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Sample records for luiseno lule sami

  1. Soboba Band of Luiseno Indians- 2011 Project

    Broader source: Energy.gov [DOE]

    The Soboba Band of Luiseno Indians would like to begin to focus on renewable sources for electricity and to actively target lowering the energy usage of the community.

  2. Project Reports for Soboba Band of Luiseno Indians- 2011 Project

    Broader source: Energy.gov [DOE]

    The Soboba Band of Luiseno Indians would like to begin to focus on renewable sources for electricity and to actively target lowering the energy usage of the community.

  3. Soboba Band of Luiseno Indians

    Office of Environmental Management (EM)

    Meter 2 16) S.W. 1 oaks Energy Evaluation Energy Consumption Planning Areas & Meters 2 Year kwh Usage Average Annual kwh Usage MW DC PV Size For 100% Offset MW AC PV Size For ...

  4. Soboba Band of Luiseno Indians

    Office of Environmental Management (EM)

    Oaks Meter 2 16) S.W. 1 oaks Energy Evaluation Energy Consumption Planning Areas & Meters 2 Year kwh Usage Average Annual kwh Usage MW DC PV Size For 100% Offset MW AC PV ...

  5. Soboba Band of Luiseno Indians - Strategic Tribal Energy Planning Project

    Energy Savers [EERE]

    Tribal Energy Program Review Denver, CO November, 2 012 By: Erica Helms---Schenk, Environmental Director Soboba Energy Efficiency and ConservaKon Project Soboba Band of Luiseño Indians Soboba Band of Luiseño Indians Soboba Band of Luiseño Indians Our Champions - Who is Involved? Gerald Wilson Soboba Tribal Environmental & Brian McDonald - Department our SCE RepresentaKves Soboba Tribal Council IT --- Steven Nino Public Works - Ken McLaughlin and Summer Willis Project Goals and ObjecKves

  6. THE SAMI GALAXY SURVEY: TOWARD A UNIFIED DYNAMICAL SCALING RELATION FOR GALAXIES OF ALL TYPES

    SciTech Connect (OSTI)

    Cortese, L.; Glazebrook, K.; Mould, J.; Fogarty, L. M. R.; Bland-Hawthorn, J.; Croom, S. M.; Scott, N.; Allen, J. T.; Bloom, J.; Bryant, J. J.; Ho, I.-T.; Bekki, K.; Colless, M.; Sharp, R.; Couch, W.; Goodwin, M.; Tonini, C.; Cluver, M.; Davies, R. L.; Drinkwater, M. J.; and others

    2014-11-10

    We take advantage of the first data from the Sydney-AAO Multi-object Integral field Galaxy Survey to investigate the relation between the kinematics of gas and stars, and stellar mass in a comprehensive sample of nearby galaxies. We find that all 235 objects in our sample, regardless of their morphology, lie on a tight relation linking stellar mass (M {sub *}) to internal velocity quantified by the S {sub 0.5} parameter, which combines the contribution of both dispersion (σ) and rotational velocity (V {sub rot}) to the dynamical support of a galaxy (S{sub 0.5}=√(0.5 V{sub rot}{sup 2}+σ{sup 2})). Our results are independent of the baryonic component from which σ and V {sub rot} are estimated, as the S {sub 0.5} of stars and gas agree remarkably well. This represents a significant improvement compared to the canonical M {sub *} versus V {sub rot} and M {sub *} versus σ relations. Not only is no sample pruning necessary, but also stellar and gas kinematics can be used simultaneously, as the effect of asymmetric drift is taken into account once V {sub rot} and σ are combined. Our findings illustrate how the combination of dispersion and rotational velocities for both gas and stars can provide us with a single dynamical scaling relation valid for galaxies of all morphologies across at least the stellar mass range 8.5 

  7. Development of High-Throughput Screens to Target SAM-I Riboswitches (2014 DOE JGI Genomics of Energy & Environment Meeting)

    SciTech Connect (OSTI)

    Hickey, Scott [UC Berkely

    2014-03-19

    Scott Hickey of the University of California Berkeley speaks at the 9th Annual Genomics of Energy & Environment Meeting on March 20, 2014 in Walnut Creek, Calif.

  8. Caldwell County, Texas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Places in Caldwell County, Texas Lockhart, Texas Luling, Texas Martindale, Texas Mustang Ridge, Texas Niederwald, Texas San Marcos, Texas Uhland, Texas Retrieved from "http:...

  9. Princeton Plasma Physics Lab - Plasma physics

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

    highlighted-imageSami%20Diagnostices12.jpg" width"2304" height"1500" alt"David Thomas and Jakob Brunner" title"Elle StarkmanOffice of Communications" >

    <...

  10. Final Report for the Soboba Strategic Tribal Energy Planning Project

    SciTech Connect (OSTI)

    Miller, Kim

    2013-09-17

    In 2011 the Tribe was awarded funds from the Department of Energy to formulate the Soboba Strategic Tribal Energy Plan. This will be a guiding document used throughout the planning of projects focused on energy reduction on the Reservation. The Soboba Strategic Tribal Energy Plan's goal is to create a Five Year Energy Plan for the Soboba Band of Luiseno Indians in San Jacinto, California. This plan will guide the decision making process towards consistent progress leading to the Tribal goal of a 25% reduction in energy consumption in the next five years. It will additionally outline energy usage/patterns and will edentify areas the Tribe can decrease energy use and increase efficiency. The report documents activities undertaken under the grant, as well as incldues the Tribe's strategif energy plan.

  11. Measurement and modeling of the refilling plasmasphere during 2001

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Krall, J.; Huba, J. D.; Jordanova, V. K.; Denton, R. E.; Carranza, T.; Moldwin, M. B.

    2016-03-18

    The Naval Research Laboratory SAMI3 (Sami3 is Also a Model of the Ionosphere) and the RAM-CPL (Ring current Atmosphere interaction Model-Cold PLasma) codes are used to model observed plasmasphere dynamics during 25 November 2001 to 1 December 2001 and 1–5 February 2001. Model results compare well to plasmasphere observations of electron and mass densities. Comparison of model results to refilling data and to each other shows good agreement, generally within a factor of 2. We find that SAMI3 plasmaspheric refilling rates and ion densities are sensitive to the composition and temperature of the thermosphere and exosphere, and to photoelectron heating.more » Furthermore, results also support our previous finding that the wind-driven dynamo significantly impacts both refilling rates and plasmasphere dynamics during quiet periods.« less

  12. Chapter 11, Sample Design Cross-Cutting Protocols: The Uniform Methods Project: Methods for Determining Energy Efficiency Savings for Specific Measures

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

    1: Sample Design Cross-Cutting Protocols M. Sami Khawaja, Josh Rushton, and Josh Keeling, The Cadmus Group, Inc. Subcontract Report NREL/SR-7A30-53827 April 2013 The Uniform Methods Project: Methods for Determining Energy Efficiency Savings for Specific Measures 11 - 1 Chapter 11 - Table of Contents 1 Introduction ............................................................................................................................ 3 1.1 Chapter Organization

  13. Integration of geothermal data along the Balcones/Ouachita trend, central Texas. Final report

    SciTech Connect (OSTI)

    Woodruff, C.M. Jr.; Gever, C.; Snyder, Fred R.; Wuerch, David Robert

    1983-01-01

    This report presents data that address possible controls on warm-water resources. Data are presented on a series of maps, and interpretations appear in the brief text accompanying the maps. It is thought that structural controls provided by the Balcones Fault Zone on the west and by the Luling-Mexia-Talco Fault Zone on the east localize the warm waters. The ultimate controlling attribute is the foundered Ouachita structural belt, which, in turn, has controlled the orientation and magnitude of displacement of the superjacent normal fault systems. This thesis is supported by maps (in pocket) showing the following: distribution of thermal waters measured in wells along the Balcones/Ouachita structural trend showing water temperature in /sup 0/F, total depth of the well measured, water salinity in parts per million, and the geologic formation producing the water; structural contours on the base of the Cretaceous System showing the configuration of the Paleozoic Ouachita basement; structural configuration of the Balcones and Luling Fault Zone, Mexia and Talco Fault Zone, and foreland areas adjacent to the Ouachita Orogen using data from the Buda Limestone, Sligo Formation, and Ellenburger Group; Landsat lineaments and Bouguer gravity contours; and geothermal gradient contours of the Balcones/Ouachita trend based on thermal values from Paleozoic and selected Mesozoic formations.

  14. Networks of the Future: Extending our senses into the physical world

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

    Extending our senses into the physical world Networks of the Future: Extending our senses into the physical world The picture of a future with wireless sensor networks is quickly coming into sharper focus through the work of Laboratory computer scientist Sami Ayyorgun. August 13, 2008 Los Alamos National Laboratory sits on top of a once-remote mesa in northern New Mexico with the Jemez mountains as a backdrop to research and innovation covering multi-disciplines from bioscience, sustainable

  15. 1

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

    Networks of the Future: Extending our senses into the physical world August 13, 2008 LOS ALAMOS, New Mexico, August 13, 2008-The picture of a future with wireless sensor networks-webs of sensory devices that function without a central infrastructure -is quickly coming into sharper focus through the work of Los Alamos National Laboratory computer scientist Sami Ayyorgun. Proponents of this new technology see a world with deployments to improve a wide range of operations. Engineers could

  16. Microsoft Word - PEP-X Status Report 6-10-08.doc

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

    1 of 51 PEP-X Light Source at SLAC Status Report Revision 0 June 10, 2008 PEP-X Study Group: Karl Bane, Lynn Bentson, Kirk Bertsche, Sean Brennan, Yunhai Cai, Alex Chao, Scott DeBarger, Valery Dolgashev, Robert Hettel,, Xiaobiao Huang, Zhirong Huang, David Kharakh, Yuri Nosochkov, Thomas Rabedeau, James Safranek, John Seeman, Joachim Stöhr, Gennady Stupakov, Sami G. Tantawi, Lanfa Wang, Min-Huey Wang, Ulrich Wienands (SLAC, Menlo Park, California), Ingolf Lindau (Stanford University, Stanford,

  17. Author for correspondence: Jennifer E

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

    SUCCESSFUL TRANSFER OF SANDIA NATIONAL LABORATORIES' OUTDOOR TEST TECHNOLOGY TO TÜV RHEINLAND PHOTOVOLTAIC TESTING LABORATORY Jennifer E. Granata 1 , William E. Boyson 1 , Jay A. Kratochvil 1 , Bo Li 2 , Venkata Abbaraju 2 , GovindaSamy TamizhMani 2 and Lawrence Pratt 3* 1 Sandia National Laboratories, Albuquerque, New Mexico, USA 2 TÜV Rheinland PTL, Tempe, Arizona, USA 3 CFV Solar Test Laboratory, Inc., Albuquerque, New Mexico, USA *Work performed while employed with Sandia National

  18. Assessment of the Potential to Reduce Emissions from Road Transportation, Notably NOx, Through the Use of Alternative Vehicles and Fuels in the Great Smoky Mountains Region

    SciTech Connect (OSTI)

    Sheffield, J.

    2001-08-30

    Air pollution is a serious problem in the region of the Great Smoky Mountains. The U.S. Environmental Protection Agency (EPA) may designate non-attainment areas by 2003 for ozone. Pollutants include nitrogen oxides (NO{sub x}), sulfur dioxide (SO{sub 2}), carbon monoxide (CO), volatile organic compounds (VOCs), lead, and particulate matter (PM), which are health hazards, damage the environment, and limit visibility. The main contributors to this pollution are industry, transportation, and utilities. Reductions from all contributors are needed to correct this problem. While improvements are projected in each sector over the next decades, the May 2000 Interim Report issued by the Southern Appalachian Mountains Initiative (SAMI) suggests that the percentage of NO{sub x} emissions from transportation may increase.

  19. Deep structure of the Texas Gulf passive margin and its Ouachita-Precambrian basement: Results of the COCORP San Marcos arch survey

    SciTech Connect (OSTI)

    Culotta, R.; Latham, T.; Oliver, J.; Brown, L.; Kaufman, S. (Cornell Univ., Ithaca, NY (United States)); Sydow, M. (Pennzoil, Houston, TX (United States))

    1992-02-01

    This COCORP deep seismic survey provides a comprehensive image of the southeast-Texas part of the Gulf passive margin and its accreted Ouachita arc foundation. Beneath the updip limit of the Cenozoic sediment wedge, a prominent antiformal structure is imaged within the interior zone of the buried late Paleozoic Ouachita orogen. The structure appears to involve Precambrian Grenville basement. The crest of the antiform is coincident with the Cretaceous-Tertiary Luling-Mexia-Talco fault zone. Some of these faults dip to the northwest, counter to the general regional pattern of down-to-the-basin faulting, and appear to sole into the top of the antiform, suggesting that the Ouachita structure has been reactivated as a hingeline to the subsiding passive margin. The antiform may be tied via this fault system and the Ouachita gravity gradient to the similar Devils River, Waco, and Benton uplifts, interpreted as Precambrian basement-cored massifs. Above the Paleozoic sequence, a possible rift-related graben is imaged near the updip limit of Jurassic salt. Paleoshelf edges of the major Tertiary depositional sequences are marked by expanded sections disrupted by growth faults and shale diapirs. Within the Wilcox Formation, the transect crosses the mouth of the 900-m-deep Yoakum Canyon, a principal pathway of sediment delivery from the Laramide belt to the Gulf. Beneath the Wilcox, the Comanchean (Lower Cretaceous) shelf edge, capped by the Stuart City reef, is imaged as a pronounced topographic break onlapped by several moundy sediment packages. Because this segment of the line parallels strike, the topographic break may be interpreted as a 2,000-m-deep embayment in the Cretaceous shelf-edge, and possibly a major submarine canyon older and deeper than the Yoakum Canyon.

  20. QUENCHING DEPENDS ON MORPHOLOGIES: IMPLICATIONS FROM THE ULTRAVIOLET-OPTICAL RADIAL COLOR DISTRIBUTIONS IN GREEN VALLEY GALAXIES

    SciTech Connect (OSTI)

    Pan, Zhizheng; Lin, Weipeng; Li, Jinrong; Kong, Xu; Wang, Jing E-mail: linwp@shao.ac.cn

    2014-09-01

    In this Letter, we analyze the radial ultraviolet-optical color distributions in a sample of low redshift green valley galaxies, with the Galaxy Evolution Explorer (GALEX)+Sloan Digital Sky Survey (SDSS) images, to investigate how the residual recent star formation is distributed in these galaxies. We find that the dust-corrected u r colors of early-type galaxies (ETGs) are flat out to R {sub 90}, while the colors monotonously turn blue when r > 0.5 R {sub 50} for late-type galaxies (LTGs). More than half of the ETGs are blue-cored and have remarkable positive NUV r color gradients, suggesting that their star formations are centrally concentrated. The rest have flat color distributions out to R {sub 90}. The centrally concentrated star formation activity in a large portion of ETGs is confirmed by the SDSS spectroscopy, showing that ?50% of the ETGs have EW(H?)>6.0 . Of the LTGs, 95% show uniform radial color profiles, which can be interpreted as a red bulge plus an extended blue disk. The links between the two kinds of ETGs, e.g., those objects having remarkable ''blue-cores'' and those having flat color gradients, are less known and require future investigations. It is suggested that the LTGs follow a general model by which quenching first occurs in the core regions, and then finally extend to the rest of the galaxy. Our results can be re-examined and have important implications for the IFU surveys, such as MaNGA and SAMI.