print Network [OSTI]

the Sahel of Africa, thus producing the low Nile flow. Future high-latitude eruptions would significantly, p. 120]. By January 1785, 1/6 of the population of Egypt had either died or left the country of Asia and North America. Recon- structed summer temperatures using tree ring maximum latewood density

Stenchikov, Georgiy L.

14

A climatology of cold air outbreaks and their impact on air-sea heat fluxes in the high-latitude South Pacific  

Science Journals Connector (OSTI)

A climatology of cold air outbreaks (CAOs) in the high-latitudes of the South Pacific and an analysis of the dynamical mechanisms leading to their formation are presented. Two major and distinct regions with frequent CAOs from autumn to spring are ...

Lukas Papritz; Stephan Pfahl; Harald Sodemann; Heini Wernli

15

EDIA-EISCAT comparison between small scale F-region irregularities and large scale electron density structures at sub-auroral latitudes  

Science Journals Connector (OSTI)

Small scale sub-auroral F-region irregularities were observed on 6ľ7 February 1984 by the two HF radars of the EDIA experiment while the EISCAT UHF system was scanning the ionosphere between 57░ and 66░ invariant latitude at a slightly different longitude. The bistatic EDIA system was mainly designed to detect the F-region irregularities at sub-auroral latitudes and to measure their perpendicular velocities. This paper is devoted to an examination of the morphology of the irregularity regions detected by the HF radars and of their production mechanisms, by comparison with the horizontal and vertical electron density profiles measured by EISCAT. It is shown that decametric irregularities observed at about 360ľ430 km height are not associated with any large scale horizontal density gradients in the F-region (350km). However, a strong north-south gradient observed at lower altitudes (150ľ200km), which is likely to indicate the southern boundary of the high energy particle precipitation zone, is well correlated with the strong scattering regions observed by the HF radars. The EISCAT electron temperature measurements at 350km height also show horizontal gradients which are well correlated with the small scale F-region irregularities. We discuss implications of these observations on the mechanisms of production of irregularities in the sub-auroral F-region.

A. Bourdillon; D. Fontaine

1988-01-01T23:59:59.000Z

16

High-Latitude Ocean and Sea Ice Surface Fluxes: Challenges for Climate Research1 Mark A. Bourassa1  

E-Print Network [OSTI]

), and in 2008, the Wilkins Ice Shelf51 collapsed equally quickly (Scambos et al. 2009). Ocean heat content1 High-Latitude Ocean and Sea Ice Surface Fluxes: Challenges for Climate Research1 2 Mark A-latitude surface fluxes will require close collaboration among meteorologists,33 oceanographers, ice physicists

Gille, Sarah T.

17

A GCM Parameterization of Ice Particle Mean Effective Sizes for High Latitude Cirrus Clouds and It's Comparison with Mid-Latitude Parmaterization  

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

GCM Parameterization of Ice Particle Mean Effective GCM Parameterization of Ice Particle Mean Effective Sizes for High Latitude Cirrus Clouds and It's Comparison with Mid-Latitude Parameterization F. S. Boudala Department of Oceanography Dalhousie University Halifax, Nova Scotia, Canada Q. Fu Department of Atmospheric Sciences University of Washington Seattle, Washington G. A. Issac Meteorological Service of Canada Toronto, Ontario, Canada Introduction Single-scattering properties of ice clouds depend on both ice water content (IWC) and effective size of cloud particles (Fu 1996; Fu et al. 1998). However, only the IWC information is provided in numerical models. Stephens et al. (1990) showed that the ice cloud feedback on a CO 2 warming simulation could be either positive or negative depending on the value of the ice particle size assumed. Parameterizations

18

On the Representation of High-Latitude Boundary Layer Mixed-Phase Cloud in the ECMWF Global Model  

Science Journals Connector (OSTI)

Supercooled liquid water (SLW) layers in boundary layer clouds are abundantly observed in the atmosphere at high latitudes, but remain a challenge to represent in numerical weather prediction (NWP) and climate models. Unresolved processes such as ...

Richard M. Forbes; Maike Ahlgrimm

2014-09-01T23:59:59.000Z

19

Uncertainty analysis of vegetation distribution in the northern high latitudes during the 21st century with a dynamic vegetation model  

E-Print Network [OSTI]

This study aims to assess how high-latitude vegetation may respond under various climate scenarios during the 21st century with a focus on analyzing model parameters induced uncertainty and how this uncertainty compares ...

Jiang, Yueyang

20

LOW-LATITUDE CORONAL HOLES, DECAYING ACTIVE REGIONS, AND GLOBAL CORONAL MAGNETIC STRUCTURE  

SciTech Connect (OSTI)

We study the relationship between decaying active-region magnetic fields, coronal holes, and the global coronal magnetic structure using Global Oscillations Network Group synoptic magnetograms, Solar TErrestrial RElations Observatory extreme-ultraviolet synoptic maps, and coronal potential-field source-surface models. We analyze 14 decaying regions and associated coronal holes occurring between early 2007 and late 2010, 4 from cycle 23 and 10 from cycle 24. We investigate the relationship between asymmetries in active regions' positive and negative magnetic intensities, asymmetric magnetic decay rates, flux imbalances, global field structure, and coronal hole formation. Whereas new emerging active regions caused changes in the large-scale coronal field, the coronal fields of the 14 decaying active regions only opened under the condition that the global coronal structure remained almost unchanged. This was because the dominant slowly varying, low-order multipoles prevented opposing-polarity fields from opening and the remnant active-region flux preserved the regions' low-order multipole moments long after the regions had decayed. Thus, the polarity of each coronal hole necessarily matched the polar field on the side of the streamer belt where the corresponding active region decayed. For magnetically isolated active regions initially located within the streamer belt, the more intense polarity generally survived to form the hole. For non-isolated regions, flux imbalance and topological asymmetry prompted the opposite to occur in some cases.

Petrie, G. J. D. [National Solar Observatory, Tucson, AZ 85719 (United States); Haislmaier, K. J. [George Mason University, Fairfax, VA 22030 (United States)

2013-10-01T23:59:59.000Z

Note: This page contains sample records for the topic "high latitude regions" 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

THE HIGH-LATITUDE BRANCH OF THE SOLAR TORSIONAL OSCILLATION IN THE RISING PHASE OF CYCLE 24  

SciTech Connect (OSTI)

We use global heliseismic data from the Global Oscillation Network Group, the Michelson Doppler Imager on board the Solar and Heliospheric Observatory, and the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory, to examine the behavior, during the rising phase of Solar Cycle 24, of the migrating zonal flow pattern known as the torsional oscillation. Although the high-latitude part of the pattern appears to be absent in the new cycle when the flows are derived by subtracting a mean across a full solar cycle, it can be seen if we subtract the mean over a shorter period in the rising phase of each cycle, and these two mean rotation profiles differ significantly at high latitudes. This indicates that the underlying high-latitude rotation has changed; we speculate that this is in response to weaker polar fields, as suggested by a recent model.

Howe, R. [School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT (United Kingdom); Christensen-Dalsgaard, J. [Stellar Astrophysics Centre, Department of Physics and Astronomy, Ny Munkegade 120, Aarhus University, DK-8000 Aarhus C (Denmark); Hill, F.; Komm, R. [National Solar Observatory, P.O. Box 26732, Tucson, AZ 85726-6732 (United States); Larson, T. P.; Schou, J. [HEPL Solar Physics, 452 Lomita Mall, Stanford University, Stanford, CA 94305-4085 (United States); Rempel, M.; Thompson, M. J., E-mail: rhowe@nso.edu [High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000 (United States)

2013-04-10T23:59:59.000Z

22

Submitted to Journal of Geophysical Research, May 11, 2000; revised July 13, 2000 Electrostatic potential patterns in the high latitude  

E-Print Network [OSTI]

potential patterns in the high latitude ionosphere constrained by SuperDARN measurements S. G. Shepherd of the electrostatic potential, #8;, associated with the `E #2; B' drift of ionospheric plasma can be reliably mapped convection according to v = E#2;B=B 2 . Measuring the velocity of the convecting ionospheric plasma allows

Shepherd, Simon

23

High-Latitude Ocean and Sea Ice Surface Fluxes: Challenges for Climate Research Mark A. Bourassa1  

E-Print Network [OSTI]

, the Wilkins Ice Shelf collapsed equally quickly (Scambos et al. 2009). Ocean heat content is rising rapidlyHigh-Latitude Ocean and Sea Ice Surface Fluxes: Challenges for Climate Research Mark A. Bourassa1 conditions for the measurement and estimation of air┬şsea and ice fluxes, limiting understanding of related

Gille, Sarah T.

24

High-Latitude Ocean and Sea Ice Surface Fluxes: Challenges for Climate Research1 Mark A. Bourassa1  

E-Print Network [OSTI]

), and in 2008, the Wilkins Ice Shelf51 collapsed equally quickly (Scambos et al. 2009). Ocean heat content1 High-Latitude Ocean and Sea Ice Surface Fluxes: Challenges for Climate Research1 2 Mark A conditions for the measurement and estimation of air┬ş27 sea and ice fluxes, limiting understanding of related

Gille, Sarah T.

25

ULF wave occurrence statistics in a high-latitude HF Doppler sounder D. M. Wright, T. K. Yeoman, T. B. Jones  

E-Print Network [OSTI]

ULF wave occurrence statistics in a high-latitude HF Doppler sounder D. M. Wright, T. K. Yeoman, T was to establish the optimum con®guration for a new high-latitude Doppler sounder experiment, called DOPE (Wright, 1996; Wright et al., 1997), and to determine the likelihood of the experiment observing pulsation eects

Paris-Sud XI, Universit├ę de

26

THE 37 MONTH MAXI/GSC SOURCE CATALOG OF THE HIGH GALACTIC-LATITUDE SKY  

SciTech Connect (OSTI)

We present a catalog of high Galactic-latitude (|b| > 10 Degree-Sign ) X-ray sources detected in the first 37 months of data of the Monitor of All-sky X-ray Image/Gas Slit Camera (MAXI/GSC). To achieve the best sensitivity, we develop a background model of the GSC that well reproduces the data based on the detailed on-board calibration. Source detection is performed through image fits with a Poisson likelihood algorithm. The catalog contains 500 objects detected with significances of s{sub D,4-10keV} {>=} 7 in the 4-10 keV band. The limiting sensitivity is Almost-Equal-To 7.5 Multiplication-Sign 10{sup -12} erg cm{sup -2} s{sup -1} ( Almost-Equal-To 0.6 mCrab) in the 4-10 keV band for 50% of the survey area, which is the highest ever achieved in an all-sky survey mission covering this energy band. We summarize the statistical properties of the catalog and results from cross matching with the Swift/BAT 70 month catalog, the meta-catalog of X-ray detected clusters of galaxies, and the MAXI/GSC 7 month catalog. Our catalog lists the source name (2MAXI), position and its error, detection significances and fluxes in the 4-10 keV and 3-4 keV bands, the hardness ratio, and the basic information of the likely counterpart available for 296 sources.

Hiroi, Kazuo; Ueda, Yoshihiro; Hayashida, Masaaki; Shidatsu, Megumi; Sato, Ryosuke; Kawamuro, Taiki [Department of Astronomy, Kyoto University, Oiwake-cho, Sakyo-ku, Kyoto 606-8502 (Japan); Sugizaki, Mutsumi; Serino, Motoko; Matsuoka, Masaru; Mihara, Tatehiro [Institute of Physical and Chemical Research (RIKEN), 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan); Nakahira, Satoshi; Tomida, Hiroshi; Ueno, Shiro [ISS Science Project Office, Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 2-1-1 Sengen, Tsukuba, Ibaraki 305-8505 (Japan); Kawai, Nobuyuki; Morii, Mikio [Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551 (Japan); Nakajima, Motoki [School of Dentistry at Matsudo, Nihon University, 2-870-1 Sakaecho-nishi, Matsudo, Chiba 101-8308 (Japan); Negoro, Hitoshi [Department of Physics, Nihon University, 1-8-14 Kanda-Surugadai, Chiyoda-ku, Tokyo 101-8308 (Japan); Sakamoto, Takanori [Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Chuo-ku, Sagamihara, Kanagawa 252-5258 (Japan); Tsuboi, Yohko [Department of Physics, Chuo University, 1-13-27 Kasuga, Bunkyo-ku, Tokyo 112-8551 (Japan); Tsunemi, Hiroshi, E-mail: hiroi@kusastro.kyoto-u.ac.jp [Department of Earth and Space Science, Osaka University, 1-1 Machikaneyama, Toyonaka, Osaka 560-0043 (Japan); and others

2013-08-15T23:59:59.000Z

27

On the solar cycle dependence of winds and planetary waves as seen from mid-latitude D1 LF mesopause region wind measurements*  

E-Print Network [OSTI]

mesospheric winds at Saskatoon, Canada, which were measured in 1978 and 1979 during high solar activityOn the solar cycle dependence of winds and planetary waves as seen from mid-latitude D1 LF-term trends and in¯uences of solar variability. The response of the prevailing wind to the 11-year solar cycle

Paris-Sud XI, Universit├ę de

28

DIFFUSE GALACTIC LIGHT IN THE FIELD OF THE TRANSLUCENT HIGH GALACTIC LATITUDE CLOUD MBM32  

SciTech Connect (OSTI)

We have conducted B-, g-, V-, and R-band imaging in a 45' Multiplication-Sign 40' field containing part of the high Galactic latitude translucent cloud MBM32, and correlated the intensity of diffuse optical light S{sub {nu}}({lambda}) with that of 100 {mu}m emission S{sub {nu}}(100 {mu}m). A {chi}{sup 2} minimum analysis is applied to fit a linear function to the measured correlation and derive the slope parameter b({lambda}) = {Delta}S{sub {nu}}({lambda})/{Delta}S{sub {nu}}(100 {mu}m) of the best-fit linear function. Compiling a sample by combining our b({lambda}) and published ones, we show that the b({lambda}) strength varies from cloud to cloud by a factor of four. Finding that b({lambda}) decreases as S{sub {nu}}(100 {mu}m) increases in the sample, we suggest that a nonlinear correlation including a quadratic term of S{sub {nu}}(100 {mu}m){sup 2} should be fitted to the measured correlation. The variation of optical depth, which is A{sub V} = 0.16-2.0 in the sample, can change b({lambda}) by a factor of 2-3. There would be some contribution to the large b({lambda}) variation from the forward-scattering characteristic of dust grains which is coupled to the non-isotropic interstellar radiation field (ISRF). Models of the scattering of diffuse Galactic light (DGL) underestimate the b({lambda}) values by a factor of two. This could be reconciled by deficiency in UV photons in the ISRF or by a moderate increase in dust albedo. Our b({lambda}) spectrum favors a contribution from extended red emission (ERE) to the diffuse optical light; b({lambda}) rises from B to V faster than the models, seems to peak around 6000 A and decreases toward long wavelengths. Such a characteristic is expected from the models in which the DGL is combined with ERE.

Ienaka, N.; Kawara, K. [Institute of Astronomy, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan)] [Institute of Astronomy, University of Tokyo, 2-21-1 Osawa, Mitaka, Tokyo 181-0015 (Japan); Matsuoka, Y.; Oyabu, S. [Graduate School of Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602 (Japan)] [Graduate School of Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602 (Japan); Sameshima, H. [Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8501 (Japan)] [Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8501 (Japan); Tsujimoto, T. [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan)] [National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588 (Japan); Peterson, B. A., E-mail: ienaka@ioa.s.u-tokyo.ac.jp [Research School of Astronomy and Astrophysics, The Australian National University, Weston Creek, ACT 2611 (Australia)

2013-04-10T23:59:59.000Z

29

Atomic and molecular interstellar absorption lines toward the high galactic latitude stars HD~141569 and HD~157841 at ultra-high resolution  

E-Print Network [OSTI]

We present ultra-high resolution (0.32 km/s) spectra obtained with the 3.9m Anglo-Australian Telescope (AAT) and Ultra-High-Resolution Facility (UHRF), of interstellar NaI D1, D2, Ca II K, K I and CH absorption toward two high galactic latitude stars HD141569 and HD157841. We have compared our data with 21-cm observations obtained from the Leiden/Dwingeloo HI survey. We derive the velocity structure, column densities of the clouds represented by the various components and identify the clouds with ISM structures seen in the region at other wavelengths. We further derive abundances, linear depletions and H2 fractional abundances for these clouds, wherever possible. Toward HD141569, we detect two components in our UHRF spectra : a weak, broad component at - 15 km/s, seen only in CaII K absorption and another component at 0 km/s, seen in NaI D1, D2, Ca II K, KI and CH absorption. In the case of the HD157841 sightline, a total of 6 components are seen on our UHRF spectra in NaI D1, D2 Ca II K, K I and CH absorption. 2 of these 6 components are seen only in a single species.

M. S. Sahu; J. C. Blades; L. He; D. Hartmann; M. J. Barlow; I. A. Crawford

1998-03-31T23:59:59.000Z

30

The microbial fate of carbon in high-latitude seas: Impact of the microbial loop on oceanic uptake of CO{sub 2}  

SciTech Connect (OSTI)

This dissertation examines pelagic microbial processes in high-latitude seas, how they affect regional and global carbon cycling, and how they might respond to hypothesized changes in climate. Critical to these interests is the effect of cold temperature on bacterial activity. Also important is the extent to which marine biological processes in general impact the inorganic carbon cycle. The study area is the Northeast Water (NEW) Polynya, a seasonally-recurrent opening in the permanent ice situated over the northeastern Greenland continental shelf. This work was part of an international, multi-disciplinary research project studying carbon cycling in the coastal Arctic. The first chapter describes a simple model which links a complex marine food web to a simplified ocean and atmosphere. The second chapter investigates the inorganic carbon inventory of the summertime NEW Polynya surface waters to establish the effect of biological processes on the air-sea pCO{sub 2} gradient. The third and fourth chapters use a kinetic approach to examine microbial activities in the NEW Polynya as a function of temperature and dissolved organic substrate concentration, testing the so-called Pomeroy hypothesis that microbial activity is disproportionately reduced at low environmental temperatures owing to increased organic substrate requirements. Together, the suite of data collected on microbial activities, cell size, and grazing pressure suggest how unique survival strategies adopted by an active population of high-latitude bacteria may contribute to, rather than detract from, an efficient biological carbon pump.

Yager, P.L.

1996-12-31T23:59:59.000Z

31

Methane Fluxes Between Terrestrial Ecosystems and the Atmosphere at Northern High Latitudes During the Past Century: A retrospective analysis with a process-based biogeochemistry model  

E-Print Network [OSTI]

We develop and use a new version of the Terrestrial Ecosystem Model (TEM) to study how rates of methane (CH4) emissions and consumption in high-latitude soils of the Northern Hemisphere have changed over the past century ...

Zhuang, Qianlai.

32

Options for improving the load matching capability of distributed photovoltaics: Methodology and application to high-latitude data  

SciTech Connect (OSTI)

At high latitudes, domestic electricity demand and insolation are negatively correlated on both an annual and a diurnal basis. With increasing integration of distributed photovoltaics (PV) in low-voltage distribution grids of residential areas, limits to the penetration level are set by voltage rise due to unmatched production and load. In this paper a methodology for determining the impacts of three options for increased load matching is presented and applied to high-latitude data. The studied options are PV array orientation, demand side management (DSM) and electricity storage. Detailed models for domestic electricity demand and PV output are used. An optimisation approach is applied to find an optimal distribution of PV systems on different array orientations and a best-case evaluation of DSM and a storage model are implemented. At high penetration levels, storage is the most efficient option for maximising the solar fraction, but at lower overproduction levels, the impact of DSM is equal or slightly better. An east-west orientation of PV arrays is suggested for high penetration levels, but the effect of the optimised orientation is small. Without an optimised storage operation, the overproduced power is more efficiently reduced by DSM than storage, although this is highly dependent on the applied DSM algorithm. Further research should be focused on the DSM potential and optimal operation of storage. (author)

Widen, Joakim; Waeckelgaard, Ewa [Department of Engineering Sciences, The Aangstroem Laboratory, Uppsala University, P.O. Box 534, SE-751 21 Uppsala (Sweden); Lund, Peter D. [Advanced Energy Systems, Helsinki University of Technology, P.O. Box 2200, FI-02015 HUT, Helsinki (Finland)

2009-11-15T23:59:59.000Z

33

MS 1603. 6 + 2600, an unusual X-ray selected binary system at high Galactic latitude  

SciTech Connect (OSTI)

The discovery of an eclipsing binary system at Galactic latitude 47 deg, found as a serendipitous X-ray source in the Einstein Extended Medium Sensitivity Survey, is described. The object has X-ray flux 1.1 x 10 to the -12th ergs/sq cm s (0.3-3.5 keV) and mean magnitude R = 19.4. An orbital period of 111 minutes is found. The problem discussed is whether the system has a white dwarf or neutron star primary, in the end preferring the neutron star primary model. If the system has either optical or X-ray luminosities typical of low mass X-ray binaries (LMXB), it must be at a very large distance (30-80 kpc). Blueshifted He I absorption is seen, indicating cool outflowing material, similar to that seen in the LMXB AC 211 in the globular cluster M15. 29 refs.

Morris, S.L.; Liebert, J.; Stocke, J.T.; Gioia, I.M.; Schild, R.E. (Observatories of the Carnegie Institution, Pasadena, CA (USA) Colorado Univ., Boulder (USA) Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (USA))

1990-12-01T23:59:59.000Z

34

Discovery of two embedded clusters with WISE in the high Galactic latitude cloud HRK 81.4-77.8  

E-Print Network [OSTI]

Molecular clouds at very high latitude ($b>60^{\\circ}$) away from the Galactic plane are rare and in general are expected to be non-star-forming. However, we report the discovery of two embedded clusters (Camargo 438 and Camargo 439) within the high-latitude molecular cloud HRK 81.4-77.8 using WISE. Camargo 439 with Galactic coordinates $\\ell=81.11^{\\circ}$ and $b=-77.84^{\\circ}$ is an $\\sim2$ Myr embedded cluster (EC) located at a distance from the Sun of $d_{\\odot}=5.09\\pm0.47$ kpc. Adopting the distance of the Sun to the Galactic centre $R_{\\odot}=7.2$ kpc we derive for Camargo 439 a Galactocentric distance of $R_{GC}=8.70\\pm0.26$ kpc and a vertical distance from the plane of $-4.97\\pm0.46$ kpc. Camargo 438 at $\\ell=79.66^{\\circ}$ and $b=-78.86^{\\circ}$ presents similar values. The derived parameters for these two ECs put HRK 81.4-77.8 in the halo at a distance from the Galactic centre of $\\sim8.7$ kpc and $\\sim5.0$ kpc from the disc. Star clusters provide the only direct means to determine the high latitu...

Camargo, Denilso; Bonatto, Charles; Salerno, Gustavo

2015-01-01T23:59:59.000Z

35

High latitudes present extreme conditions for the measurement and estimation of airsea and ice fluxes, limiting understanding of related physical processes and  

E-Print Network [OSTI]

High latitudes present extreme conditions for the measurement and estimation of air┬şsea and ice of the Earth's climate. HigH-LatitudE OcEan and SEa icE SurfacE fLuxES: cHaLLEngES fOr cLimatE rESEarcH by Mark change can manifest itself in astonishing ways. Arctic sea ice extent at the end of the melt season

Renfrew, Ian

36

The effects of coronal mass ejection on galactic cosmic rays in the high latitude heliosphere: Observations from Ulysses` first orbit  

SciTech Connect (OSTI)

During its first solar orbit the Ulysses spacecraft detected several coronal mass ejections (CMEs) at high heliographic latitudes. The authors present first observations on the effects of these high latitude CMEs on galactic cosmic rays (GCRs) using measurements from the Kiel Electron Telescope (KET) which is part of the Cosmic Ray and Solar Particle Investigation (COSPIN) experiment, the Los Alamos SWOOPS (Solar Wind Observations Over the Poles of the Sun) experiment and the magnetic field experiments. They find the passage of these CMEs over the spacecraft to be associated with short term decreases of GCR intensities The relatively weak shocks in these events, driven by the CMEs` over-expansion, had no strong influence on the GCRs. The intensity minimums of GCRs occurred on closed magnetic field lines inside the CMEs themselves as indicated by bidirectional fluxes of suprathermal electrons. Short episodes of intensity increases of GCRs inside CMEs at times when the bidirectional fluxes of suprathermal electrons disappeared, can be interpreted as evidence that GCRs can easily access the interior of those CMEs in which open magnetic field lines are embedded.

Bothmer, V.; Heber, B.; Kunow, H.; Mueller-Mellin, R.; Wibberenz, G. [Univ. of Kiel (Germany). Institut fuer Kernphysik; Gosling, J.T. [Los Alamos National Lab., NM (United States); Balogh, A. [Imperial College, London (United Kingdom). Blackett Lab.; Raviart, A. [CEA, Gif-sur-Yvette (France). Service d`Astrophysique; Paizis, C. [Univ. di Milano (Italy). Istituto di Fisica Cosmica CNR

1997-10-01T23:59:59.000Z

37

Interactions of Water and Energy Mediate Responses of High-Latitude Terrestrial Ecosystems to Climate Change  

E-Print Network [OSTI]

into the numerical weather prediction model COSMO. Borealinto the numerical weather prediction model COSMO. BorealCurrent numerical weather prediction (NWP) models, regional

Subin, Zachary Marc

2012-01-01T23:59:59.000Z

38

STORM TIME SEASONAL VARIATION OF TEC IN THE SOUTHERN HEMISPHERE MID-LATITUDE REGIONS USING SIGNALS FROM GPS SATELLITE  

E-Print Network [OSTI]

region. The main source of this heating is the joule dissipation of electric currents (F├Ârster & Jakowski SIGNALS FROM GPS SATELLITE E. Yizengaw1 and E. A. Essex Cooperative Research Center for Satellite Systems AND METHODS During an ionospheric storm there is heating of the lower part of the thermosphere in the auroral

Kassie, Endawoke Yizengaw

39

Imaging ion outflow in the high-latitude magnetosphere using low-energy neutral atoms  

SciTech Connect (OSTI)

The measurement of neutral atom fluxes generated by charge exchange with the Earth's geocorona has recently been shown to provide the capability to image the magnetosphere. The authors investigate neutral oxygen fluxes produced by charge exchange from the cusp/cleft ion fountain population. Using an empirical cusp/cleft ion fountain model, an empirical variation of the geocoronal neutral hydrogen density with distance, and typical values for charge-exchange cross sections, line-of-sight integrations are performed to calculate the neutral oxygen flux at arbitrary locations in space. The resulting images are evaluated for a set of orbital positions of the proposed HI-LITE small explorer spacecraft. The resulting neutral oxygen fluxes are high enough for imaging with a low-energy neutral atom imaging instrument (ILENA) onboard the spacecraft.

Hesse, M.; Smith, M.F.; Herrero, F. (NASA, Greenbelt, MD (United States). Goddard Space Flight Center); Ghielmetti, A.G.; Shelley, E.G. (Lockheed Palo Alto Research Lab., CA (United States)); Wurz, P.; Bochsler, P. (Univ. of Bern (Switzerland)); Gallagher, D.L.; Moore, T.E. (NASA, Huntsville, AL (United States). Marshall Space Flight Center); Stephen, T.S. (Univ. of Denver, CO (United States))

1993-12-01T23:59:59.000Z

40

A Geochemical and Sedimentary Record of High Southern Latitude Holocene Climate Evolution from Lago Fagnano, Tierra del Fuego  

SciTech Connect (OSTI)

Situated at the southern margin of the hemispheric westerly wind belt and immediately north of the Antarctic Polar Frontal zone, Tierra del Fuego is well-positioned to monitor coupled changes in the ocean-atmosphere system of the high southern latitudes. Here we describe a Holocene paleoclimate record from sediment cores obtained from Lago Fagnano, a large lake in southern Tierra del Fuego at 55{sup o}S, to investigate past changes in climate related to these two important features of the global climate system. We use an AMS radiocarbon chronology for the last 8,000 years based on pollen concentrates, thereby avoiding contamination from bedrock-derived lignite. Our chronology is consistent with a tephrochronologic age date for deposits from the middle Holocene Volcan Hudson eruption. Combining bulk organic isotopic ({delta}{sup 13}C and {delta}{sup 15}N) and elemental (C and N) parameters with physical sediment properties allow us to better understand sediment provenance and transport mechanisms and to interpret Holocene climate and tectonic change during the last 8,000 years. Co-variability and long-term trends in C/N ratio, carbon accumulation rate, and magnetic susceptibility reflect an overall Holocene increase in the delivery of terrestrial organic and lithogenic material to the deep eastern basin. We attribute this variability to westerly wind-derived precipitation. Increased wind strength and precipitation in the late Holocene drives the Nothofagus forest eastward and enhances run-off and terrigenous inputs to the lake. Superimposed on the long-term trend are a series of abrupt 9 negative departures in C/N ratio, which constrain the presence of seismically-driven mass flow events in the record. We identify an increase in bulk {delta}{sup 13}C between 7,000 and 5,000 cal yr BP that we attribute to enhanced aquatic productivity driven by warmer summer temperatures. The Lago Fagnano {delta}{sup 13}C record shows similarities with Holocene records of sea surface temperature from the mid-latitude Chilean continental shelf and Antarctic air temperatures from the Taylor Dome ice core record in East Antarctica. Mid-Holocene warming occurred simultaneously across the Antarctic Frontal Zone, and in particular, in locations currently influenced by the Antarctic Circumpolar Current.

Moy, C M; Dunbar, R B; Guilderson, T P; Waldmann, N; Mucciarone, D A; Recasens, C; Austin, J A; Anselmetti, F S

2010-11-19T23:59:59.000Z

Note: This page contains sample records for the topic "high latitude regions" 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

Nuclear Interactions in Super High Energy Region  

Science Journals Connector (OSTI)

......research-article Articles Nuclear Interactions in Super High Energy Region Jose F. Bellandi a...Tokyo 188 We formulate the energy spectrum of produced particles...Atmospheric diffusion of high energy cosmic rays is calculated analytically......

Jose F. Bellandi; Sergio Q. Brunetto; Jose A. Chinellato; Carola Dobrigkeit; Akinori Ohsawa; Kotaro Sawayanagi; Edison H. Shibuya

1990-01-01T23:59:59.000Z

42

LOW-FREQUENCY IMAGING OF FIELDS AT HIGH GALACTIC LATITUDE WITH THE MURCHISON WIDEFIELD ARRAY 32 ELEMENT PROTOTYPE  

SciTech Connect (OSTI)

The Murchison Widefield Array (MWA) is a new low-frequency, wide-field-of-view radio interferometer under development at the Murchison Radio-astronomy Observatory in Western Australia. We have used a 32 element MWA prototype interferometer (MWA-32T) to observe two 50 Degree-Sign diameter fields in the southern sky, covering a total of {approx}2700 deg{sup 2}, in order to evaluate the performance of the MWA-32T, to develop techniques for epoch of reionization experiments, and to make measurements of astronomical foregrounds. We developed a calibration and imaging pipeline for the MWA-32T, and used it to produce {approx}15' angular resolution maps of the two fields in the 110-200 MHz band. We perform a blind source extraction using these confusion-limited images, and detect 655 sources at high significance with an additional 871 lower significance source candidates. We compare these sources with existing low-frequency radio surveys in order to assess the MWA-32T system performance, wide-field analysis algorithms, and catalog quality. Our source catalog is found to agree well with existing low-frequency surveys in these regions of the sky and with statistical distributions of point sources derived from Northern Hemisphere surveys; it represents one of the deepest surveys to date of this sky field in the 110-200 MHz band.

Williams, Christopher L.; Hewitt, Jacqueline N.; Levine, Alan M. [MIT Kavli Institute for Astrophysics and Space Research, Cambridge, MA (United States); De Oliveira-Costa, Angelica; Hernquist, Lars L.; Bernardi, Gianni [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States); Bowman, Judd D. [School of Earth and Space Exploration, Arizona State University, Tempe, AZ (United States); Briggs, Frank H. [Research School of Astronomy and Astrophysics, The Australian National University, Canberra (Australia); Gaensler, B. M.; Mitchell, Daniel A.; Subrahmanyan, Ravi; Sadler, Elaine M. [ARC Centre of Excellence for All-sky Astrophysics (CAASTRO) (Australia); Morales, Miguel F. [Department of Physics, University of Washington, Seattle, WA (United States); Sethi, Shiv K. [Raman Research Institute, Bangalore (India); Arcus, Wayne; Crosse, Brian W. [International Centre for Radio Astronomy Research, Curtin University, Perth (Australia); Barnes, David G. [Center for Astrophysics and Supercomputing, Swinburne University of Technology, Melbourne (Australia); Bunton, John D. [CSIRO Astronomy and Space Science, Epping (Australia); Cappallo, Roger C.; Corey, Brian E., E-mail: clmw@mit.edu [MIT Haystack Observatory, Westford, MA (United States); and others

2012-08-10T23:59:59.000Z

43

latitude | OpenEI  

Open Energy Info (EERE)

42 42 Varnish cache server Browse Upload data GDR 429 Throttled (bot load) Error 429 Throttled (bot load) Throttled (bot load) Guru Meditation: XID: 2142278742 Varnish cache server latitude Dataset Summary Description (Abstract): Latitude Tilt Irradiance NASA Surface meteorology and Solar Energy (SSE) Release 6.0 Data Set (Jan 2008)22-year Monthly & Annual Average (July 1983 - June 2005) Parameter: Latitude Tilt Radiation (kWh/m^2/day) Internet: http://eosweb.larc.nasa.gov/sse/ Note 1: SSE Methodology & Accuracy sections online Source U.S. National Aeronautics and Space Administration (NASA), Surface meteorology and Solar Energy (SSE) Date Released March 31st, 2009 (5 years ago) Date Updated April 01st, 2009 (5 years ago) Keywords GIS global irradiance latitude

44

DC High School Science Bowl Regionals | Department of Energy  

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

DC High School Science Bowl Regionals DC High School Science Bowl Regionals February 22, 2014 1:15PM to 8:15PM EST Department of Energy headquarters - 1000 Independence Ave SW,...

45

Ulysses solar wind plasma observations from peak southerly latitude through perihelion and beyond  

Science Journals Connector (OSTI)

We present Ulysses solar wind plasma data from the peak southerly latitude of ?80.2░ through +64.9░ latitude on June 7 1995. Ulysses encountered fast wind throughout this time except for a 43░ equatorial band. Mass flux was nearly constant with latitude while speed (density) had positive (negative) poleward gradients. Momentum flux was highest at high latitudes suggesting a latitudinal asymmetry in the heliopause cross section. Solar wind energy flux density was also highest at high latitudes.

J. L. Phillips; S. J. Bame; W. C. Feldman; J. T. Gosling; D. J. McComas; B. E. Goldstein; M. Neugebauer; C. M. Hammond

1996-01-01T23:59:59.000Z

46

West Windsor-Plainsboro High School South wins regional Science...  

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

West Windsor-Plainsboro High School South wins regional Science Bowl at PPPL A dramatic ending to High School Bowl sends local team to nationals By Jeanne Jackson DeVoe February...

47

Isentropic diagnostics of mid-latitude circulation and transport  

E-Print Network [OSTI]

This thesis examines the mid-latitude circulation and tracer transport using zonal average isentropic diagnostics. The Underworld (i.e. the region roughly below the 300K-isentrope) is targeted by our research. Currently, ...

Koh, Tieh-Yong, 1972-

2001-01-01T23:59:59.000Z

48

latitude tilt | OpenEI  

Open Energy Info (EERE)

latitude tilt latitude tilt Dataset Summary Description (Abstract): Monthly Average Solar Resource for flat-plate collectors tilted at latitude for Nepal. (Purpose): Provide information on the solar resource potential for the data domain. The insolation values represent the average solar energy available to a flat plate collector, such as a photovoltaic panel, oriented due south at an angle from horizontal equal to the latitude of the collector location. Source U.S. National Renewable Energy Laboratory (NREL) Date Released April 12th, 2005 (9 years ago) Date Updated October 30th, 2007 (7 years ago) Keywords atmospheric water vapor GIS latitude tilt Nepal NREL solar SWERA TILT UNEP Data application/zip icon Download Shapefile (zip, 25.6 KiB) text/csv icon Download Data (csv, 36.2 KiB)

49

Turbine component casting core with high resolution region  

DOE Patents [OSTI]

A hollow turbine engine component with complex internal features can include a first region and a second, high resolution region. The first region can be defined by a first ceramic core piece formed by any conventional process, such as by injection molding or transfer molding. The second region can be defined by a second ceramic core piece formed separately by a method effective to produce high resolution features, such as tomo lithographic molding. The first core piece and the second core piece can be joined by interlocking engagement that once subjected to an intermediate thermal heat treatment process thermally deform to form a three dimensional interlocking joint between the first and second core pieces by allowing thermal creep to irreversibly interlock the first and second core pieces together such that the joint becomes physically locked together providing joint stability through thermal processing.

Kamel, Ahmed; Merrill, Gary B.

2014-08-26T23:59:59.000Z

50

Ulysses solar wind plasma observations from peak southerly latitude through perihelion and beyond  

SciTech Connect (OSTI)

We present Ulysses solar wind plasma data from the peak southerly latitude of {minus}80.2{degrees} through +64.9{degrees} latitude on June 7, 1995. Ulysses encountered fast wind throughout this time except for a 43{degrees} band centered on the solar equator. Median mass flux was nearly constant with latitude, while speed and density had positive and negative poleward gradients, respectively. Solar wind momentum flux was highest at high latitudes, suggesting a latitudinal asymmetry in the heliopause cross section. Solar wind energy flux density was also highest at high latitudes.

Phillips, J.L.; Bame, S.J.; Feldman, W.C.; Gosling, J.T.; McComas, D.J. [Los Alamos National Lab., NM (United States); Goldstein, B.E.; Neugebauer, M. [Jet Propulsion Lab., Pasadena, CA (United States); Hammond, C.M. [SRI International, Menlo Park, CA (United States)

1995-09-01T23:59:59.000Z

51

We Have a Winner - DC High School Regional Science Bowl Competition...  

Office of Environmental Management (EM)

We Have a Winner - DC High School Regional Science Bowl Competition Held Last Saturday We Have a Winner - DC High School Regional Science Bowl Competition Held Last Saturday...

52

Resolution limits and process latitude of comformable contact nano-lithography  

E-Print Network [OSTI]

Conformable Contact Lithography enables researchers to attain high-resolution lithographic patterning at manageable cost. This thesis characterizes the minimum resolvable feature size and process latitude of Conformable ...

Fucetola, Corey Patrick

2007-01-01T23:59:59.000Z

53

An Optical Survey of the Position Error Contours of Unidentified High Energy Gamma-Ray Sources at Galactic Latitude b >|20| degrees  

E-Print Network [OSTI]

We present the most recent results of an optical survey of the position error contours ("error boxes") of unidentified high energy gamma-ray sources.

S. D. Bloom; D. A. Dale; R. Cool; K. Dupczak; C. Miller; A. Haugsjaa; C. Peters; M. Tornikoski; P. Wallace; M. Pierce

2004-04-02T23:59:59.000Z

54

Does High[Plasma]-Beta Dynamics "Load" Active Regions?  

E-Print Network [OSTI]

Using long-duration observations in the He II 304 Angstrom passband of the Solar and Heliospheric Observatory (SOHO) Extreme-ultraviolet Imaging Telescope (EIT) we investigate the spatial and temporal appearance of impulsive intensity fluctuations in the pixel light curves. These passband intensity fluctuations come from plasma emitting in the chromosphere, transition region and lowest portions of the corona. We see that they are spatially tied to the supergranular scale and that their rate of occurrence is tied to the unsigned imbalance of the magnetic field in which they are observed. The signature of the fluctuations (in space and time) is consistent with their creation by magnetoconvection forced reconnection that is driven by the flow field in the high-beta plasma. The signature of the intensity fluctuations around an active region suggest that the bulk of the mass and energy supplied into the active region complex observed in the hotter coronal plasma is supplied by this process, dynamically forcing the looped structure from beneath.

Scott W. McIntosh

2007-02-04T23:59:59.000Z

55

THE LOCATION OF THE HIGH-DENSITY BOUNDARY IN SATURN'S INNER  

E-Print Network [OSTI]

density. Dur- ing seven consecutive high-latitude passes in the northern hemisphere from Septem- ber to detect modulations in the high-latitude auroral hiss emissions at a 10.6 hour rotational modulation rate and periodic modulations in the density profiles indicate that Cassini is passing in and out of a plasma region

Gurnett, Donald A.

56

High Schools Served by Regional Admissions Representatives (by County) Lisa Overstreet  

E-Print Network [OSTI]

High Schools Served by Regional Admissions Representatives (by County) Region 1 Lisa Overstreet San Joaquin El Dorado San Mateo Fresno Sierra Kings Solano Lake Sonoma Madera Stanislaus Mariposa

Belanger, David P.

57

THE ACCIMA PROJECT COUPLED MODELING OF THE HIGH SOUTHERN LATITUDES K.M. Hines1* , D.H. Bromwich1,2, L.-S. Bai1, J.P. Nicolas1,2, D.M. Holland3, J.M. Klinck4, M. Dinniman4, C. Yoo3, and E.P. Gerber3  

E-Print Network [OSTI]

THE ACCIMA PROJECT ┬ş COUPLED MODELING OF THE HIGH SOUTHERN LATITUDES K.M. Hines1* , D.H. Bromwich1 including surface and bottom layer formulations; as well as procedures for data assimilation. Numerical balance of the Antarctic ice sheet is critical for projecting global sea-level change. Also, Antarctica

Howat, Ian M.

58

Arizona Regional High Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Arizona Regions » Arizona Regional High Arizona Regions » Arizona Regional High Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Arizona Regions Arizona Regional High Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Castle Catherine Email: ccastle@wapa.gov Regional Event Information Date: Saturday, March 1, 2014 Maximum Number of Teams: 32 Maximum Number of Teams per School: 3

59

Alaska Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Alaska Regions » Alaska Regional High School Alaska Regions » Alaska Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Alaska Regions Alaska Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Cindy Carl Email: WellnessWorks_4u2@yahoo.com Regional Event Information Date: Saturday, February 8, 2014 Maximum Number of Teams: 12

60

Arkansas Regional High Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Arkansas Regions » Arkansas Regional High Arkansas Regions » Arkansas Regional High Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Arkansas Regions Arkansas Regional High Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: David Burkey Email: david.burkey@uafs.edu Regional Event Information Date: Saturday, January 25, 2014 Maximum Number of Teams: 16

Note: This page contains sample records for the topic "high latitude regions" 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

DC Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

DC Regions » DC Regional High DC Regions » DC Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Washington DC Regions DC Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Jamie T. Scipio Email: jamie.scipio@hq.doe.gov Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 12

62

SWPA Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Pennsylvania Regions » SWPA Regional High Pennsylvania Regions » SWPA Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Pennsylvania Regions SWPA Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Lilas Soukup Email: lilas.soukup@netl.doe.gov Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 48

63

Wisconsin Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Wisconsin Regions » Wisconsin Regional High Wisconsin Regions » Wisconsin Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Wisconsin Regions Wisconsin Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Julie Schuster Email: schuster@msoe.edu Regional Event Information Date: Saturday, January 25, 2014 Maximum Number of Teams: 20

64

Michigan Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Michigan Regions » Michigan Regional High Michigan Regions » Michigan Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Michigan Regions Michigan Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Andrew Chubb Email: achubb@svsu.edu Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 15

65

Nevada Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Nevada Regions » Nevada Regional High School Nevada Regions » Nevada Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Nevada Regions Nevada Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Daniel Burns Email: burnsdb@nv.doe.gov Regional Event Information Date: Saturday, February 1, 2014 Maximum Number of Teams: 32

66

BPA Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Oregon Regions » BPA Regional High School Oregon Regions » BPA Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Oregon Regions BPA Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Christy Adams Email: cfadams@bpa.gov Regional Event Information Date: Saturday, February 1, 2014 Maximum Number of Teams: 64 Maximum Number of Teams per School: 3

67

Maryland Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Maryland Regions » Maryland Regional High Maryland Regions » Maryland Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Maryland Regions Maryland Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Michael Mehalick Email: michael.mehalick@montgomerycollege.edu Regional Event Information Date: Saturday, January 18, 2014

68

Maine Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Maine Regions » Maine Regional High School Maine Regions » Maine Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Maine Regions Maine Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Rob Sanford Email: rsanford@usm.maine.edu Regional Event Information Date: Saturday, March 1, 2014 Maximum Number of Teams: 20

69

Indiana Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Indiana Regions » Indiana Regional High School Indiana Regions » Indiana Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Indiana Regions Indiana Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Bala Dhungana Email: bkrishnad@hotmail.com Regional Event Information Date: Saturday, March 8, 2014 Maximum Number of Teams: 10

70

Kansas Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Kansas Regions » Kansas Regional High School Kansas Regions » Kansas Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Kansas Regions Kansas Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Myra Everette Email: meverette@kcp.com Regional Event Information Date: February 1, 2014 Maximum Number of Teams: 32 Maximum Number of Teams per School: 3

71

Iowa Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Iowa Regions » Iowa Regional High School Iowa Regions » Iowa Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Iowa Regions Iowa Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Steve Karsjen Email: karsjen@ameslab.gov Regional Event Information Date: Saturday, January 25, 2014 Maximum Number of Teams: 40

72

Nebraska Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Nebraska Regions » Nebraska Regional High Nebraska Regions » Nebraska Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Nebraska Regions Nebraska Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Todd Young Email: toyoung1@wsc.edu Regional Event Information Date: Saturday, February 8, 2014 Maximum Number of Teams: 40

73

Montana Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Montana Regions » Montana Regional High School Montana Regions » Montana Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Montana Regions Montana Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Josie Daggett Email: daggett@wapa.gov Regional Event Information Date: Saturday, March 8, 2014 Maximum Number of Teams: 30

74

Virginia Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Virginia Regions » Virginia Regional High Virginia Regions » Virginia Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Virginia Regions Virginia Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Jan Tyler Email: tyler@jlab.org Regional Event Information Date: Saturday, February 1, 2014 Maximum Number of Teams: 23

75

Missouri Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Missouri Regions » Missouri Regional High Missouri Regions » Missouri Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Missouri Regions Missouri Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Myra Everette Email: meverette@kcp.com Regional Event Information Date: February 1, 2014 Maximum Number of Teams: 32

76

Georgia Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Georgia Regions » Georgia Regional High School Georgia Regions » Georgia Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Georgia Regions Georgia Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Donna Mullenax Email: donna.mullenax@armstrong.edu Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 72

77

Florida Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Florida Regions » Florida Regional High School Florida Regions » Florida Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Florida Regions Florida Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Michael Chiang Email: michaelraymondchiang@gmail.com Regional Event Information Date: Saturday, February 8, 2014 Maximum Number of Teams: 24

78

Colorado Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Colorado Region » Colorado Regional High Colorado Region » Colorado Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Colorado Region Colorado Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Linda Lung Email: linda.lung@nrel.gov Regional Event Information Date: Saturday, March 1, 2014 Maximum Number of Teams: 48

79

Oklahoma Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Oklahoma Regions » Oklahoma Regional High Oklahoma Regions » Oklahoma Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Oklahoma Regions Oklahoma Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Gail Bliss Email: gnbliss@carnegienet.net Regional Event Information Date: Saturday, February 1, 2014 Maximum Number of Teams: 32

80

Minnesota Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Minnesota Regions » Minnesota Regional High Minnesota Regions » Minnesota Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Minnesota Regions Minnesota Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Barbara Donoho Email: bdonoho@mnmas.org Regional Event Information Date: Friday, January 24, 2014 Maximum Number of Teams: 32

Note: This page contains sample records for the topic "high latitude regions" 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 Region Thesaurus Approach for High-Level Concept Detection in the Natural Disaster Domain  

Science Journals Connector (OSTI)

This paper presents an approach on high-level feature detection using a region thesaurus. MPEG-7 features are locally extracted from ... This set of region types defines the region thesaurus. Using this thesaurus

Evaggelos Spyrou; Yannis Avrithis

2007-01-01T23:59:59.000Z

82

Fermi LAT detection of two high Galactic latitude gamma-ray sources, Fermi J1049.7+0435 and J1103.2+1145  

E-Print Network [OSTI]

The Second Fermi LAT source catalog (Nolan et al. 2012) includes as many as 1,873 sources, but initial attempts to identify counterparts at other wavelengths resulted in 575 sources remaining unidentified. The 2FGL catalog is based on the first 24 months of LAT observation since its launch in 2008, but the LAT has now accumulated more than 5 years of high-energy gamma-ray data almost flawlessly, presenting the possibility of finding new sources which were too faint to be detected in the first two years of data or showed flaring activity after the catalog was created. In this paper we report on two new gamma-ray sources serendipitously discovered in the constellation Leo and discuss possible counterparts based on radio observations.

Nishimichi, Masaki; Mori, Masaki; Edwards, Philip G; Stevens, Jamie

2014-01-01T23:59:59.000Z

83

West Virginia Regional High School Science Bowl | U.S. DOE Office of  

Office of Science (SC) Website

West Virginia Regions » West Virginia Regional West Virginia Regions » West Virginia Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov West Virginia Regions West Virginia Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Kirk Gerdes Email: Kirk.Gerdes@NETL.DOE.GOV Regional Event Information Date: Saturday, February 1, 2014

84

Puerto Rico Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Puerto Rico Regions » Puerto Rico Regional Puerto Rico Regions » Puerto Rico Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Puerto Rico Regions Puerto Rico Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Julienne Sanchez Email: julienne.sanchez@upr.edu Regional Event Information Date: Saturday, February 22, 2014

85

Mississippi Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Mississippi Regions » Mississippi Regional Mississippi Regions » Mississippi Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Mississippi Regions Mississippi Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Dionne Fortenberry Email: dfortenberry@as.muw.edu Regional Event Information Date: Friday, January 31, 2014

86

Northeast Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Massachusetts Regions » Northeast Regional Massachusetts Regions » Northeast Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Massachusetts Regions Northeast Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Kevin McLaughlin Email: kjm@engr.uconn.edu Regional Event Information Date: Saturday, March 1, 2014

87

South Dakota Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Daktoa Regions » South Dakota Regional Daktoa Regions » South Dakota Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov South Daktoa Regions South Dakota Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Lesley Berg Email: lberg@wapa.gov Regional Event Information Date: Saturday, March 1, 2014 Maximum Number of Teams: 32

88

Connecticut Regional High School Science Bowl| U.S. DOE Office of Science  

Office of Science (SC) Website

Connecticut Regions » Connecticut Regional Connecticut Regions » Connecticut Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Connecticut Regions Connecticut Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Kevin McLaughlin Email: kjm@engr.uconn.edu Regional Event Information Date: Saturday, March 1, 2014

89

North Dakota Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Dakota Regions » North Dakota Regional Dakota Regions » North Dakota Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov North Dakota Regions North Dakota Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Tom Atkinson Phone: 701-221-4559 Email: tatkinson@wapa.gov Regional Event Information Date: Saturday, February 8, 2014

90

UIC Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

UIC Regional High School UIC Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Illinois Regions UIC Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Anita Ramirez Email: chicago.regional.science.bowl@gmail.com Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 24

91

Tennessee Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Tennessee Regions » Tennessee Regional High Tennessee Regions » Tennessee Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Tennessee Regions Tennessee Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Martha Hammond Email: Martha.Hammond@orau.org Additional Contact: Name: Marolyn Randolph Email: Marolyn.Randolph@orau.org

92

West Kentucky Regional High School Science Bowl | U.S. DOE Office of  

Office of Science (SC) Website

Kentucky Regions » West Kentucky Regional High Kentucky Regions » West Kentucky Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Kentucky Regions West Kentucky Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Robert Smith Email: robert.smith@lex.doe.gov Additional Contact: Name: Donald Dihel Email: don.dihel@lex.doe.gov

93

New Jersey Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Jersey Regions » New Jersey Regional High Jersey Regions » New Jersey Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov New Jersey Regions New Jersey Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Please Note: All slots for the High School Science Bowl have been filled. Any team registering after December 17, 2013, will be placed on the wait-list. Should a school drop out of the competition, a new team will be

94

U.S. Virgin Islands Regional High School Science Bowl | U.S. DOE Office of  

Office of Science (SC) Website

U.S. Virgin Islands Regions » U.S. Virgin U.S. Virgin Islands Regions » U.S. Virgin Islands High School Regional Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov U.S. Virgin Islands Regions U.S. Virgin Islands High School Regional Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Gerald Walters Email: gwalters@sttj.k12.vi Regional Event Information

95

Savannah River Regional High School Science Bowl | U.S. DOE Office of  

Office of Science (SC) Website

Carolina Regions » Savannah River Carolina Regions » Savannah River Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov South Carolina Regions Savannah River Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Kim Mitchell Email: kimberly.mitchell@srs.gov Regional Event Information Date: Saturday, March 1, 2014

96

North Carolina Regional High School Science Bowl | U.S. DOE Office of  

Office of Science (SC) Website

Carolina Regions » North Carolina Carolina Regions » North Carolina Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov North Carolina Regions North Carolina Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Fredrick Johnson Email: fjohnson@nccu.edu Regional Event Information Date: Saturday, January 25, 2014

97

JPL Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

JPL Regional High School JPL Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov California Regions JPL Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Kimberly Lievense Email: Klievense@jpl.nasa.gov Regional Event Information Date: Saturday, February 1, 2014 Maximum Number of Teams: 24 Maximum Number of Teams per School: 1

98

PNNL Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

PNNL Regional High School PNNL Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Washington Regions PNNL Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Beth Perry Email: bethperry13@msn.com Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 24 Maximum Number of Teams per School: 3

99

SHPE NYC Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

SHPE NYC Regional High SHPE NYC Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov New York Regions SHPE NYC Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Dora Maria Abreu Email: Doramaria@gmail.com Regional Event Information Date: Saturday, March 1, 2014 Maximum Number of Teams: 20 Maximum Number of Teams per School: 3

100

LADWP Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

LADWP Regional High LADWP Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov California Regions LADWP Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Walter Zeisl Email: walter.zeisl@ladwp.com Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 55 Maximum Number of Teams per School: 2

Note: This page contains sample records for the topic "high latitude regions" 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

Kern County Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Kern County Regional High Kern County Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov California Regions Kern County Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Thomas Meyer Email: tmeyer@csub.edu Regional Event Information Date: Saturday, February 8, 2014 Maximum Number of Teams: 32 Maximum Number of Teams per School: 3

102

San Diego Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

San Diego Regional High San Diego Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov California Regions San Diego Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Ronald Lewis Email: sandiegonobcche@earthlink.net Regional Event Information Date: Saturday, February 8, 2014 Maximum Number of Teams: 24

103

Sacramento Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Sacramento Regional High Sacramento Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov California Regions Sacramento Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Anita Wiley Email: wiley@wapa.gov Regional Event Information Date: March 1, 2014 Maximum Number of Teams: 26 Maximum Number of Teams per School: 2

104

Modesto Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Modesto Regional High Modesto Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov California Regions Modesto Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Mike Zweifel Email: mikez@mid.org Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 24 Maximum Number of Teams per School: 2

105

North Texas Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

North Texas Regional High North Texas Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Texas Regions North Texas Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Rommel Alonzo Email: rommel.alonzo@mavs.uta.edu Regional Event Information Date: Saturday, February 15, 2014 Maximum Number of Teams: 12

106

Pantex Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Pantex Regional High School Pantex Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Texas Regions Pantex Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Debra Halliday Email: dhallida@pantex.com Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 40 Maximum Number of Teams per School: 3

107

UTPA Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

UTPA Regional High School UTPA Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Texas Regions UTPA Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Joel Ruiz Email: jruiz@utpa.edu Additional Contacts: Name: Jessica Salinas Email: lopezj@utpa.edu Name: Karen Dorado Email: kadorado@utpa.edu Regional Event Information

108

NOBCChE Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

NOBCChE Regional High NOBCChE Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov New York Regions NOBCChE Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Thomas Whitt Email: twhitt523@gmail.com Regional Event Information Date: Saturday, February 8, 2014 Maximum Number of Teams: 10 Maximum Number of Teams per School: 2

109

San Antonio Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

San Antonio Regional High San Antonio Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Texas Regions San Antonio Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Bobby Blount Email: bb@mitre.org Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 35 Maximum Number of Teams per School: 3

110

Redding Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Redding Regional High Redding Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov California Regions Redding Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Matt Madison Email: mmadison@reupower.com Regional Event Information Date: Saturday, March 1, 2014 Maximum Number of Teams: 28 Maximum Number of Teams per School: 3

111

SLAC Regional High School Science Bowl| U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

SLAC Regional High School SLAC Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov California Regions SLAC Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Farah Rahbar Email: farah.rahbar@slac.stanford.edu Regional Event Information Date: Saturday, February 8, 2014 Maximum Number of Teams: 18

112

STEP Regional High School Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

STEP Regional High School STEP Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov New York Regions STEP Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Peter Macchia Email: mrmacchia@gmail.com Regional Event Information Date: Saturday, March 1, 2014 Maximum Number of Teams: 16 Maximum Number of Teams per School: 3

113

Inland Northwest Regional High School Science Bowl | U.S. DOE Office of  

Office of Science (SC) Website

Inland Northwest Regional Inland Northwest Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Washington Regions Inland Northwest Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Kaye Kamp Email: kkamp@whitworth.edu Regional Event Information Date: February 8, 2014 Maximum Number of Teams: 42

114

Capital District Regional High School Science Bowl | U.S. DOE Office of  

Office of Science (SC) Website

Capital District Regional Capital District Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov New York Regions Capital District Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Dominic Fulgieri Email: dominic.fulgieri@unnpp.gov Regional Event Information Date: Saturday, March 1, 2014 Maximum Number of Teams: 18

115

South Central Ohio Regional High School Science Bowl | U.S. DOE Office of  

Office of Science (SC) Website

South Central Ohio Regional South Central Ohio Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Ohio Regions South Central Ohio Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Greg Simonton Email: greg.simonton@lex.doe.gov Regional Event Information Date: Friday, March 7, 2014 Maximum Number of Teams: 32

116

Greater Cincinnati Regional High School Science Bowl | U.S. DOE Office of  

Office of Science (SC) Website

Greater Cincinnati Regional Greater Cincinnati Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Ohio Regions Greater Cincinnati Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Betsy Volk Email: betsy.volk@emcbc.doe.gov Regional Event Information Date: Saturday, February 22, 2014 Maximum Number of Teams: 24

117

We Have a Winner - DC High School Regional Science Bowl Competition Held  

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

We Have a Winner - DC High School Regional Science Bowl Competition We Have a Winner - DC High School Regional Science Bowl Competition Held Last Saturday We Have a Winner - DC High School Regional Science Bowl Competition Held Last Saturday February 11, 2013 - 10:30am Addthis We Have a Winner - DC High School Regional Science Bowl Competition Held Last Saturday Annie Whatley Annie Whatley Deputy Director, Office of Minority Economic Impact As part of the National Science Bowl, more than 9,500 high school students take place in 70 high school regional competitions around the United States and Puerto Rico. The winners of these regions advance to the National Science Bowl competition held every April in Chevy Chase, Maryland. On Saturday, February 9, the Office of Economic Impact and Diversity hosted the Washington, D.C. High School Regional Science Bowl competition at Cesar

118

High School Regionals | U.S. DOE Office of Science (SC)  

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

Regionals Regionals National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School High School Regionals Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Team Registration For more information, please visit the High School Coach page. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

119

The Chimalapas Region, Oaxaca, Mexico: a high-priority region for bird conservation in Mesoamerica  

E-Print Network [OSTI]

have been few (Binford 1989). Aside from occasional collecting by W. B. Richardson at the end of the nineteenth century (specimens principally at the British Museum), and intensive collecting in the mid-twentieth century near Sarabia and Matias Romero... scienti?c collections in North America and Europe (Peterson et al. 1998b). For Oaxaca east of Matias Figure 2. Vegetation types in the Selva Zoque priority region of the Chimalapas, Mexico. Data from http://www.conabio.gob.mx. The Chimalapas Region, Oaxaco...

Peterson, A. Townsend; Navarro-Sigü enza, Adolfo G.; Herná ndez-Bañ os, Blanca E.; Escalona-Segura, Griselda; Rebó n-Gallardo, Fanny; Rodrí guez-Ayala, Emir; Figueroa-Esquivel, Elsa M.; Cabrera-Garcí a, Leonardo

2003-01-01T23:59:59.000Z

120

Planning for a regional rail system : analysis of high speed and high quality rail in the Basque region  

E-Print Network [OSTI]

The goal of this thesis is to provide guidance for regional rail network planning to achieve the maximum benefits in terms of economic growth, passenger satisfaction, and environmental sustainability. The hypothesis is ...

Lewis, Paul R. S. (Paul Robinson S.)

2011-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "high latitude regions" 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

Brookhaven National Lab Regional High School Science Bowl | U.S. DOE Office  

Office of Science (SC) Website

Brookhaven National Lab Brookhaven National Lab Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov New York Regions Brookhaven National Lab Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Catherine Osiecki Email: Osiecki@bnl.gov Regional Event Information Date: Saturday, January 25, 2014 Maximum Number of Teams: 20

122

Sandia National Laboratories Regional High School Science Bowl | U.S. DOE  

Office of Science (SC) Website

Sandia National Sandia National Laboratories Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov California Regions Sandia National Laboratories Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Timothy Shepodd Email: tjshepo@sandia.gov Regional Event Information Date: January 25, 2014

123

GEF. latitude tilt | OpenEI  

Open Energy Info (EERE)

GEF. latitude tilt GEF. latitude tilt Dataset Summary Description (Abstract): Latitude tilted solar radiation in kWh/m2/day for 1 year organized into cells with 40km x 40km (Purpose): To provide a set of consistent, reliable, verifiable, and accessible global data sets for international and in-country investors and other stakeholders Source INPE (National Institute for Spatial Research) and LABSOLAR (Laboratory of Solar Energy/Federal University of Santa Catarina) - Brazil Date Released August 08th, 2009 (5 years ago) Date Updated August 08th, 2009 (5 years ago) Keywords Brazil GEF. latitude tilt INPE LABSOLAR solar SWERA TILT UNEP Data application/zip icon Download Shapefile (zip, 706.1 KiB) text/csv icon Download Data (csv, 999.1 KiB) Quality Metrics Level of Review Some Review

124

High-Speed Extraction Model of Interest Region in the Parcel Image of Large Size  

Science Journals Connector (OSTI)

This paper deals with a model for the high-speed extraction of ROI (Region Of Interest) during the process of logistics transported on conveyor belt. The objective of this paper is to extract various ROIs from...

Moon-sung Park; Il-sook Kim; Eun-kyung Choů

2005-01-01T23:59:59.000Z

125

Groundwater Nitrogen Source Identification and Remediation in the Texas High Plains and Rolling Plains Regions  

E-Print Network [OSTI]

Groundwater nitroGen source identification and remediation in the texas hiGh plains and rollinG plains reGions Paul Delaune, Bridget R. Scanlon, Robert C. Reedy, Robert C. Schwartz, Louis Baumhardt, Lucas F. Gregory Texas Water Resources... Institute TR-451 September 2013 GROUNDWATER NITROGEN SOURCE IDENTIFICATION AND REMEDIATION IN THE TEXAS HIGH PLAINS AND ROLLING PLAINS REGIONS FINAL REPORT FUNDING PROVIDED BY THE TEXAS STATE SOIL AND WATER CONSERVATION BOARD THROUGH A CLEAN...

Delaune, P.; Scanlon, B.; Reedy, R.; Schwartz, R.; Baumhardt, L.; Gregory, L.

2013-01-01T23:59:59.000Z

126

A SYSTEMATIC SURVEY OF HIGH-TEMPERATURE EMISSION IN SOLAR ACTIVE REGIONS  

SciTech Connect (OSTI)

The recent analysis of observations taken with the EUV Imaging Spectrometer and X-Ray Telescope instruments on Hinode suggests that well-constrained measurements of the temperature distribution in solar active regions can finally be made. Such measurements are critical for constraining theories of coronal heating. Past analysis, however, has suffered from limited sample sizes and large uncertainties at temperatures between 5 and 10 MK. Here we present a systematic study of the differential emission measure distribution in 15 active region cores. We focus on measurements in the 'inter-moss' region, that is, the region between the loop footpoints, where the observations are easier to interpret. To reduce the uncertainties at the highest temperatures we present a new method for isolating the Fe XVIII emission in the AIA/SDO 94 A channel. The resulting differential emission measure distributions confirm our previous analysis showing that the temperature distribution in an active region core is often strongly peaked near 4 MK. We characterize the properties of the emission distribution as a function of the total unsigned magnetic flux. We find that the amount of high-temperature emission in the active region core is correlated with the total unsigned magnetic flux, while the emission at lower temperatures, in contrast, is inversely related. These results provide compelling evidence that high-temperature active region emission is often close to equilibrium, although weaker active regions may be dominated by evolving million degree loops in the core.

Warren, Harry P. [Space Science Division, Naval Research Laboratory, Washington, DC 20375 (United States); Winebarger, Amy R. [NASA Marshall Space Flight Center, VP 62, Huntsville, AL 35812 (United States); Brooks, David H. [College of Science, George Mason University, 4400 University Drive, Fairfax, VA 22030 (United States)

2012-11-10T23:59:59.000Z

127

Mats Lindroos, Cristina Oyon and Stevey OECD "A High Power Spallation Source in each Global Region"  

E-Print Network [OSTI]

ESS Mats Lindroos, Cristina Oyon and Stevey Peggs #12;ESS 2 #12;OECD "A High Power Spallation Source in each Global Region" SNS Oak Ridge J-PARC Tokai ESS in Lund #12;ESS: Site selection process ┬Ě ESS high up on the ESFRI list Th ti biddi f th it (Bilb L d d┬Ě Three consortia bidding for the site

McDonald, Kirk

128

Texas A&M Regional High School Science Bowl | U.S. DOE Office of Science  

Office of Science (SC) Website

Texas A&M Regional High School Texas A&M Regional High School Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Texas Regions Texas A&M Regional High School Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Vince Schielack Email: vinces@math.tamu.edu Regional Event Information Date: Saturday, February 1, 2014 Maximum Number of Teams: 32

129

**NO SCIENCE ON SATURDAY TODAY** NJ Regional High School Science Bowl |  

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

February 23, 2013, 8:00am February 23, 2013, 8:00am Science Education Lab-wide Event **NO SCIENCE ON SATURDAY TODAY** NJ Regional High School Science Bowl Teams of students are invited to participate in the Department of Energy's National Science Bowl Competition. Each year PPPL hosts the New Jersey Regional Science Bowl which decides which teams from the local area can continue onto the national competition in Washington, D.C. The Science Bowl is a double elimination contest with oral question and answer rounds in the fields of chemistry, biology, physics, astronomy and mathematics plus general and earth sciences. Questions are given in a toss-up with a bonus format. For more information, visit our Science Bowl website! Contact Information Website: NJ Regional High School Science Bowl

130

Temperature dependence of the gaps of high-temperature superconductors in the Fermi-arc region  

Science Journals Connector (OSTI)

It is shown how in a high-temperature superconductor, the length of the Fermi arc can be obtained from the doping dependence of the pseudogap and the superconducting gap. In the momentum region spanned by the Fermi arc, the pseudogap temperature dependence follows that of the superconducting gap. The close interconnection of the two gaps suggests that they are both an essential part of the high-temperature superconductivity.

S. HŘfner and F. MŘller

2008-07-23T23:59:59.000Z

131

High-Speed extraction model of interest region in the parcel image of large size  

Science Journals Connector (OSTI)

This paper deals with a model for the high-speed extraction of ROI (Region Of Interest) during the process of logistics transported on conveyor belt. The objective of this paper is to extract various ROIs from large size image of logistics more than ...

Moon-sung Park; Il-sook Kim; Eun-kyung Cho; Young-hee Kwon; Jong-heung Park

2005-09-01T23:59:59.000Z

132

REGIONAL BINNING FOR CONTINUED STORAGE OF SPENT NUCLEAR FUEL AND HIGH-LEVEL WASTES  

SciTech Connect (OSTI)

In the Continued Storage Analysis Report (CSAR) (Reference 1), DOE decided to analyze the environmental consequences of continuing to store the commercial spent nuclear fuel (SNF) at 72 commercial nuclear power sites and DOE-owned spent nuclear fuel and high-level waste at five Department of Energy sites by region rather than by individual site. This analysis assumes that three commercial facilities pairs--Salem and Hope Creek, Fitzpatrick and Nine-Mile Point, and Dresden and Moms--share common storage due to their proximity to each other. The five regions selected for this analysis are shown on Figure 1. Regions 1, 2, and 3 are the same as those used by the Nuclear Regulatory Commission in their regulatory oversight of commercial power reactors. NRC Region 4 was subdivided into two regions to more appropriately define the two different climates that exist in NRC Region 4. A single hypothetical site in each region was assumed to store all the SNF and HLW in that region. Such a site does not exist and has no geographic location but is a mathematical construct for analytical purposes. To ensure that the calculated results for the regional analyses reflect appropriate inventory, facility and material degradation, and radionuclide transport, the waste inventories, engineered barriers, and environmental conditions for the hypothetical sites were developed from data for each of the existing sites within the given region. Weighting criteria to account for the amount and types of SNF and HLW at each site were used in the development of the environmental data for the regional site, such that the results of the analyses for the hypothetical site were representative of the sum of the results of each actual site if they had been modeled independently. This report defines the actual site data used in development of this hypothetical site, shows how the individual site data was weighted to develop the regional site, and provides the weighted data used in the CSAR analysis. It is divided into Part 1 that defines time-dependent releases from each regional site, Part 2 that defines transport conditions through the groundwater, and Part 3 that defines transport through surface water and populations using the surface waters for drinking.

W. Lee Poe, Jr

1998-10-01T23:59:59.000Z

133

Direct injection of ionospheric O sup + into the dayside low latitude boundary layer  

SciTech Connect (OSTI)

Observations from the AMPTE/Charge Composition Explorer (AMPTE/CCE) indicate the presence of two distinct O{sup +} populations in the dayside subsolar low latitude boundary layer during some periods of northward Interplanetary Magnetic Field (IMF). The first population is O{sup +} convected into the boundary layer from the outer magnetosphere and has been reported previously. It is suggested here that the new, second, O{sup +} population is injected into the dayside boundary layer directly from the high latitude ionosphere. This second population can have a significant density and distinct characteristics such as field-aligned flow relative to boundary layer H{sup +} that modify both the plasma composition and dynamics in the low latitude boundary layer. {copyright} American Geophysical Union 1989

Fuselier, S.A.; Klumpar, D.M.; Peterson, W.K.; Shelley, E.G. (Lockheed Palo Alto Research Laboratory, Palo Alto, California (US))

1989-10-01T23:59:59.000Z

134

Neogene Low-latitude Seasonal Environmental Variations: Stable Isotopic and Trace Elemental Records in Mollusks from the Florida Platform and the Central American Isthmus  

E-Print Network [OSTI]

to examine low-latitude temperature and salinity variations recorded in Plio-Pleistocene (3.5-1.6 Ma) fossils from western Florida during periods of high-latitude warming and "global" cooling. The middle Pliocene Pinecrest Beds (Units 7 and 4...

Tao, Kai

2012-10-19T23:59:59.000Z

135

Radiation damage considerations in a high luminosity collider: The interaction region  

SciTech Connect (OSTI)

The interaction region in a high luminosity collider will be a source of radiation for all components in the vicinity and will place stringent requirements on their design. The major components in the vicinity and will place stingent requirements on their design. The major components in the vicinity of the interaction region are the physics detectors that surround the beam pipe and the focusing quadrupole magnets nearby. We will present the radiation levels in such a physics detector and the power in the forward direction that will be deposited in the forward calorimeters and quad magnets. The implications of the levels on a variety of detector components and electronics will be presented. The calculational techniques and limitation will be reviewed.

Lee, D.M.

1992-01-01T23:59:59.000Z

136

Radiation damage considerations in a high luminosity collider: The interaction region  

SciTech Connect (OSTI)

The interaction region in a high luminosity collider will be a source of radiation for all components in the vicinity and will place stringent requirements on their design. The major components in the vicinity and will place stingent requirements on their design. The major components in the vicinity of the interaction region are the physics detectors that surround the beam pipe and the focusing quadrupole magnets nearby. We will present the radiation levels in such a physics detector and the power in the forward direction that will be deposited in the forward calorimeters and quad magnets. The implications of the levels on a variety of detector components and electronics will be presented. The calculational techniques and limitation will be reviewed.

Lee, D.M.

1992-10-01T23:59:59.000Z

137

The Pipe-Quadrupole, an Alternative for High Gradient Interaction Region Quadrupole Designs  

SciTech Connect (OSTI)

In the design of interaction region (IR) quadrupoles for high luminosity colliders such as the LHC or a possible upgrade of the Tevatron, the radiation heating of the coil windings is an important issue. Two obvious solutions to this problem can be chosen. The first is to reduce the heat load by added shielding, increased cooling with fins or using Nb{sub 3}Sn to increase the temperature margin. The second solution eliminates the conductor from the areas with the highest radiation intensity, which are located on the symmetry-axes of the midplanes of the coils. A novel quadrupole design is presented, in which the conductor is wound on four half-moon shaped supports, forming elongated toroid sections. The assembly of the four shapes yields a quadrupole field with an active flux return path, and a void in the high radiation area. This void can be occupied by a liquid helium cooling pipe to lower the temperature of the windings from the inside. The coil layout, harmonic optimization and mechanical design are shown, together with the calculated temperature rise for the radiation load of the LHC interaction region quadrupoles.

Oort, J.M. van; Scanlan, R.M.

1996-12-12T23:59:59.000Z

138

Cosmic-ray latitude surveys in the Atlantic Ocean area  

SciTech Connect (OSTI)

Vertical cutoff rigidities were re-determined for the locations of the stratospheric balloon measurements made during the 22nd Soviet Antarctic Expedition (1975-1976). These cutoff rigidities were determined for the month of each measurement using a method that interpolates between the world grids of trajectory-derived vertical cutoff rigidities calculated for Epoch 1965.0 and Epoch 1980.0. In comparing these values with other calculated using the 1975.0 field models which under-estimated the secular variations, small increases in the vertical cutoff rigidities were noted in the North Atlantic area and small decreases were noted in the South Atlantic, consistent with the secular changes in the world grid of vertical cutoff rigidities. These results emphasize the necessity of determining cutoff rigidity values of the year in which latitude measurements are made if these measurements are in the region of the world (particularly the Atlantic Ocean area) where the cutoff-rigidity values are rapidly changing.

Shea, M.A.; Smart, D.F.; Stozhkov, Y.I.; Svirzhevsky, N.S.; Svirzhevskaya, A.K.

1987-01-01T23:59:59.000Z

139

High-resolution Bent-crystal Spectrometer for the Ultra-soft X-ray Region  

DOE R&D Accomplishments [OSTI]

A multichannel vacuum Brag-crystal spectrometer has been developed for high-resolution measurements of the line emission from tokamak plasmas in the wavelength region between 4 and 25 angstrom. The spectrometer employs a bent crystal in Johann geometry and a microchannel-plate intensified photodiode array. The instrument is capable of measuring high-resolution spectra (lambda/..delta..lambda approx. 3000) with fast time resolution (4 msec per spectrum) and good spatial resolution (3 cm). The spectral bandwidth is ..delta..lambda/lambda{sub 0} = 8 angstrom. A simple tilt mechanism allows access to different wavelength intervals. In order to illustrate the utility of the new spectrometer, time- and space-resolved measurements of the n = 3 to n = 2 spectrum of selenium from the Princeton Large Torus tokamak plasmas are presented. The data are used to determine the plasma transport parameters and to infer the radial distribution of fluorinelike, neonlike, and sodiumlike ions of selenium in the plasma. The new ultra-soft x-ray spectrometer has thus enabled us to demonstrate the utility of high-resolution L-shell spectroscopy of neonlike ions as a fusion diagnostic.

Beiersdorfer, P.; von Goeler, S.; Bitter, M.; Hill, K. W.; Hulse, R. A.; Walling, R. S.

1988-10-00T23:59:59.000Z

140

High-resolution observations of active region moss and its dynamics  

E-Print Network [OSTI]

The \\textit{High resolution Coronal Imager (Hi-C)} has provided the sharpest view of the EUV corona to date. In this paper we exploit its impressive resolving power to provide the first analysis of the fine-scale structure of moss in an active region. The data reveal that the moss is made up of a collection of fine threads, that have widths with a mean and standard deviation of $440\\pm190$~km (Full Width Half Maximum). {The brightest moss emission is located at the visible head of the fine-scale structure and the fine structure appears to extend into the lower solar atmosphere.} The emission decreases along the features implying the lower sections are most likely dominated by cooler transition region plasma. These threads appear to be the cool, lower legs of the hot loops. In addition, the increased resolution allows for the first direct observation {of physical displacements of the moss fine-structure in a direction transverse to its central axis. Some of these transverse displacements demonstrate periodic b...

Morton, R J

2014-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "high latitude regions" 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
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141

Solar: monthly and annual average latitude tilt irradiance GIS data at  

Open Energy Info (EERE)

irradiance GIS data at irradiance GIS data at one-degree resolution of the World from NASA/SSE Dataset Summary Description (Abstract): Latitude Tilt Irradiance NASA Surface meteorology and Solar Energy (SSE) Release 6.0 Data Set (Jan 2008)22-year Monthly & Annual Average (July 1983 - June 2005) Parameter: Latitude Tilt Radiation (kWh/m^2/day) Internet: http://eosweb.larc.nasa.gov/sse/ Note 1: SSE Methodology & Accuracy sections online Note 2: Lat/Lon values indicate the lower left corner of a 1x1 degree region. Negative values are south and west; positive values are north and east. Boundaries of the -90/-180 region are -90 to -89 (south) and -180 to -179 (west). The last region, 89/180, is bounded by 89 to 90 (north) and 179 to 180 (east). The mid-point of the region is +0.5 added to the the Lat/Lon value. These data are regional averages; not point data.

142

CHEMICAL EVOLUTION IN HIGH-MASS STAR-FORMING REGIONS: RESULTS FROM THE MALT90 SURVEY  

SciTech Connect (OSTI)

The chemical changes of high-mass star-forming regions provide a potential method for classifying their evolutionary stages and, ultimately, ages. In this study, we search for correlations between molecular abundances and the evolutionary stages of dense molecular clumps associated with high-mass star formation. We use the molecular line maps from Year 1 of the Millimetre Astronomy Legacy Team 90 GHz (MALT90) Survey. The survey mapped several hundred individual star-forming clumps chosen from the ATLASGAL survey to span the complete range of evolution, from prestellar to protostellar to H II regions. The evolutionary stage of each clump is classified using the Spitzer GLIMPSE/MIPSGAL mid-IR surveys. Where possible, we determine the dust temperatures and H{sub 2} column densities for each clump from Herschel/Hi-GAL continuum data. From MALT90 data, we measure the integrated intensities of the N{sub 2}H{sup +}, HCO{sup +}, HCN and HNC (1-0) lines, and derive the column densities and abundances of N{sub 2}H{sup +} and HCO{sup +}. The Herschel dust temperatures increase as a function of the IR-based Spitzer evolutionary classification scheme, with the youngest clumps being the coldest, which gives confidence that this classification method provides a reliable way to assign evolutionary stages to clumps. Both N{sub 2}H{sup +} and HCO{sup +} abundances increase as a function of evolutionary stage, whereas the N{sub 2}H{sup +} (1-0) to HCO{sup +} (1-0) integrated intensity ratios show no discernable trend. The HCN (1-0) to HNC(1-0) integrated intensity ratios show marginal evidence of an increase as the clumps evolve.

Hoq, Sadia; Jackson, James M.; Foster, Jonathan B.; Sanhueza, Patricio; Claysmith, Christopher [Institute for Astrophysical Research, Boston University, Boston, MA 02215 (United States); Guzmßn, AndrÚs [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Whitaker, J. Scott [Physics Department, Boston University, Boston, MA 02215 (United States); Rathborne, Jill M. [Australia Telescope National Facility, CSIRO Astronomy and Space Science, Epping, NSW (Australia); Vasyunina, Tatiana; Vasyunin, Anton, E-mail: shoq@bu.edu, E-mail: jackson@bu.edu, E-mail: patricio@bu.edu, E-mail: claysmit@bu.edu, E-mail: jonathan.b.foster@yale.edu, E-mail: aguzmanf@cfa.harvard.edu, E-mail: scott@bu.edu, E-mail: rathborne@csiro.au, E-mail: tv3h@virginia.edu, E-mail: aiv3f@virginia.edu [Department of Chemistry, University of Virginia, Charlottesville, VA 22904 (United States)

2013-11-10T23:59:59.000Z

143

Holocene climate evolution in the high-latitude Southern Hemisphere  

E-Print Network [OSTI]

through the iceÁ/albedo and iceÁ/insulation feedbacks. Our experiments can help to improve our atmosphereÁ/sea iceÁ/oceanÁ/vegetation model Hans Renssen,1* Hugues Goosse,2 Thierry Fichefet,2 Vale-long transient experiment performed with the ECBilt-CLIO-VECODE coupled atmosphereÁ/sea ice

Renssen, Hans

144

The variability of high-frequency acoustic backscatter from the region near the sea surface  

Science Journals Connector (OSTI)

The temporal variability of acoustic backscattering from the region near the sea surface is examined for frequencies in the 30ľ70 kHz range. A variance spectrum of the scattering strength exhibits effects associated with three different processes. Below about 0.1 Hz the spectrum contains a large contribution associated with temporal variations in the advection of bubble clouds through the measurement volume by large-scale processes. At high frequencies the spectrum asymptotes to a level characteristic of a Gaussian backscatteredpressure field from randomly moving bubbles within the scattering volume. The overall variability is treated as a slow modulation of this Gaussian process by larger-scale processes and a probability density function is derived for the scattering strength using Bayesĺ theorem. Finally in some cases the spectrum exhibits a peak at the frequency of the dominant surface waves. Attempts to compute coherence functions between the backscattered acoustic power and surface wave orbital velocities measured by a microwave system observing the same spot as the acoustic system resulted in very low values. This leads to the belief that the wave-induced peak in the acoustic backscatter variance spectrum is caused by highly nonlinear processes. A time series of acoustic backscatter from a vertically pointing system confirms the existence of this modulation at the dominant wave frequency and also suggests its nonlinear character.

Peter H. Dahl; William J. Plant

1997-01-01T23:59:59.000Z

145

Fault structure and kinematics of the Long Valley Caldera region, California, revealed by high-accuracy earthquake hypocenters and  

E-Print Network [OSTI]

Fault structure and kinematics of the Long Valley Caldera region, California, revealed by high that occurred between 1980 and 2000 in the Long Valley caldera area using a double- difference earthquake a series of east/west-striking right-lateral strike-slip faults beneath the caldera's south moat

Waldhauser, Felix

146

The Impact of Energy Shortage and Cost on Irrigation for the High Plains and Trans Pecos Regions of Texas  

E-Print Network [OSTI]

Plains and Trans Pecos regional economies is much greater than these statistics show. On the High Plains 86 percent of the cotton, 90 percent of the grain sorghum, and 75 percent of the wheat produced in 1974 was harvested from irrigated acreage. Rainfall...

Lacewell, R. D.; Condra, G. D.; Hardin, D. C.; Zavaleta, L.; Petty, J. A.

1978-01-01T23:59:59.000Z

147

ELUSIVE ETHYLENE DETECTED IN SATURN'S NORTHERN STORM REGION  

SciTech Connect (OSTI)

The massive eruption at 40 Degree-Sign N (planetographic latitude) on Saturn in 2010 December has produced significant and lasting effects in the northern hemisphere on temperature and species abundances. The northern storm region was observed on many occasions in 2011 by Cassini's Composite Infrared Spectrometer (CIRS). In 2011 May, temperatures in the stratosphere greater than 200 K were derived from CIRS spectra in the regions referred to as 'beacons' (warm regions in the stratosphere). Ethylene has been detected in the beacon region in Saturn's northern storm region using CIRS. Ground-based observations using the high-resolution spectrometer Celeste on the McMath-Pierce Telescope on 2011 May 15 were used to confirm the detection and improve the altitude resolution in the retrieved profile. The derived ethylene profile from the CIRS data gives a C{sub 2}H{sub 4} mole fraction of 5.9 {+-} 4.5 Multiplication-Sign 10{sup -7} at 0.5 mbar, and from Celeste data it gives 2.7 {+-} 0.45 Multiplication-Sign 10{sup -6} at 0.1 mbar. This is two orders of magnitude higher than the amount measured in the ultraviolet at other latitudes prior to the storm. It is also much higher than predicted by photochemical models, indicating that perhaps another production mechanism is required or a loss mechanism is being inhibited.

Hesman, B. E.; Achterberg, R. K.; Nixon, C. A. [Department of Astronomy, University of Maryland, College Park, MD 20742 (United States); Bjoraker, G. L.; Romani, P. N. [NASA/GSFC Code 693, Greenbelt, MD 20771 (United States); Sada, P. V. [Departamento de Fisica y Matematicas, Universidad de Monterrey, Garza Garcia, NL 66238 (Mexico); Jennings, D. E. [NASA/GSFC Code 693 and Code 500, Greenbelt, MD 20771 (United States); Lunsford, A. W. [Department of Physics, Catholic University of America, Washington, DC 20064 (United States); Fletcher, L. N.; Irwin, P. G. J. [Atmospheric, Oceanic and Planetary Physics, Clarendon Laboratory, Parks Road, Oxford OX1 3PU (United Kingdom); Boyle, R. J. [Department of Physics and Astronomy, Dickinson College, Carlisle, PA 17013 (United States); Simon-Miller, A. A., E-mail: brigette.e.hesman@nasa.gov [NASA/GSFC Code 690, Greenbelt, MD 20771 (United States)

2012-11-20T23:59:59.000Z

148

The domination of Saturn's low latitude ionosphere by ring `rain'  

E-Print Network [OSTI]

Saturn's ionosphere is produced when the otherwise neutral atmosphere is exposed to a flow of energetic charged particles or solar radiation. At low latitudes the latter should result in a weak planet-wide glow in infrared (IR), corresponding to the planet's uniform illumination by the Sun. The observed low-latitude ionospheric electron density is lower and the temperature higher than predicted by models. A planet-ring magnetic connection has been previously suggested in which an influx of water from the rings could explain the lower than expected electron densities in Saturn's atmosphere. Here we report the detection of a pattern of features, extending across a broad latitude band from ~25 to 60 degrees, that is superposed on the lower latitude background glow, with peaks in emission that map along the planet's magnetic field lines to gaps in Saturn's rings. This pattern implies the transfer of charged water products from the ring-plane to the ionosphere, revealing the influx on a global scale, flooding betw...

O'Donoghue, J; Melin, H; Jones, G H; Cowley, S W H; Miller, S; Baines, K H; Blake, J S D

2013-01-01T23:59:59.000Z

149

Heavy Primary Cosmic Rays at Geomagnetic Latitude of 41░N  

Science Journals Connector (OSTI)

This report includes the results from 9 balloon flights at geomagnetic latitude 41░N of altitude range from 70 000 to 100 000 feet. Only primaries of Z>~10 are considered. 2410 tracks are involved, in Ilford G-5 and G-0 emulsion exposures. Given are the charge spectra, flux, mean free paths, and angular distributions.

O. B. Young and H. Y. Chen

1959-09-15T23:59:59.000Z

150

LARGE SCALE CHANGES IN THE HIGHLY ENERGETIC CHARGED PARTICLES IN THE REGION OF THE IO TORUS  

E-Print Network [OSTI]

that they are caused by energetic trapped particles. On the C22 pass through the torus region the count rates were pass, the background count rate was low until inside the orbit of Io with a dip in the count rate 1 Institute of Geophysics and Planetary Physics, University of California Los Angeles, CA 90095

Russell, Christopher T.

151

Spitzer IRAC and MIPS Imaging of Clusters and Outflows in 9 High-mass Star Forming Regions  

E-Print Network [OSTI]

We present Spitzer Space Telescope IRAC and MIPS observations toward a sample of nine high-mass star forming regions at a distance of around 2 kpc. Based on IRAC and MIPS 24 $\\mu$m photometric results and 2MASS JHKs data, we carry out a census of young stellar objects (YSOs) in a 5' by 5' field toward each region. Toward seven out of the nine regions, we detect parsec sized clusters with around 20 YSOs surrounded by a more extended and sparse distribution of young stars and protostars. For the other two regions, IRAS 20126+4104 and IRAS 22172+5549, the former has the lowest number of YSOs in the sample and shows no obvious cluster, and the latter appears to be part of a larger, potentially more evolved cluster. The deep IRAC imaging reveals at least twelve outflows in eight out of the nine regions, with nine outflows prominent in the 4.5 $\\mu$m band most probably attributed to shocked H$_2$ emission, two outflows dominated by scattered light in the 3.6 and 4.5 $\\mu$m bands, and one outflow standing out from its hydrocarbon emission in the 8.0 $\\mu$m band. In comparison with previous ground-based observations, our IRAC observations reveal new outflow structures in five regions. The dramatically different morphologies of detected outflows can be tentatively interpreted in terms of possible evolution of massive outflows. The driving sources of these outflows are deeply embedded in dense dusty cores revealed by previous millimeter interferometric observations. We detect infrared counterparts of these dusty cores in the IRAC or MIPS 24 $\\mu$m bands. Reflection nebulae dominated by the emission from UV heated hydrocarbons in the 8 $\\mu$m band can be found in most regions and they may imply the presence of young B stars.

Keping Qiu; Qizhou Zhang; S. Thomas Megeath; Robert A. Gutermuth; Henrik Beuther; Debra S. Shepherd; T. K. Sridharan; L. Testi; C. G. De Pree

2008-06-16T23:59:59.000Z

152

High-frequency spectra of regional phases from earthquakes and chemical explosions  

Science Journals Connector (OSTI)

...realistic oceanic Pn wave trains, J. Geophys. Res. 90 , 12755-12776. Smith A. T. (1989). High-frequency seismic observations...realistic oceanic Pn wave trains, J. Geophys. Res. 90, 12755-12776. Smith, A. T. (1989). High-frequency seismic observations...

W. Y. Kim; D. W. Simpson; P. G. Richards

153

WIND-DRIVEN NEAR INERTIAL OCEAN RESPONSE AND MIXING AT THE CRITICAL LATITUDE  

E-Print Network [OSTI]

? latitude. Near 30? latitude, the maximum oceanic response to sea breeze moves offshore slowly because of the near-zero group speed of Poincare waves at this latitude. The lateral energy flux convergence plus the energy input from the wind is maximum near...

Zhang, Xiaoqian

2010-07-14T23:59:59.000Z

154

High resolution far-infrared observations of the evolved H II region M16  

SciTech Connect (OSTI)

M16 is an evolved, extremely density bounded H II region, which now consists only of a series of ionization fronts at molecular cloud boundaries. The source of ionization is the OB star cluster (NGC 6611) which is about 5 x 10/sup 6/ years old. We used the CFA/UA 102 cm balloon-borne telescope to map this region and detected three far-infrared (far-IR) sources embedded in an extended ridge of emission. Source I is an unresolved far-IR source embedded in a molecular cloud near a sharp ionization front. An H/sub 2/O maser is associated with this source, but no radio continuum emission has been observed. The other two far-IR sources (II and III) are associated with ionized gas-molecular cloud interfaces, with the far-IR radiation arising from dust at the boundary heated by the OB cluster. Source II is located at the southern prominent neutral intrusion with its associated bright rims and dark ''elephant trunk'' globules that delineate the current progress of the ionization front into the neutral material, and Source III arises at the interface of the northern molecular cloud fragment.

McBreen, B.; Fazio, G.G.; Jaffe, D.T.

1982-03-01T23:59:59.000Z

155

A New Microwave Temperature Profiler ┬ů First Measurements in Polar Regions  

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

Microwave Temperature Profiler - First Microwave Temperature Profiler - First Measurements in Polar Regions E. N. Kadygrov, A. V. Koldaev, and A. S. Viazankin Central Aerological Observatory Moscow, Russia A. Argentini, and A. Conidi Institute of Atmospheric Physics CNR, Italy Introduction Temperature inversions are a ubiquitous feature of the high latitude atmospheric boundary layer (ABL). In Polar Regions, the temperature inversion is a complicated phenomenon involving interactions between surface radiative cooling, subsidence and warm air advection. In the period 1997-2002, several microwave temperature profilers were used to measure temperature inversion parameters at one of the three sites of the U.S. Department of Energy (DOE) Atmospheric Radiation Measurement (ARM)

156

Neutral Pion Electroproduction in the Resonance Region at High $Q^2$  

E-Print Network [OSTI]

The process $ep \\to e^{\\prime}p^{\\prime}\\pi^0$ has been measured at $Q^2$ = 6.4 and 7.7 GeV/c$^2$)$^2$ in Jefferson Lab's Hall C. Unpolarized differential cross sections are reported in the virtual photon-proton center of mass frame considering the process $\\gamma^{\\ast}p \\to p^{\\prime}\\pi^0$. Various details relating to the background subtractions, radiative corrections and systematic errors are discussed. The usefulness of the data with regard to the measurement of the electromagnetic properties of the well known $\\Delta(1232)$ resonance is covered in detail. Specifically considered are the electromagnetic and scalar-magnetic ratios $R_{EM}$ and $R_{SM}$ along with the magnetic transition form factor $G_M^{\\ast}$. It is found that the rapid fall off of the $\\Delta(1232)$ contribution continues into this region of momentum transfer and that other resonances

A. N. Villano; P. Stoler; P. E. Bosted; S. H. Connell; M. M. Dalton; M. K. Jones; V. Kubarovsky; G. S Adams; A. Ahmidouch; J. Arrington; R. Asaturyan; O. K. Baker; H. Breuer; M. E. Christy; S. Danagoulian; D. Day; J. A. Dunne; D. Dutta; R. Ent; H. C. Fenker; V. V. Frolov; L. Gan; D. Gaskell; W. Hinton; R. J. Holt; T. Horn; G. M. Huber; K. Joo; N. Kalantarians; C. E. Keppel; Y. Li; A. Lung; D. Mack; S. Malace; P. Markowitz; D. G. Meekins; H. Mkrtchyan; J. Napolitano; G. Niculescu; I. Niculescu; D. H. Potterveld; Paul E. Reimer; J. Reinhold; J. Roche; S. E. Rock; G. R. Smith; S. Stepanyan; V. Tadevosyan; V. Tvaskis; M. Ungaro; A. Uzzle; S. Vidakovic; F. R. Wesselmann; B. Wojtsekhowski; S. A. Wood; L. Yuan; X. Zheng; H. Zhu

2009-09-26T23:59:59.000Z

157

High Q-value resonators for the SHF-region based on TBCCO-films  

SciTech Connect (OSTI)

The authors used a sapphire dielectric resonator with a copper cylindrical shield and two endplates replaced by HTS layers for very accurate surface resistance measurements of TBCCO films made by the two step method. This technique allows for the preparation of high quality 2-in diameter Tl-2223 superconducting films with surface resistance values (R{sub s}) smaller than 100 {micro}{Omega} at 5.6 GHz and 77 K. The use of these films in sapphire dielectric resonators yields resonators for the C-band with very high unloaded quality factors (Q{sub o} > 2 {times} 10{sup 6} at 77 K). Such high Q{sub o}-values are not reached with any conventional resonators of comparable size.

Manzel, M.; Huber, S.; Bruchlos, H.; Bornmann, S.; Goernert, P. [Inst. fuer Physikalische Hochtechnologie, Jena (Germany)] [Inst. fuer Physikalische Hochtechnologie, Jena (Germany); Klinger, M.; Stiller, M. [Forschungsgesellschaft fuer Informationstechnik, Bad Salzdetfurth (Germany)] [Forschungsgesellschaft fuer Informationstechnik, Bad Salzdetfurth (Germany)

1996-07-01T23:59:59.000Z

158

Beyond Basic Region Caching: Specializing Cache Structures for High Performance and Energy  

E-Print Network [OSTI]

's usage char- acteristics provides many potential benefits: faster access times, lower energy con a small heap footprint, we save energy by using the smaller structure and turn off the larger. For applications with larger footprints, we use both structures, but save energy by keeping highly used "hot" data

McKee, Sally A.

159

Analytical investigation of collector optimum tilt angle at low latitude  

Science Journals Connector (OSTI)

An analytical investigation on the optimum tilt angle for solar collectors at low latitude a case study of Universiti Teknologi PETRONAS (UTP) 4.39░N and 100.98░E Malaysia is presented in this work. The study employed Hay Davies Klucher and Reindl (HDKR) anisotropic sky model to evaluate the available hourly solar radiation on inclined surface using the location metrological data. The tilt angles considered were 0░ to 30░ in step of 3░ with the inclusion of the location latitude angle. The study employed the ratio of global solar radiation on tilted surface to the global solar radiation on horizontal surface in the decision of the optimum tilt. The system equations were converted to MATLAB codes to solve for the optimum tilt angles. The results show that the optimum tilt varies monthly but gave zero degree for south facing collector for the months of April to August; thus the investigation also considered north facing orientation for the months of April to September. The optimum annual tilt angle for the location using the tilt to horizontal radiation ratio was found to be equal to the location latitude angle. Using the conventional average of the monthly optimum tilt angles the annual optimum tilt angle was found to be 9.75░ for south facing collector. Considering seasonal optimum tilt angle for the location using the tilt to horizontal radiation ratio 18░ facing south was found to be the optimum tilt angle for rainy season (September to March) and 15░ facing north for dry season (April to August). Employing the average of monthly optimum tilt method the seasonal optimum tilt angle was found to be 17░ for rainy season and 12░ facing north dry season. The effect of dust on the collector was considered with reference to literature and the annual tilt angle of 15░ facing south was recommended for the location in the case of large solar collector that cannot be monthly or seasonally adjusted.

Ogboo Chikere Aja; Hussain H. Al-Kayiem; Zainal Ambri Abdul Karim

2013-01-01T23:59:59.000Z

160

Exploration of Quench Initiation Due to Intentional Geometrical Defects in a High Magnetic Field Region of an SRF Cavity  

SciTech Connect (OSTI)

A computer program which was used to simulate and analyze the thermal behaviors of SRF cavities has been developed at Jefferson Lab using C++ code. This code was also used to verify the quench initiation due to geometrical defects in high magnetic field region of SRF cavities. We built a CEBAF single cell cavity with 4 artificial defects near equator, and this cavity has been tested with T-mapping. The preheating behavior and quench initiation analysis of this cavity will be presented here using the computer program.

J. Dai, K. Zhao, G.V. Eremeev, R.L. Geng, A.D. Palczewski; Dai, J. [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Palczewski, A. D. [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Eremeev, G. V. [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Geng, R. L. [Thomas Jefferson National Accelerator Facility, Newport News, VA (United States); Zhao, K. [Institute of Heavy Ion Physics, Peking University, Beijing (China)

2011-07-01T23:59:59.000Z

Note: This page contains sample records for the topic "high latitude regions" 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

Molecular Outflows in Low- and High-Mass Star Forming Regions  

E-Print Network [OSTI]

We review the known properties of molecular outflows from low- and high-mass young stars. General trends among outflows are identified, and the most recent studies on the morphology, kinematics, energetics, and evolution of molecular outflows are discussed, focusing on results from high-resolution millimeter observations. We review the existing four broad classes of outflow models and compare numerical simulations with the observational data. A single class of models cannot explain the range of morphological and kinematic properties that are observed, and we propose a possible solution. The impact of outflows on their cloud is examined, and we review how outflows can disrupt their surrounding environment, through the clearing of gas and the injection of momentum and energy onto the gas at distances from their powering sources from about 0.01 to a few pc. We also discuss the effects of shock-induced chemical processes on the ambient medium, and how these processes may act as a chemical clock to date outflows. Lastly, future outflow research with existing and planned millimeter and submillimeter instruments is presented.

Hector G. Arce; Debra Shepherd; Frederic Gueth; Chin-Fei Lee; Rafael Bachiller; Alexander Rosen; Henrik Beuther

2006-03-03T23:59:59.000Z

162

High-frequency absorption of the dynamic mixed state in the surface superconductivity region  

SciTech Connect (OSTI)

We analyze the absorption of a high-frequency electromagnetic field in the type II superconductor Pb{sub 0.8}In{sub 0.2} in magnetic fields H{sub c2} < H < H{sub c3}. The absorption component proportional to the rate of variation of the external magnetic field is detected. We assume that this absorption component is associated with the dynamic mixed state of the superconducting shell containing 2D magnetic flux vortices (Kulik vortices). The motion of these vortices under the action of the critical current ensures the required difference between the external and internal magnetic inductions of the superconducting shell upon a change in the external magnetic field. This model correctly describes the observed behavior of absorption of rf electromagnetic radiation.

Berezin, V. A., E-mail: berezin@iptm.ru; Tulin, V. A., E-mail: tulin@iptm.ru [Russian Academy of Sciences, Institute of Microelectronics Technology and High-Purity Materials (Russian Federation)

2013-03-15T23:59:59.000Z

163

Specification of fields quality in the interaction region magnets of the high luminosity LHC based on dynamic aperture  

E-Print Network [OSTI]

New large aperture Inner Triplet quadrupoles, separation dipoles and the nearby matching quadrupoles will be installed in the low-beta interaction regions (IR) of the high luminosity LHC upgrade (HL-LHC) [1]. The large aperture is necessary for accommodating the increased beam size due to much higher beta functions in these magnets for the low collision optics. The high beta functionswill amplify the effects of field errors in the new magnets leading to a smaller dynamic aperture (DA). It is, therefore, critical to evaluate the impact of these errors on the DA and specify the magnet field quality (FQ) satisfying an acceptable DA while being realistically achievable. The study is performed for the HL-LHC lattice layouts SLHCV3.1b and HLLHCV1.0 for collision and injection energies.

Nosochkov, Y; Wang, M H; Fartoukh, S; Giovannozzi, M; De Maria, R; McIntosh, E

2014-01-01T23:59:59.000Z

164

GALACTIC ALL-SKY SURVEY HIGH-VELOCITY CLOUDS IN THE REGION OF THE MAGELLANIC LEADING ARM  

SciTech Connect (OSTI)

We present a catalog of high-velocity clouds in the region of the Magellanic Leading Arm. The catalog is based on neutral hydrogen (H I) observations from the Parkes Galactic All-Sky Survey. Excellent spectral resolution allows clouds with narrow-line components to be resolved. The total number of detected clouds is 419. We describe the method of cataloging and present the basic parameters of the clouds. We discuss the general distribution of the high-velocity clouds and classify the clouds based on their morphological type. The presence of a significant number of head-tail clouds and their distribution in the region is discussed in the context of Magellanic System simulations. We suggest that ram-pressure stripping is a more important factor than tidal forces for the morphology and formation of the Magellanic Leading Arm and that different environmental conditions might explain the morphological difference between the Magellanic Leading Arm and Magellanic Stream. We also discuss a newly identified population of clouds that forms the LA IV and a new diffuse bridge-like feature connecting the LA II and III complexes.

For, Bi-Qing; Staveley-Smith, Lister [International Centre for Radio Astronomy Research, University of Western Australia, 35 Stirling Hwy, Crawley, WA 6009 (Australia)] [International Centre for Radio Astronomy Research, University of Western Australia, 35 Stirling Hwy, Crawley, WA 6009 (Australia); McClure-Griffiths, N. M., E-mail: biqing.for@uwa.edu.au [Australia Telescope National Facility, CSIRO Astronomy and Space Science, PO Box 76, Epping, NSW 1710 (Australia)

2013-02-10T23:59:59.000Z

165

Major shifts in calcareous phytoplankton assemblages through the Eocene-Oligocene transition of Tanzania and their implications for low-latitude primary production  

E-Print Network [OSTI]

in the deep sea, significant glaciomarine sedimen- tation commences around the margins of both East and West Antarctica indicating the first Cenozoic advance of conti- nental-scale ice sheets in southern high latitudes [Breza and Wise, 1992; Ivany et al., 2006... patterns. In low south- ern latitudes the present-day western boundary of the Indian Ocean is dominated by the northward flowing East African Coastal Current (EACC), which is sourced from the west- ward flowing South Equatorial Current (SEC) [Swallow et al...

Jones, Tom Dunkley; Bown, Paul R.; Pearson, Paul N.; Wade, Bridget S.; Coxall, Helen K.; Lear, Caroline H.

166

Magnetic Landscape of Sun's Polar Region  

E-Print Network [OSTI]

We present the magnetic landscape of the polar region of the Sun that is unprecedented in terms of high spatial resolution, large field of view, and polarimetric precision. These observations were carried out with the Solar Optical Telescope aboard \\emph{Hinode}. Using a Milne-Eddington inversion, we found many vertically-oriented magnetic flux tubes with field strength as strong as 1 kG that are scattered in latitude between 70-90 degree. They all have the same polarity, consistent with the global polarity of the polar region. The field vectors were observed to diverge from the center of the flux elements, consistent with a view of magnetic fields that expand and fan out with height. The polar region is also covered with ubiquitous horizontal fields. The polar regions are the source of the fast solar wind channelled along unipolar coronal magnetic fields whose photospheric source is evidently rooted in the strong field, vertical patches of flux. We conjecture that vertical flux tubes with large expansion around the photosphere-corona boundary serve as efficient chimneys for Alfven waves that accelerate the solar wind.

S. Tsuneta; K. Ichimoto; Y. Katsukawa; B. W. Lites; K. Matsuzaki; S. Nagata; D. Orozco Suarez; T. Shimizu; M. Shimojo; R. A. Shine; Y. Suematsu; T. K. Suzuki; T. D. Tarbell; A. M. Title

2008-08-08T23:59:59.000Z

167

Carbon dioxide in Arctic and subarctic regions  

SciTech Connect (OSTI)

A three year research project was presented that would define the role of the Arctic ocean, sea ice, tundra, taiga, high latitude ponds and lakes and polar anthropogenic activity on the carbon dioxide content of the atmosphere. Due to the large physical and geographical differences between the two polar regions, a comparison of CO/sub 2/ source and sink strengths of the two areas was proposed. Research opportunities during the first year, particularly those aboard the Swedish icebreaker, YMER, provided additional confirmatory data about the natural source and sink strengths for carbon dioxide in the Arctic regions. As a result, the hypothesis that these natural sources and sinks are strong enough to significantly affect global atmospheric carbon dioxide levels is considerably strengthened. Based on the available data we calculate that the whole Arctic region is a net annual sink for about 1.1 x 10/sup 15/ g of CO/sub 2/, or the equivalent of about 5% of the annual anthropogenic input into the atmosphere. For the second year of this research effort, research on the seasonal sources and sinks of CO/sub 2/ in the Arctic will be continued. Particular attention will be paid to the seasonal sea ice zones during the freeze and thaw periods, and the tundra-taiga regions, also during the freeze and thaw periods.

Gosink, T. A.; Kelley, J. J.

1981-03-01T23:59:59.000Z

168

Thermo-physical and structural studies of sodium zinc borovanadate glasses in the region of high concentration of modifier oxides  

SciTech Connect (OSTI)

Highlights: ? Highly modified sodium zinc borovanadate glasses. ? Structural model for borovanadate glasses. ? Network forming tendency of ZnO in borovanadate glasses. ? Fragility can be limited to NBO concentration in borovanadate glasses. -- Abstract: This paper reports investigation of Na{sub 2}O and ZnO modified borovanadate glasses in the highly modified regime of compositions. These glasses have been prepared by microwave route. Ultraviolet (UV) and visible, infrared (IR), Magic Angle Spinning Nuclear Magnetic Resonance (MAS NMR) and Electron Paramagnetic Resonance (EPR) spectroscopies have been used to characterize the speciation in the glasses. Together with the variation of properties such as molar volume and glass transition temperatures, spectroscopic data indicate that at high levels of modification, ZnO tends to behave like network former. It is proposed that the observed variation of all the properties can be reasonably well understood with a structural model. The model considers that the modification and speciation in glasses are strongly determined by the hierarchy of group electronegativities. Further, it is proposed that the width of the transitions of glasses obtained under same condition reflects the fragility of the glasses. An empirical expression has been suggested to quantify fragility on the basis of width of the transition regions.

Chethana, B.K. [Solid State and Structural Chemistry Unit, Indian Institute of Science, Bangalore 560 012 (India)] [Solid State and Structural Chemistry Unit, Indian Institute of Science, Bangalore 560 012 (India); Reddy, C. Narayana [Maharani's Science College for Women, Bangalore 560 001 (India)] [Maharani's Science College for Women, Bangalore 560 001 (India); Rao, K.J., E-mail: kalyajrao@yahoo.co.in [Solid State and Structural Chemistry Unit, Indian Institute of Science, Bangalore 560 012 (India)

2012-07-15T23:59:59.000Z

169

Effects of solar activity on myocardial infarction deaths in low geomagnetic latitude regions  

Science Journals Connector (OSTI)

We study the effect of solar activity on the incidence of myocardial infarction deaths (MID) in Mexico. We work with 129,917 cases along ... by sex and age, and considering the solar cycle phases. At higher frequ...

Blanca Mendoza; Rosa Diaz-Sandoval

2004-05-01T23:59:59.000Z

170

Classical dynamics and localization of resonances in the high energy region of the hydrogen atom in crossed fields  

E-Print Network [OSTI]

When superimposing the potentials of external fields on the Coulomb potential of the hydrogen atom a saddle point appears, which is called the Stark saddle point. For energies slightly above the saddle point energy one can find classical orbits, which are located in the vicinity of this point. We follow those so-called quasi-Penning orbits to high energies and field strengths observing structural changes and uncovering their bifurcation behavior. By plotting the stability behavior of those orbits against energy and field strength the appearance of a stability apex is reported. A cusp bifurcation, located in the vicinity of the apex, will be investigated in detail. In this cusp bifurcation another orbit of similar shape is found, which becomes completely stable in the observed region of positive energy, i.e., in a region of parameter space, where the Kepler-like orbits located around the nucleus are already unstable. By quantum-mechanically exact calculations we prove the existence of signatures in quantum spectra belonging to those orbits. Husimi distributions are used to compare quantum-Poincar\\'e sections with the extension of the classical torus structure around the orbits. Since periodic orbit theory predicts that each classical periodic orbit contributes an oscillating term to photoabsorption spectra, we finally give an estimation for future experiments, which could verify the existence of the stable orbits.

Frank Schweiner; J÷rg Main; Holger Cartarius; GŘnter Wunner

2014-12-10T23:59:59.000Z

171

Large methane emission upon spring thaw from natural wetlands in the northern permafrost region  

SciTech Connect (OSTI)

The permafrost carbon climate feedback is one of the major mechanisms in controlling the climate ecosystem interactions in northern high latitudes. Of this feedback, methane (CH4) emission from natural wetlands is critically important due to its high warming potential. The freeze thaw transition has been confirmed to play an important role in annual CH4 budget, yet the magnitude of this effect is uncertain. An intensive field campaign was carried out in the Sanjiang Plain, Northeast China to estimate the CH4 emission in the spring freeze thaw transition period. The observation concluded that a large CH4 source was caused by spring thaw; the maximum hourly emission rate was 48.6 g C m 2 h 1, more than three orders of the regularly observed CH4 emission rate in the growing season. In some sporadically observed 'hot spots', the spring thawing effect contributed to a large CH4 source of 31.3 10.1 g C m 2, which is approximately 80% of the previously calculated annual CH4 emission in the same study area. If our results are typical for natural wetlands in the Northern Hemisphere permafrost region, we estimate a global CH4 source strength of 0.5 1.0 Tg C (1 Tg =1012 g) caused by spring thaw in the Northern Hemisphere permafrost region in the year 2011. Combining with available satellite and flask data, a regional extrapolation reaches a temporal pattern of CH4 emission during 2003 2009 which is consistent with recently observed changes in atmospheric CH4 concentration in the high latitudes. This suggests that the CH4 emission upon spring thaw in the high latitudes might be enhanced by the projected climate warming. These findings indicate that the spring thawing effect is an important mechanism in the permafrost carbon climate feedback and needs to be incorporated in Earth system models.

Song, Changchun [Chinese Academy of Sciences; Xu, Xiaofeng [ORNL; Sun, Xiaoxin [Chinese Academy of Sciences; Tian, Hanqin [Auburn University, Auburn, Alabama; Sun, Li [Chinese Academy of Sciences; Miao, Yuqing [Chinese Academy of Sciences; Wang, Xianwei [Chinese Academy of Sciences; Guo, Yuedong [Chinese Academy of Sciences

2012-01-01T23:59:59.000Z

172

Structural impacts of the 1985 farm bill on typical farms in the Texas Southern High Plains and delta region of Mississippi  

E-Print Network [OSTI]

STRUCTURAL IMPACTS OF THK 1985 FARM BILL ON TYPICAL FARMS IN THK TEXAS SOUTHERN HIGH PLAINS AND DELTA REGION OF MISSISSIPPI A Thesis by CHARLES FREDERICK MILLER Submitted to the Graduate College of Texas A&M University in partial fulfillment... of the requirement for the degree of MASTER OF SCIENCE August 1988 Major Subject: Agricultural Economics STRUCTURAL IMPACTS OF THE 1985 FARM BILL ON TYPICAL FARMS IN THE TEXAS SOUTHERN HIGH PLAINS AND DELTA REGION OF MISSISSIPPI A Thesis by CHARLES FREDERICK...

Miller, Charles Frederick

2012-06-07T23:59:59.000Z

173

Building America Best Practices Series, Volume 7.1 - High-Performance Home Technologies: Guide to Determining Climate Regions by County  

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

HOT-HUMID HOT-HUMID MIXED-HUMID COLD / VERY COLD HOT-DRY / MIXED-DRY MARINE PREPARED BY Pacific Northwest National Laboratory & Oak Ridge National Laboratory August 2010 August 2010 * PNNL-17211 CLIMATE REGIONS VOLUME 7.1 R HIGH-PERFORMANCE HOME TECHNOLOGIES Guide to Determining Climate Regions by County BUILDING AMERICA BEST PRACTICES SERIES BUILDING AMERICA BEST PRACTICES SERIES VOLUME 7.1 High-Performance Home Technologies: Guide to Determining Climate Regions by County PREPARED BY Pacific Northwest National Laboratory Michael C. Baechler Jennifer Williamson, Theresa Gilbride, Pam Cole, and Marye Hefty

174

Detection and Attribution of Regional Climate Change  

SciTech Connect (OSTI)

We developed a high resolution global coupled modeling capability to perform breakthrough studies of the regional climate change. The atmospheric component in our simulation uses a 1{sup o} latitude x 1.25{sup o} longitude grid which is the finest resolution ever used for the NCAR coupled climate model CCSM3. Substantial testing and slight retuning was required to get an acceptable control simulation. The major accomplishment is the validation of this new high resolution configuration of CCSM3. There are major improvements in our simulation of the surface wind stress and sea ice thickness distribution in the Arctic. Surface wind stress and ocean circulation in the Antarctic Circumpolar Current are also improved. Our results demonstrate that the FV version of the CCSM coupled model is a state of the art climate model whose simulation capabilities are in the class of those used for IPCC assessments. We have also provided 1000 years of model data to Scripps Institution of Oceanography to estimate the natural variability of stream flow in California. In the future, our global model simulations will provide boundary data to high-resolution mesoscale model that will be used at LLNL. The mesoscale model would dynamically downscale the GCM climate to regional scale on climate time scales.

Bala, G; Mirin, A

2007-01-19T23:59:59.000Z

175

latitude 2100 What if you could get fast internet access to check emails on the  

E-Print Network [OSTI]

the same┬Ě image commonality as the rest of your corporate notebooks? discover smart Functionality Smart, with Linux┬« or Microsoft┬« options. You can also make your laptop an extension of your business brand of the Latitude family, giving you the power to take advantage of our Latitude commitment to manageability, image

Fiebig, Peter

176

The Influence of Meridional Shear on Planetary Waves. Part 2: Critical Latitudes  

Science Journals Connector (OSTI)

With the simplifying assumption that the mean zonal wind is a function of latitude only, numerical and analytical methods are applied to study the effects of critical latitudes (where the Doppler-shifted frequency is 0) on planetary waves. On the ...

John P. Boyd

1982-04-01T23:59:59.000Z

177

First VUV full-Sun spectrum of the transition region with high spectral resolution compared to cool stars  

E-Print Network [OSTI]

This paper reports the first full-Sun vacuum ultraviolet (VUV) emission line profile originating from the transition region from the chromosphere to the corona. It is based on a raster scan of the whole solar disk using SUMER/SOHO. The full-Sun spectrum has a spectral resolution which allows an investigation of details in the line profile as well as a thorough comparison to stellar spectra as obtained, e.g. with FUSE or STIS/HST. The full-Sun spectrum shows enhanced emission in the wings, and is well described by a double Gaussian fit with a narrow and a broad component. It is shown that the broad component is due to structures on the solar surface, especially those related to the magnetic chromospheric network. Thus it is proposed that the broad components of other solar-like stars are also a consequence of the mixture of surface structures, and not necessarily a signature of small-scale heating processes like explosive events, as it is commonly argued. A comparison to spectra of luminous cool stars shows that the line asymmetries of these stars might also be a surface structure effect and not or only partly due to opacity effects in their cool dense winds. These comparisons show the potential of high quality full-Sun VUV spectra and their value for the study of solar-stellar connections. As an example, this study proposes that alpha Cen A has a considerably higher amount of magnetic flux concentrated in the chromospheric magnetic network than the Sun.

Hardi Peter

2005-10-11T23:59:59.000Z

178

Hybrid thermal model for swimming pools based on artificial neural networks for southeast region of Brazil  

Science Journals Connector (OSTI)

Nowadays, the usage of systems based on solar energy have been largely stimulated. The correct designing and efficiency of these systems are highly dependent of the seasonal climatic characteristics of the regions where they will be installed. In this work, we propose a hybrid structure to simulate the thermodynamic behavior of pools, which uses neural computational models to incorporate the climatic information of the regions being analyzed. The neural models have as input variables data of geographic position such as: elevation, latitude and longitude, what permits to delineate the climatic profile of the region being considered. The human activity is another factor that directly influences the thermodynamic behavior of pools and, therefore, is also considered. In this work, changes of volume are estimated in order to track losses due to the human activity.

Enock T. Santos; Luis E. Zßrate; Elizabeth M.D. Pereira

2013-01-01T23:59:59.000Z

179

Emission in the 50ľ80-┼ region from highly ionized silver in Princeton Large Torus tokamak plasmas  

Science Journals Connector (OSTI)

The spectrum of silver emitted by Princeton Large Torus tokamak plasmas has been recorded in the 25ľ150-┼ region by a multichannel time-resolving grazing-incidence spectrometer. Silver...

Schwob, J L; Finkenthal, M; Wouters, A; Suckewer, S; Cohen, S A

1986-01-01T23:59:59.000Z

180

COLLABORATIVE RESEARCH: TOWARDS ADVANCED UNDERSTANDING AND PREDICTIVE CAPABILITY OF CLIMATE CHANGE IN THE ARCTIC USING A HIGH-RESOLUTION REGIONAL ARCTIC CLIMATE SYSTEM MODEL  

SciTech Connect (OSTI)

The motivation for this project was to advance the science of climate change and prediction in the Arctic region. Its primary goals were to (i) develop a state-of-the-art Regional Arctic Climate system Model (RACM) including high-resolution atmosphere, land, ocean, sea ice and land hydrology components and (ii) to perform extended numerical experiments using high performance computers to minimize uncertainties and fundamentally improve current predictions of climate change in the northern polar regions. These goals were realized first through evaluation studies of climate system components via one-way coupling experiments. Simulations were then used to examine the effects of advancements in climate component systems on their representation of main physics, time-mean fields and to understand variability signals at scales over many years. As such this research directly addressed some of the major science objectives of the BER Climate Change Research Division (CCRD) regarding the advancement of long-term climate prediction.

Gutowski, William J.

2013-02-07T23:59:59.000Z

Note: This page contains sample records for the topic "high latitude regions" from the National Library of EnergyBeta (NLEBeta).
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to obtain the most current and comprehensive results.


181

Solar: monthly latitude tilt GIS data at 40km resolution for Bangladesh  

Open Energy Info (EERE)

latitude tilt GIS data at 40km resolution for Bangladesh latitude tilt GIS data at 40km resolution for Bangladesh from NREL Dataset Summary Description (Abstract): Monthly Average Solar Resource for flat-plate collectors tilted at latitude for Bangladesh. (Purpose): Provide information on the solar resource potential for the data domain. The insolation values represent the average solar energy available to a flat plate collector, such as a photovoltaic panel, oriented due south at an angle from horizontal equal to the latitude of the collector location. (Supplemental Information): These data provide monthly average and annual average daily total solar resource averaged over surface cells of approximately 40 km by 40 km in size. The solar resource value is represented as watt-hours per square meter per day for each month. The

182

Why do model tropical cyclones intensify more rapidly at low latitudes?  

Science Journals Connector (OSTI)

We examine the problem of why model tropical cyclones intensify more rapidly at low latitudes. Our answer to this question touches on practically all facets of the dynamics and thermodynamics of tropical cyclones. The answer invokes the ...

Roger K. Smith; Gerard Kilroy; Michael T. Montgomery

183

Solar: monthly and annual latitude tilt horizontal GIS data at 40km  

Open Energy Info (EERE)

latitude tilt horizontal GIS data at 40km latitude tilt horizontal GIS data at 40km resolution for Nepal from NREL Dataset Summary Description (Abstract): Monthly Average Solar Resource for flat-plate collectors tilted at latitude for Nepal. (Purpose): Provide information on the solar resource potential for the data domain. The insolation values represent the average solar energy available to a flat plate collector, such as a photovoltaic panel, oriented due south at an angle from horizontal equal to the latitude of the collector location. (Supplemental Information): These data provide monthly average and annual average daily total solar resource averaged over surface cells of approximately 40 km by 40 km in size. The solar resource value is represented as watt-hours per square meter per day for each month. The

184

Altitude and latitude variations in avionics SEU and atmospheric neutron flux  

SciTech Connect (OSTI)

The direct cause of single event upsets in SRAMs at aircraft altitudes by the atmospheric neutrons has previously been documented. The variation of the in-flight SEU rate with latitude is demonstrated by new data over a wide range of geographical locations. New measurements and models of the atmospheric neutron flux are also evaluated to characterize its variation with altitude, latitude and solar activity.

Normand, E.; Baker, T.J. (Boeing Defense and Space Group, Seattle, WA (United States))

1993-12-01T23:59:59.000Z

185

Resampling Methods and High-Dimensional Data, Texas A&M, 3/25/2010 Analyzing and Combining Regional  

E-Print Network [OSTI]

, snowpack, etc. ┬ş Skiing, fire, water, crops, public health, power, etc. ┬Ě Generating regional climate in to Geosciences National Center for Atmospheric Research Boulder, CO Claudia Tebaldi, Climate Central; Cari. ┬Ě An atmosphere-ocean general circulation model (AOGCM or GCM) couples an atmosphere model with an ocean model

Sain, Steve

186

Solar desalination in the southwest United States| A thermoeconomic analysis utilizing the sun to desalt water in high irradiance regions.  

E-Print Network [OSTI]

?? Water scarcity and high irradiance overlap in the southwestern United States. This thesis explores solar energy as a method to power desalination in theů (more)

Stroud, Matthew

2012-01-01T23:59:59.000Z

187

Supplemental Guide for Seasonal High Water Table Indicators in Georgia's Onsite Wastewater Manual Section C: Flatwoods Region  

E-Print Network [OSTI]

1 Supplemental Guide for Seasonal High Water Table Indicators in Georgia's Onsite Wastewater Manual) are part of the Atlantic Coast Flatwoods that run along the eastern shore of the US. They fall within

Ma, Lena

188

Transforming the representation of the boundary layer and low clouds for high-resolution regional climate modeling: Final report  

SciTech Connect (OSTI)

Stratocumulus and shallow cumulus clouds in subtropical oceanic regions (e.g., Southeast Pacific) cover thousands of square kilometers and play a key role in regulating global climate (e.g., Klein and Hartmann, 1993). Numerical modeling is an essential tool to study these clouds in regional and global systems, but the current generation of climate and weather models has difficulties in representing them in a realistic way (e.g., Siebesma et al., 2004; Stevens et al., 2007; Teixeira et al., 2011). While numerical models resolve the large-scale flow, subgrid-scale parameterizations are needed to estimate small-scale properties (e.g. boundary layer turbulence and convection, clouds, radiation), which have significant influence on the resolved scale due to the complex nonlinear nature of the atmosphere. To represent the contribution of these fine-scale processes to the resolved scale, climate models use various parameterizations, which are the main pieces in the model that contribute to the low clouds dynamics and therefore are the major sources of errors or approximations in their representation. In this project, we aim to 1) improve our understanding of the physical processes in thermal circulation and cloud formation, 2) examine the performance and sensitivity of various parameterizations in the regional weather model (Weather Research and Forecasting model; WRF), and 3) develop, implement, and evaluate the advanced boundary layer parameterization in the regional model to better represent stratocumulus, shallow cumulus, and their transition. Thus, this project includes three major corresponding studies. We find that the mean diurnal cycle is sensitive to model domain in ways that reveal the existence of different contributions originating from the Southeast Pacific land-masses. The experiments suggest that diurnal variations in circulations and thermal structures over this region are influenced by convection over the Peruvian sector of the Andes cordillera, while the mostly dry mountain-breeze circulations force an additional component that results in semi-diurnal variations near the coast. A series of numerical tests, however, reveal sensitivity of the simulations to the choice of vertical grid, limiting the possibility of solid quantitative statements on the amplitudes and phases of the diurnal and semidiurnal components across the domain. According to our experiments, the Mellor-Yamada-Nakanishi-Niino (MYNN) boundary layer scheme and the WSM6 microphysics scheme is the combination of schemes that performs best. For that combination, mean cloud cover, liquid water path, and cloud depth are fairly wellsimulated, while mean cloud top height remains too low in comparison to observations. Both microphysics and boundary layer schemes contribute to the spread in liquid water path and cloud depth, although the microphysics contribution is slightly more prominent. Boundary layer schemes are the primary contributors to cloud top height, degree of adiabaticity, and cloud cover. Cloud top height is closely related to surface fluxes and boundary layer structure. Thus, our study infers that an appropriate tuning of cloud top height would likely improve the low-cloud representation in the model. Finally, we show that entrainment governs the degree of adiabaticity, while boundary layer decoupling is a control on cloud cover. In the intercomparison study using WRF single-column model experiments, most parameterizations show a poor agreement of the vertical boundary layer structure when compared with large-eddy simulation models. We also implement a new Total-Energy/Mass- Flux boundary layer scheme into the WRF model and evaluate its ability to simulate both stratocumulus and shallow cumulus clouds. Result comparisons against large-eddy simulation show that this advanced parameterization based on the new Eddy-Diffusivity/Mass-Flux approach provides a better performance than other boundary layer parameterizations.

Huang, Hsin-Yuan; Hall, Alex

2013-07-24T23:59:59.000Z

189

Solar: annual and seasonal average latitude tilt GIS data (contours) for  

Open Energy Info (EERE)

latitude tilt GIS data (contours) for latitude tilt GIS data (contours) for Brazil from INPE and LABSOLAR Dataset Summary Description (Abstract): Annual and seasonal mean of Latitude Tilt Solar Radiation in kWh/m2/day based on data from 1995 to 2002 (Purpose): To provide a set of consistent, reliable, verifiable, and accessible global data sets for international and in-country investors and other stakeholders (Supplemental Information): The cross-calibration process worked with data from 3 ground stations: Caic├│ (located in the Northeast of Brazil), Florian├│polis (located in the South) and Balbina (located in Amazonia). These data have been used for validation and comparison of radiation transfer models operated in SWERA to estimate the incidence of solar radiation on the surface of the country from satellite images

190

A study of mid-latitude tropopause characteristics over eastern North America  

E-Print Network [OSTI]

- parable latitudes in other parts of the worldf Some correlation 34 0. 7 4J n e W W c 0 al w n 0 0. 6 0. 5 0. 4 0. 3 0. 2 0. 1 BUF PIT Gg0 C@S 60 55 50 45 40 35 Latitude (degrees north) Figure 7. Average of the absolute values... tropopauses during summer 2. Profile of mean zonal wind during summer 3. Occurrence of multiple tropopauses during winter 4. Profile of mean zonal wind during winter 20 21 5. Mean and standard deviation of primary tropopause height during summer 25 6...

Houston, Ben Howard

1962-01-01T23:59:59.000Z

191

Occurrence of high-speed solar wind streams over the Grand Modern Maximum  

E-Print Network [OSTI]

In the declining phase of the solar cycle, when the new-polarity fields of the solar poles are strengthened by the transport of same-signed magnetic flux from lower latitudes, the polar coronal holes expand and form non-axisymmetric extensions toward the solar equator. These extensions enhance the occurrence of high-speed solar wind streams (HSS) and related co-rotating interaction regions in the low-latitude heliosphere, and cause moderate, recurrent geomagnetic activity in the near-Earth space. Here, using a novel definition of geomagnetic activity at high (polar cap) latitudes and the longest record of magnetic observations at a polar cap station, we calculate the annually averaged solar wind speeds as proxies for the effective annual occurrence of HSS over the whole Grand Modern Maximum (GMM) from 1920s onwards. We find that a period of high annual speeds (frequent occurrence of HSS) occurs in the declining phase of each solar cycle 16-23. For most cycles the HSS activity clearly maximizes during one year...

Mursula, Kalevi; Holappa, Lauri

2015-01-01T23:59:59.000Z

192

D.C. Middle and High School Students Get a Chance to Experience the Regional Science Bowl Competition Setting  

Broader source: Energy.gov [DOE]

The U.S. Department of Energyĺs Office of Minority Education and Community Development will demonstrate how middle schools and high schools in D.C. can get involved by providing a hands-on, interactive science bowl demonstration. The mock competition allows students to get a feel for the competition style, practice answering science questions at rapid pace, and meet staff from the Department of Energy.

193

High-Resolution Soft X-Ray Spectral Analysis in the CK Region of Titanium Carbide (TiC) using the DV-X alpha Molecular Orbital Method  

SciTech Connect (OSTI)

We used the DV-X alpha method to analyze the high-resolution soft X-ray emission and absorption spectra in the CK region of titanium carbide (TiC). The spectral profiles of the X-ray emission and absorption can be ssuscfucelly reproduced by the occupied and unoccupied density of states (DOS ), respectively, in the C2p orbitals of the center carbon atoms in a Ti62C63 cluster model, suggesting that the center carbon atom in a large cluster model expanded to the cubic-structured 53 (= 125) atoms provides sufficient DOS for the X-ray spectral analysis of rock-salt structured metal carbides.

Shimomura, Kenta; Muramatsu, Yasuji; Denlinger, Jonathan D.; Gullikson, Eric M.

2008-10-31T23:59:59.000Z

194

Some unusual discrete VLF emissions observed at a low-latitude ground station at Agra  

E-Print Network [OSTI]

Some unusual discrete VLF emissions observed at a low-latitude ground station at Agra B. Singh February 1997 / Accepted: 17 February 1997 Abstract. A detailed analysis of the VLF emissions data obtained°1¢ N, L = 1.15) has yielded some unusual discrete VLF emissions of the rising type. These include (1

Paris-Sud XI, Universit├ę de

195

Friction in Mid-latitude Bob Plant, Stephen Belcher, Bob Beare, Andy Brown  

E-Print Network [OSTI]

Friction in Mid-latitude Cyclones Ian Boutle Bob Plant, Stephen Belcher, Bob Beare, Andy Brown #12;Motivation ┬Ě Many studies have shown the significance of friction in formation and dissipation of cyclones Dt = + ├? . F . Diabatic Term: ┬Ě Surface heat fluxes ┬Ě Latent heat fluxes Frictional Term

Plant, Robert

196

7Tracking a Sea Turtle from a Satellite Day Number Latitude Longitude Distance  

E-Print Network [OSTI]

7Tracking a Sea Turtle from a Satellite Day Number Latitude Longitude Distance (km) 1 0 +5o North in the table above to track the sea turtle from the start of its journey to its end. Use your map to answer these questions: Question 1 - In what part of the world did it begin its trip? Question 2 - Where did the turtle

Christian, Eric

197

Discovery of Eight Recycled Pulsars - The Swinburne Intermediate Latitude Pulsar Survey  

E-Print Network [OSTI]

We have conducted a pulsar survey of intermediate Galactic latitudes (15deg 0.57 Mo and > 1.2 Mo), while anotherhas a low mass (~0.2 Mo) companion in a 23.3-d orbit, residing the well-known orbital period ``gap''.

R. T. Edwards

1999-11-19T23:59:59.000Z

198

The Mackenzie GEWEX Study: A Contribution to Cold Region Atmospheric and Hydrologic Sciences  

Science Journals Connector (OSTI)

The Mackenzie GEWEX Study (MAGS) is a collaborative study with the goals of understanding and modeling the high-latitude energy and water cycles, and improving our ability to assess the changes to the water re...

Ming-ko Woo; Wayne R. Rouseů

2008-01-01T23:59:59.000Z

199

Effects of Soil Moisture on the Responses of Soil Temperatures to Climate Change in Cold Regions  

Science Journals Connector (OSTI)

At high latitudes, changes in soil moisture could alter soil temperatures independently of air temperature changes by interacting with the snow thermal rectifier. The authors investigated this mechanism with model experiments in the Community Land ...

Zachary M. Subin; Charles D. Koven; William J. Riley; Margaret S. Torn; David M. Lawrence; Sean C. Swenson

2013-05-01T23:59:59.000Z

200

Quantifying Climate Feedbacks from Abrupt Changes in High-Latitude Trace-Gas Emissions  

SciTech Connect (OSTI)

Our overall goal was to quantify the potential for threshold changes in natural emission rates of trace gases, particularly methane and carbon dioxide, from pan-arctic terrestrial systems under the spectrum of anthropogenically forced climate warming, and the extent to which these emissions provide a strong feedback mechanism to global climate warming. This goal is motivated under the premise that polar amplification of global climate warming will induce widespread thaw and degradation of the permafrost, and would thus cause substantial changes in the extent of wetlands and lakes, especially thermokarst (thaw) lakes, over the Arctic. Through a coordinated effort of field measurements, model development, and numerical experimentation with an integrated assessment model framework, we have investigated the following hypothesis: There exists a climate-warming threshold beyond which permafrost degradation becomes widespread and thus instigates strong and/or sharp increases in methane emissions (via thermokarst lakes and wetland expansion). These would outweigh any increased uptake of carbon (e.g. from peatlands) and would result in a strong, positive feedback to global climate warming.

Schlosser, Courtney Adam [MIT; Walter-Anthony, Katey [University of Alaska; Zhuang, Qianlai [Purdue University; Melillo, Jerry [Marine Biological Laboratory

2013-04-26T23:59:59.000Z

Note: This page contains sample records for the topic "high latitude regions" 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

A COMPARISON OF FAR-IR AND H I AS REDDENING PREDICTORS AT HIGH GALACTIC LATITUDE  

SciTech Connect (OSTI)

Both the Galactic 21 cm line flux from neutral hydrogen (H I) in interstellar medium and the far-infrared (FIR) emission from Galactic dust grains have been used to estimate the strength of Galactic reddening of distant sources. In this work we use a collection of uniform color distant galaxies as color standards to determine whether the H I method or the FIR method is superior. We find that the two methods both produce reasonably accurate maps, but that both show significant errors as compared to the typical color of the background galaxies. We find that a mixture of the FIR and H I maps in roughly a 2-to-1 ratio is clearly superior to either map alone. We recommend that future reddening maps should use both sets of data, and that well-constructed FIR and H I maps should both be vigorously pursued.

Peek, J. E. G., E-mail: jegpeek@gmail.com [Department of Astronomy, Columbia University, New York, NY 10027 (United States)

2013-03-20T23:59:59.000Z

202

Conditions governing localized high-latitude dayside aurora H. Korth and B. J. Anderson  

E-Print Network [OSTI]

-aligned currents observed by the Iridium constellation for 25 events of prolonged steady IMF orientation with both with an estimate for the particle precipitation energy density based on the Knight relation, using the measured the Iridium constellation, which consists of $70 satellites distributed over six equally-spaced orbit planes

California at Berkeley, University of

203

Teleconnections Between the Subtropical Monsoons and High-Latitude Climates During the Last Deglaciation  

Science Journals Connector (OSTI)

...peri-ods). The 1450-year and 1150-year periods have also been found in the 5180 (temper-ature) record of the Camp Century ice core in Greenland (33). Thus, all of the frequen-cies observed in the monsoonal climate ap-pear to be part...

F. Sirocko; D. Garbe-Sch÷nberg; A. McIntyre; B. Molfino

1996-04-26T23:59:59.000Z

204

Diversification at high latitudes: speciation of buntings in the genus Plectrophenax inferred from mitochondrial  

E-Print Network [OSTI]

-294X.2009.04513.x #12;corroborating the signal of divergence with a large nuclear dataset mitochondrial and nuclear markers JAMES M. MALEY* and KEVIN WINKER University of Alaska Museum and Institute for a mitochondrial DNA (mtDNA) dataset, and in Correspondence: James Maley, Fax: +1 225 578 3075; E-mail: jmaley1@lsu

Winker, Kevin

205

High-latitude ionospheric convection models derived from Defense Meteorological Satellite Program ion drift  

E-Print Network [OSTI]

Vladimir O. Papitashvili Space Physics Research Laboratory, University of Michigan, Ann Arbor, Michigan to the average solar wind (i.e., the ``quasi-viscous'' interaction) and to changes in the IMF By, Bz 0, and Bz, plasma convection, current systems 1. Introduction [2] Earth's magnetosphere is immersed in the solar

Michigan, University of

206

The contribution of CHONS particles to the diffuse high-Galactic-latitude IR emission  

Science Journals Connector (OSTI)

......powder of beta-silicon carbide), AC (soot from an arc discharge in argon) and BE (soot from benzene burned in air...of motions of all atoms in each mode. This gives the electric polarizability and, hence A and then alpha. It is......

R. Papoular

2014-01-01T23:59:59.000Z

207

High-Latitude Dust Over the North Atlantic: Inputs from Icelandic Proglacial Dust Storms  

Science Journals Connector (OSTI)

...agustsson H. Olafsson H. , Forecasting wind gusts in complex terrain . Meteorol. Atmos...composition of African dust measured in trade wind aerosols at Barbados and Miami...version of this article illus. incl. sketch maps United States 201225 10.1126/science...

Joseph M. Prospero; Joanna E. Bullard; Richard Hodgkins

2012-03-02T23:59:59.000Z

208

Intense 2.3-Hz electric field pulsations in the stratosphere at high auroral latitude  

SciTech Connect (OSTI)

A survey has been performed of the power spectra of the electric field measured by stratospheric balloon-borne instruments during the 1985-1986 South Pole Balloon Campaign. The survey reviewed all 468 hours of available data and covered the frequency range from 0 to 4 Hz. Three episodes of narrow-band emissions were detected in this frequency range. These narrow-band emissions had frequencies in the horizontal component between 2 and 2.5 Hz. The frequencies observed in the vertical component were different, with several bands present. The fundamental frequency in the vertical component was around 0.8 to 1.4 Hz depending on event. The spectra of the events in the vertical component showed multiple emission bands, not all harmonically spaced. The vertical component showed much more pronounced time variations of the frequencies of the emission bands than the horizontal component showed. The ratio E{sub V}/E{sub H} was typically {approximately}2-3. The amplitude of the horizontal components of the emissions was quite large in one of the three events, with individual bursts having amplitudes of 60 mV/m. The polarization was complicated. An extensive list of possible explanations for these emissions was considered. Distant sources associated with tropospheric storms were considered in detail. During the most intense of the 2-Hz emission events, the nearest bad weather was more than 1000 km away. It proved impossible to account for the amplitude and polarization of the horizontal component with any reasonable tropospheric source. Explaining the narrow-band tuning was also a problem for any weather source model. An ionospheric model based on the concept of the ionospheric Alfven resonator is capable of accounting for the tuning, amplitude, and polarization of the horizontal components. However, this model has moderate difficulty in accounting for the observed vertical component of the emissions. 36 refs., 15 figs., 6 tabs.

Bering, E.A.; Benbrook, J.R. [Univ. of Houston, TX (United States)] [Univ. of Houston, TX (United States)

1995-05-01T23:59:59.000Z

209

Interactions of Water and Energy Mediate Responses of High-Latitude Terrestrial Ecosystems to Climate Change  

E-Print Network [OSTI]

air, water, and ice content, snow insulation is modeledinhibition of ice formation from snow insulation (Brown andeliminating snow insulation caused declines in ice surface

Subin, Zachary Marc

2012-01-01T23:59:59.000Z

210

Energy Conversions and Mean Vertical Motions in the High Latitude Summer Mesosphere and Lower Thermosphere  

Science Journals Connector (OSTI)

As is well known, an appreciable part of the solar energy initially absorbed in the upper atmosphere is not immediately converted to kinetic energy, but appears in chemical form (dissociation energy or energy ...

Paul J. Crutzen

1971-01-01T23:59:59.000Z

211

National Aeronautics and Space Administration On clear, dark nights at high northern latitudes,  

E-Print Network [OSTI]

scientists want to learn when, where, and why solar wind energy stored within the Earth's magneto- sphere

Waliser, Duane E.

212

Letter to the Editor Temperature anomalies in high northerly latitudes and their link  

E-Print Network [OSTI]

meteorological records which led extremes in the Southern Oscillation Index (SOI) by a number of months and hourly wind directional and velocity measurements (in each 10┬░ sector) were available for one monitoring continuous time series of coastal SSTs and concomitant surface wind conditions between January 1961 and April

Boyer, Edmond

213

Characterisation of CH3X fluxes from Scottish and high latitude wetlandsá  

E-Print Network [OSTI]

Methyl bromide (CH3Br) and methyl chloride (CH3Cl) are two halocarbons that are unique in that they play a significant role in stratospheric ozone destruction, and are mainly produced by natural systems. The current ...

Hardacre, Catherine

2010-01-01T23:59:59.000Z

214

Geology of the Yucca Mountain Region, Chapter in Stuckless, J.S., ED., Yucca Mountain, Nevada - A Proposed Geologic Repository for High-Level Radioactive Waste  

SciTech Connect (OSTI)

Yucca Mountain has been proposed as the site for the Nation's first geologic repository for high-level radioactive waste. This chapter provides the geologic framework for the Yucca Mountain region. The regional geologic units range in age from late Precambrian through Holocene, and these are described briefly. Yucca Mountain is composed dominantly of pyroclastic units that range in age from 11.4 to 15.2 Ma. The proposed repository would be constructed within the Topopah Spring Tuff, which is the lower of two major zoned and welded ash-flow tuffs within the Paintbrush Group. The two welded tuffs are separated by the partly to nonwelded Pah Canyon Tuff and Yucca Mountain Tuff, which together figure prominently in the hydrology of the unsaturated zone. The Quaternary deposits are primarily alluvial sediments with minor basaltic cinder cones and flows. Both have been studied extensively because of their importance in predicting the long-term performance of the proposed repository. Basaltic volcanism began about 10 Ma and continued as recently as about 80 ka with the eruption of cones and flows at Lathrop Wells, approximately 10 km south-southwest of Yucca Mountain. Geologic structure in the Yucca Mountain region is complex. During the latest Paleozoic and Mesozoic, strong compressional forces caused tight folding and thrust faulting. The present regional setting is one of extension, and normal faulting has been active from the Miocene through to the present. There are three major local tectonic domains: (1) Basin and Range, (2) Walker Lane, and (3) Inyo-Mono. Each domain has an effect on the stability of Yucca Mountain.

J.S. Stuckless; D. O'Leary

2006-09-25T23:59:59.000Z

215

Solar: monthly and annual average latitude tilt GIS data at 40km resolution  

Open Energy Info (EERE)

Mexico, Central America, and the Caribbean Islands from NREL Mexico, Central America, and the Caribbean Islands from NREL Dataset Summary Description (Abstract): Monthly Average Solar Resource for flat-plate collectors tilted at latitude, for Mexico, Central America, and the Caribbean Islands. (Purpose): Provide information on the solar resource potential for the data domain. The insolation values represent the average solar energy available to a flat plate collector, such as a photovoltaic panel, oriented due south at an angle from horizontal equal to the latitude of the collector location. (Supplemental Information): These data provide monthly average and annual average daily total solar resource averaged over surface cells of approximately 40 km by 40 km in size. The solar resource value is represented as watt-hours per square meter per day for each month. The

216

Hard X-ray latitude effect measured during a transatlantic balloon flight  

SciTech Connect (OSTI)

The hard X-ray latitude effect is reported in the range of McIlwain shell parameter L from 1.4 to 2.6 (earth radius units). The data were obtained with two X-ray scintillator detectors flown on board a transatlantic balloon launched from Trapani, Sicily. The data analysis method for measuring the flux from weak X-ray sources is also described.

Frontera, F. (CNR, Istituto Plasma Spazio, Frascati, Italy); Fuligni, F. (CNR, Istituto di Tecnologie e Studio delle Radiazioni Extraterrestri, Bologna, Italy)

1981-01-01T23:59:59.000Z

217

Solar wind energy transfer regions inside the dayside magnetopauseŚII. Evidence for an MHD generator process  

Science Journals Connector (OSTI)

In this paper a quantitative analysis of magnetosheath injection regions observed by PROGNOZ-7 in the dayside high latitude boundary layer is performed. Particular emphasis is laid on describing the consequences of the observed excess transverse momentum of solar wind ions (H+ and He2+) as compared to the magnetospheric ions (e.g. He+ and O+) in the magnetosheath injection regions, hereafter referred to as energy transfer regions. An important result of this study is that the observed excess drift velocity of the solar wind ions as compared to the magnetospheric ions can be interpreted as a negative inertia current being present in the boundary layer. This means that the inertia current goes against the local electric field and that particle kinetic energy is converted into electric energy there. The dayside high-latitude boundary layer therefore constitutes a voltage generator (at least with respect to the injected magnetosheath plasma). The MHD-theory predicts a strong coupling of the energy transfer process in the boundary layer and the ionosphere, both regions being connected by field aligned currents. The rate of decay of the inertia current in the injected plasma element is in the range of a few minutes, a value which is directly proportional to the ionospheric resistance. By taking into account both the Hall and the Pedersen conductivities in the ionosphere, the theory also predicts a strong coupling between ionospheric East/West and North/South currents. A considerable part of the inertia current may actually flow in the tangential (East/West) direction due to this coupling. Thus, a consequence of the boundary layer energy transfer process is that it may generate currents, powering other magnetospheric plasma processes, down to ionospheric heights.

R. Lundin

1984-01-01T23:59:59.000Z

218

South America Latitude Tilted SR Solar Model from INPE and LABSOLAR |  

Open Energy Info (EERE)

Latitude Tilted SR Solar Model from INPE and LABSOLAR Latitude Tilted SR Solar Model from INPE and LABSOLAR Dataset Summary Description (Abstract): Mean values of Latitude Tilted Solar Radiation in kWh/m2/day for 40km cells for 1 year (month, season, year) based on data from 1995 to 2005 (Purpose): To provide a set of consistent, reliable, verifiable, and accessible global data sets for international and in-country investors and other stakeholders (Supplemental Information): The BRASIL-SR model (developed by INPE - National Institute for Space Research) and the ARCVIEW software were used to produce the dataset and SHAPE files.The assessment of reliability levels of the BRASIL-SR model were performed through the evaluation of the deviations shown by the estimated values for solar radiation flux vis-à-vis the values measured at the surface (ground truth). This evaluation was done in two phases. The first phase consisted in an inter-comparison between the core radiation transfer models adopted by the SWERA Project to map the solar energy in the various countries participating in the project. The HELIOSAT model took part in this phase like benchmark due to its employment to map solar energy resources in countries from European Union. In the second phase, the solar flux estimates provided by the BRASIL-SR model were compared with measured values acquired at several solarimetric stations spread along the Brazilian territory. The BRASIL-SR model is not validated for areas covered by snow.

219

High  

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

the pitch of B (r), and B(r), flips toroidally, such that the unidirectional toroidal electric field drives current in opposite directions, with respect to B, in the regions...

220

High-Resolution Soft X-Ray Spectral Analysis in the CK Region of Titanium Carbide (TiC) using the DV-X alpha Molecular Orbital Method  

E-Print Network [OSTI]

in the CK Region of Titanium Carbide (TiC) using the DV-X?USA Keyword titanium carbide, soft X-ray spectroscopy,C K region of titanium carbide (TiC). The spectral profiles

Shimomura, Kenta

2010-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "high latitude regions" 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

Continental and oceanic crustal structure of the Pampean flat slab region, western Argentina, using receiver function analysis: new high-resolution results  

Science Journals Connector (OSTI)

......out that the largest seismic energy release is in flat slab regions...coupling. In central Chile/Argentina, for example, the upper plate energy release associated with the...slab region beneath western Argentina. An improved depth to continental......

Christine R. Gans; Susan L. Beck; George Zandt; Hersh Gilbert; Patricia Alvarado; Megan Anderson; Lepolt Linkimer

2011-07-01T23:59:59.000Z

222

Low-latitude Western North Atlantic climate variability during the past millennium : insights from proxies and models  

E-Print Network [OSTI]

Estimates of natural climate variability during the past millennium provide a frame of reference in which to assess the significance of recent changes. This thesis investigates new methods of reconstructing low-latitude ...

Saenger, Casey Pearce

2009-01-01T23:59:59.000Z

223

Population Studies of Gamma Ray Sources Using Stacking Analysis at Low Galactic Latitudes  

SciTech Connect (OSTI)

We studied the problem of the treatment of uncertainties in the diffuse gamma radiation apparent in stacking analysis of EGRET data at low Galactic latitudes for several classes of sources like PSRs. For those classes of sources we co-added maps of counts, exposure and diffuse background, and residuals, in varying numbers for different sub-categories. Finally we tested for gamma-ray excess emission in those maps and attempt to quantify the systematic biases in such approach. Such kinds of analysis will support and provide confidence in the classification processes of sources and source populations in the GLAST era.

Cillis, Analia N.; /NASA, Goddard; Reimer, Olaf; /Stanford U., HEPL /KIPAC, Menlo Park; Torres, Diego F.; /ICREA, Barcelona /Barcelona, Autonoma U.

2007-11-13T23:59:59.000Z

224

Regional Purchasing  

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

Regional Purchasing Regional Purchasing Regional Purchasing Pursuant to Appendix M of Prime Contract No. DE-AC52-06NA25396 between DOE/NNSA and Los Alamos National Security, LLC (LANS), LANS is committed to building a strong supplier base with Northern New Mexico businesses and the local Native American pueblos in the purchases of goods and services. Contact Small Business Office (505) 667-4419 Email We seek out and utilize known Northern New Mexico business as suppliers The Northern New Mexico counties included are Los Alamos Santa Fe Rio Arriba Taos Mora San Miguel Sandoval The eight regional pueblos included are Nambe Ohkay Owingeh (formerly known as San Juan) Picuris Pojoaque San Ildefonso Santa Clara Taos Tesuque When the Laboratory cannot identify regional firms, it will expand its

225

A method to discriminate solar and antisolar differential rotation in high-precision light curves  

E-Print Network [OSTI]

Surface differential rotation (DR) is one major ingredient of the magnetic field generation process in the Sun and likely in other stars. The term solar-like differential rotation describes the observation that solar equatorial regions rotate faster than polar ones. The opposite effect of polar regions rotating faster than equatorial ones (termed as antisolar DR) has only been observed in a few stars, although there is evidence from theoretical dynamo models. We present a new method to detect the sign of DR (i.e. solar-like or antisolar DR) by analyzing long-term high-precision light curves with the Lomb-Scargle periodogram.We compute the Lomb-Scargle periodogram and identify a set of significant periods $P_k$, which we associate with active regions located at different latitudes on the the stellar surface. If detectable, the first harmonics ($P_k'$) of these periods were identified to compute their peak-height-ratios $r_k:=h(P_k')/h(P_k)$. Spots rotating at lower latitudes generate less sine-shaped light cur...

Reinhold, T

2015-01-01T23:59:59.000Z

226

Solar wind energy transfer regions inside the dayside magnetopauseŚI. Evidence for magnetosheath plasma penetration  

Science Journals Connector (OSTI)

PROGNOZ-7 high temporal resolution measurements of the ion composition and hot plasma distribution in the dayside high latitude boundary layer near noon have revealed that magnetosheath plasma may penetrate the dayside magnetopause and form high density, high ?, magnetosheath-like regions inside the magnetopause. We will from these measurements demonstrate that the magnetosheath injection regions most probably play an important role in transferring solar wind energy into the magnetosphere. The transfer regions are characterized by a strong perpendicular flow towards dawn or dusk (depending on local time) but are also observed to expand rapidly along the boundary layer field lines. This increased flow component transverse to the local magnetic field corresponds to a predominantly radial electric field of up to several mV m?1, which indicates that the injected magnetosheath plasma causes an enhanced polarization of the boundary layer. Polarization of the boundary layer can therefore be considered a result of a local MHD-process where magnetosheath plasma excess momentum is converted into electromagnetic energy (electric field), i.e. we have primarily an MHD-generator there. We state primarily because we also observe acceleration of ôcoldö ions inside the magnetopause as a result of this radial electric field. A few cases of polarity reversals suggest that the polarization is sometimes quite localized. The perhaps most significant finding is that the boundary layer is observed to be charged up to tens of kilovolts, a potential which may be highly variable depending on e.g. the presence of a momentum exchange by the energy transfer regions.

R. Lundin; E. Dubinin

1984-01-01T23:59:59.000Z

227

Solar: monthly and annual average latitude tilt GIS data at 40km resolution  

Open Energy Info (EERE)

China from NREL China from NREL Dataset Summary Description (Abstract): Monthly Average Solar Resource for flat-plate collectors tilted at latitude for China. (Purpose): Provide information on the solar resource potential for the data domain. The insolation values represent the average solar energy available to a flat plate collector, such as a photovoltaic panel, oriented due south at an angle from horizontal equal to the latitude of the collector location. (Supplemental Information): These data provide monthly average and annual average daily total solar resource averaged over surface cells of approximately 40 km by 40 km in size. The solar resource value is represented as watt-hours per square meter per day for each month. The data were developed from NREL's Climatological Solar Radiation (CSR) Model. This model uses information on cloud cover, atmospheric water vapor and trace gases, and the amount of aerosols in the atmosphere to calculate the monthly average daily total insolation (sun and sky) falling on a horizontal surface. Existing ground measurement stations

228

Regional Inventories  

Gasoline and Diesel Fuel Update (EIA)

5 5 Notes: This year has not started well for gasoline inventories, with inventories being low across regions of the country. The Midwest region (PADD II) had been running lower than most regions, but began to catch up during the last week in April. Gasoline inventories ran about 9% below their 5-year average for this time of year and about 4% below where they were last year. The recent refinery problems in the Midwest, though, could erase some of that recovery. The impacts of Tosco's Wood River refinery and Marathon's St Paul refinery are not fully realized. But inventories were also precariously low along the East Coast (PADD I) and are extremely low in the Rocky Mountain region (PADD IV), although the size of this market mitigates any national impact. While the

229

High-Resolution Soft X-Ray Spectral Analysis in the CK Region of Titanium Carbide (TiC) using the DV-X alpha Molecular Orbital Method  

E-Print Network [OSTI]

of rock-salt structured metal carbides. K. Shimomura et al.in metals, such as metal carbides and carbon/metal alloys,the CK region of metal carbides, and analyzed the spectral

Shimomura, Kenta

2010-01-01T23:59:59.000Z

230

Solar: monthly and annual average latitude tilt GIS data at 40km resolution  

Open Energy Info (EERE)

Ghana from NREL Ghana from NREL Dataset Summary Description (Abstract): Monthly Average Solar Resource for flat-plate collectors tilted at latitude for Ghana. (Purpose): Provide information on the solar resource potential for the data domain. The insolation values represent the average solar energy available to a flat plate collector, such as a photovoltaic panel, oriented horizontally. (Supplemental Information): These data provide monthly average and annual average daily total solar resource averaged over surface cells of approximately 40 km by 40 km in size. The solar resource value is represented as watt-hours per square meter per day for each month. The data were developed from NREL's Climatological Solar Radiation (CSR) Model. This model uses information on cloud cover, atmospheric water vapor and trace gases, and the amount of aerosols in the atmosphere to

231

Brazil Latitude Tilted Solar Radiation Model (40km) from INPE and LABSOLAR  

Open Energy Info (EERE)

40km) from INPE and LABSOLAR 40km) from INPE and LABSOLAR Dataset Summary Description (Abstract): Latitude tilted solar radiation in kWh/m2/day for 1 year organized into cells with 40km x 40km (Purpose): To provide a set of consistent, reliable, verifiable, and accessible global data sets for international and in-country investors and other stakeholders (Supplemental Information): The BRASIL-SR model and the SPRING software (both developed by INPE - National Institute for Space Research) were used to produce the dataset and SHAPE files.The assessment of reliability levels of the BRASIL-SR model were performed through the evaluation of the deviations shown by the estimated values for solar radiation flux vis-à-vis the values measured at the surface (ground truth). This evaluation was done in two phases. The first phase

232

The Penumbra at Geomagnetic Latitude 20░ and the Energy Spectrum of Primary Cosmic Radiation  

Science Journals Connector (OSTI)

The method of obtaining the penumbra presented in a previous paper is applied to the following energies: r=0.385,0.400,0.425,0.450áandá0.500 St÷rmer at a geomagnetic latitude of 20░. Two graphs showing the variation of the penumbra with the energy are derived from the (?1,?) diagrams of these energies: one at a constant zenith angle of 60░, and the other along the east-west plane. If the number of primaries is assumed to vary inversely as the 2.8 power of their energy, the contribution of the penumbra to the directional intensity at a zenith angle of 60░ is calculated, and is shown to be far from negligible. The calculated intensities are quite sensitive to the energy distribution used, and this suggests a possible method for determining the energy spectrum of primary cosmic rays.

R. Albagli Hutner

1939-04-01T23:59:59.000Z

233

PACIFIC HIGHLY MIGR ATORY PEL AGIC FISHERIES pacific highly migratory  

E-Print Network [OSTI]

the Pacific Ocean, from the tropics to temperate latitudes. Many of these fishes routinely travel great highly migratory species throughout the Pacific Ocean. Some of the fleets are capable of operating across the Pacific as well as in other oceans during a single fishing season. These fleets use larger purse

234

high  

Gasoline and Diesel Fuel Update (EIA)

0 0 Summary Our short-term outlook for a wide array of energy prices has been adjusted upward as international and domestic energy supply conditions have tightened. We think that crude oil prices are as likely as not to end the year $2 to $3 per barrel higher than our previous projections. Thus, we think that the probability of West Texas Intermediate costing an average of $30 per barrel or more at midwinter is about 50 percent. On their current track, heating oil prices are likely to be about 30 percent above year-ago levels in the fourth quarter. Prices for Q1 2001 seem more likely now to match or exceed the high level seen in Q1 2000. Tight oil markets this year and an inherent propensity for high gas utilization in incremental power supply have resulted in rising North American natural gas

235

Optimizing the Probability of Flying in High Ice Water Content Conditions in the Tropics Using a Regional-Scale Climatology of Convective Cell Properties  

Science Journals Connector (OSTI)

In this paper, statistical properties of rainfall are derived from 14 years of Tropical Rainfall Measuring Mission data to optimize the use of flight hours for the upcoming High Altitude Ice Crystals (HAIC)/High Ice Water Content (HIWC) program. ...

A. Protat; S. Rauniyar; V. V. Kumar; J. W. Strapp

2014-11-01T23:59:59.000Z

236

Collaborative Research: Towards Advanced Understanding and Predictive Capability of Climate Change in the Arctic using a High-Resolution Regional Arctic Climate System Model  

SciTech Connect (OSTI)

Primary activities are reported in these areas: climate system component studies via one-way coupling experiments; development of the Regional Arctic Climate System Model (RACM); and physical feedback studies focusing on changes in Arctic sea ice using the fully coupled model.

Lettenmaier, Dennis P

2013-04-08T23:59:59.000Z

237

Identification of a novel homozygous deletion region at 6q23.1 in medullobalstomas using high-resolution array CGH analysis  

Science Journals Connector (OSTI)

...markers confined a 0.887Mb minimal region of homozygous deletion at 6q23.1 which was flanked by markers SHGC-14149 (6q22.33) and SHGC-110551 (6q23.1). Quantitative RT-PCR analysis showed complete loss of expression of 2 genes located...

Angela Bik-Yu Hui; Hirokuni Takano; Kwok Wai Lo; Wen Lin Kuo; Joe Gray; Ho Keung Ng

2005-05-01T23:59:59.000Z

238

A unique seasonal pattern in phytoplankton biomass in low-latitude waters in the South China Sea  

E-Print Network [OSTI]

A unique seasonal pattern in phytoplankton biomass in low-latitude waters in the South China Sea in phytoplankton biomass was observed at the South East Asian Time- series Study (SEATS) station (18┬░N, 116┬░E became readily detectable in the winter. The elevation of phytoplankton biomass coincided approximately

Wu, Chau-Ron

239

The Interannual Relationship between the Latitude of the Eddy-Driven Jet and the Edge of the Hadley Cell  

Science Journals Connector (OSTI)

A strong correlation between the latitudes of the eddy-driven jet and of the Hadley cell edge, on interannual time scales, is found to exist during austral summer, in both the NCEPľNCAR reanalysis and the models participating in the Coupled Model ...

Sarah M. Kang; Lorenzo M. Polvani

2011-01-01T23:59:59.000Z

240

high  

Gasoline and Diesel Fuel Update (EIA)

0 0 Highlights International Oil Markets Prices. We have raised our world oil price projection by about $2 per barrel for this month because of assumed greater compliance by OPEC to targeted cuts, especially for the second quarter of 2000 (Figure 1). The expected decline in world petroleum inventories continues (Figure 2), and, given the generally stiff resolve of OPEC members to maintain production cuts, any sign of a turnaround in stocks may be postponed until later this year than previously assumed (Q3 instead of Q2). Our current estimate for the average import cost this past January is now $25 per barrel, a nearly $15-per-barrel increase from January 1999. Crude oil prices are expected to remain at relatively high levels for the first half of 2000, but

Note: This page contains sample records for the topic "high latitude regions" 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

Variable numbers of pepsinogen genes are located in the centromeric region of human chromosome 11 and determine the high-frequency electrophoretic polymorphism  

Science Journals Connector (OSTI)

...labeled to high specific activity (1-3 x 108 cpm/gg) by nick-translation using standard procedures. We used high-stringency...pp. 829-838. 4. Taggart, R. T., Karn, R. C., Merritt, A. D., Yu, P. L. & Conneally, P. M. (1979) Hum...

R T Taggart; T K Mohandas; T B Shows; G I Bell

1985-01-01T23:59:59.000Z

242

Variable numbers of pepsinogen genes are located in the centromeric region of human chromosome 11 and determine the high-frequency electrophoretic polymorphism  

Science Journals Connector (OSTI)

...labeled to high specific activity (1-3 x 108 cpm/gg) by nick-translation using standard procedures. We used high-stringency...for their invaluable suggestions. This work was supported by Merit AM 32015, GM 20454, and HD 05196 from the National Institutes...

R T Taggart; T K Mohandas; T B Shows; G I Bell

1985-01-01T23:59:59.000Z

243

Global Lifetime Measurements of Highly-Deformed and Other Rotational Structures in the A~135 Light Rare-Earth Region: Probing the Single-Particle Motion in a Rotating Potential  

E-Print Network [OSTI]

It has been possible, using GAMMASPHERE plus Microball,to extract differential lifetime measurements free from common systematic errors for over 15 different nuclei (various isotopes of Ce, Pr, Nd, Pm, and Sm) at high spin within a single experiment. This comprehensive study establishes the effective single-particle quadrupole moments in the A~135 light rare-earth region. Detailed comparisons are made with calculations using the self-consistent cranked mean-field theory.

M. A. Riley; R. W. Laird; F. G. Kondev; D. J. Hartley; D. E. Archer; T. B. Brown; R. M. Clark; M. D evlin; P. Fallon; I. M. Hibbert; D. T. Joss; D. R. LaFosse; P. J. Nolan; N. J. O'Brien; E. S. Paul; J. Pfohl; D. G. Sarantites; R. K. Sheline; S. L. Shepherd; J. Simpson; R. Wadsworth; M. T. Matev; A. V. Afanasjev; J. Dobaczewski; G. A. Lalazissis; W. Nazarewicz; W. Satula

2001-05-15T23:59:59.000Z

244

Brazil Latitude Tilted Solar Radiation Model (10km) from INPE and LABSOLAR  

Open Energy Info (EERE)

10km) from INPE and LABSOLAR 10km) from INPE and LABSOLAR Dataset Summary Description (Abstract): Latitude tilted solar radiation in kWh/m2/day for 1 year organized into cells with 10km x 10km (Purpose): The BRASIL-SR model and the SPRING software (both developed by INPE -National Institute for Space Research) were used to produce the dataset and SHAPE files (Supplemental Information): The assessment of reliability levels of the BRASIL-SR model were performed through the evaluation of the deviations shown by the estimated values for solar radiation flux vis-à-vis the values measured at the surface (ground truth). This evaluation was done in two phases. The first phase consisted in an inter-comparison between the core radiation transfer models adopted by the SWERA Project to map the solar energy in the various countries participating in the project. The HELIOSAT model took part in this phase like benchmark due to its employment to map solar energy resources incountries from European Union. In the second phase, the solar flux estimates providedby the BRASIL-SR model were compared with measured values acquired at several solarimetric stations spread along the Brazilian territory

245

CAPITAL REGION  

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

t 09/20/07 15:28 FAX 301 903 4656 t 09/20/07 15:28 FAX 301 903 4656 CAPITAL REGION 0 j002 SDOE F 1325.8 (8-89) EFG (0790) Energy United States Government Department of Energy Memorandum DATE. September 18, 2007 Audit Report No.: OAS-L-07-23 REPLY TO: IG-34 (A07TG036) SUBJECT: Evaluation of "The Federal Energy Regulatory Commission's Cyber Security Program-2007" TO: Chairman, Federal Energy Regulatory Commission The purpose of this report is to inform you of the results o Four evaluation of the Federal Energy Regulatory Commission's (Commission) cyber security program. The evaluation was initiated in May 2007, and our fieldwork was conducted through September 2007. Our methodology is described in the attachment to this report. . INTRODUCTION AND OBJECTIVE The Commission reports that it is constantly improving thl stability, reliability, and

246

High density polyethylene (HDPE) containers as an alternative to polyethylene terephthalate (PET) bottles for solar disinfection of drinking water in northern region, Ghana  

E-Print Network [OSTI]

The purpose of this study is to investigate the technical feasibility of high density polyethylene (HDPE) containers as an alternative to polyethylene terephthalate (PET) bottles for the solar disinfection of drinking water ...

Yazdani, Iman

2007-01-01T23:59:59.000Z

247

Extensive study of the optical spectra for high-temperature superconducting oxides and their related materials from the infrared to the vacuum-ultraviolet energy region  

Science Journals Connector (OSTI)

Optical reflectivity spectra of (La, Sr)2CuO4 and YBa2Cu3Oy have been measured over a wide spectral range as high as 40 eV. Although overall...

Tajima, S; Seki, M; Hidaka, Y; Oka, K; Unoki, H; Suzuki, M; Suga, S; Ishii, H; Nakahashi, T; Murakami, T; Takagi, T; Uchida, S

1989-01-01T23:59:59.000Z

248

Forcing and Sampling of Ocean General Circulation Models: Impact of High-Frequency Motions  

Science Journals Connector (OSTI)

Significant inertial oscillations are present in all primitive equation ocean general circulation models when they are forced with high-frequency (period order of days) wind stress fields. At specific latitudes the energy of the wind stress ...

Steven R. Jayne; Robin Tokmakian

1997-06-01T23:59:59.000Z

249

E-Print Network 3.0 - anomalously high number Sample Search Results  

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

1999 3043F E L D S T E I N 1999 American Meteorological Society Summary: anomalous friction and mountain torques do extend into high latitudes. The most striking of these...

250

The qWR star HD 45166. II. Fundamental stellar parameters and evidence of a latitude-dependent wind  

E-Print Network [OSTI]

The enigmatic object HD 45166 is a qWR star in a binary system with an orbital period of 1.596 day, and presents a rich emission-line spectrum in addition to absorption lines from the companion star (B7 V). As the system inclination is very small (i=0.77 +- 0.09 deg), HD 45166 is an ideal laboratory for wind-structure studies. The goal of the present paper is to determine the fundamental stellar and wind parameters of the qWR star. A radiative transfer model for the wind and photosphere of the qWR star was calculated using the non-LTE code CMFGEN. The wind asymmetry was also analyzed using a recently-developed version of CMFGEN to compute the emerging spectrum in two-dimensional geometry. The temporal-variance spectrum (TVS) was calculated for studying the line-profile variations. Abundances, stellar and wind parameters of the qWR star were obtained. The qWR star has an effective temperature of Teff=50000 +- 2000 K, a luminosity of log(L/Lsun)=3.75 +- 0.08, and a corresponding photospheric radius of Rphot=1.00 Rsun. The star is helium-rich (N(H)/N(He) = 2.0), while the CNO abundances are anomalous when compared either to solar values, to planetary nebulae, or to WR stars. The mass-loss rate is Mdot = 2.2 . 10^{-7} Msun/yr, and the wind terminal velocity is vinf=425 km/s. The comparison between the observed line profiles and models computed under different latitude-dependent wind densities strongly suggests the presence of an oblate wind density enhancement, with a density contrast of at least 8:1 from equator to pole. If a high velocity polar wind is present (~1200 km/s), the minimum density contrast is reduced to 4:1. The wind parameters determined are unusual when compared to O-type stars or to typical WR stars. (abridged)

J. H. Groh; A. S. Oliveira; J. E. Steiner

2008-04-10T23:59:59.000Z

251

FIRST DETECTION OF THE [O III] 88 {mu}m LINE AT HIGH REDSHIFTS: CHARACTERIZING THE STARBURST AND NARROW-LINE REGIONS IN EXTREME LUMINOSITY SYSTEMS  

SciTech Connect (OSTI)

We have made the first detections of the 88 {mu}m [O III] line from galaxies in the early universe, detecting the line from the lensed active galactic nucleus (AGN)/starburst composite systems APM 08279+5255 at z = 3.911 and SMM J02399-0136 at z = 2.8076. The line is exceptionally bright from both systems, with apparent (lensed) luminosities {approx}10{sup 11} L {sub sun}. For APM 08279, the [O III] line flux can be modeled in a star formation paradigm, with the stellar radiation field dominated by stars with effective temperatures, T {sub eff} > 36,000 K, similar to the starburst found in M82. The model implies {approx}35% of the total far-IR luminosity of the system is generated by the starburst, with the remainder arising from dust heated by the AGN. The 88 {mu}m line can also be generated in the narrow-line region of the AGN if gas densities are around a few 1000 cm{sup -3}. For SMM J02399, the [O III] line likely arises from H II regions formed by hot (T {sub eff} > 40,000 K) young stars in a massive starburst that dominates the far-IR luminosity of the system. The present work demonstrates the utility of the [O III] line for characterizing starbursts and AGN within galaxies in the early universe. These are the first detections of this astrophysically important line from galaxies beyond a redshift of 0.05.

Ferkinhoff, C.; Hailey-Dunsheath, S.; Nikola, T.; Parshley, S. C.; Stacey, G. J. [Department of Astronomy, Cornell University, Ithaca, NY 14853 (United States); Benford, D. J.; Staguhn, J. G., E-mail: cferkinh@astro.cornell.ed, E-mail: steve@mpe.mpg.d [Observational Cosmology Laboratory (Code 665), NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)

2010-05-01T23:59:59.000Z

252

Enhanced terrestrial carbon uptake in the Northern High Latitudes in the 21st century from the Coupled Carbon  

E-Print Network [OSTI]

the Coupled Carbon Cycle Climate Model Intercomparison Project model projections H A I F E N G Q I A N *, R E Carbon Cycle Climate Model Intercomparison Project. Our analysis suggests that the NHL will be a carbon the intense warming there enhances SOM decomposition, soil organic carbon (SOC) storage continues to increase

Zeng, Ning

253

Dependencies of high-latitude plasma convection: Consideration of interplanetary magnetic field, seasonal, and universal time factors in  

E-Print Network [OSTI]

measurements were collected over the period 1998┬ş2002. The data were first used to derive a new statistical is kept in motion by processes that couple energy and momentum from the solar wind into Earth, seasonal, and universal time factors in statistical patterns J. M. Ruohoniemi and R. A. Greenwald Johns

Shepherd, Simon

254

Halogen-driven low-altitude O3 and hydrocarbon losses in spring at northern high latitudes  

E-Print Network [OSTI]

; Vogt et al., 1996; Foster et al., 2001]. HOBr ├ż Br├? ├ż H├ż ! Br2 ├ż H2O├░R3├? HOBr ├ż Cl├? ├ż H├ż ! BrCl ├ż H2O├░, National Center for Atmospheric Research, Boulder, Colorado, USA. Copyright 2

Chance, Kelly

255

The seasonal evolution of NMHCs and light alkyl nitrates at middle to high northern latitudes during TOPSE  

E-Print Network [OSTI]

Meinardi,1 Oliver W. Wingenter,3 Elliot L. Atlas,4 Frank Flocke,4 Brian A. Ridley,4 and F. Sherwood Rowland with meteorological trajectory analysis, different trace gas signatures provided significant clues to the origins here provide a unique picture of NH trace gas evolution from winter to summer that will be invaluable

Wingenter, Oliver W.

256

In search of long-term hemispheric asymmetry in the geomagnetic field: Results from high northern latitudes  

E-Print Network [OSTI]

of Nordvestkapp lavas and unconsolidated beach and lagoonalNord-Jan Spitsbergen ck Marine unconsolidated depositsOther unconsolidated deposits Inndalen Fmn. (Holocene) b) Bo

Cromwell, G.; Tauxe, L.; Staudigel, H.; Constable, C. G; Koppers, A. A. P; Pedersen, R.-B.

2013-01-01T23:59:59.000Z

257

Regional University Alliance  

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

Alliance Alliance Developed by the National Energy Technology Laboratory in collaboration with NETL-Regional University Alliance WVU National Research Center for Coal and Energy Fossil Consulting Services, Inc. The AVESTAR(tm) Center provides a state-of- the-art, highly realistic, dynamic simulator for a coal-fired power plant using Integrated Gasification Combined Cycle (IGCC) technology with CO 2 capture. The system is based on Invensys' DYNSIM ® software

258

Region 9: Pacific Rim Region, Regional Sustainability Plan  

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

REGION 9: PACIFIC RIM REGION REGION 9: PACIFIC RIM REGION Regional Sustainability Plan Presented by Ruth Cox Region 9 Regional Administrator Federal Utility Partnership Working Group (FUPWG) May 22 nd , 2013 REGION 9 INFORMATION MANAGE Federal space ´ü 36 million RSF in Region Nine * 173 owned buildings, 955 leased buildings * 100,000 Federal workers housed DESIGN & CONSTRUCT new Federal buildings ´üÂ$1.4 billion in FY12 capital construction projects ´üÂ$318 million in FY13 - Los Angeles Courthouse project PROVIDE PROCUREMENT LEADERSHIP across the Federal government ´ü $1.24 billion in total GSA Schedule sales in FY12 ´ü $468 million to small businesses ´ü 34,000 fleet vehicles, 53% of which are Alternative Fuel Vehicles Pacific Rim Profile - CA, AZ, NV, HI

259

Time series of high resolution photospheric spectra in a quiet region of the Sun. II. Analysis of the variation of physical quantities of granular structures  

E-Print Network [OSTI]

From the inversion of a time series of high resolution slit spectrograms obtained from the quiet sun, the spatial and temporal distribution of the thermodynamical quantities and the vertical flow velocity is derived as a function of logarithmic optical depth and geometrical height. Spatial coherence and phase shift analyzes between temperature and vertical velocity depict the height variation of these physical quantities for structures of different size. An average granular cell model is presented, showing the granule-intergranular lane stratification of temperature, vertical velocity, gas pressure and density as a function of logarithmic optical depth and geometrical height. Studies of a specific small and a specific large granular cell complement these results. A strong decay of the temperature fluctuations with increasing height together with a less efficient penetration of smaller cells is revealed. The T -T coherence at all granular scales is broken already at log tau =-1 or z~170 km. At the layers beyon...

Puschmann, K G; Vazquez, M; Bonet, J A; Hanslmeier, A; 10.1051/0004-6361:20047193

2012-01-01T23:59:59.000Z

260

High-energy radiation visualizer (HERV): A new system for imaging in x-ray and gamma-ray emission regions  

SciTech Connect (OSTI)

The authors present a description and results of the operation for {gamma}-ray and X-ray objects for the compact visualization system high-energy radiation visualizer (HERV). The imaging in this system is based on use of a conical collimator, scintillator plate, and image intensifier as a detector and CCD matrix as a readout device. The use of HERV as a two-dimensional X-ray image visualizer for the Compton scatter inspection system was considered and first results are discussed. The possibility of using different hexagonal-coded apertures imaging for HERV is discussed and results of Monte Carlo simulation and experiments with optical analog of coded aperture are presented.

Sudarkin, A.N.; Ivanov, O.P.; Stepanov, V.E.; Volkovich, A.G.; Turin, A.S.; Danilovich, A.S.; Rybakov, D.D.; Urutskoev, L.I. [RECOM Ltd., Moscow (Russian Federation)] [RECOM Ltd., Moscow (Russian Federation)

1996-08-01T23:59:59.000Z

Note: This page contains sample records for the topic "high latitude regions" 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

State & Regional Resources  

Broader source: Energy.gov [DOE]

The Bioenergy Technologies Office partners with the National Biomass State and Regional Partnerships' five regional organizations that provide leadership in their regions with regard to policies...

262

Regional Summary Pacific Region Management Context  

E-Print Network [OSTI]

, for the Eastern Pacific Ocean, and the Western and Central Pacific Fishery Commission, for the Western PacificRegional Summary Pacific Region Management Context The Pacific Region includes California, Oregon, and Washington. Federal fisheries in this region are managed by the Pacific Fishery Management Council (PFMC

263

Interaction Region Papers  

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

IR (Interaction Region) Magnets with Ramesh Gupta IR (Interaction Region) Magnets with Ramesh Gupta as the major author (unless noted): R. Gupta, et. al, "React & Wind Nb3Sn Common Coil Dipole", ASC 2006, August 27- September 1, 2006 in Seattle, WA, USA . *** Click Here for Talk ***. R. Gupta, "Modular Design and Modular Program for High Gradient Quadrupoles", ASC 2006, August 27- September 1, 2006 in Seattle, WA, USA. *** Click Here for Poster ***. Racetrack Magnet Designs and Technologies, WAMDO@CERN, April 2-6, 2006 (Click here for the oral presentation). R. Gupta, et. al, "Optimization of Open Midplane Dipole Design for LHC IR Upgrade," Presented at the 2005 Particle Accelerator Conference, Knoxville, TN, USA (2005). *** Click Here for Poster *** R. Gupta, et al., “Open Midplane Dipole Design for LHC IR

264

Grating formation by a high power radio wave in near-equator ionosphere  

SciTech Connect (OSTI)

The formation of a volume grating in the near-equator regions of ionosphere due to a high power radio wave is investigated. The radio wave, launched from a ground based transmitter, forms a standing wave pattern below the critical layer, heating the electrons in a space periodic manner. The thermal conduction along the magnetic lines of force inhibits the rise in electron temperature, limiting the efficacy of heating to within a latitude of few degrees around the equator. The space periodic electron partial pressure leads to ambipolar diffusion creating a space periodic density ripple with wave vector along the vertical. Such a volume grating is effective to cause strong reflection of radio waves at a frequency one order of magnitude higher than the maximum plasma frequency in the ionosphere. Linearly mode converted plasma wave could scatter even higher frequency radio waves.

Singh, Rohtash; Sharma, A. K.; Tripathi, V. K. [Department of Physics, Indian Institute of Technology Delhi, New Delhi-110016 (India)

2011-11-15T23:59:59.000Z

265

2014 REGIONAL ECONOMIC OUTLOOK  

E-Print Network [OSTI]

2014 REGIONAL ECONOMIC OUTLOOK #12;2014 REGIONAL ECONOMIC OUTLOOK 2014 Overview The Cincinnati USA Partnership for Economic Development and the Northern Kentucky Chamber of Commerce are pleased to present the 2014 Regional Economic Outlook. This report was prepared by the Cincinnati USA Partnership's Regional

Boyce, Richard L.

266

Intensity of the Soft and Hard Component of the Cosmic Radiation as a Function of Altitude at Geomagnetic Latitudes of 28░N, 41░N, and 55░N  

Science Journals Connector (OSTI)

Counter telescopes have been flown with plastic balloons to a maximum altitude of 94,000 ft. Intensity vs pressure curves have been obtained at geomagnetic latitudes of ?=55?,41?,áandá28? for the total cosmic radiation and for the components capable of traversing several thickness of lead. The energy spectrum of primary cosmic-ray particles has been derived from the extrapolation of the intensity of the total radiation to the top of the atmosphere. The integral momentum spectrum of the total primary radiation is given by N(>pcZe)=0.49(pcZe)-1.0. The results show that the radiation originating from primaries in the energy range 1 to 4 Bev (cut-off energies at ?=55?áandá41?) is predominantly of a nucleonic nature. The absence of an appreciable electronic component can be explained by assuming that, close to the top of the atmosphere, electrons originate predominantly from the decay of neutral mesons and that, within this energy range, the over-all probability of nucleon emission is greater than that of meson production. In sharp contrast, the soft component originating from primaries in the range from 4 to 8 Bev (cut-off at ?=41?áandá28?) multiplies rapidly in the atmosphere. This large transition effect in air with a maximum at about 10 cm Hg pressure is very characteristic of electron showers. It is concluded that the probability of neutral mesons being produced is comparatively high at primary energies between 4 and 8 Bev. At energies higher than 8 Bev this effect is even more pronounced, due to the contribution of the plural and multiple production of mesons.

Marcello L. Vidale

1952-10-15T23:59:59.000Z

267

PROCEEDINGS OF RIKEN BNL RESEARCH CENTER WORKSHOP ON RHIC SPIN PHYSICS III AND IV, POLARIZED PARTONS AT HIGH Q2 REGION, AUGUST 3, 2000 AT BNL, OCTOBER 14, 2000 AT KYOTO UNIVERSITY.  

SciTech Connect (OSTI)

International workshop on II Polarized Partons at High Q2 region 11 was held at the Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto, Japan on October 13-14, 2000, as a satellite of the international conference ''SPIN 2000'' (Osaka, Japan, October 16-21,2000). This workshop was supported by RIKEN (The Institute of Physical and Chemical Research) and by Yukawa Institute. The scientific program was focused on the upcoming polarized collider RHIC. The workshop was also an annual meeting of RHIC Spin Collaboration (RSC). The number of participants was 55, including 28 foreign visitors and 8 foreign-resident Japanese participants, reflecting the international nature of the RHIC spin program. At the workshop there were 25 oral presentations in four sessions, (1) RHIC Spin Commissioning, (2) Polarized Partons, Present and Future, (3) New Ideas on Polarization Phenomena, (4) Strategy for the Coming Spin Running. In (1) the successful polarized proton commissioning and the readiness of the accelerator for the physics program impressed us. In (2) and (3) active discussions were made on the new structure function to be firstly measured at RHIC, and several new theoretical ideas were presented. In session (4) we have established a plan for the beam time requirement toward the first collision of polarized protons. These proceedings include the transparencies presented at the workshop. The discussion on ''Strategy for the Coming Spin Running'' was summarized by the chairman of the session, S. Vigdor and G. Bunce.

BUNCE, G.; VIGDOR, S.

2001-03-15T23:59:59.000Z

268

Alaska Geothermal Region | Open Energy Information  

Open Energy Info (EERE)

Geothermal Region Geothermal Region Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Alaska Geothermal Region Details Areas (54) Power Plants (1) Projects (2) Techniques (0) Assessment of Moderate- and High-Temperature Geothermal Resources of the United States[1] Assessment of Moderate- and High-Temperature Geothermal Resources of the United States[2] References ÔćĹ "Assessment of Moderate- and High-Temperature Geothermal Resources of the United States" ÔćĹ "Assessment of Moderate- and High-Temperature Geothermal Resources of the United States" Geothermal Region Data State(s) Alaska Area 1,717,854 km┬▓1,717,854,000,000 m┬▓ 663,091.644 mi┬▓ 18,490,808,670,600 ft┬▓ 2,054,553,384,000 yd┬▓ 424,490,312.67 acres USGS Resource Estimate for this Region Identified Mean Potential 677 MW677,000 kW

269

arXiv:0908.1824v2[physics.comp-ph]24Feb2010 The calculation of longitude and latitude from geodesic measurements  

E-Print Network [OSTI]

arXiv:0908.1824v2[physics.comp-ph]24Feb2010 The calculation of longitude and latitude from geodesic, 2009; revised: February 24, 2010) 1. INTRODUCTION Consider a geodesic line between two points A and B by deriving the fundamental properties of geodesic lines on a spheroid of revolution. Even though aspects

Karney, Charles

270

Western Regional Partnership Overview  

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

Regional Partnership Overview Regional Partnership Overview June 2013 Briefing Overview ´éĘ WRP Background ´éĘ Importance of Region ´éĘ WRP Tribal Relations Committee ´éĘ WRP Energy Committee WRP Region's Uniqueness ´éĘ 5 states stretching from the Great Plains to the Pacific Ocean ´éĘ Diverse terrain ranging from desert valleys to forested mountains ´éĘ Significant State Trust Landholdings ´éĘ Approximately 188 Federally recognized Tribes ´éĘ Significant amounts of Federally managed land ´éĄ According to GSA 2004 study, WRP states range from 41.8% - 84.5% of total state land WRP Region's Importance to DoD ´éĘ Extensive Training Ranges ´éĄ Interconnected ground/air ranges provide unmatched warfighter training opportunities

271

HIGH-ACCURACY QUARTIC FORCE FIELD CALCULATIONS FOR THE SPECTROSCOPIC CONSTANTS AND VIBRATIONAL FREQUENCIES OF 1{sup 1} A' l-C{sub 3}H{sup -}: A POSSIBLE LINK TO LINES OBSERVED IN THE HORSEHEAD NEBULA PHOTODISSOCIATION REGION  

SciTech Connect (OSTI)

It has been shown that rotational lines observed in the Horsehead nebula photodissociation region (PDR) are probably not caused by l-C{sub 3}H{sup +}, as was originally suggested. In the search for viable alternative candidate carriers, quartic force fields are employed here to provide highly accurate rotational constants, as well as fundamental vibrational frequencies, for another candidate carrier: 1 {sup 1} A' C{sub 3}H{sup -}. The ab initio computed spectroscopic constants provided in this work are, compared to those necessary to define the observed lines, as accurate as the computed spectroscopic constants for many of the known interstellar anions. Additionally, the computed D{sub eff} for C{sub 3}H{sup -} is three times closer to the D deduced from the observed Horsehead nebula lines relative to l-C{sub 3}H{sup +}. As a result, 1 {sup 1} A' C{sub 3}H{sup -} is a more viable candidate for these observed rotational transitions. It has been previously proposed that at least C{sub 6}H{sup -} may be present in the Horsehead nebular PDR formed by way of radiative attachment through its dipole-bound excited state. C{sub 3}H{sup -} could form in a similar way through its dipole-bound state, but its valence excited state increases the number of relaxation pathways possible to reach the ground electronic state. In turn, the rate of formation for C{sub 3}H{sup -} could be greater than the rate of its destruction. C{sub 3}H{sup -} would be the seventh confirmed interstellar anion detected within the past decade and the first C{sub n}H{sup -} molecular anion with an odd n.

Fortenberry, Ryan C.; Lee, Timothy J. [NASA Ames Research Center, Moffett Field, CA 94035-1000 (United States); Huang, Xinchuan [SETI Institute, 189 Bernardo Avenue, Suite 100, Mountain View, CA 94043 (United States); Crawford, T. Daniel, E-mail: Timothy.J.Lee@nasa.gov [Department of Chemistry, Virginia Tech, Blacksburg, VA 24061 (United States)

2013-07-20T23:59:59.000Z

272

Climatology of Mid-latitude Ionospheric Disturbances from the Very Large Array Low-frequency Sky Survey  

E-Print Network [OSTI]

The results of a climatological study of ionospheric disturbances derived from observations of cosmic sources from the Very Large Array (VLA) Low-frequency Sky Survey (VLSS) are presented. We have used the ionospheric corrections applied to the 74 MHz interferometric data within the VLSS imaging process to obtain fluctuation spectra for the total electron content (TEC) gradient on spatial scales from a few to hundreds of kilometers and temporal scales from less than one minute to nearly an hour. The observations sample nearly all times of day and all seasons. They also span latitudes and longitudes from 28 deg. N to 40 deg. N and 95 deg. W to 114 deg. W, respectively. We have binned and averaged the fluctuation spectra according to time of day, season, and geomagnetic (Kp index) and solar (F10.7) activity. These spectra provide a detailed, multi-scale account of seasonal and intraday variations in ionospheric activity with wavelike structures detected at wavelengths between about 35 and 250 km. In some cases,...

Helmboldt, J F; Cotton, W D

2012-01-01T23:59:59.000Z

273

Regional Comparisons, Spatial Aggregation,  

Gasoline and Diesel Fuel Update (EIA)

Regional Regional Comparisons, Spatial Aggregation, and Asymmetry of Price Pass-Through in U.S. Gasoline Markets MICHAEL YE*, JOHN ZYREN**, JOANNE SHORE**, AND MICHAEL BURDETTE** Abstract Spot to retail price pass-through behavior of the U.S. gasoline market was investigated at the national and regional levels, using weekly wholesale and retail motor gasoline prices from January 2000 to the present. Asymmetric pass-through was found across all regions, with faster pass-through when prices are rising. Pass-through patterns, in terms of speed and time for completion, were found to vary from region to region. Spatial aggregation was investigated at the national level and the East Coast with the aggregated cumulative pass-through being greater than the volume-weighted regional pass-through when spot prices increase. These results are useful to the petroleum industry, consumers,

274

Hawaii Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Hawaii Regions Hawaii Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Hawaii Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Hawaii Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

275

Delaware Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Delaware Regions Delaware Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Delaware Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Delaware Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

276

Utah Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Utah Regions Utah Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Utah Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Utah Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

277

Arkansas Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Arkansas Regions Arkansas Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Arkansas Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Arkansas Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

278

Minnesota Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Minnesota Regions Minnesota Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Minnesota Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Minnesota Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

279

Tennessee Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Tennessee Regions Tennessee Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Tennessee Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Tennessee Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

280

Connecticut Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Connecticut Regions Connecticut Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Connecticut Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Connecticut Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

Note: This page contains sample records for the topic "high latitude regions" 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

Massachusetts Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Massachusetts Regions Massachusetts Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Massachusetts Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Massachusetts Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

282

Alaska Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Alaska Regions Alaska Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Alaska Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Alaska Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

283

Ohio Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Ohio Regions Ohio Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Ohio Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Ohio Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

284

Kentucky Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Kentucky Regions Kentucky Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Kentucky Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Kentucky Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

285

Pennsylvania Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Pennsylvania Regions Pennsylvania Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Pennsylvania Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Pennsylvania Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

286

Indiana Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Indiana Regions Indiana Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Indiana Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Indiana Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

287

Oklahoma Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Oklahoma Regions Oklahoma Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Oklahoma Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Oklahoma Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

288

Michigan Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Michigan Regions Michigan Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Michigan Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Michigan Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

289

Iowa Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Iowa Regions Iowa Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Iowa Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Iowa Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

290

Washington Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Regions Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Washington Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Washington Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

291

Arizona Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Arizona Regions Arizona Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Arizona Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Arizona Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

292

Nebraska Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Nebraska Regions Nebraska Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Nebraska Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Nebraska Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

293

Oregon Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Oregon Regions Oregon Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Oregon Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Oregon Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

294

Louisiana Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Louisiana Regions Louisiana Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Louisiana Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Louisiana Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

295

Kansas Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Kansas Regions Kansas Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Kansas Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Kansas Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

296

Wyoming Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Wyoming Regions Wyoming Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Wyoming Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Wyoming Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

297

Idaho Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Idaho Regions Idaho Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Idaho Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Idaho Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

298

Vermont Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Vermont Regions Vermont Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Vermont Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Vermont Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

299

Georgia Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Georgia Regions Georgia Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Georgia Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Georgia Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

300

Colorado Region | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Colorado Region Colorado Region National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Colorado Region Print Text Size: A A A RSS Feeds FeedbackShare Page Colorado Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

Note: This page contains sample records for the topic "high latitude regions" 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

Missouri Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Missouri Regions Missouri Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Missouri Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Missouri Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

302

Texas Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Texas Regions Texas Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Texas Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Texas Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

303

California Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

California Regions California Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals California Regions Print Text Size: A A A RSS Feeds FeedbackShare Page California Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

304

Mississippi Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Mississippi Regions Mississippi Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Mississippi Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Mississippi Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

305

Maine Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Maine Regions Maine Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Maine Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Maine Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

306

Wisconsin Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Wisconsin Regions Wisconsin Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Wisconsin Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Wisconsin Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

307

Montana Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Montana Regions Montana Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Montana Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Montana Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

308

Virginia Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Virginia Regions Virginia Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Virginia Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Virginia Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

309

Nevada Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Nevada Regions Nevada Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Nevada Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Nevada Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

310

Florida Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Florida Regions Florida Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Florida Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Florida Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

311

Illinois Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Illinois Regions Illinois Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Illinois Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Illinois Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

312

Maryland Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Maryland Regions Maryland Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Maryland Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Maryland Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

313

Alabama Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Alabama Regions Alabama Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Alabama Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Alabama Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

314

Spin asymmetries A[sub 1] of the proton and the deuteron in the low [ital x] and low Q[sup 2] region from polarized high energy muon scattering  

SciTech Connect (OSTI)

We present the results of the spin asymmetries A[sub 1] of the proton and the deuteron in the kinematic region extending down to x=6[times]10[sup [minus]5] and Q[sup 2]=0.01 hthinsp;GeV[sup 2]. The data were taken with a dedicated low [ital x] trigger, which required hadron detection in addition to the scattered muon, so as to reduce the background at low [ital x]. The results complement our previous measurements and the two sets are consistent in the overlap region. No significant spin effects are found in the newly explored region. thinsp [copyright] [ital 1999] [ital The American Physical Society

Baum, G.; Bueltmann, S.; Kraemer, D.; Kyynaeraeinen, J.; Tripet, A. (University of Bielefeld, Physics Department, D-33501 Bielefeld (Germany)); Arik, E.; Cuhadar, T.; Ozben, C.; Unel, G. (Bogazici University and Istanbul Technical University, 80676 Istanbul (Turkey)); Goertz, S.; Meyer, W.; Reicherz, G. (University of Bochum, Physics Department, D-44780 Bochum (Germany)); Derro, B.; Dulya, C.; Igo, G.; Whitten, C. (University of California, Department of Physics, Los Angeles, California 90024 (United States)); Hautle, P.; Heusch, C.A.; Kroeger, W.; Niinikoski, T.O.; Raedel, G.; Stiegler, U.; Voss, R. (CERN, CH-1211 Geneva 23 (Switzerland)); Gilly, H.; Kessler, H.J.; Landgraf, U.; Witzmann, A. (University of Freiburg, Physics Department, D-79104 Freiburg (Germany)); Stuhrmann, H.; Willumeit, R.; Zhao, J. (GKSS, D-21494 Geesthacht (Germany)); Berglund, P.; Kyynaeraeinen, J. (Helsinki University of Technology, Low Temperature Laboratory and Institute of Particle Physics Technology,

1999-10-01T23:59:59.000Z

315

About Rocky Mountain Region  

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

Rates About the Rocky Mountain Region RM Office The Platte River Power Authority in Colorado, Nebraska Public Power District, Kansas Electric Power Cooperative and Wyoming...

316

Hydrogen Regional Infrastructure Program in Pennsylvania  

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

REGIONAL REGIONAL INFRASTRUCTURE PROGRAM IN PENNSYLVANIA HYDROGEN REGIONAL INFRASTRUCTURE PROGRAM IN PENNSYLVANIA Melissa Klingenberg, PhD Melissa Klingenberg, PhD Hydrogen Program Hydrogen Program Air Products and Chemicals, Inc. (APCI) Hydrogen Separation Hydrogen Sensors Resource Dynamics Corporation (RDC) Tradeoff/Sensitivity Analyses of Hydrogen Delivery Approaches EDO Fiber Science High Pressure/High Strength Composite Material Development and Prototyping CTC * Program Management * Hydrogen Delivery - CH 4 /H 2 co-transport - H 2 separation - Delivery approaches * Advanced Materials - Characterization - Testing/Analyses - Predictive Modeling * Sensors SRNL Pipeline Life Management Program Develop infrastructure technology for a H 2 economy Aims to serve as "go-to" organization to catalyze PA Hydrogen

317

HYDROGEN REGIONAL INFRASTRUCTURE PROGRAM  

E-Print Network [OSTI]

to serve as "go-to" organization to catalyze PA Hydrogen and Fuel Cell Economy development #12;FundingHYDROGEN REGIONAL INFRASTRUCTURE PROGRAM IN PENNSYLVANIA HYDROGEN REGIONAL INFRASTRUCTURE PROGRAM IN PENNSYLVANIA Melissa Klingenberg, PhDMelissa Klingenberg, PhD #12;Hydrogen ProgramHydrogen Program Air Products

318

Regional Analysis Briefs  

Reports and Publications (EIA)

Regional Analysis Briefs (RABs) provide an overview of specific regions that play an important role in world energy markets, either directly or indirectly. These briefs cover areas that are currently major producers (Caspian Sea), have geopolitical importance (South China Sea), or may have future potential as producers or transit areas (East Africa, Eastern Mediterranean).

2028-01-01T23:59:59.000Z

319

Regional Competitions - EERE Commercialization Office  

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

Regional Competitions Six Regional Clean Energy Business Plan Competitions are taking place across the country- representing all of the United States' distinct regions. The...

320

Regional TectonicsRegional Tectonics Geology 200  

E-Print Network [OSTI]

, WV Thrusting of the Wills Mtn Duplex created open folds to the west.g p p Seneca RocksPlateau Valley ┬Ě Appalachian Plateau ┬ş Low and High ┬Ě Valley and Ridge ┬Ě Great Valley ┬Ě Blue Ridge #12;Great High Plateau Low Plateau Valley and Ridge Valley Bl RidBlue Ridge #12;Relief Map #12;Fig. 23.15. Differential erosion

Kammer, Thomas

Note: This page contains sample records for the topic "high latitude regions" 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

Wideband noise observed at ground level in the auroral region  

SciTech Connect (OSTI)

A sideband noise event was detected at ground level from the Andoya Rocket Range in Norway in January 1989. The signals were observed on four commercial communication receivers (tuned to 159, 515, 905, and 1200 kHz), an ionosonde (200-kHz to 3.5-MHz interference-free observations) and a riometer (32.5 MHz). The event, which occurred during a period of magnetic disturbance near magnetic midnight, was the only one observed during nearly 3 weeks of operations. This low frequency-of-occurrence is attributed partly to high local noise levels. The ease with which this event was identified on the ionograms produced by the local ionosonde suggests that routine ionosonde recordings should be inspected in search for such events. Such an effort would enhance existing research directed toward developing techniques for identifying quiet communication channels and help to identify the origin and frequency-of-occurrence of high-latitude wideband noise events. 20 refs.

Benson, R.F.; Desch, M.D. (NASA, Goddard Space Flight Center, Greenbelt, MD (United States))

1991-08-01T23:59:59.000Z

322

Regional Planning | Data.gov  

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

Regional Planning Regional Planning Ocean Data Tools Technical Guide Map Gallery Regional Planning Feedback Ocean You are here Data.gov ┬╗ Communities ┬╗ Ocean Regional Planning Efforts Alias (field_alias) Apply California, Oregon, Washington Regional Ocean Partnership West Coast Governors' Alliance Regional Data Portal In Development U.S. Virgin Islands, Puerto Rico Regional Ocean Partnership U.S. Caribbean Regional Ocean Partnership-currently being formally established Regional Data Portal To be developed Georgia, Florida, North Carolina, South Carolina Regional Ocean Partnership Governors' South Atlantic Alliance Regional Data Portal Currently in development American Samoa, Commonwealth of the Northern Mariana Islands (CNMI), Federated States of Micronesia, Guam, Hawaii, Marshall Islands, Palau

323

the Regional Development Corporation  

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

carry out this work, CPO partners carry out this work, CPO partners with the Los Alamos National Laboratory Foundation for education, the Regional Development Corporation for economic development, and the regional United Way organizations for community giving. Education Los Alamos National Security (LANS) invests more than $1 million each year to enhance regional educational opportunities in science, technology, engineering, and math (STEM) education. Education Focus Areas Our education commitments address four focus areas: * Workforce Development * Student Internships * Teacher and Faculty Professional Development * Public Understanding of Science In 2011, more than 1,100 students

324

Development of heavy mineral and heavy element database of soil sediments in Japan using synchrotron radiation X-ray powder diffraction and high-energy (116ákeV) X-ray fluorescence analysis: 1. Case study of Kofu and Chiba region  

Science Journals Connector (OSTI)

We have started the construction of a nationwide forensic soil sediment database for Japan based on the heavy mineral and trace heavy element compositions of stream sediments collected at 3024 points all over Japan obtained by high-resolution synchrotron X-ray powder diffraction (SR-XRD) and high-energy synchrotron X-ray fluorescence analysis (HE-SR-XRF). In this study, the performance of both techniques was demonstrated by analyzing soil sediments from two different geological regions, the Kofu and Chiba regions in Kanto province, to construct database that can be applied in the future to provenance analysis of soil evidence from a crime scene. The sediments from the quaternary volcanic lithology of the Chiba region were found to be dominated by heavy minerals of volcanic origin ľ orthopyroxene, clinopyroxene, and amphibole, and the \\{REEs\\} (rare earth elements) within the region showed similar geochemical behavior. On the other hand, four distinct heavy mineral groups were identified in the sediments of the Kofu region, where there is a great variety of underlying bedrock, and the geochemical behavior of the \\{REEs\\} in the sediments also varied accordingly to their geological origins. As such, our study shows that high-resolution SR-XRD data can provide information on the spatial distribution patterns of heavy minerals in stream sediments, playing an important role in determining their likely geographical origin. Meanwhile, the highly sensitive HE-SR-XRF data allow us to study the geochemical behavior of trace heavy elements, especially the \\{REEs\\} in the sediments, providing additional support to further constrain the likely geographical origin of the sediments determined by heavy minerals.

Willy Shun Kai Bong; Izumi Nakai; Shunsuke Furuya; Hiroko Suzuki; Yoshinari Abe; Keiichi Osaka; Takuya Matsumoto; Masayoshi Itou; Noboru Imai; Toshio Ninomiya

2012-01-01T23:59:59.000Z

325

Regional and Global Data  

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

Products > Regional/Global Products > Regional/Global Regional and Global Data Biogeochemical Dynamics Data Regional and global biogeochemical dynamics data can be used to improve our understanding of the structure and function of various ecosystems; to enable prediction across spatial and temporal scales; and to parameterize and validate terrestrial ecosystem models. The ORNL DAAC compiles, archives, and distributes more than 150 products from the following projects: Climate Collections Hydroclimatology Collections ISLSCP II Project Net Primary Productivity (NPP) River Discharge (RIVDIS) Russian Land Cover (RLC) Soil Collections Vegetation Collections Vegetation-Ecosystem Modeling (VEMAP) Climate Collections Climate collections include measured and modeled values for variables such as temperature, precipitation, humidity, radiation, wind velocity, and

326

Regional Districts (Texas)  

Broader source: Energy.gov [DOE]

Adjacent Water Control and Improvement Districts and Municipal Utility Districts can opt to form a Regional District to oversee water issues. Such districts may be created:(1) to purchase, own,...

327

Regional assessment of aquifers for thermal energy storage. Volume 1. Regions 1 through 6  

SciTech Connect (OSTI)

This volume contains information on the geologic and hydrologic framework, major aquifers, aquifers which are suitable and unsuitable for annual thermal energy storage (ATES) and the ATES potential of the following regions of the US: the Western Mountains; Alluvial Basins; Columbia LAVA Plateau; Colorado Plateau; High Plains; and Glaciated Central Region. (LCL)

Not Available

1981-06-01T23:59:59.000Z

328

Media Advisory - Virginia Regional Middle School Science Bowl...  

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

http:science.energy.govwdtsnsb Science Bowl rules, the locations of regional high school competitions and sample questions are posted at: http:science.energy.govwdts...

329

Improving image segmentation by learning region affinities  

SciTech Connect (OSTI)

We utilize the context information of other regions in hierarchical image segmentation to learn new regions affinities. It is well known that a single choice of quantization of an image space is highly unlikely to be a common optimal quantization level for all categories. Each level of quantization has its own benefits. Therefore, we utilize the hierarchical information among different quantizations as well as spatial proximity of their regions. The proposed affinity learning takes into account higher order relations among image regions, both local and long range relations, making it robust to instabilities and errors of the original, pairwise region affinities. Once the learnt affinities are obtained, we use a standard image segmentation algorithm to get the final segmentation. Moreover, the learnt affinities can be naturally unutilized in interactive segmentation. Experimental results on Berkeley Segmentation Dataset and MSRC Object Recognition Dataset are comparable and in some aspects better than the state-of-art methods.

Prasad, Lakshman [Los Alamos National Laboratory; Yang, Xingwei [TEMPLE UNIV.; Latecki, Longin J [TEMPLE UNIV.

2010-11-03T23:59:59.000Z

330

Regional Retail Gasoline Prices  

Gasoline and Diesel Fuel Update (EIA)

7 7 Notes: Retail gasoline prices, like those for distillate fuels, have hit record prices nationally and in several regions this year. The national average regular gasoline price peaked at $1.68 per gallon in mid-June, but quickly declined, and now stands at $1.45, 17 cents higher than a year ago. Two regions, in particular, experienced sharp gasoline price runups this year. California, which often has some of the highest prices in the nation, saw prices peak near $1.85 in mid-September, while the Midwest had average prices over $1.87 in mid-June. Local prices at some stations in both areas hit levels well over $2.00 per gallon. The reasons for the regional price runups differed significantly. In the Midwest, the introduction of Phase 2 RFG was hampered by low stocks,

331

regional | OpenEI  

Open Energy Info (EERE)

regional regional Dataset Summary Description The UK Department of Energy and Climate Change (DECC) releases annual statistics on domestic and industrial/commercial electricity and gas consumption (and number of meters) at the Middle Layer Super Output Authority (MLSOA) and Intermediate Geography Zone (IGZ) level (there are over 950 of these subregions throughout England, Scotland and Wales). Both MLSOAs (England and Wales) and IGZs (Scotland) include a minimum of approximately 2,000 households. Source UK Department of Energy and Climate Change (DECC) Date Released March 01st, 2008 (6 years ago) Date Updated Unknown Keywords Electricity Consumption gas regional UK Data application/zip icon Guidance document for interpreting data (zip, 1.2 MiB) application/vnd.ms-excel icon Excel file: 2005 MLSOA and IGZ gas and electricity (xls, 10 MiB)

332

Establishing Regional Resource Centers  

Wind Powering America (EERE)

Establishing Regional Resource Centers Establishing Regional Resource Centers July 25, 2013 Coordinator: Welcome and thank you for standing by. At this time all participants are in a listen only mode. To ask a question later during the question and answer session please press star then 1 on your touchtone phone. Today's conference is being recorded. If you have any objections you may disconnect. And I would like to turn it over to Mr. Jonathan Bartlett. Sir, you may begin. Jonathan Bartlett: Thank you very much. This is Jonathan Bartlett from the Department of Energy's Wind and Water Power Technologies Office. Today's WPA Webinar will be on the subject of establishing regional resource centers. I will be joined by Ian Baring-Gould at the National Renewable Energy Laboratory and the

333

A Near-Infrared Photometric Study of the Low Latitude Globular Clusters Liller 1, Djorgovski 1, HP 1, and NGC 6528  

E-Print Network [OSTI]

Images recorded through J, H, Ks, 2.2 micron continuum, and 2.3 micron CO filters are used to investigate the stellar contents of the low Galactic latitude globular clusters NGC 6528, Liller 1, Djorgovski 1, and HP 1, as well as surrounding bulge fields. Metallicities are estimated for the latter three clusters by comparing the colors and CO indices of giant branch stars with those in other clusters and the bulge, while reddenings are estimated from the colors of bright bulge stars in the surrounding fields. In some cases the metallicities and reddenings are significantly different from previous estimates.

T. J. Davidge

1999-09-23T23:59:59.000Z

334

Prediction of disordered regions in proteins based on the meta approach  

Science Journals Connector (OSTI)

Motivation: Intrinsically disordered regions in proteins have no unique stable structures without their partner molecules, thus these regions sometimes prevent high-quality structure determination. Furthermore, proteins with disordered regions ...

Takashi Ishida; Kengo Kinoshita

2008-06-01T23:59:59.000Z

335

The Holocene climate evolution in the high-latitude Southern Hemisphere simulated by a coupled atmosphere-sea ice-ocean-vegetation model  

E-Print Network [OSTI]

CO2 a) b) Sea-ice area -2.0 -1.5 -1.0 -0.5 0.0 0.5 -9000 -8000 -7000 -6000 -5000 -4000 -3000 -2000 concentrations 500 550 600 650 700 750 -9000 -8000 -7000 -6000 -5000 -4000 -3000 -2000 -1000 0 Time [yr] CH4conc -8000 -7000 -6000 -5000 -4000 -3000 -2000 -1000 0 Time [yr] W/m 2 JAN FEBDEC MAR AUG NOV OCTSEP JUL CH4

Renssen, Hans

336

Variability in Springtime Thaw in the Terrestrial High Latitudes: Monitoring a Major Control on the Biospheric Assimilation of Atmospheric CO2 with Spaceborne Microwave Remote Sensing  

Science Journals Connector (OSTI)

Evidence is presented from the satellite microwave remote sensing record that the timing of seasonal thawing and subsequent initiation of the growing season in early spring has advanced by approximately 8 days from 1988 to 2001 for the pan-Arctic ...

Kyle C. McDonald; John S. Kimball; Eni Njoku; Reiner Zimmermann; Maosheng Zhao

2004-12-01T23:59:59.000Z

337

Regional Service Plan South Plains Region  

E-Print Network [OSTI]

planning process; only one has done so. Various agencies purchase bus passes for distribution to their clients: Agency Average monthly purchase 1 Texas Tech University Health Sciences Center $17 LakeRidge Rehab $20 Covenant Medical Center $30....3% +1,638,202 16.0% 15.4% 9.9% In FY2005, Citibus carried a total of 3,779,325 passengers; due in large part to high gasoline prices, FY2006 ridership increased in all services with the exception of the Texas Tech University system. The ridership...

South Plains Association of Governments

2010-10-27T23:59:59.000Z

338

Northeast Region Standardized Bycatch  

E-Print Network [OSTI]

Flexibility Act Assessment, and a Regulatory Impact Review June 2007 Prepared by the New England Fishery Management Plans of the Mid-Atlantic and New England Regional Fishery Management Councils June 2007 #12;This Management Plan (FMP); Amendment 2 to the Atlantic Herring FMP; Amendment 2 to the Atlantic Salmon FMP

339

architecture architecture urban & regional  

E-Print Network [OSTI]

in architectural design, history, building construction, structures, and environmental technology from ourlandscape architecture architecture urban & regional planning environment + design college of fine-disciplinary studies. 18-to-1 Student-Teacher Ratio You'll enjoy individual, one-on-one attention in your architecture

Hwu, Wen-mei W.

340

Geothermal Regions | Open Energy Information  

Open Energy Info (EERE)

Regions Regions Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Geothermal Regions RegionsMap2012.jpg Geothermal regions were outlined for the western United States (including Alaska and Hawaii) to identify geothermal areas, projects, and exploration trends for each region. These regions were developed based on the USGS physiographic regions (U.S. Geological Survey), and then adjusted to fit geothermal exploration parameters such as differences in geologic regime, structure, heat source, surface effects (weather, vegetation patterns, groundwater flow), and other relevant factors. The 21 regions can be seen outlined in red and overlain on the 2008 USGS Geothermal Favorability Map in Figure 1.[1] Add a new Geothermal Region List of Regions Area (km2) Mean MW

Note: This page contains sample records for the topic "high latitude regions" 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

Northwest Regional Meeting  

Science Journals Connector (OSTI)

Northwest Regional Meeting ... Organizers are planning symposia on instrumental experiments in the general chemistry laboratory, active learning in chemical education, bio-based products, environmental molecular sciences laboratory user research, green chemistry, Hanford site analytical chemistry, management of the chemical enterprise, noninvasive diagnostics, radioisotopes and radiopharmaceuticals, semiconductor materials, the chemistry of advanced nuclear systems, thermodynamic models in geochemistry, sensors and sensor technology, women in chemistry, agricultural and public health protection chemistry, and public response to chemical exposure emergencies. ...

2007-02-12T23:59:59.000Z

342

Total Cross Section Measurements of Highly Enriched Isotopic Mo in the Resolved and Unresolved Energy Regions R.M. Bahran, A.M. Daskalakis, B.J. McDermott, E.J. Blain and Y. Danon  

E-Print Network [OSTI]

section data in particular are important because molybdenum can exist in reactors as a high yield fission structure based on fluctuations in the data. The analysis in this paper is limited to the unresolved energy reflective surfaces. The modular design allows operational reliability, functional versatility, relatively

Danon, Yaron

343

Regional Algal Feedstock Testbed  

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

for Collaboration * Production of algal biomass for a variety of applications - Fuel - Feed - High value Products * Cultivation of genetically modified algae * Design and...

344

CLOUD AND HAZE IN THE WINTER POLAR REGION OF TITAN OBSERVED WITH VISUAL AND INFRARED MAPPING SPECTROMETER ON BOARD CASSINI  

SciTech Connect (OSTI)

A large cloud in the north polar region of Titan was first observed by the Visual and Infrared Mapping Spectrometer (VIMS) in 2005 and then in 2006. This cloud, confined beyond the latitude 62 Degree-Sign N, is surrounded by a mixture of aerosol and mist probably lying in the low stratosphere and troposphere. Subsequent images of this region of Titan show a gradual vanishing of this cloud which was reported previously. In this paper, we characterize the physical properties of this cloud, haze, and mist as well as their time evolutions. We note several details on the images such as a secondary cloud above the main cloud and latitudes beyond 70 Degree-Sign N. We also show that the cloud disappearance leaves the polar region poorly loaded in aerosols, yielding an annular zone of aerosols between 50 Degree-Sign N and 65 Degree-Sign N. Our analysis suggests that this structure observed by VIMS in the near-IR is an annular structure observed by ISS on board Voyager one Titan year ago in 1980.

Rannou, P. [GSMA, UMR CNRS 7331, Universite de Reims Champagne-Ardenne (France); Le Mouelic, S. [LPGN, UMR CNRS 6112, Universite de Nantes (France); Sotin, C. [JPL, California Institute of Technology, PA (United States); Brown, R. H., E-mail: pascal.rannou@univ-reims.fr [LPL, University of Arizona, Tucson, AZ (United States)

2012-03-20T23:59:59.000Z

345

Geology and tectonics of Mendana Fracture Zone between latitudes 10S?-12S? and longitudes 80W?-83W?  

E-Print Network [OSTI]

ridges. The southern area has an average overall depth of nearly 4700 m. Two structural trends are present. The spreading fabric from the northern area is observed in this area and strikes N 45 W. A second set cf lineaments strike N 35 W and are only... in the southeastern region of the Pacific Ocean. The boundaries of this plate consist of three divergent plate margins and one convergent plate margin. These boundaries are the Galapagos Fift, East Pacific Rise, Chile Rise, and Peru-Chile Trench which...

Bullion, David Nelson

1988-01-01T23:59:59.000Z

346

Cascades Geothermal Region | Open Energy Information  

Open Energy Info (EERE)

Cascades Geothermal Region Cascades Geothermal Region Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Cascades Geothermal Region Details Areas (21) Power Plants (0) Projects (3) Techniques (5) Map: {{{Name}}} The Cascade Range is part of a vast mountain chain that extends from British Columbia to northern California and has been volcanically active for ~ 40 million years as a result of the convergence of the of the Juan de Fuca and Pacific plates. Two physiographic sub-provinces make up the Cascade Range; the Western Cascades and the High Cascades on the east. Middle Eocene to early Pliocene (40 - 5 million years) thick mafic lava flows, primarily of andesitic composition are associated with ash flows, tuffs, and silicic intrusive bodies and stocks that decrease in age eastward to the High Cascades. Miocene to Holocene volcanic rocks make up

347

JOURNAL DE PHYSIQUE CoZloque C7, suppZdment au n07, Tome 40, JuiZZet 1979, page C7-463 ANODE REGION OF HIGH CURRENT ARC DISCHARGE  

E-Print Network [OSTI]

JOURNAL DE PHYSIQUE CoZloque C7, suppZdment au n07, Tome 40, JuiZZet 1979, page C7- 463 ANODE investigations of the anode near-electrode layer i n high current arc ( I "102- 1 0 ~ 8 )burning freely i n of near-anode plasma with cathode erosion ma- terial, which is inherent i n spot operation mode

Paris-Sud XI, Universit├ę de

348

Compilationof Regional to Global Inventoriesof Anthropogenic Emissions  

E-Print Network [OSTI]

Compilationof Regional to Global Inventoriesof Anthropogenic Emissions CarmenM. Benkovitz, Hajime inventories of emissions of the trace species included in the study at the appropriate sectoral, spatial on emissions is also required at high resolution for the design of policies aimed at reducing emissions

349

Pennsylvania Regional Infrastructure Project  

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

CTC Team CTC Team 1 Pennsylvania Regional Infrastructure Project Presentation by: The Concurrent Technologies Corporation (CTC) Team January 6, 2004 The CTC Team 2 Presentation Outline Introduction of CTC Team CTC Background Technical Approach - CTC Team Member Presentations Conclusions The CTC Team 3 The CTC Project Team Concurrent Technologies Corporation Program Management and Coordination Hydrogen Delivery and Storage Material Development Hydrogen Sensors Concurrent Technologies Corporation Program Management and Coordination Hydrogen Delivery and Storage Material Development Hydrogen Sensors Air Products and Chemicals, Inc. Hydrogen Separation Hydrogen Sensors Air Products and Chemicals, Inc. Hydrogen Separation Hydrogen Sensors Resource Dynamics Corp. Tradeoff Analyses of Hydrogen

350

Regional Energy Baseline  

E-Print Network [OSTI]

ESL-TR-11-09-02 REGIONAL ENERGY BASELINE (1960 ~ 2009) 0 100 200 300 400 500 600 700 800 1960 1965 1970 1975 1980 1985 1990 1995 2000 2005 To tal En erg y U se pe r C ap ita (M MB tu) Year Total Energy... Use per Capita (1960-2009) US SEEC 12-States TX Hyojin Kim Juan-Carlos Baltazar, Ph.D. Jeff S. Haberl, Ph.D., P.E. September 2011 ENERGY SYSTEMS LABORATORY Texas Engineering Experiment Station Texas A&M University...

Kim, H.; Baltazar, J.C.; Haberl, J.

351

Sierra Nevada Region  

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

Sierra Nevada Region Sierra Nevada Region Power Revenue Requirement Forecast FY 2014 - FY 2017 Expenses Revenues Expenses Revenues Expenses Revenues Expenses Revenues Expenses Revenues O&M Expense: /1 Reclamation $41,172,013 $43,590,771 $45,797,325 $47,108,786 $49,408,075 Western $56,601,261 $58,299,299 $60,048,278 $61,849,726 $63,705,218 Total O&M Expense $97,773,274 $101,890,070 $105,845,603 $108,958,512 $113,113,292 Purchase Power Expense: Custom Product & Suppl. Power /2 $211,016,136 $211,016,136 $215,236,459 $215,236,459 $219,541,188 $219,541,188 $223,932,012 $223,932,012 $228,410,652 $228,410,652 HBA Costs /3 $2,310,408 $2,379,720 $2,451,112 $2,524,645 $2,600,385 Purchases for Project Use /4 $1,025,800 $0 $0 $0 $0 Washoe Cost for BR $471,500 $471,500 $471,500 $194,000 $194,000 Total Purchase Power

352

Coronal Heating and Acceleration of the High/Low-Speed Solar Wind by Fast/Slow MHD Shock Trains  

E-Print Network [OSTI]

We investigate coronal heating and acceleration of the high- and low-speed solar wind in the open field region by dissipation of fast and slow magnetohydrodynamical (MHD) waves through MHD shocks. Linearly polarized \\Alfven (fast MHD) waves and acoustic (slow MHD) waves travelling upwardly along with a magnetic field line eventually form fast switch-on shock trains and hydrodynamical shock trains (N-waves) respectively to heat and accelerate the plasma. We determine one dimensional structure of the corona from the bottom of the transition region (TR) to 1AU under the steady-state condition by solving evolutionary equations for the shock amplitudes simultaneously with the momentum and proton/electron energy equations. Our model reproduces the overall trend of the high-speed wind from the polar holes and the low-speed wind from the mid- to low-latitude streamer except the observed hot corona in the streamer. The heating from the slow waves is effective in the low corona to increase the density there, and plays an important role in the formation of the dense low-speed wind. On the other hand, the fast waves can carry a sizable energy to the upper level to heat the outer corona and accelerate the high-speed wind effectively. We also study dependency on field strength, $B_0$, at the bottom of the TR and non-radial expansion of a flow tube, $f_{\\rm max}$, to find that large $B_0/f_{\\rm max}\\gtrsim 2$ but small $B_0\\simeq 2$G are favorable for the high-speed wind and that small $B_0/f_{\\rm max}\\simeq 1$ is required for the low-speed wind.

Takeru K. Suzuki

2003-12-22T23:59:59.000Z

353

E-Print Network 3.0 - astrophysical energy region Sample Search...  

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

Radiation Field Summary: absorb- ing) region I 0( ) Free space I Ray s 0 s s1 Emergent intensity High Energy Astrophysics... High Energy Astrophysics: Radiation Field 36111...

354

Southern Rockies Geothermal Region | Open Energy Information  

Open Energy Info (EERE)

Southern Rockies Geothermal Region Southern Rockies Geothermal Region Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Southern Rockies Geothermal Region Details Areas (0) Power Plants (0) Projects (0) Techniques (0) Assessment of Moderate- and High-Temperature Geothermal Resources of the United States[1] References ÔćĹ "Assessment of Moderate- and High-Temperature Geothermal Resources of the United States" Geothermal Region Data State(s) Colorado, New Mexico Area 128,454 km┬▓128,454,000,000 m┬▓ 49,583.244 mi┬▓ 1,382,666,010,600 ft┬▓ 153,630,984,000 yd┬▓ 31,741,625.67 acres USGS Resource Estimate for this Region Identified Mean Potential 0 MW0 kW 0 W 0 mW 0 GW 0 TW Undiscovered Mean Potential 1,010 MW1,010,000 kW 1,010,000,000 W 1,010,000,000,000 mW 1.01 GW 0.00101 TW Planned Capacity

355

Received 16 Aug 2013 | Accepted 12 Dec 2013 | Published 21 Jan 2014 Asian pollution climatically modulates mid-latitude  

E-Print Network [OSTI]

.5) reaching unprecedented high levels across many cities in recent winters. In addition to the impacts radiative transfer and indirectly by influencing cloud formation8,9. By serving as cloud condensation nuclei efficiency13┬ş18. Presently, the estimates of the cloud adjustment by aerosols range from ├? 0.06 to ├? 1.33Wm

356

Regional GHG Emissions Stat s Greenhouse Gas and the Regional  

E-Print Network [OSTI]

6/5/2013 1 Regional GHG Emissions Stat s Greenhouse Gas and the Regional Power System Symposium Regional GHG Emissions ┬ş Status June 4, 2013 Gillian Charles A few clarifications This presentation and ┬Ż Valmy coal plants) 2 #12;6/5/2013 2 GHG Emissions by Economic Sector in the Pacific Northwest (2010

357

Regional GHG Emissions O tlook Greenhouse Gas and the Regional  

E-Print Network [OSTI]

6/5/2013 1 Regional GHG Emissions O tlook Greenhouse Gas and the Regional Power System Symposium Regional GHG Emissions ┬ş Outlook June 4, 2013 Steven Simmons CO2 Emission Outlook for the Pacific NW (ID MW Centralia 1 Centralia WA 1972 2020 730 MW Centralia 2 Centralia WA 1973 2025 730 MW 5 GHG Emission

358

Appendix K: Regional Definitions  

Gasoline and Diesel Fuel Update (EIA)

K K Regional Definitions The six basic country groupings used in this report (Figure K1) are defined as follows: *OECD (18 percent of the 2008 world population): North America-United States, Canada, and Mexico; OECD Europe-Austria, Belgium, Czech Republic, Denmark, Finland, France, Germany, Greece, Hungary, Iceland, Ireland, Italy, Luxem- bourg, the Netherlands, Norway, Poland, Portugal, Slovakia, Spain, Sweden, Switzerland, Turkey, and the United Kingdom. OECD Asia-Japan, South Korea, Australia, and New Zealand. *Non-OECD (82 percent of the 2008 world popula- tion): - Non-OECD Europe and Eurasia (5 percent of the 2008 world population)-Albania, Armenia, Azerbaijan, Belarus, Bosnia and Herzegovina, Bulgaria, Croatia, Estonia, Georgia, Kazakhstan, Kyrgyzstan, Latvia, Lithuania, Macedonia, Malta, Moldova, Montenegro, Romania, Russia, Serbia, Slovenia,

359

New Mexico Regional Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Mexico Regions » New Mexico Regional Mexico Regions » New Mexico Regional Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov New Mexico Regions New Mexico Regional Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Cheryl Garcia Email: cagarci@Sandia.gov Regional Event Information Date: January 25, 2014 Maximum Number of Teams: 40 Maximum Number of Teams per School: 3

360

Wyoming Regional Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Wyoming Regions » Wyoming Regional Science Wyoming Regions » Wyoming Regional Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Wyoming Regions Wyoming Regional Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Anne Theriault Email: anne@wyrsb.org Regional Event Information Date: February 8, 2014 Maximum Number of Teams: 16 Maximum Number of Teams per School: 3

Note: This page contains sample records for the topic "high latitude regions" 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

Louisiana Regional Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Louisiana Regions » Louisiana Regional Science Louisiana Regions » Louisiana Regional Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Louisiana Regions Louisiana Regional Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Tammy James Email: Tammy.James@SPR.DOE.GOV Regional Event Information Date: Saturday, February 15, 2014 Maximum Number of Teams: 30 Maximum Number of Teams per School: 2

362

High Energy Solar Particles  

Science Journals Connector (OSTI)

6 May 1976 research-article High Energy Solar Particles J. J. Quenby Protons, heavy nuclei and electrons are seen to be emitted from solar flares with energies extending up to the relativistic region. Three different...

1976-01-01T23:59:59.000Z

363

Americas Region Partnerships and Projects  

Office of Energy Efficiency and Renewable Energy (EERE)

The Office of Energy Efficiency and Renewable Energy (EERE) engages in the Americas through regional partnerships, as well as bilaterally with individual countries. In addition to the regional and...

364

Regional air quality in the Four Corners study region  

SciTech Connect (OSTI)

The body of information presented in this paper is directed to policy makers, regulators, and energy planners concerned with the effect of energy development and alternative regulatory policies on regional air quality in the Four Corners Study Region. This study was one of 5 regional studies conducted for the National Commission on Air Quality (NCAQ). Potential regional air quality impacts were evaluated out to the year 1995 for alternative energy scenarios under current and alternative regulatory policies. Highlights of the results from the regional air quality analysis are discussed in this paper.

Nochumson, D.H.

1982-01-01T23:59:59.000Z

365

Regional Summary Pacific Management Context  

E-Print Network [OSTI]

. Bocaccio, Pacific ocean perch, cowcod, and darkblotched and widow rockfish are currently in rebuildingRegional Summary Pacific Management Context The Pacific Region includes California, Oregon, and Washington. Federal fisheries in this region are managed by the Pacific Fishery Management Council (PFMC

366

Cascades Geothermal Region | Open Energy Information  

Open Energy Info (EERE)

Cascades Geothermal Region Cascades Geothermal Region (Redirected from Cascades) Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Cascades Geothermal Region Details Areas (21) Power Plants (0) Projects (3) Techniques (5) Map: {{{Name}}} The Cascade Range is part of a vast mountain chain that extends from British Columbia to northern California and has been volcanically active for ~ 40 million years as a result of the convergence of the of the Juan de Fuca and Pacific plates. Two physiographic sub-provinces make up the Cascade Range; the Western Cascades and the High Cascades on the east. Middle Eocene to early Pliocene (40 - 5 million years) thick mafic lava flows, primarily of andesitic composition are associated with ash flows, tuffs, and silicic intrusive bodies and stocks that decrease in age

367

Arizona Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Arizona Regions Arizona Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Arizona Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Arizona Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

368

Oregon Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Oregon Regions Oregon Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Oregon Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Oregon Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

369

Iowa Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Iowa Regions Iowa Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Iowa Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Iowa Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

370

Georgia Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Georgia Regions Georgia Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Georgia Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Georgia Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

371

Florida Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Florida Regions Florida Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Florida Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Florida Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

372

Wyoming Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Wyoming Regions Wyoming Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Wyoming Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Wyoming Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

373

Alaska Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Alaska Regions Alaska Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Alaska Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Alaska Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

374

Minnesota Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Minnesota Regions Minnesota Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Minnesota Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Minnesota Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

375

Idaho Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Idaho Regions Idaho Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Idaho Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Idaho Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

376

Michigan Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Michigan Regions Michigan Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Michigan Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Michigan Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

377

Texas Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Texas Regions Texas Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Texas Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Texas Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

378

Missouri Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Missouri Regions Missouri Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Missouri Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Missouri Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

379

California Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

California Regions California Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals California Regions Print Text Size: A A A RSS Feeds FeedbackShare Page California Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

380

Virginia Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Virginia Regions Virginia Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Virginia Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Virginia Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

Note: This page contains sample records for the topic "high latitude regions" 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

Montana Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Montana Regions Montana Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Montana Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Montana Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

382

Tennessee Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Tennessee Regions Tennessee Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Tennessee Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Tennessee Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

383

Massachusetts Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Massachusetts Regions Massachusetts Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Massachusetts Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Massachusetts Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

384

Washington Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Regions Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Washington Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Washington Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

385

Mississippi Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Mississippi Regions Mississippi Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Mississippi Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Mississippi Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

386

Nebraska Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Nebraska Regions Nebraska Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Nebraska Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Nebraska Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

387

Arkansas Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Arkansas Regions Arkansas Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Arkansas Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Arkansas Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

388

Colorado Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Colorado Regions Colorado Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Colorado Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Colorado Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

389

Maine Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Maine Regions Maine Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Maine Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Maine Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

390

Utah Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Utah Regions Utah Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Utah Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Utah Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

391

Maryland Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Maryland Regions Maryland Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Maryland Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Maryland Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

392

Indiana Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Indiana Regions Indiana Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Indiana Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Indiana Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

393

Oklahoma Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Oklahoma Regions Oklahoma Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Oklahoma Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Oklahoma Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

394

Illinois Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Illinois Regions Illinois Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Illinois Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Illinois Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

395

Pennsylvania Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Pennsylvania Regions Pennsylvania Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Pennsylvania Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Pennsylvania Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

396

Kentucky Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Kentucky Regions Kentucky Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Kentucky Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Kentucky Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

397

Alabama Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Alabama Regions Alabama Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Alabama Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Alabama Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

398

Vermont Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Vermont Regions Vermont Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Vermont Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Vermont Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

399

Nevada Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Nevada Regions Nevada Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Nevada Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Nevada Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

400

Delaware Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Delaware Regions Delaware Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Delaware Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Delaware Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

Note: This page contains sample records for the topic "high latitude regions" 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

Connecticut Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Connecticut Regions Connecticut Regions National Science Bowl® (NSB) NSB Home About High School Middle School Middle School Students Middle School Coaches Middle School Regionals Middle School Rules, Forms, and Resources Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Middle School Regionals Connecticut Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Connecticut Coaches can review the middle school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

402

An empirical examination of trade flows in the SAARC region  

Science Journals Connector (OSTI)

South Asia combines a low level of regional integration and the presence of relatively high trade barriers. The proportion of trade originating in the region has increased in the last decade but still lags behind many similar regional arrangements. The present study employs an augmented gravity model to examine the impact of a set of macroeconomic and other policy factors on trade flows in the South Asian Association for Regional Cooperation (SAARC) region. The interesting finding is that export between two countries would increase by 152.2%, if there exists a bilateral trade agreement between countries compared to country-pairs without having bilateral trade ties. The empirical analysis reveals that reduction in tariff level is also a better measure to improve trade in the region. Further, the study supports specialisation in the region based on the relative factor endowments and cost advantage as well.

P.R. Madhusoodanan

2010-01-01T23:59:59.000Z

403

Regional Partnerships | Department of Energy  

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

Regional Regional Partnerships Regional Partnerships DOE's Regional Carbon Sequestration Partnerships Program DOE has created a network of seven Regional Carbon Sequestration Partnerships (RCSPs) to help develop the technology, infrastructure, and regulations to implement large-scale CO2 storage (also called carbon sequestration) in different regions and geologic formations within the Nation. Collectively, the seven RCSPs represent regions encompassing: 97 percent of coal-fired CO2 emissions; 97 percent of industrial CO2 emissions; 96 percent of the total land mass; and essentially all the geologic sequestration sites in the U.S. potentially available for carbon storage. We launched this initiative in 2003. It's being completed in phases (I, II, and III) and forms the centerpiece of national efforts to develop the

404

Rhode Island Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Rhode Island Regions Rhode Island Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Rhode Island Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Rhode Island Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

405

South Daktoa Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Daktoa Regions Daktoa Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals South Daktoa Regions Print Text Size: A A A RSS Feeds FeedbackShare Page South Dakota Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

406

North Dakota Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Dakota Regions Dakota Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals North Dakota Regions Print Text Size: A A A RSS Feeds FeedbackShare Page North Dakota Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

407

New York Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

York Regions York Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals New York Regions Print Text Size: A A A RSS Feeds FeedbackShare Page New York Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

408

West Virginia Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

West Virginia Regions West Virginia Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals West Virginia Regions Print Text Size: A A A RSS Feeds FeedbackShare Page West Virginia Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

409

New Jersey Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Jersey Regions Jersey Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals New Jersey Regions Print Text Size: A A A RSS Feeds FeedbackShare Page New Jersey Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

410

New Mexico Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Mexico Regions Mexico Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals New Mexico Regions Print Text Size: A A A RSS Feeds FeedbackShare Page New Mexico Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your school's state, county, city, or district.

411

Puerto Rico Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Puerto Rico Regions Puerto Rico Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Puerto Rico Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Puerto Rico Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

412

North Carolina Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Carolina Regions Carolina Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals North Carolina Regions Print Text Size: A A A RSS Feeds FeedbackShare Page North Carolina Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

413

Washington DC Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Washington DC Regions Washington DC Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals Washington DC Regions Print Text Size: A A A RSS Feeds FeedbackShare Page Washington, DC Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

414

New Hampshire Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Hampshire Regions Hampshire Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals New Hampshire Regions Print Text Size: A A A RSS Feeds FeedbackShare Page New Hampshire Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

415

U.S. Virgin Islands Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

U.S. Virgin Islands Regions U.S. Virgin Islands Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals U.S. Virgin Islands Regions Print Text Size: A A A RSS Feeds FeedbackShare Page U.S. Virgin Islands Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

416

South Carolina Regions | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Carolina Regions Carolina Regions National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov High School Regionals South Carolina Regions Print Text Size: A A A RSS Feeds FeedbackShare Page South Carolina Coaches can review the high school regional locations listed below. Please note: Registrations are based on the location of your school. Please be sure to select the regional that is designated for your

417

Understanding Regional Economic Growth in IndiaUnderstanding Regional Economic Growth in India Understanding Regional Economic  

E-Print Network [OSTI]

Understanding Regional Economic Growth in IndiaUnderstanding Regional Economic Growth in India Understanding Regional Economic Growth in India* Jeffrey D. Sachs Director The Earth Institute at Columbia_ramiah@yahoo.co.uk Asian Economic Papers 1:3 ┬ę 2002 The Earth Institute at Columbia University and the Massachusetts

418

Multilateral, regional and bilateral energy trade governance  

SciTech Connect (OSTI)

The current international energy trade governance system is fragmented and multi-layered. Streamlining it for greater legal cohesiveness and international political and economic cooperation would promote global energy security. The current article explores three levels of energy trade governance: multilateral, regional and bilateral. Most energy-rich countries are part of the multilateral trading system, which is institutionalized by the World Trade Organization (WTO). The article analyzes the multilateral energy trade governance system by focusing on the WTO and energy transportation issues. Regionally, the article focuses on five major regional agreements and their energy-related aspects and examines the various causes that explain the proliferation of regional trade agreements, their compatibility with WTO law, and then provides several examples of regional energy trade governance throughout the world. When it comes to bilateral energy trade governance, this article only addresses the European Unionĺs (EU) bilateral energy trade relations. The article explores ways in which gaps could be filled and overlaps eliminated whilst remaining true to the high-level normative framework, concentrating on those measures that would enhance EU energy security.

Leal-Arcas, Rafael; Grasso, Costantino; Rios, Juan Alemany (Queen Mary Univ. of London (United Kingdom))

2014-12-01T23:59:59.000Z

419

Polarimetric modeling of corotating interaction regions (CIRs) threading massive-star winds  

E-Print Network [OSTI]

Massive star winds are complex radiation-hydrodynamic (sometimes magnetohydrodynamic) outflows that are propelled by their enormously strong luminosities. The winds are often found to be structured and variable, but can also display periodic or quasi-periodic behavior in a variety of wind diagnostics. The regular variations observed in putatively single stars, especially in UV wind lines, have often been attributed to corotating interaction regions (CIRs) like those seen in the solar wind. We present light curves for variable polarization from winds with CIR structures. We develop a model for a time-independent CIR based on a kinematical description. Assuming optically thin electron scattering, we explore the range of polarimetric light curves that result as the curvature, latitude, and number of CIRs are varied. We find that a diverse array of variable polarizations result from an exploration of cases. The net polarization from an unresolved source is weighted more toward the inner radii of the wind. Given t...

Ignace, R; Proulx-Giraldeau, F

2015-01-01T23:59:59.000Z

420

Global and Regional Solutions  

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

Robyn Rock Robyn Rock Robyn Rock Manager, BNL Proposal Center rrock@bnl.gov, (631)-344-5468 Photo of Robyn Rock Responsibilities Robyn is responsible for establishing a new Brookhaven National Laboratory (BNL) Proposal Center to support the Laboratory's development of high-quality, competitive proposals to sponsor organizations; for providing oversight for BNL proposal process, organizational performance and optimization in proposal execution; supporting the Laboratory's growth initiative through collaborations with BNL's research organizations and with external funding organizations and partners. She is also responsible for providing leadership in advising BNL's research organizations on funding opportunity requirements. Experience Robyn's strengths include 15 years of experience in Government

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


421

Appendix B Sierra Nevada Region Customer Groups and Economic Regions  

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

A- Not available electronically. A- Not available electronically. Appendix B Sierra Nevada Region Customer Groups and Economic Regions The list included in this appendix shows the Sierra Nevada Region customers with contracts expiring in the year 2004. The list indicates which customer group each customer is considered a part of for purposes of analysis. The list also shows which economic region each customer is located in. Some customers are not included in a subregion of the central and northern California region. Further discussion of the economic regions is included in Section 4.9.4 and in Appendix L. Appendix C Renewable Technology Cost Information Matrix The development of the renewable technology matrix (RTM) was undertaken to determine the primary cost and performance characteristics of renewable technologies in

422

CDKN-CARICOM-A Regional Implementation Plan for CARICOM's Regional  

Open Energy Info (EERE)

CARICOM-A Regional Implementation Plan for CARICOM's Regional CARICOM-A Regional Implementation Plan for CARICOM's Regional Climate Change Resilience Framework Jump to: navigation, search Name CDKN-CARICOM-A Regional Implementation Plan for CARICOM's Regional Climate Change Resilience Framework Agency/Company /Organization Climate and Development Knowledge Network (CDKN), United Kingdom Department for International Development Partner Caribbean Community Climate Change Centre (CCCCC), Caribbean Community Heads of State (CARICOM) Sector Climate, Energy, Land Topics Background analysis, Market analysis, Pathways analysis Website http://cdkn.org/project/planni Program Start 2010 Country Antigua and Barbuda, The Bahamas, Barbados, Belize, Dominica, Grenada, Guyana, Haiti, Jamaica, Montserrat, Saint Lucia, St. Kitts and Nevis, St. Vincent and the Grenadines, Suriname, Trinidad and Tobago

423

Southeast Texas Region Regional Public Transportation Coordination Plan  

E-Print Network [OSTI]

in the southeast Texas region include local, regional, and state entities that provide transportation, medical, workforce, and aging and disability assistance services. The SETRPC acts as the lead planning partner for the southeast Texas region. Established... opportunities for Texas Workforce Development Board clientele. Operational Projects Several of the recommendations already listed provide means to explore, plan, and implement improvements that will enhance the operational effectiveness of the transit...

Southeast Texas Regional Planning Commission

424

supplemental information for Improved regional temperature predictions  

E-Print Network [OSTI]

-EH GISS-ER INM-CM3.0 year 1850 1900 1950 2000 IPSL-CM4 MIROC3.2(hires) ECHO-G ECHAM5 MRI-CGCM2.3.2 CCSM3.1 GISS-EH GISS-ER INM-CM3.0 latitude -50 0 50 IPSL-CM4 MIROC3.2(hires) ECHO-G ECHAM5 MRI-CGCM2.3.2 CCSM3

Huybers, Peter

425

Limitations in solar module azimuth and tilt angles in building integrated photovoltaics at low latitude tropical sites in Brazil  

Science Journals Connector (OSTI)

Abstract Photovoltaic (PV) generation depends directly on the amount of radiation received by solar modules at a given temperature, and annual irradiation varies according to site location and PV array position. In this paper, the limitations and the solar irradiation levels received by building surfaces in different positions (with azimuth and tilt angle variation) in capital cities in Brazil are shown, making use of the Brazilian global horizontal solar irradiation data provided by the SWERA (Solar and Wind Energy Resource Assessment) project. These data were processed to generate figures on the irradiation at various PV module orientations and slopes for each city, which show the relative radiation levels received on specific azimuth and tilt angles in relation to the ideal position. Results were validated using four real and operating PV systems. In general, variations in azimuth or slope did not cause large annual irradiation losses up to around 20░ tilt angles. This shows to PV system planners that under these fairly flexible conditions it is possible to install PV on any orientation, keeping high levels of annual irradiation, and that limitations in orientation and tilt can be relatively low. It also allows a quick analysis of PV retrofit in building-applied photovoltaics (BAPV), when seeking the best building surfaces to incorporate PV.

═sis Portolan dos Santos; Ricardo RŘther

2014-01-01T23:59:59.000Z

426

Category:Geothermal Regions | Open Energy Information  

Open Energy Info (EERE)

Geothermalpower.jpg Geothermalpower.jpg Looking for the Geothermal Regions page? For detailed information on Geothermal Regions, click here. Category:Geothermal Regions Add.png Add a new Geothermal Region Pages in category "Geothermal Regions" The following 22 pages are in this category, out of 22 total. A Alaska Geothermal Region C Cascades Geothermal Region Central Nevada Seismic Zone Geothermal Region G Gulf of California Rift Zone Geothermal Region H Hawaii Geothermal Region Holocene Magmatic Geothermal Region I Idaho Batholith Geothermal Region N Northern Basin and Range Geothermal Region N cont. Northern Rockies Geothermal Region Northwest Basin and Range Geothermal Region O Outside a Geothermal Region R Rio Grande Rift Geothermal Region S San Andreas Geothermal Region San Andreas Split Geothermal Region

427

Figure 1. Census Regions and Divisions  

U.S. Energy Information Administration (EIA) Indexed Site

US Federal Region Map US Federal Region Map US Federal Regions/> Region 1 Connecticut, Maine, Massachusetts, New Hampshire, Rhode Island, Vermont Region 2 New Jersey, New York Region 3 Delaware, District of Columbia, Maryland, Pennsylvania, Virginia, West Virginia Region 4 Alabama, Florida, Georgia, Kentucky, Mississippi, North Carolina, South Carolina, Tennessee Region 5 Illinois, Indiana, Michigan, Minnesota, Ohio, Wisconsin Region 6 Arkansas, Louisiana, New Mexico, Oklahoma, Texas Region 7 Iowa, Kansas, Missouri, Nebraska Region 8 Colorado, Montana, North Dakota, South Dakota, Utah, Wyoming Region 9 Arizona, California, Hawaii, Nevada Region 10 Alaska, Idaho, Oregon, Washington Source: Energy Information Administration, Office of Coal, Nuclear, Electric and Alternate Fuels.

428

HIGH ENERGY DENSITY PHYSICS EXPERIMENTS WITH INTENSE HEAVY ION BEAMS  

E-Print Network [OSTI]

used to inject plasma into the final focus region right inplasma flow is slowed down once entering the high field region of the final focus

Bieniosek, F.M.

2008-01-01T23:59:59.000Z

429

HIGH ENERGY DENSITY PHYSICS EXPERIMENTS WITH INTENSE HEAVY ION BEAMS  

E-Print Network [OSTI]

used to inject plasma into the final focus region right inplasma flow is slowed down once entering the high field region of the final focus

Henestroza, E.

2012-01-01T23:59:59.000Z

430

" Level: National Data and Regional...  

U.S. Energy Information Administration (EIA) Indexed Site

6 Capability to Switch Electricity to Alternative Energy Sources, 2002; " " Level: National Data and Regional Totals;" " Row: NAICS Codes, Value of Shipments and Employment Sizes;"...

431

" Level: National Data and Regional...  

U.S. Energy Information Administration (EIA) Indexed Site

0 Capability to Switch Coal to Alternative Energy Sources, 2006; " " Level: National Data and Regional Totals;" " Row: NAICS Codes, Value of Shipments and Employment Sizes;" "...

432

" Level: National Data and Regional...  

U.S. Energy Information Administration (EIA) Indexed Site

0 Capability to Switch Coal to Alternative Energy Sources, 2002; " " Level: National Data and Regional Totals;" " Row: NAICS Codes, Value of Shipments and Employment Sizes;" "...

433

WINDExchange: About Regional Resource Centers  

Wind Powering America (EERE)

Development Siting About Regional Resource Centers Significant expansion of wind energy deployment will be required to achieve the President's goal of doubling renewable...

434

The tropics may be defined as the region between the Tropic of Cancer and the Tropic of1 Capricorn (i.e., within 23.5E N and S latitude), or according to ecozone, based on temperature,  

E-Print Network [OSTI]

transiting from socialism. Among the top1 30 countries ranked by 1994 per capita GDP, only four small million in 1994. Of these, 27 are outside of Europe. The richest of these are Turkemenistan (1994 GDP per income levels to natural resources, energy in the cases of Turkmenistan and Kazakhstan, and diamonds

435

Coordinated Regional Public Transportation Plan: Heart of Texas Region  

E-Print Network [OSTI]

Coordinated Regional Public Transportation Plan Heart of Texas Region Bosque, Falls, Freestone, Hill, Limestone & McLennan Counties December 1, 2006 TABLE OF CONTENTS Acknowledgements... of Texas Council of Governments (HOTCOG) and the McLennan County Youth Collaboration (MCYC) ---21 Central Texas Senior Ministries (CTSM), Hill County Transit (HCT) and Scott and White (S&W) Medical Facilities...

Heart of Texas Council of Governments

2006-12-01T23:59:59.000Z

436

Regional Systems Development for Geothermal Energy Resources Pacific Region  

Open Energy Info (EERE)

Systems Development for Geothermal Energy Resources Pacific Region Systems Development for Geothermal Energy Resources Pacific Region (California and Hawaii). Task 3: water resources evaluation. Topical report Jump to: navigation, search GEOTHERMAL ENERGYGeothermal Home Report: Regional Systems Development for Geothermal Energy Resources Pacific Region (California and Hawaii). Task 3: water resources evaluation. Topical report Details Activities (1) Areas (1) Regions (0) Abstract: The fundamental objective of the water resources analysis was to assess the availability of surface and ground water for potential use as power plant make-up water in the major geothermal areas of California. The analysis was concentrated on identifying the major sources of surface and ground water, potential limitations on the usage of this water, and the

437

Temporal changes in greenspace in a highly urbanized region  

Science Journals Connector (OSTI)

...cities. Such a dramatic shift in land use coincides with policy reforms in 2000, which favoured densification. Here, we illustrate...cities. Such a dramatic shift in land use coincides with policy reforms in 2000, which favoured densification. Here, we illustrate...

2011-01-01T23:59:59.000Z

438

WIND DATA REPORT Old Rochester Regional High School  

E-Print Network [OSTI]

version 3.1 Renewable Energy Research Laboratory University of Massachusetts, Amherst 160 Governors Drive This report was prepared by the Renewable Energy Research Laboratory (RERL) at the University of Massachusetts, Amherst in the course of performing work sponsored by the Renewable Energy Trust (RET), as administered

Massachusetts at Amherst, University of

439

ANNUAL WIND DATA REPORT Old Rochester Regional High School  

E-Print Network [OSTI]

Report template version 1.3 Renewable Energy Research Laboratory University of Massachusetts, Amherst 160 AND ACKNOWLEDGEMENTS This report was prepared by the Renewable Energy Research Laboratory (RERL) at the University of Massachusetts, Amherst in the course of performing work sponsored by the Renewable Energy Trust (RET

Massachusetts at Amherst, University of

440

WIND DATA REPORT Old Rochester Regional High School  

E-Print Network [OSTI]

version 2.0 Renewable Energy Research Laboratory University of Massachusetts, Amherst 160 Governors Drive This report was prepared by the Renewable Energy Research Laboratory (RERL) at the University of Massachusetts, Amherst in the course of performing work sponsored by the Renewable Energy Trust (RET), as administered

Massachusetts at Amherst, University of

Note: This page contains sample records for the topic "high latitude regions" 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

HIGH ENERGY EXCITATION FUNCTIONS IN THE HEAVY REGION  

E-Print Network [OSTI]

145, 777 (1940). F19(d,H3)F18 - R. S. Krishnan, NatureProtons 4 Mev: 018(p,n)F18 _ L. A. DuBridge, S. W. Barnes,

Meinke, W.W.; Wick, G.C.; Seaborg, G.T.

2008-01-01T23:59:59.000Z

442

Energy-efficient housing for low-income students in a highly variable environment of central Argentina  

Science Journals Connector (OSTI)

Socio-economic, educational and environmental reasons have driven the building of energy-efficient dwellings for low-income students in University of La Pampa. The buildings are located in the central region of Argentina (35░ 70? of South latitude), an area of warm temperate climate. Energy conservation devices, passive solar heating, natural ventilation and solar protection were the main strategies of design. The resulting design comprised three blocks of housing with a useful floor area of 900ám2. Two bedrooms, a dining room and essential services make up each house. Solar gains through transparent areas to the North are provided for all main spaces. Northern shading devices and metallic pergolas protect all windows in summer. In spite of high external temperature variability, the simulated performance during the design stage showed a remarkable internal thermal stability. The thermal and energy monitoring started in September 1999 and had two phases: (a) under real conditions of use and (b) during student's summer holidays (when the buildings were not inhabited). The results from the monitoring process suggest that interpretations about the building behaviour cannot be restricted to constructive issues. Useful inferences cannot be done from design and building technology only. The thermal behaviour was the result of construction, non-construction factors like dwellers habits, and their interaction. Energy saving in heating during the winter season was around 50%.

C. FilippÝn; A. Beascochea

2007-01-01T23:59:59.000Z

443

Market Statistics Northern Colorado Region  

E-Print Network [OSTI]

Market Statistics RE Northern Colorado Region #12;┬ę2013 Everitt Real Estate Center, All Rights. The EREC Market Statistics for the Northern Colorado region details historical closing and inventory trends. The EREC Market Statistics report is available for download at http

444

NORTHEAST REGIONAL REFINED PETROLEUM PRODUCT RESERVE | Department...  

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

NORTHEAST REGIONAL REFINED PETROLEUM PRODUCT RESERVE NORTHEAST REGIONAL REFINED PETROLEUM PRODUCT RESERVE The Northeast region of the U.S. is particularly vulnerable to gasoline...

445

Regional Energy Efficiency Programs | Department of Energy  

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

Regional Energy Efficiency Programs Regional Energy Efficiency Programs This presentation covers regional industrial energy efficiency programs in the Midwest, Southeast, and...

446

Regional Science Bowl | netl.doe.gov  

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

Regional Science Bowl West Virginia Regional Site SWPA Regional Site The U.S. Department of Energy (DOE) National Science Bowl is a nationwide academic competition that tests...

447

WINDExchange: Wind Energy Regional Resource Centers  

Wind Powering America (EERE)

Bookmark and Share Regional Resource Centers About Economic Development Siting Wind Energy Regional Resource Centers The U.S. Department of Energy's Regional Resource Centers...

448

Property:GeothermalRegion | Open Energy Information  

Open Energy Info (EERE)

Property Name GeothermalRegion Property Name GeothermalRegion Property Type Page Pages using the property "GeothermalRegion" Showing 25 pages using this property. (previous 25) (next 25) A Abraham Hot Springs Geothermal Area + Northern Basin and Range Geothermal Region + Adak Geothermal Area + Alaska Geothermal Region + Aidlin Geothermal Facility + Holocene Magmatic Geothermal Region + Akun Strait Geothermal Area + Alaska Geothermal Region + Akutan Fumaroles Geothermal Area + Alaska Geothermal Region + Akutan Geothermal Project + Alaska Geothermal Region + Alum Geothermal Area + Walker-Lane Transition Zone Geothermal Region + Alum Geothermal Project + Walker-Lane Transition Zone Geothermal Region + Alvord Hot Springs Geothermal Area + Northwest Basin and Range Geothermal Region +

449

Local FIRST robotics teams dominate regionals, advance to world  

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

Features Features 2014 2013 2012 2011 2010 News Home | ORNL | News | Features | 2013 SHARE News Feature Local FIRST robotics teams dominate regionals, advance to world championship UT-Battelle continues third year of support for high school engineering event (From left) Students from Hardin Valley Academy, Halls High School and Oak Ridge High School celebrate winning the 2013 championship title at the FIRST robotics Smoky Mountains regionals on March 30. UT-Battelle, managing contractor of ORNL, has supported the program for the last three years. Photo courtesy of Michael Messing. (From left) Students from Hardin Valley Academy, Halls High School and Oak Ridge High School celebrate winning the 2013 championship title at the FIRST robotics Smoky Mountains regionals on March 30. UT-Battelle, managing

450

New Jersey Regional Science Bowl | Princeton Plasma Physics Lab  

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

New Jersey Regional Science Bowl New Jersey Regional Science Bowl Competition Overview: Each year PPPL hosts the New Jersey Regional Science Bowl which decides which teams from the local area can continue onto the national competition in Washington, D.C.! The Science Bowl is a double elimination contest with question and answer rounds in the fields of chemistry, biology, physics, astronomy, mathematics and general and earth sciences. Middle School: Teams of a coach and five middle school students (four members and an alternate) in grades 6-8 from middle schools and home schools are invited to enter. High School: Teams of a coach and five high school students (four members and an alternate) in grades 9-12 from high schools and home schools are invited to enter. The NJ Regional Competition is open to all of NJ and surrounding areas that

451

Mass Flows in Cometary UCHII Regions  

E-Print Network [OSTI]

High spectral and spatial resolution, mid-infrared fine structure line observations toward two ultracompact HII (UCHII) regions (G29.96 -0.02 and Mon R2) allow us to study the structure and kinematics of cometary UCHII regions. In our earlier study of Mon R2, we showed that highly organized mass motions accounted for most of the velocity structure in that UCHII region. In this work, we show that the kinematics in both Mon R2 and G29.96 are consistent with motion along an approximately paraboloidal shell. We model the velocity structure seen in our mapping data and test the stellar wind bow shock model for such paraboloidal like flows. The observations and the simulation indicate that the ram pressures of the stellar wind and ambient interstellar medium cause the accumulated mass in the bow shock to flow along the surface of the shock. A relaxation code reproduces the mass flow's velocity structure as derived by the analytical solution. It further predicts that the pressure gradient along the flow can accelerate ionized gas to a speed higher than that of the moving star. In the original bow shock model, the star speed relative to the ambient medium was considered to be the exit speed of ionized gas in the shell.

Qing-Feng Zhu; John H. Lacy; Daniel T. Jaffe; Thomas K. Greathouse; Matthew J. Richter

2005-06-06T23:59:59.000Z

452

Eastern Idaho Regional Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Eastern Idaho Regional Science Eastern Idaho Regional Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Idaho Regions Eastern Idaho Regional Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Steve Zollinger Email: zollingers@byui.edu Regional Event Information Date: TBD Maximum Number of Teams: 20 Maximum Number of Teams per School: 2 Registration Fee: N/A

453

Illinois State Regional Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Illinois State Regional Illinois State Regional Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Illinois Regions Illinois State Regional Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Ken Wester Email: kwester@ilstu.edu Regional Event Information Date: February 8, 2014 Maximum Number of Teams: 24 Maximum Number of Teams per School: 3

454

Western Idaho Regional Science Bowl | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Western Idaho Regional Science Western Idaho Regional Science Bowl National Science Bowl® (NSB) NSB Home About High School High School Students High School Coaches High School Regionals High School Rules, Forms, and Resources Middle School Attending National Event Volunteers 2013 Competition Results News Media WDTS Home Contact Information National Science Bowl® U.S. Department of Energy SC-27/ Forrestal Building 1000 Independence Ave., SW Washington, DC 20585 P: 202-586-6702 E: National.Science.Bowl@science.doe.gov Idaho Regions Western Idaho Regional Science Bowl Print Text Size: A A A RSS Feeds FeedbackShare Page Regional Coordinator Information Name: Kami Faylor Email: ksfaylor@micron.com Regional Event Information Date: TBD Maximum Number of Teams: 26 Maximum Number of Teams per School: 2 Registration Fee: N/A

455

Annual training event instrumental in regionĺs safety culture  

Broader source: Energy.gov [DOE]

OREM is participating in Safety Fest Tennessee. The annual event provides training on important safety disciplines that are helping local workers create one of the safest workplaces in the region.

456

Indonesia Geothermal Region | Open Energy Information  

Open Energy Info (EERE)

Indonesia Geothermal Region Retrieved from "http:en.openei.orgwindex.php?titleIndonesiaGeothermalRegion&oldid706190...

457

China Geothermal Region | Open Energy Information  

Open Energy Info (EERE)

China Geothermal Region Retrieved from "http:en.openei.orgwindex.php?titleChinaGeothermalRegion&oldid70619...

458

Composition of saturn's atmosphere at northern temperate latitudes from Voyager iris spectra: NH/sub 3/, PH/sub 3/, C/sub 2/H/sub 2/, C/sub 2/H/sub 6/, CH/sub 3/D, CH/sub 4/, and the saturnian D/H isotopic ratio  

SciTech Connect (OSTI)

The abundances of minor atmospheric constituents at northern Saturnian latitudes have been inferred from infrared emission spectra recorded by Voyager. The NH/sub 3/, PH/sub 3/, C/sub 2/H/sub 2/, and C/sub 2/H/sub 6/ vertical distributions have been determined from spectra selected in a cloud-free region centered approximately at the latitude of the Voyager 2 radio-occultation point (36.5 N). The NH/sub 3/ mixing ratio in the upper troposphere is found to be compatible with the saturated partial pressure. The inferred PH/sub 3//H/sub 2/ ratio of 1.4 +- 0.8 x 10/sup -6/ is higher than the value derived from the solar P/H ratio, and the PH/sub 3/ vertical profile may extend somewhat into the stratosphere, up to a few millibars. The stratospheric C/sub 2/H/sub 2//H/sub 2/ and C/sub 2/H/sub 6//H/sub 2/ ratios are, respectively, 2.1 +- 1.4 x 10/sup -7/ and 3.0 x 1.1 x 10/sup -6/; the latter decreases sharply below the 20-50 mbar level. A larger selection of spectra yields CH/sub 3/D/H/sub 2/ = 3.9 +- 2.5 x 10/sup -7/ and CH/sub 4//H/sub 2/ = 4.5/sup +2.4//sub -1.9/ x 10/sup -3/. This result implies an enrichment of Saturn's upper atmosphere is carbon by at least a factor of 3 over the solar abundance. The D/H value resulting from our CH/sub 3/D/CH/sub 4/ ratio is 1.6/sup +1.3//sub -1.2/ x 10/sup -5/, significantly lower than previous determinations obtained from HD lines; it is also less than half of the IRIS-inferred Jovian value. Finally, the interpretation of two NH/sub 3/ lines in the 5 ..mu..m window suggests a NH/sub 3/H/sub 2/ ratio at the 2 bar level below the solar value.

Courtin, R.; Gautier, D.; Marten, A.; Bezard, B.; Hanel, R.

1984-12-15T23:59:59.000Z

459

interconnect region | OpenEI  

Open Energy Info (EERE)

interconnect region interconnect region Dataset Summary Description Datasets are for the US electricity grid system interconnect regions (ASCC, FRCC, HICC, MRO, NPCC, RFC, SERC, SPP, TRE, WECC) for 2008. The data is provided in life cycle inventory (LCI) forms (both xls and xml). A module report and a detailed spreadsheet are also included. Source US Life Cycle Inventory Database Date Released May 01st, 2011 (3 years ago) Date Updated Unknown Keywords ASCC FRCC HICC interconnect region LCI life cycle inventory MRO NPCC RFC SERC SPP TRE unit process US utilities WECC Data application/zip icon interconnect_lci_datasets_2008.zip (zip, 6.3 MiB) Quality Metrics Level of Review Some Review Comment Temporal and Spatial Coverage Frequency Time Period License License Open Data Commons Public Domain Dedication and Licence (PDDL)

460

Urban and Regional Air Quality  

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

equipment equipment Urban and Regional Air Quality Research in this area is concerned with regional air quality issues such as: Controlling nitrogen oxides (NOx) and volatile organic compounds, to manage tropospheric ozone pollution. Hazardous air pollutants: using science to base standards on rigorously studied risks. Air quality and climate: how does climate influence air quality at a regional or local level? Current modeling practices often do not capture variations in pollutants such as ozone-they represent a limited sample of the diverse meteorology and human behavior that affect air pollution. Improved modeling of regional air quality will help understand variability, reveal patterns of behavior, and pollutant transport issues. Controlled experiments in lab and field can help validate improved models.

Note: This page contains sample records for the topic "high latitude regions" 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

RAFT Regional Algal Feedstock Testbed  

Broader source: Energy.gov [DOE]

Breakout Session 3BŚIntegration of Supply Chains III: Algal Biofuels Strategy RAFT Regional Algal Feedstock Testbed Kimberly Ogden, Professor, University of Arizona, Engineering Technical Lead, National Alliance for Advanced Biofuels and Bioproducts

462

Anomalous Emission from HII regions  

E-Print Network [OSTI]

Spinning dust appears to be the best explanation for the anomalous emission that has been observed at $\\sim 10-60$ GHz. One of the best examples of spinning dust comes from a HII region in the Perseus molecular cloud. Observations of other HII regions also show tentative evidence for excess emission at frequencies $\\sim 30$ GHz, although at lower emissivity levels. A new detection of excess emission at 31 GHz in the HII region RCW175 has been made. The most plausible explanation again comes from spinning dust. HII regions are a good place to look for spinning dust as long as accurate radio data spanning the $\\sim 5-100$ GHz range is available.

C. Dickinson

2008-08-04T23:59:59.000Z

463

High School Students | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

Students National Science Bowl (NSB) NSB Home About High School High School Students High School Coaches High School Regionals Middle School Attending National Event Volunteers...

464

High-resolution stratospheric tracer fields estimated from satellite observations using Lagrangian trajectory calculations  

SciTech Connect (OSTI)

A technique is introduced by which high-resolution tracer fields may be constructed from low-resolution satellite observations. The technique relies upon the continual cascade of tracer variance from large to small scales and makes use of wind fields generated by a data assimilation scheme. To demonstrate its usefulness, the technique has been applied in a study of isentropic distributions of nitrous oxide in the winter midstratosphere, using measurements made by the Improved Stratospheric and Mesospheric Sounder (ISAMS) instrument on the Upper Atmosphere Research Satellite (UARS). The results show that the high-resolution fields significantly increase the amount of information that is available from the satellite observations. The fields give insights into the characteristic structure and evolution of tracer distributions at scales that are normally obscured from view. Two results are particularly noteworthy. First, at the interface between low and middle latitudes there is evidence of active mixing. This mixing occurs on the eastern, equatorward side of air that is being drawn toward high latitudes around the polar vortex. Second, in the anticyclone, a complex pattern of transport is revealed. Air drawn in from low latitudes spirals together with ambient midlatitude air. Small scales are generated relatively slowly in the organized flow, and persistent filamentary structures, with transverse scales of hundreds of kilometers or greater, are seen.

Sutton, R.T.; Maclean, H.; Swinbank, R.; O`Neill, A.; Taylor, F.W. [Oxford Univ., Oxford (United Kingdom)] [Oxford Univ., Oxford (United Kingdom); [Meteorological Office, Bracknell, Berkshire (United Kingdom); [Univ. of Reading, Reading (United Kingdom)

1994-10-01T23:59:59.000Z

465