Sample records for foothill vineyard euclid

  1. Euclid Programming

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

    Programming Programming Compiling and linking programs on Euclid. Compiling Codes How to compile and link MPI codes on Euclid. Read More Using the ACML Math Library How to...

  2. Euclid File Systems

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

    File storage File storage Disk Quota Change Request Form Euclid File Systems Euclid has 3 kinds of file systems available to users: home directories, scratch directories and...

  3. Foothills Model Forest Business Strategy

    E-Print Network [OSTI]

    Foothills Model Forest Business Strategy 2007 ­ 2012 November 2006 #12;Page ii TABLE OF CONTENTS FOOTHILLS MODEL FOREST Business Strategy for April 2007 to March 2012 1.0 INTRODUCTION....................................................................................................................... 4 2.4 Foothills Model Forest Values

  4. Running jobs on Euclid

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

    Running jobs Running jobs Overview and Basic Description Euclid is a single node system with 48 processors. It supports both multiprocessing (MPI) and multithreading programming...

  5. Compiling Codes on Euclid

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

    Compiling Codes Compiling Codes Overview Open Mpi is the the only MPI library available on Euclid. This implementation of MPI-2 is described at Open MPI: Open Source High...

  6. Texas Vineyard Guide.

    E-Print Network [OSTI]

    McEachern, George Ray; Stein, Larry A.; Gan, Peretz; Lipe, William N.; Stockton, L. Austin; Helmers, Sammy G.

    1982-01-01T23:59:59.000Z

    in the following years. The cordons may "wrap" the wire and become self supportive. CANE TRAINING Most vineyards in Texas are cordon trained and pruned, but this is not always the case. Cane pruning is recommended for varieties which do not produce fruit... avoids undue damage to endposts and anchor Wires when equipment turns at the end of rows. Number vineyard rows so that work assignments, irrigation schedules, etc., can be understood and sites located easily. PLANTING THE VINES Plant vines...

  7. Using the ACML Math Library on Euclid

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

    ACML Math Library Using the ACML Math Library The AMD ACML math library is available on Euclid. This library is described at the ACML Math Library. To compile and link with it,...

  8. Foothills Energy Ventures | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdf Jump to:ar-80m.pdfFillmoreGabbs Valley Area(Sasada,Foothills Energy Ventures

  9. Foothills Parkway Section 8B Final Environmental Report, Volume 1

    SciTech Connect (OSTI)

    Blasing, T.J.; Cada, G.F.; Carer, M.; Chin, S.M.; Dickerman, J.A.; Etnier, D.A.; Gibson, R.; Harvey, M.; Hatcher, B.; Lietzske, D.; Mann, L.K.; Mulholland, P.J.; Petrich, C.H.; Pounds, L.; Ranney, J.; Reed, R.M.; Ryan, P.F.; Schweitzer, M.; Smith, D.; Thomason, P.; Wade, M.C.

    1999-07-01T23:59:59.000Z

    In 1994, Oak Ridge National Laboratory (ORNL) was tasked by the National Park Service (NPS) to prepare an Environmental Report (ER) for Section 8B of the Foothills Parkway in the Great Smoky Mountains National Park (GSMNP). Section 8B represents 27.7 km (14.2 miles) of a total of 115 km (72 miles) of the planned Foothills Parkway and would connect the Cosby community on the east to the incorporated town of Pittman Center to the west.

  10. Cosmology and fundamental physics with the Euclid satellite

    E-Print Network [OSTI]

    Luca Amendola; Stephen Appleby; David Bacon; Tessa Baker; Marco Baldi; Nicola Bartolo; Alain Blanchard; Camille Bonvin; Stefano Borgani; Enzo Branchini; Clare Burrage; Stefano Camera; Carmelita Carbone; Luciano Casarini; Mark Cropper; Claudia deRham; Cinzia di Porto; Anne Ealet; Pedro G. Ferreira; Fabio Finelli; Juan Garcia-Bellido; Tommaso Giannantonio; Luigi Guzzo; Alan Heavens; Lavinia Heisenberg; Catherine Heymans; Henk Hoekstra; Lukas Hollenstein; Rory Holmes; Ole Horst; Knud Jahnke; Thomas D. Kitching; Tomi Koivisto; Martin Kunz; Giuseppe La Vacca; Marisa March; Elisabetta Majerotto; Katarina Markovic; David Marsh; Federico Marulli; Richard Massey; Yannick Mellier; David F. Mota; Nelson Nunes; Will Percival; Valeria Pettorino; Cristiano Porciani; Claudia Quercellini; Justin Read; Massimiliano Rinaldi; Domenico Sapone; Roberto Scaramella; Constantinos Skordis; Fergus Simpson; Andy Taylor; Shaun Thomas; Roberto Trotta; Licia Verde; Filippo Vernizzi; Adrian Vollmer; Yun Wang; Jochen Weller; Tom Zlosnik

    2012-06-06T23:59:59.000Z

    Euclid is a European Space Agency medium class mission selected for launch in 2019 within the Cosmic Vision 2015-2025 programme. The main goal of Euclid is to understand the origin of the accelerated expansion of the Universe. Euclid will explore the expansion history of the Universe and the evolution of cosmic structures by measuring shapes and redshifts of galaxies as well as the distribution of clusters of galaxies over a large fraction of the sky. Although the main driver for Euclid is the nature of dark energy, Euclid science covers a vast range of topics, from cosmology to galaxy evolution to planetary research. In this review we focus on cosmology and fundamental physics, with a strong emphasis on science beyond the current standard models. We discuss five broad topics: dark energy and modified gravity, dark matter, initial conditions, basic assumptions and questions of methodology in the data analysis. This review has been planned and carried out within Euclid's Theory Working Group and is meant to provide a guide to the scientific themes that will underlie the activity of the group during the preparation of the Euclid mission.

  11. WIND DATA REPORT Tisbury, Martha's Vineyard,

    E-Print Network [OSTI]

    Massachusetts at Amherst, University of

    WIND DATA REPORT Tisbury, Martha's Vineyard, Massachusetts September 1, 2007 ­ November 30, 2007...................................................................................................................... 8 Wind Speed Time Series............................................................................................................. 9 Wind Speed Distributions

  12. The Euclid space-time diagram of the theory of relativity

    E-Print Network [OSTI]

    W. LiMing

    2014-06-03T23:59:59.000Z

    A conventional space-time diagram is $r-ct$ one, which satisfies the Minkowski geometry. This geometry conflict the intuition from the Euclid geometry. In this work an Euclid space-time diagram is proposed to describe relativistic world lines with an exact Euclid geometry. The relativistic effects such as the dilation of moving clocks, the contraction of moving length, and the twin paradox can be geometrically expressed in the Euclid space-time diagram. It is applied to the case of a satellite clock to correct the gravitational effect. It is found that this Euclid space-time diagram is much more intuitive than the conventional space-time diagram.

  13. Fortuna Foothills, Arizona: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualPropertyd8c-a9ae-f8521cbb8489Information HydroFontana,dataset nameFortFortuna Foothills,

  14. Catalina Foothills, Arizona: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:EzfeedflagBiomassSustainableCSLInformationMissouri: EnergyCastleton,Catalina Foothills,

  15. Thrust belt architecture of the central and southern Western Foothills of Taiwan

    E-Print Network [OSTI]

    Rodriguez-Roa, Fernando Antonio

    2009-05-15T23:59:59.000Z

    segments. The restored position of the preexisting normal faults places the current trace of the Western Foothills-Slate Belt boundary beneath the Coastal Range. The restoration of WFFTB’s rocks to their depositional locations also supports the tectonic...

  16. EXTENSION CENTER FOR COMMUNITY VITALITY Economic Contribution: Vineyards

    E-Print Network [OSTI]

    Amin, S. Massoud

    EXTENSION CENTER FOR COMMUNITY VITALITY Economic Contribution: Vineyards and Wineries of the North of Applied Economics IN PARTNERSHIP WITH: NORTHERN GRAPES PROJECT USDA, SPECIALTY CROPS RESEARCH INITIATIVE: ECONOMIC CONTRIBUTION i Partners/Sponsors: Northern Grapes Project, which is funded by USDA's Specialty

  17. Cusiana trend exploration, Llanos Foothills thrustbelt, Colombia: The opening of a new hydrocarbon province

    SciTech Connect (OSTI)

    O'Leary, J.; Hayward, T.; Addison, F. (BP Exploration, Bogota (Colombia)); Espinosa, G. (Ecopetrol, Bogota (Colombia))

    1996-01-01T23:59:59.000Z

    The Llanos Foothills petroleum trend of the Eastern Cordillera in Colombia containing the giant Cusiana Field has proven to be one of the most exciting hydrocarbon provinces discovered in recent years. The Llanos Foothills trend is a fold and thrust belt with cumulative discovered reserves to date of nearly 6 billion barrels of oil equivalent. This paper summarizes the critical exploration techniques used in unlocking the potential of this major petroleum system. The first phase of exploration in the Llanos Foothills lasted from the early 1960's to the mid-70's. Several large structures defined by surface geology and seismic data were drilled. Although no major discoveries were made, evidence of a petroleum play was found. The seismic imaging and drilling technology combined with the geological understanding which was then available did not allow the full potential of the trend to be realized. In the late 1980's better data and a revised geological perception of the trend led BP, Triton and Total into active exploration, which resulted in the discovery of the Cusiana Field. The subsequent discovery of the Cupiagua, Volcanera, Florena and Pauto Sur Fields confirmed the trend as a major hydrocarbon province. The exploration programme has used a series of geological and geophysical practices and techniques which have allowed the successful exploitation of the trend. The critical success factor has been the correct application of technology in seismic acquisition and recessing and drilling techniques.

  18. Horticultural & Forest crops 2014 Grapes: Weed Control in Vineyards 3-19

    E-Print Network [OSTI]

    Liskiewicz, Maciej

    Horticultural & Forest crops 2014 Grapes: Weed Control in Vineyards 3-19 Weed Control in Vineyards and postemergence herbicides can be made to control existing vegetation and control weeds germinating from seed oz) Vines must be established at least 5 years. Do not use in soils high in sand or gravel. Apply

  19. Vineyard Energy Project Smart Grid Project | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualProperty Edit withTianlin BaxinUmweltVillage ofInformationVineyard Energy Project Country

  20. Euclid Announcements

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) Environmental Assessments (EA) /

  1. Euclid Programming

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) Environmental Assessments (EA) /Email Announcements Archive EmailKnown Problems

  2. Euclid Timeline

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) Environmental Assessments (EA) /Email Announcements Archive EmailKnownTimeline

  3. An Integrated Assessment of the Influences of Upland Thermal-Erosional Features on Landscape Structure and Function in the Foothills of the Brooks Range, Alaska

    E-Print Network [OSTI]

    Crosby, Benjamin T.

    The Rubenstein School of Environment and Natural Resources, University of Vermont, USA B.T. Crosby, K. Krieger in foothill and mountain terrain are less well known than similar dynamics on coastal plains and peat plateaus

  4. Foothills Parkway Section 8B Final Environmental Report, Volume 6, Appendix N

    SciTech Connect (OSTI)

    Blasing, T.J.; Cada, G.F.; Carer, M.; Chin, S.M.; Dickerman, J.A.; Etnier, D.A.; Gibson, R.; Harvey, M.; Hatcher, B.; Lietzske, D.; Mann, L.K.; Mulholland, P.J.; Petrich, C.H.; Pounds, L.; Ranney, J.; Reed, R.M.; Ryan, P.F.; Schweitzer, M.; Smith, D.; Thomason, P.; Wade, M.C.

    1999-07-01T23:59:59.000Z

    In 1994, Oak Ridge National Laboratory (ORNL) was tasked by the National Park Service (NPS) to prepare an Environmental Report (ER) for Section 8B of the Foothills Parkway in the Great Smoky Mountains National Park (GSMNP). Section 8B represents 27.7 km (14.2 miles) of a total of 115 km (72 miles) of the planned Foothills Parkway and would connect the Cosby community on the east to the incorporated town of Pittman Center to the west. The major deliverables for the project are listed. From August 1995 through October 1996, NPS, GSMNP, and ORNL staff interacted with Federal Highway Administration staff to develop a conceptual design plan for Section 8B with the intent of protecting critical resources identified during the ER process to the extent possible. In addition, ORNL arranged for bioengineering experts to discuss techniques that might be employed on Section 8B with NPS, GSMNP, and ORNL staff during September 1996. For the purposes of this ER, there are two basic alternatives under consideration: (1) a build alternative and (2) a no-build alternative. Within the build alternative are a number of options including constructing Section 8B with no interchanges, constructing Section 8B with an interchange at SR 416 or U.S. 321, constructing Section 8B with a spur road on Webb Mountain, and considering operation of Section 8B both before and after the operation of Section 8C. The no-build alternative is considered the no-action alternative and is not to construct Section 8B. This volume of the ER documents the results of the architectural, historical, and cultural resources assessment for the entire Section 8B ROW that was completed in May 1995 to document the architectural, historical, and cultural resources located within the project area. The assessment included evaluation of the potential for cultural (i.e., rural historic) landscapes in the area of the ROW. The assessment showed that one National Register-listed property is located 0.3 mile south of the ROW, and seven properties appear to meet National Register criteria. For six of these seven sites, no audible or visual effects were predicted to result from the construction and operation of the build alternatives of Section 8B. Three areas were evaluated to determine if they could be considered rural historic landscapes: the Cosby Valley, Pittman Center, and Rocky Flats. None of these landscapes met National Register criteria for rural historic landscapes.

  5. Foothills Parkway Section 8B Final Environmental Report, Volume 4, Appendices E-I

    SciTech Connect (OSTI)

    Blasing, T.J.; Cada, G.F.; Carer, M.; Chin, S.M.; Dickerman, J.A.; Etnier, D.A.; Gibson, R.; Harvey, M.; Hatcher, B.; Lietzske, D.; Mann, L.K.; Mulholland, P.J.; Petrich, C.H.; Pounds, L.; Ranney, J.; Reed, R.M.; Ryan, P.F.; Schweitzer, M.; Smith, D.; Thomason, P.; Wade, M.C.

    1999-07-01T23:59:59.000Z

    In 1994, Oak Ridge National Laboratory (ORNL) was tasked by the National Park Service (NPS) to prepare an Environmental Report (ER) for Section 8B of the Foothills Parkway in the Great Smoky Mountains National Park (GSMNP). Section 8B represents 27.7 km (14.2 miles) of a total of 115 km (72 miles) of the planned Foothills Parkway and would connect the Cosby community on the east to the incorporated town of Pittman Center to the west. The major deliverables for the project are listed. From August 1995 through October 1996, NPS, GSMNP, and ORNL staff interacted with Federal Highway Administration staff to develop a conceptual design plan for Section 8B with the intent of protecting critical, resources identified during the ER process to the extent possible. In addition, ORNL arranged for bioengineering experts to discuss techniques that might be employed on Section 8B with NPS, GSMNP, and ORNL staff during September 1996. For the purposes of this ER, there are two basic alternatives under consideration: (1) a build alternative and (2) a no-build alternative. Within the build alternative are a number of options including constructing Section 8B with no interchanges, constructing Section 8B with an interchange at SR 416 or U.S. 321, constructing Section 8B with a spur road on Webb Mountain, and considering operation of Section 8B both before and after the operation of Section 8C. The no-build alternative is considered the no-action alternative and is not to construct Section 8B. This volume of the ER consists of Appendices E through I (all ecological survey reports), which are summarized individually in the sections that follow. The following conclusions result from the completion of these surveys and the ER impact analysis: (1) Forest clearing should be limited as much as possible; (2) Disturbed areas should be replanted with native trees; (3) Drainages should be bridged rather than leveled with cut and fill; (4) For areas of steep slopes and potential erosion, bioengineering techniques should be implemented; (5) The Webb Mt. spur road is not recommended. If the spur road is built no grass shoulders should be used (to minimize forest fragmentation impacts); and (6) Transplanting of protected plants should be done when possible. Construction in wetland areas should be avoided and erosion and sedimentation mitigation measures discussed under water resources and aquatic ecology should be implemented.

  6. Constraining neutrino properties with a Euclid-like galaxy cluster survey

    SciTech Connect (OSTI)

    Cerbolini, M. Costanzi Alunno; Sartoris, B.; Borgani, S. [Universitá di Trieste, Dipartimento di Fisica, via Valerio, 2, 34127 Trieste (Italy); Xia, Jun-Qing [Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Science, P.O.Box 918-3, Beijing 100049, P.R.China (China); Biviano, A.; Viel, M., E-mail: costanzi@oats.inaf.it, E-mail: sartoris@oats.inaf.it, E-mail: xiajq@ihep.ac.cn, E-mail: borgani@oats.inaf.it, E-mail: viel@oats.inaf.it, E-mail: biviano@oats.inaf.it [INAF-Osservatorio Astronomico di Trieste, via Tiepolo 11, 34143 Trieste (Italy)

    2013-06-01T23:59:59.000Z

    We perform a forecast analysis on how well a Euclid-like photometric galaxy cluster survey will constrain the total neutrino mass and effective number of neutrino species. We base our analysis on the Monte Carlo Markov Chains technique by combining information from cluster number counts and cluster power spectrum. We find that combining cluster data with Cosmic Microwave Background (CMB) measurements from Planck improves by more than an order of magnitude the constraint on neutrino masses compared to each probe used independently. For the ?CDM+m{sub ?} model the 2? upper limit on total neutrino mass shifts from ?m{sub ?} < 0.35 eV using cluster data alone to ?m{sub ?} < 0.031 eV when combined with Planck data. When a non-standard scenario with N{sub eff}?3.046 number of neutrino species is considered, we estimate an upper limit of N{sub eff} < 3.14 (95%CL), while the bounds on neutrino mass are relaxed to ?m{sub ?} < 0.040 eV. This accuracy would be sufficient for a 2? detection of neutrino mass even in the minimal normal hierarchy scenario (?m{sub ?} ? 0.05 eV). In addition to the extended ?CDM+m{sub ?}+N{sub eff} model we also consider scenarios with a constant dark energy equation of state and a non-vanishing curvature. When these models are considered the error on ?m{sub ?} is only slightly affected, while there is a larger impact of the order of ? 15% and ? 20% respectively on the 2? error bar of N{sub eff} with respect to the standard case. To assess the effect of an uncertain knowledge of the relation between cluster mass and optical richness, we also treat the ?CDM+m{sub ?}+N{sub eff} case with free nuisance parameters, which parameterize the uncertainties on the cluster mass determination. Adopting the over-conservative assumption of no prior knowledge on the nuisance parameter the loss of information from cluster number counts leads to a large degradation of neutrino constraints. In particular, the upper bounds for ?m{sub ?} are relaxed by a factor larger than two, ?m{sub ?} < 0.083 eV (95%CL), hence compromising the possibility of detecting the total neutrino mass with good significance. We thus confirm the potential that a large optical/near-IR cluster survey, like that to be carried out by Euclid, could have in constraining neutrino properties, and we stress the importance of a robust measurement of masses, e.g. from weak lensing within the Euclid survey, in order to full exploit the cosmological information carried by such survey.

  7. A Feasibility Study of a Wind/Hydrogen System for Martha's Vineyard, Massachusetts

    E-Print Network [OSTI]

    Massachusetts at Amherst, University of

    systems (SAPS). Their work specifically concentrated on non-grid connected systems that included local project have been carried out. These projects both show the technical feasibility of wind/hydrogen systems1 A Feasibility Study of a Wind/Hydrogen System for Martha's Vineyard, Massachusetts American Wind

  8. A new HST/Herschel deep field at the North Ecliptic Pole: preparing the way for JWST, SPICA and Euclid

    E-Print Network [OSTI]

    Serjeant, Stephen; Burgarella, Denis; Clements, Dave; De Zotti, Gianfranco; Goto, Tomo; Hatsukade, Bunyo; Hopwood, Rosalind; Hwang, Narae; Inami, Hanae; Jeong, Woong-Seob; Kim, Seong Jin; Krumpe, Mirko; Lee, Myung Gyoon; Malkan, Matt; Matsuhara, Hideo; Miyaji, Takamitsu; Oyabu, Shinki; Pearson, Chris; Takeuchi, Tsutomu; Vaccari, Mattia; Valtchanov, Ivan; van der Werf, Paul; Wada, Takehiko; White, Glenn

    2012-01-01T23:59:59.000Z

    We propose a co-ordinated multi-observatory survey at the North Ecliptic Pole. This field is the natural extragalactic deep field location for most space observatories (e.g. containing the deepest Planck, WISE and eROSITA data), is in the continuous viewing zones for e.g. Herschel, HST, JWST, and is a natural high-visibility field for the L2 halo orbit of SPICA with deep and wide-field legacy surveys already planned. The field is also a likely deep survey location for the forthcoming Euclid mission. It is already a multi-wavelength legacy field in its own right (e.g. AKARI, LOFAR, SCUBA-2): the outstanding and unparalleled continuous mid-IR photometric coverage in this field and nowhere else enables a wide range of galaxy evolution diagnostics unachievable in any other survey field, by spanning the wavelengths of redshifted PAH and silicate features and the peak energy output of AGN hot dust. We argue from the science needs of Euclid and JWST, and from the comparative multiwavelength depths, that the logical ...

  9. This book is compiled to provide a printer-friendly e-book for you who want to read Euclid's Elements in the original Greek language. The Greek text is borrowed from Perseus Digital Library 1

    E-Print Network [OSTI]

    Beligiannis, Apostolos

    Digital Library 1 and as for the drawings I have reproduced with a geometrical drawing language named on David Joyce's Euclid's Elements Web Page 3 . At the Perseus Digital Library each word is linked. But the digitalized version, and especially the morphological tools serviced on Perseus Digital Library are protected

  10. Process Limits on Euclid

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

    Process Limits Process Limits Limit Hard Soft core file size (blocks) 0 unlimited data seg size (kbytes) unlimited unlimited scheduling priority 0 0 file size (blocks) unlimited...

  11. Compiling Codes on Euclid

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625govInstrumentstdmadapInactiveVisiting theCommercialization and Innovation2010 2010About Us >Effective

  12. Process Limits on Euclid

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)IntegratedSpeedingTechnical News, informationPriority FirmTechxx by ASME 31

  13. Running jobs on Euclid

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Scienceand Requirements RecentlyElectronicResourcesjobs Running jobs Quick Instructions

  14. Getting Started on Euclid

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    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) Environmental AssessmentsGeoffrey(SC) Getting More ElectricityStarted

  15. Euclid Email Announcements Archive

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  16. Euclid File Systems

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  17. Euclid Known Problems

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  18. Euclid Software and Tools

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  19. Euclid Updates and Status

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) Environmental Assessments (EA) /Email Announcements Archive EmailKnownTimelineStatus

  20. Long-Term Results from Evaluation of Advanced New Construction Packages in Test Homes: Martha's Vineyard, Massachusetts

    SciTech Connect (OSTI)

    Stecher, D.; Allison, K.; Prahl, D.

    2012-10-01T23:59:59.000Z

    This report presents a cold climate project that examines the relationships among very energy efficient single-family residential thermal enclosures, room-to-room temperature variations, and simplified space conditioning systems. The project is located in West Tisbury, Massachusetts, on the island of Martha's Vineyard, and allowed for the comparison of room-to-room temperatures in four virtually identical houses that were all built to the same construction standard. The four homes each has a single ductless heat pump unit (DHU) located in the main living space and radiant electric resistance panels in each bedroom with individual thermostatic controls. Results indicate that temperature fluctuations in the living room due to aggressive setup and setback of the DHU may contribute to higher percentages of time where the bedroom temperatures were within +/-2 degrees F of the living room temperatures. Solar gains in the living room, door opening/closure and occupant manipulation of thermostats appear to have had a significant impact on room-to-room temperature differences, as would be expected.

  1. LEES EUCLIDES! I Jan Hogendijk

    E-Print Network [OSTI]

    Hogendijk, Jan P.

    worden vergeleken, maar niet met elkaar worden vermenigvuldigd. In de rest van dit stuk zullen we af en

  2. Euclid Hardware and Software Configuration

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) Environmental Assessments (EA) /Email Announcements Archive Email

  3. Foothills Bio Energies | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdf Jump to:ar-80m.pdfFillmoreGabbs Valley Area(Sasada,

  4. ` Barbara R. Snyder 10900 Euclid Avenue

    E-Print Network [OSTI]

    Rollins, Andrew M.

    and the Nobel Prize-winning creator of the "bubble chamber" ­ a development essential for a series of subsequent ­ and a $10,000 prize. And, finally, Carbon Origins, designers of reusable rockets that carry science

  5. 1607 Matteo Ricci EuclidElements

    E-Print Network [OSTI]

    Siu, M.K.

    ;6 Thomas Jefferson, 1743-1826 (Bedini, 1990) ... Tacitus Thucydides (Jefferson, 1984) 1776 Declaration

  6. Euclid, Ohio: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model,DOEHazelPennsylvania: Energy Resources(RECP) in DevelopingEtowah,

  7. Using the ACML Math Library on Euclid

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of ScienceandMesa del SolStrengthening aTurbulence mayUndergraduateAboutUserHadoopon-package memoryACML

  8. Euclid, NERSC's Sunfire Shared Memory Analytics System

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC) Environmental Assessments (EA) /Email Announcements Archive EmailKnownTimelineStatus

  9. Estudia con estilo www.ShopFoothillsMall.com

    E-Print Network [OSTI]

    Rhoads, James

    esco- lar en Arizona y Sonora, el binomio edu- car-aprender parece tomar una nueva di- námica frente

  10. Foothill Farms, California: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualPropertyd8c-a9ae-f8521cbb8489Information HydroFontana, California: Energy ResourcesIV

  11. East Foothills, California: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model,DOE FacilityDimondale,South,Earlsboro,Canton, Ohio:Information

  12. Tustin Foothills, California: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro IndustriesTown of Ladoga, IndianaTurtle Airships Jump to: navigation,TuscarawasTussol Jump

  13. 2009 Update UCSF Planning Group GearyEuclid

    E-Print Network [OSTI]

    Lim, Wendell

    2727 Mariposa Street 19 3360 Geary Boulevard 20 250 Executive Park Boulevard 8 Hunters Point 9 Oyster

  14. PGI version 11.3 available on Euclid

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What's Possible for RenewableSpeedingBiomass and4/26/11: eliza18 emergency3 , 2

  15. South Euclid, Ohio: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro Industries Pvt LtdShawangunk, NewSingaporeSonix Japan

  16. VineyardS i t e S e l e c t i o n Vineyard Site Selection

    E-Print Network [OSTI]

    Liskiewicz, Maciej

    Murray, Loudoun County Cooperative Extension. We thank Scott D. Klopfer, GIS and Remote Sensing Division- enced by their proximity to large bodies of water, which are tremendous heat sinks. Water absorbs heat

  17. Viticulture Instructor / Vineyard Manager Job Description

    E-Print Network [OSTI]

    as one course during the summer - teaching workshops may count as partial credit-hour teaching load. 5 this position includes a teaching load of approximately 8-9 credits per semester and one course during summer management, spray scheduling, crop load management, and coordinate with HCC Winery regarding harvest

  18. Vineyard Energy Project | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-fTri Global EnergyUtility Rate HomeVela

  19. Vineyard, California: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-fTri Global EnergyUtility Rate HomeVelaCalifornia: Energy Resources Jump to:

  20. Vineyard, Utah: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro IndustriesTown of Ladoga,planningFlowmeterUtah: Energy Resources Jump to: navigation, search

  1. BY M. MITCHELL WALDROP n the foothills above Palo Alto, California, physicists have set up

    E-Print Network [OSTI]

    Uppsala Universitet

    . All rights reserved #12;SLAC machine, known as the Linac Coherent LightSource(LCLS since the LCLS began operation in 2009, says

  2. Investigation of Groundwater Flow in Foothill and Mountain regions using Heat Flow measurements

    E-Print Network [OSTI]

    Fogg, Graham E.; Trask, James C

    2009-01-01T23:59:59.000Z

    or shortly after drilling for each well. We performed one orft amsl. However, drilling of the peak well may have short-Gondola well dropped substantially as drilling progressed to

  3. Soil-landscape model helps predict potassium supply in vineyards

    E-Print Network [OSTI]

    O'Geen, Anthony T; Pettygrove, Stuart; Southard, Randal; Minoshima, Hideomi; Verdegaal, Paul S.

    2008-01-01T23:59:59.000Z

    for making and inter- preting soil surveys (2nd ed. ). USDA-K S, V, K Depth inches Color* moist soil Sand Silt Clay Claymineralogy† pH CEC cmol(+)/kg soil‡ Exchangeable K K

  4. The State Energy Program Helps Promote that Bigger IS Better in Euclid, Ohio

    Broader source: Energy.gov [DOE]

    Highlighting how one Ohio-based manufacturer is saving energy and money through the Energy Department's State Energy Program.

  5. Unraveling the Timing of Fluid Migration and Trap Formation in the Brooks Range Foothills: A Key to Discovering Hydrocarbons

    SciTech Connect (OSTI)

    Catherine L. Hanks

    2008-12-31T23:59:59.000Z

    Naturally occurring fractures can play a key role in the evolution and producibility of a hydrocarbon accumulation. Understanding the evolution of fractures in the Brooks Range/Colville basin system of northern Alaska is critical to developing a better working model of the hydrocarbon potential of the region. This study addressed this problem by collecting detailed and regional data on fracture distribution and character, structural geometry, temperature, the timing of deformation along the Brooks Range rangefront and adjacent parts of the Colville basin, and the in situ stress distribution within the Colville basin. This new and existing data then were used to develop a model of how fractures evolved in northern Alaska, both spatially and temporally. The results of the study indicate that fractures formed episodically throughout the evolution of northern Alaska, due to a variety of mechanisms. Four distinct fracture sets were observed. The earliest fractures formed in deep parts of the Colville basin and in the underlying Ellesmerian sequence rocks as these rocks experienced compression associated with the growing Brooks Range fold-and-thrust belt. The orientation of these deep basin fractures was controlled by the maximum in situ horizontal stress in the basin at the time of their formation, which was perpendicular to the active Brooks Range thrust front. This orientation stayed consistently NS-striking for most of the early history of the Brooks Range and Colville basin, but changed to NW-striking with the development of the northeastern Brooks Range during the early Tertiary. Subsequent incorporation of these rocks into the fold-and-thrust belt resulted in overprinting of these deep basin fractures by fractures caused by thrusting and related folding. The youngest fractures developed as rocks were uplifted and exposed. While this general order of fracturing remains consistent across the Brooks Range and adjacent Colville basin, the absolute age at any one location varies. Fracturing started in the southwest deep in the stratigraphic section during the Late Jurassic and Early Cretaceous, moving northeastward and upsection as the Colville basin filled from the west. Active fracturing is occurring today in the northeastern parts of the Colville basin, north of the northeastern Brooks thrust front. Across northern Alaska, the early deep basin fractures were probably synchronous with hydrocarbon generation. Initially, these early fractures would have been good migration pathways, but would have been destroyed where subsequently overridden by the advancing Brooks Range fold-and-thrust belt. However, at these locations younger fracture sets related to folding and thrusting could have enhanced reservoir permeability and/or served as vertical migration pathways to overlying structural traps.

  6. Phantom Canyon Preserve and Laramie Foothills Stewardship Intern Time Period: available between late May through mid August 2013 (dates flexible)

    E-Print Network [OSTI]

    late May through mid August 2013 (dates flexible) CSU Compensation: as available CSU class credit and

  7. Birds of the Laguna Kaucaya Area, a Semi-Humid Valley in the Andean Foothills of Departamento Santa Cruz, Bolivia.

    E-Print Network [OSTI]

    Robb. T. Brumfield, Oswaldo Maillard Z., Robert C. Faucett, Gustavo Sanchez, Vanya G. Rohwer, Juan Carlos Catari, C. Gregory Schmitt, Donna C. Schmitt, Rosa Strem and Ana Maria Mamani ...

  8. EIS-0280: Proposed Clean Power from Integrated Coal/Ore Reduction Project (CPICOR) at Vineyard, Utah

    Broader source: Energy.gov [DOE]

    This EIS assesses the potential environmental and human health impacts of a proposed project under the Clean Coal Technology Program that would integrate the production of molten iron for steelmaking with the production of electricity.

  9. Converting oak woodland or savanna to vineyards may stress groundwater supply in summer

    E-Print Network [OSTI]

    Grismer, Mark E; Asato, Caitlin

    2012-01-01T23:59:59.000Z

    processes as root water extraction (ET c ), infiltration byprocesses as root water extraction (ET c ), infiltration byc ): Root extraction of available soil water used in plant

  10. Vineyard managers and researchers seek sustainable solutions for mealybugs, a changing pest complex

    E-Print Network [OSTI]

    2008-01-01T23:59:59.000Z

    genus Ferrisia Fullaway (Hemiptera: Pseudococcidae) from theto control Planococcus ficus (Hemiptera: Pseudococcidae) inof Planococcus spp. (Hemiptera: Pseudo- coccidae), with

  11. Effects of Weather Variables on Pedestrian Volumes in Alameda County, California

    E-Print Network [OSTI]

    Attaset, Vanvisa; Schneider, Robert J.; Arnold, Lindsay S.; Ragland, David R

    2010-01-01T23:59:59.000Z

    Telegraph Avenue  Weather Station  Oakland Foothills Oakland Foothills  Several weather variables were derivedCombined Pedestrian Count and Weather Condition Database The

  12. Woody biomass plots at Sierra Foothill Range Field Station. RichardB. Standiford o Dean R. Donaldson u Roy M. Sachs 0 Janine K. Hasey

    E-Print Network [OSTI]

    Standiford, Richard B.

    and rapidly increasing energy costs,wood cameto be viewed asa po- tential alternative source of renewable with the effortsof several state and federal agencies, and a cooperative group of interested private and public energy. Firewood and co- generation technology, two already-developed uses of wood for energy

  13. Bravo Araby Navy Base Holtville

    E-Print Network [OSTI]

    Mesquite Loveland Imperial Highline Descanso Calexico Sand Hill Navy Base Holtville Glencliff Foothills

  14. Safe Routes to School Safety and Mobility Analysis

    E-Print Network [OSTI]

    Orenstein, Marla R.; Gutierrez, Nicolas; Rice, Thomas M.; Cooper, Jill F.; Ragland, David R.

    2007-01-01T23:59:59.000Z

    Elementary Diamond View Happy Valley Elementary ParadiseHigh Cornell Elementary Happy Valley Elementary Foothill

  15. The kingdom and its subjects : charisms, language, economy, and the birth of a progressive politics in the vineyard

    E-Print Network [OSTI]

    Bialecki, Jon

    2009-01-01T23:59:59.000Z

    Public Culture 20(3):453-459. Graeber, David 2001 Toward anformalist debate (see Graeber 2001: 9-12). revenue-

  16. Cross-shelf circulation and momentum and heat balances over the inner continental shelf near Martha's Vineyard, Massachusetts

    E-Print Network [OSTI]

    Fewings, Melanie Rinn

    2007-01-01T23:59:59.000Z

    The water circulation and evolution of water temperature over the inner continental shelf are investigated using observations of water velocity, temperature, density, and bottom pressure; surface gravity waves; wind stress; ...

  17. PhD Project: Understanding adaptation to climate in the UK: 1800-2000 Supervisors: Professor Mike Hulme (Environmental Sciences), Dr Paul Warde (History)

    E-Print Network [OSTI]

    Hulme, Mike

    insurance), behavioural (vineyards), engineering (1970s Thames Barrier), economic (1980s cold weather

  18. An intertextual study of Euclides Da Cunha's Os serto?es, R.B. Cunninghame Graham's A Brazilian mystic, and Mario Vargas Llosa's La guerra del fin del mundo 

    E-Print Network [OSTI]

    Erickson, Sandra Sassetti Fernandes

    1990-01-01T23:59:59.000Z

    known) fictions inspired by Q~~m. In" rr I fin I m n de Mario Vargas Llosa: un estudio transtextual, " Marcos Leopoldo Bernucci discussed a variety of texts used by Llosa in the writing of ~Lrr~. In this study Bernucci examined the relationship... American Case Studies, " and Marcos Leopoldo Bernucci, " ' de Mario Vargas Llosa: Un estudio transtextual. " , and is suggested in Llosa's text itself by Gall's phrenology, a major theme of Hegel's P~hn~m~~nlggy. Both in regard to ~~ and La~~rr we...

  19. An intertextual study of Euclides Da Cunha's Os serto?es, R.B. Cunninghame Graham's A Brazilian mystic, and Mario Vargas Llosa's La guerra del fin del mundo

    E-Print Network [OSTI]

    Erickson, Sandra Sassetti Fernandes

    1990-01-01T23:59:59.000Z

    . Newman Dr. Stephen J. Miller. L rr I fin I m n is not just a story about the saga of Canudos, but rather a "tree of stories, " composed of several metatexts telling that story. Structurally it illustrates two Hegelian themes, namely, the dialectics..., represents the achievement of historical consciousness in the Hegelian sense; at another level, ~~rr illustrates the full dialectical structure of its principal metatext, Quad~. DEDICATION To my parents, Lourdinha and Paulo Pires Fernandes, as a token...

  20. 2013 UCSC Second Harvest Holiday Food Drive Raffle Raffle Guidelines

    E-Print Network [OSTI]

    California at Santa Cruz, University of

    One bottle Odonata Winery River Skimmer One Annie Glass glass plate - value $40 Two Zip car - Chancellor One bottle Saintsbury Vineyards Carneros Chardonnay One bottle Saintsbury Vineyards Carneros Pinot

  1. Plant Pathology (Geneva) Seminars FALL 2013 All Seminars--3:30 PM (Coffee @ 3:00)

    E-Print Network [OSTI]

    Lazzaro, Brian

    , fruit composition, and leaching of agrochemicals in a Finger Lakes vineyard December 4 12:20 PM Bruce Mc

  2. Cost & Registration The cost of the tour is $65 per person for

    E-Print Network [OSTI]

    Holsinger, Kent

    for lunch at Priam Vineyards in Colchester- - the discovery of a new Champion tree on the property! While

  3. acid-assisted phosphine catalysis: Topics by E-print Network

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

    Washington University School of Medicine, 660 S. Euclid Avenue, St. Louis, MO 63110 Marshall, Garland R. 37 Catalytic Hydrogenolysis of Biphenylene with Platinum, Palladium,...

  4. SSL Workshop - Walmart

    Energy Savers [EERE]

    *Timeline *Euclid *Opportunities 2 "LEDs have become an integral part of our energy efficiency model for our stores and play a key role in achieving our overall sustainability...

  5. Generation and transport of a low energy intense ion beam

    E-Print Network [OSTI]

    2004-01-01T23:59:59.000Z

    and J. K. Walters Tri Alpha Energy Inc. , Foothill Ranch,supported by UCI and Tri Alpha Energy, Inc. R. N. Sudan and

  6. Transmission Right Of Way

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

    About SNR > Right Of Way Right Of Way Preferred Vegetation List - Redding & Foothills (XLS - 23K) Preferred Vegetation List - Sacramento Valley (XLS - 170K) WESTERN AREA POWER...

  7. CAMPUSDRIVEWEST SANTA TERESA ST

    E-Print Network [OSTI]

    QUARRYRD UNIVERSITY AVE PALO RD OLM STED PANAMAST TEUR DR K RD YALE ARBORETUM RD PAM PASLN W I VINEYARD LN

  8. Assessment of Technologies for Compliance with the Low Carbon Fuel Standard

    E-Print Network [OSTI]

    Yeh, Sonia; Lutsey, Nicholas P.; Parker, Nathan C.

    2009-01-01T23:59:59.000Z

    from municipal solid waste, agricultural residue, herbaceousbiofuels from waste streams, agricultural residue, algae, orLCE-Orchard/vineyard waste LCE-Agricultural residue LCE-

  9. Essays in Environmental Economics

    E-Print Network [OSTI]

    Foreman, Kathleen

    2013-01-01T23:59:59.000Z

    vineyards due to these water shortages (DWR, 2012). Whilecosts of irrigation water shortages. Bibliography [1] Alexto a severe shortage of surface irrigation water. In one of

  10. Environmental and Resource Science 336H -2009 WI Agriculture and Agricultural Alternatives

    E-Print Network [OSTI]

    Fox, Michael

    with deer, buffalo and ratites, paralleled with increases in berry crops, vineyards, hemp, sugar beet, hemp, sugar beet, ginseng - guest lecturer. 11. Alternative meat sources: venison, buffalo, ratites

  11. This Page Left Blank Intentionally Nutrient and Sediment Transport From a

    E-Print Network [OSTI]

    Standiford, Richard B.

    them use best management practices to protect water quality when these conversions are made (Dahlgren quality protection measures at the Cuesta Ridge Vineyard. Water samples were taken during storm events of the vineyard system, with the severity of leakage depending upon specific management practices in a given

  12. ___ L....-------Bo/l. Zool. agr. Bachic.

    E-Print Network [OSTI]

    Rider, David A.

    of Hemiptera, Heteroptera in vineyards of Valtellina (Northern Italy) Abstract - Research on the biodiversity of Hemiptera was carried out in 1997- 1999 in two viticultural areas of Valtellina. The first site the biocenosis of Hemiptera. In the Sassella vineyard with weeds, whose vegetation has become richer during

  13. Alcune difficolt con il caro vecchio Teorema di Prospettive per una ricerca

    E-Print Network [OSTI]

    Spagnolo, Filippo

    razionale. L'ipotesi di Zeuthen ha avuto molta fortuna ed è stata ripresa dagli studiosi anche recentemente2 . La dimostrazione data da Euclide nella I,47 ebbe varia fortuna nella didattica del teorema di

  14. EDITED--LS-332-DWA_FEL_August16

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

    32 August 2012 A Compact Soft X-ray Free-Electron Laser Facility based on a Dielectric Wakefield Accelerator C. Jing, P. Schoessow, A. Kanareykin, Euclid Techlabs LLC, Solon, OH...

  15. Diurnal cycle of air pollution in the Kathmandu Valley, Nepal: Observations

    E-Print Network [OSTI]

    Panday, Arnico K.

    During the dry season of 2004–2005 we carried out field measurements of air pollution and meteorology in the Kathmandu Valley, Nepal, a bowl-shaped urban basin in the Himalayan foothills of Nepal. We measured the trace ...

  16. J. Field Ornithol. 79(4):381390, 2008 DOI: 10.1111/j.1557-9263.2008.00195.x Distribution of California Black Rails

    E-Print Network [OSTI]

    Beissinger, Steven R.

    en la regi´on del valle de Sacramento para determinar la distribuci´on y residencia del Ralido Negro foothills and Sacramento Valley region to determine the distribution and residency of Black Rails, estimate

  17. 531Proc. VIIth IS on Kiwifruit

    E-Print Network [OSTI]

    Crisosto, Carlos H.

    15.1%, but DM varied among vineyards and seasons. DM did not change during cold storage. Thus, DM proposed the use of DM concentration as a quality index. Thus, some industries have started its use

  18. Developing algorithms for healthcare insurers to systematically monitor surgical site infection rates

    E-Print Network [OSTI]

    2007-01-01T23:59:59.000Z

    7. Sands K, Vineyard G, Platt R: Surgical site infectionsNottebart VF, Hameed SR, Platt R: Automated post- dischargeDS, Shapiro M, Simchen E, Platt R: Use of antibiotic expo-

  19. Smaller loads reduce risk of back injuries during wine grape harvest

    E-Print Network [OSTI]

    2006-01-01T23:59:59.000Z

    of manual lifting tasks. Ergonomics 36(7):749-76. Waters T,back disorder risk. Ergonomics Meyers J, Miles J, Faucett J,field work: Vineyard ergonomics. J Agromed 8(1):37-52. [NRC-

  20. 20 University of Kentucky College of Health Sciences 21University of Kentucky College of Health Sciences Connection | College of Health Sciences Connection | College of Health Sciences

    E-Print Network [OSTI]

    Hayes, Jane E.

    Cincinnati Reds Clean Sweep Carwash Comedy Off Broadway Elk Creek Vineyards Embassy Suites Hotel Griffin Gate Marriott Resort and Spa Heaven Hill Distilleries, Inc. Heavenly Ham Homewood Suites by Hilton Lexington

  1. H

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

    views of the area's mountains and vineyards. Wines will be available for purchase by the glass or by the bottle. The price is 40 per person (must be 21 to attend) and non-wine...

  2. Researchers study grapevine microbiota | Argonne National Laboratory

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

    To survey the microbes living in the roots and in the soil near grapevines, Argonne researchers took soil samples in several vineyards over the course of all four seasons. (Photo...

  3. J. Agric. Food Chem. 1994, 42, 301-309 301 Synthesis of Haptens and Derivation of Monoclonal Antibodies for

    E-Print Network [OSTI]

    Hammock, Bruce D.

    , potatoes, cotton, corn, beans, cereals, and ornamentals and in orchards and vineyards. They * Author towhom- water and surface water. In 1990,40of 782wellssampled in California were contaminated with 0.06-3.95 ppb

  4. Introduzione In questo libretto sono illustrati i quesiti di informatica che sono stati

    E-Print Network [OSTI]

    Monga, Mattia

    5 1. Trettrerob`ot 6 2. Sul pianeta Alber 8 3. Euclide 10 4. Analisi grammaticale 12 5. Pseudo 2009 #12;Parte I. Quesiti nel volantino #12;Quesito 1: Trettrerob`ot Trettrerobot e in grado di corrispondere ad ogni porzione di frase un movi- mento di Trettrerobot: ad esempio A3 fa procedere il robot di 3

  5. New Book Information Crossroads in the History

    E-Print Network [OSTI]

    Sriraman, Bharath

    and for mathematics education courses aimed at teachers. CONTENTS: TOPICS IN HISTORY AND DIDACTICS OF CALCULUS infinitesimals and formal mathematical analysis, Mikhail Katz (Israel) & David Tall (UK). The didactical nature AND DIDACTICS OF GEOMETRY AND NUMBER. Euclid's Book on the Regular Solids: Its Place in the Elements and Its

  6. The activities of the Department are sup-ported by a combination of government

    E-Print Network [OSTI]

    projects funds from na- tional, international and EU programmes and fully commercial industrial contracts) Materials Science Materials Engineering Materials Technology Symposium EUCLID, EUREKA BRITE-EURAM, JOULE, EU$ Project funding 35.144.000 4.604.000 Government funding Income 34.988.000 4.583.000 Central Risø

  7. UNCORRECTED 2 Spall strength of a zirconium-based bulk metallic glass under

    E-Print Network [OSTI]

    Rollins, Andrew M.

    of Mechanical and Aerospace Engineering, Case Western Reserve University, 10900 Euclid Avenue, Glennan 616 B. Introduction 40 Bulk amorphous metals, also referred to as bulk metallic 41 glasses (BMG), are alloys in which super-cooling of a liquid 42 alloy produces a metastable phase, thus preventing forma- 43 tion

  8. Updated by Malana Bey 6/2013 Postbaccalaureate Research Education

    E-Print Network [OSTI]

    Yang, Sichun

    1 Updated by Malana Bey 6/2013 Postbaccalaureate Research Education Program (PREP) Scholar Handbook Education Program Office of Graduate Education, Ground floor TG-1 CWRU School of Medicine, 10900 Euclid://gradresed.meds.cwru.edu/PREP/index.html #12;2 Updated by Malana Bey 6/2013 Topic Table of Contents Page # Checklist ­ what to do when you

  9. 2001 The Society for the Study of Evolution. All rights reserved. Evolution, 55(12), 2001, pp. 25762600

    E-Print Network [OSTI]

    Cheverud, James M.

    structure relatively stable during evolutionary diversification of South American monkeys. Key words, 660 South Euclid Avenue, Campus Box 8108, Saint Louis, Missouri, 63110 5E-mail: cheverud habits. Finally, common patterns and levels of morphological integration are found among Plat- yrrhine

  10. SPARC Japan>> 20(2008)93()

    E-Print Network [OSTI]

    Hattori, Tetsuya

    2008-01-01T23:59:59.000Z

    1 SPARC Japan>> 20(2008)93() National Institute of Informatics 20(2008)93() RIMS 4 SPARC Japan 2008 SPARC JapanSPARC Japan UniBio Press J-STAGE Project Euclid SPARC Japan 3 (2000) ( 144 63 74 5 2 3 676 1 396 2 105 206 55 ISIJCRNCR 3,676 1,396 2,105 206

  11. MATERIALS RESEARCH DEPARTMENT 2000 A n n u a l R e p o r t 2 0 0 0

    E-Print Network [OSTI]

    MATERIALS RESEARCH DEPARTMENT 2000 35 A n n u a l R e p o r t 2 0 0 0 Finances Finances), 13% BRITE-EURAM, JOULE, EU-Fusion, 23% EUCLID,EUREKA, 5% Research areas (hours) Materials Science, 37% Materials Technology, 41% Materials engineering, 22% 36 501 000 DKK 4 551 000 USS 36 598 000 DKK 4 563 000

  12. Experimental and Molecular Pathology 71, 4054 (2001) doi:10.1006/exmp.2001.2380, available online at http://www.idealibrary.com on

    E-Print Network [OSTI]

    Burnstock, Geoffrey

    2001-01-01T23:59:59.000Z

    Experimental and Molecular Pathology 71, 40­54 (2001) doi:10.1006/exmp.2001.2380, available online, School of Medicine, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, Ohio 44106 in humans and other animals (Verbeuren et al., 1986, macrophages and smooth muscle showed a different

  13. Reprint from the Bulletin of the Belgian Mathematical Society Simon Stevin Lagrangian submanifolds in 3-dimensional

    E-Print Network [OSTI]

    Li, Haizhong

    of Project Euclid (Cornell University Library), an aggregation of electronic journals. It is available online classification of the Lagrangian submanifolds in 3-dimensional complex space forms with isotropic cubic tensor. 1 Mathematics Subject Classification : Primary 53C20; Secondary 53C42. Key words and phrases : Lagrangian

  14. This article appeared in a journal published by Elsevier. The attached copy is furnished to the author for internal non-commercial research

    E-Print Network [OSTI]

    Simon, Dan

    maintenance schedules. Reliable health eval- uations are used to anticipate future maintenance needs.elsevier.com/locate/aescte A comparison of filtering approaches for aircraft engine health estimation Dan Simon Cleveland State University, Department of Electrical Engineering, Stilwell Hall Room 332, 2121 Euclid Avenue, Cleveland, OH 44115, USA

  15. ADAPTIVE FILTERING FOR DETECTING MYOCARDIAL INFARCTION USING NONINVASIVE CONDUCTING POLYMER COMPOSITE SENSORS

    E-Print Network [OSTI]

    Simon, Dan

    , is the leading cause of death among firefighters in the United States [1]. The need to carry heavy equipment long) (1) (3) (1) (1) Cleveland State University, 2121 Euclid Ave, Cleveland, Ohio 44115 (2) Arcon software produces a diagnostic-friendly ECG signal and then determines the patient's heart rate. When

  16. In The News Wednesday, April 06, 2011

    E-Print Network [OSTI]

    Arizona, University of

    In The News Wednesday, April 06, 2011 Tonight on campus: Free CPR training 04/06/2011 Arizona Daily Star (blog) View Clip Couture for Cancer in Tucson 04/06/2011 Arizona Foothills Magazine View Clip Poison Control's Bitter Budget Pill 04/05/2011 Arizona Public Media View Clip Gabrielle Giffords' surgeon

  17. Assistant, Associate or Full Professor with Research Emphasis in Neuroendocrinology Department of Biomedical Sciences

    E-Print Network [OSTI]

    Birner, Thomas

    research areas in the department and within these PRSEs include stress, reproduction, energy balance of ~150,000 people located in the foothills of the Rocky Mountains. The city offers outstanding outdoor recreational opportunities and excellent quality of life. Additional information on the city of Fort Collins

  18. CSMRI Bagged Soil Disposal Summary Report

    E-Print Network [OSTI]

    Radiological Instrumentation Calibration Records Appendix D Truck Manifests, Weigh Tickets, and Incoming/Outgoing Radiological Surveys Appendix E Truck Departure Record Forms Appendix F Final Radiological Surveys of Trucks (Stoller 2005b). The soil was loaded into trucks and shipped to BFI Foothills facility under the Stoller

  19. Lifestyle and Mercury Contamination of Amerindian Populations along the Beni River

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    1 Lifestyle and Mercury Contamination of Amerindian Populations along the Beni River (Lowland (Corresponding author), M.D., Ph.D. Abstract The objective of this paper was to document mercury contamination at the foothills of the Andes. Hair mercury content (H-Hg) served as a bioindicator of mercury contamination

  20. NIRS/NUTBAL nutritional profiling system for grazingland animal management

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    . The NUTBAL-Nutritional Balance Analyser was designed to link the NIRS technology with site specific conditions of an individual herd to allow determination of crude protein, net energy of maintenance pastures, subtropical rangeland and marshes, temperate native prairie and woodlands, foothill woodlands

  1. Structure and evolution of the active fold and thrust belt of southwestern Taiwan using GPS geodesy

    E-Print Network [OSTI]

    Hickman, John Bibb

    1999-01-01T23:59:59.000Z

    ) from north to south, a dramatic change in the width of the deformation front of the fold and thrust belt which is accentuated across the Michih fault, and 4) the Tulungwan fault, a bounding fault between the Western Foothills and the Slate Belt, appears...

  2. ROCKY MOUNTAIN CLIFF, CANYON AND MASSIVE BEDROCK extent exaggerated for display

    E-Print Network [OSTI]

    Vegetation Overview: This ecological system is found from foothill to subalpine elevations and includes hydraulic pressure retaining water within the rock, so liquid water is more consistently found than roads. Human disturbance to this system may include road construction and maintenance, recreation

  3. IIDA Hidefusa Sungbin Ha The Graduate School of Law (GSL) and the

    E-Print Network [OSTI]

    Banbara, Mutsunori

    of Commerce (Kobe University of Economics). Sparing no effort in its quest to become a leading institution a reputable academic center that is highly ranked in Japan. Located on the foothills of the lush green Rokko provide a five-year graduate program consisting of a two-year program leading to a Master's degree

  4. Monte Vista Springfield

    E-Print Network [OSTI]

    ,000 solar panels. Research Innovation Center (RIC) · Hot-water preheating system at the boiler that allows Hall O.T. Annex Gibbons Bldg. Heating Plant Chiller BuildingAdmin. Annex Student Vocational Education tour.They are located on CSU's Foothills Campus. Solar Plant · A public-private partnership among CSU

  5. Borehole stability analysis at the Coporo-1 well, Colombia

    E-Print Network [OSTI]

    Arias, Henry

    2000-01-01T23:59:59.000Z

    Coporo-1 is an 18,000-ft dry hole located in the tectonically active foothills of the Eastern Cordillera of Colombia. A mechanical stability analysis allowed explaining most of the drilling stability-related problems and elaborating an optimal mud...

  6. Andean deformation and rift inversion, eastern edge of Cordillera Oriental (GuatequeMedina area), Colombia

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    ), Colombia Y. Branquet, a , A. Cheilletzb , P. R. Cobboldc , P. Babyd , B. Laumoniere and G. Giulianif; Colombia; Cordillera Oriental; Guateque­Medina area hal-00076871,version1-16Nov2006 Author manuscript Oriental (CO) and adjacent Llanos foothills, which produce much of the oil in Colombia. The CO resulted

  7. Seismic reprocessing, interpretation and petroleum prospectivity of the East Cano Rondon Area, Llanos Basin, Colombia

    E-Print Network [OSTI]

    Molina, German D

    1999-01-01T23:59:59.000Z

    The Llanos Basin, in Eastern Colombia, is the major oil-producing province in the country. In recent years, exploration in this basin has been focused towards plays in the Llanos foothills, where proven thrust traps present the possibility of large...

  8. Rainfall-Runoff Modelling of Meso-Scale Catchments in the Upper Ewaso

    E-Print Network [OSTI]

    Richner, Heinz

    , but growing demand for irrigation water on its foothills produces water shortage in the lowlands. Water founded River Water Users Associations, but their work is hindered by a lack of knowledge on the present and future availability of water resources. This study tries to make a contribution to better water

  9. New Horizons Environmental Consultants, Inc. November 12, 2003

    E-Print Network [OSTI]

    as demolition debris for disposal at BFI's Foothills Landfill (BFI) near Golden (a solid waste facility/Solidification · Off-Site Disposal at a Solid Waste Landfill · Off-Site Disposal at a Solid Waste and/or Special Waste/Institutional Controls · On-Site In Place Closure · On-Site Below Ground Repository with Waste Stabilization

  10. Non-Campus Property7 2010 2011 2012 2010 2011 2012 2010 2011 2012 2010 2011 2012

    E-Print Network [OSTI]

    Sze, Lawrence

    action and/or in which arrest(s) occurred and/or criminal prosecution was sought. These referrals reflect Disciplinary Action - Disciplinary referrals (non-arrests) from UPD, Housing and other University Officials of the intersection with Monte Vista Crandall Avenue: north of the intersection with Foothill Boulevard Private Road

  11. Blood lead concentrations in a remote Himalayan population

    SciTech Connect (OSTI)

    Piomelli, S.; Corash, L.; Corash, M.B.; Seaman, C.; Mushak, P.; Glover, B.; Padgett, R.

    1980-12-05T23:59:59.000Z

    The lead content in the air at the foothills of the Himalayas in Nepal was found to be negligible. The concentration of lead in the blood of 103 children and adults living in this region was found to average 3.4 micrograms per deciliter, a level substantially lower than that found in industrialized populations.

  12. Optimizing Warehouse Forklift Dispatching Using a Sensor Network and Stochastic Learning

    E-Print Network [OSTI]

    Paschalidis, Ioannis "Yannis"

    , detecting biological, chemical, and nuclear attacks [6, 7]. More examples of security applications come from]. Agriculture may also benefit from sensor networks. For example, [18] studied the potential use of sensor network in vineyard management; see also [19] on precision agriculture. Sensor networks have also been

  13. Marine Biological Laboratory Semester in Environmental Science 2011

    E-Print Network [OSTI]

    Vallino, Joseph J.

    bacteria can use sulfur compounds in energy-yielding reactions, called dissimilatory sulfur metabolism neighborhood of Falmouth, MA. The pond has a history of slight eutrophication (Moore 2009, Unpublished Report intrusion through a small channel that connects the pond to Martha's Vineyard Sound during large storms

  14. MVYLI Team Explores Sustainable Development Best Practices Cerina Gordon has big dreams for her life and for her island. A senior at MVRHS, she aspires to become an

    E-Print Network [OSTI]

    Schweik, Charles M.

    with Professor John Gerber, a Sustainable Agriculture leader and a frequent Vineyard sailor. He leads the Living of sustainable living in eco-villages around the world. During their College Field Trip, MVYLI youth stayedMVYLI Team Explores Sustainable Development Best Practices Cerina Gordon has big dreams for her

  15. Alson H. Smith Jr. Agricultural Research and Extension Center Physical Resources

    E-Print Network [OSTI]

    Liskiewicz, Maciej

    and soil management in orchards, hard cider production, high density orchard systems, sweet cherry cultivar Sustainable vineyard management practices to improve wine grape quality. Current focus on managementAlson H. Smith Jr. Agricultural Research and Extension Center Physical Resources Land

  16. QWhat are viable strategies for Iowa grape growers to successfully manage weeds and/or reduce pesticide usage while maintaining

    E-Print Network [OSTI]

    Debinski, Diane M.

    . Sustainable weed management that includes living or soil mulches minimizes some of the environmental risks for achieving weed management in Iowa vineyards will enable growers to sustainably manage this unique and encourage the use of sustainable land management practices that are environmentally sound, economically

  17. dddddddddddddddddddddddddddddddddddddd United States

    E-Print Network [OSTI]

    Hubbard, Susan

    , and is on the verge of a major water shortage. As vineyards consume more rural acre- age, competition for water irrigation. However, California uses the largest volume of water of any state in the nation resources is increasing, which has increased the pres- sure on California vintners to use water more

  18. Real Time Emulations: Foundation and Applications Azalia Mirhoseini

    E-Print Network [OSTI]

    vineyards, there are often several rose bushes planted throughout. The reason is not the romantic nature on the first page. To copy otherwise, to republish, to post on servers or to redistribute to lists, requires prior specific permission and/or a fee. DAC'10, June 13­18, 2010, Anaheim, California, USA. Copyright

  19. May 2011 Regional Fruit Grower Newsletter CALENDAR OF EVENTS

    E-Print Network [OSTI]

    @msu.edu, 517-355-5191, x 1302 6/3 Parallel 45 "First Friday" Meeting Crane Hill Vineyards, Leelanau Co. Shoot of Elk Rapids on the southeast side of M-31 Dates: May 10, May 24, June 7, June 21 Time: 10-12 pm TRELLIS

  20. Northern Michigan FruitNet 2014 Northwest Michigan Horticultural Research Center

    E-Print Network [OSTI]

    Northern Michigan FruitNet 2014 Northwest Michigan Horticultural Research Center Weekly Update, Grand Rapids 2015 1/13-14 NW Michigan Orchard & Vineyard Show Grand Traverse Resort, Acme, MI 2 ­ Kellogg Hotel & Conference Center 3/4-6 Michigan Grape & Wine Conference MSU ­ Kellogg Hotel & Conference

  1. Cornell University, Office of Sponsored Programs

    E-Print Network [OSTI]

    ,400.00 ALEXANDER, JAMES P Cornell Lab Accelerator Sciences & Ed NSF MPS PARTICLE PHYSICS AT THE ENERGY FRONTIER AND INNOVATION IN ETHIOPIA 62088 $ 20,000.00 BATES, TERENCE R CALS Horticulture NY WINE/GRAPE A SYSTEM APPROACH R CALS Horticulture NY WINE/GRAPE SPATIAL VINEYARD MANAGEMENT FOR PRODUCTION EFFICIENCY

  2. ANDREW J. PLANTINGA Department of Agricultural and Resource Economics

    E-Print Network [OSTI]

    Tullos, Desiree

    -1993). Research Assistant, Resources for the Future, Energy and Natural Resources Division, Washington, DC (1990.N. Stavins. 2011. The Value of Terroir: Hedonic Estimation of Vineyard Sale Prices. Journal of Wine Economics of Voluntary Incentive Policies for Preventing Biodiversity Loss. Resource and Energy Economics 33

  3. In addition to the intensive focus on operational energy reduction, the client and

    E-Print Network [OSTI]

    In addition to the intensive focus on operational energy reduction, the client and design team carbon emissions of the building materials as well as the produced carbon emissions resulting from energy decommissioned Sebastiani vineyard wine vats. Due to the tight- grained quality of this old-growth wood no sealer

  4. www.agbioresearch.anr.msu.edu Northern Michigan FruitNet 2013

    E-Print Network [OSTI]

    : $15 CMI Luncheon, January 22: Free to cherry growers; pre-register with CMI Sponsors: Grand Traverse:35 First Year Report on Bird Damage Studies in Tree Fruit Dr. Catherine Lindell, Michigan State University:35 First Year Report on Bird Damage Studies in Vineyards Dr. Catherine Lindell, Michigan State University

  5. Probing Neutrino Hierarchy and Chirality via Wakes

    E-Print Network [OSTI]

    Hong-Ming Zhu; Ue-Li Pen; Xuelei Chen; Derek Inman

    2014-12-04T23:59:59.000Z

    The relic neutrinos are expected to acquire a bulk relative velocity with respect to the dark matter at low redshifts, and downstream of dark matter halos neutrino wakes are expected to develop. We propose a method of measuring the neutrino mass based on this mechanism. The neutrino wake will cause a dipole distortion of the galaxy-galaxy lensing pattern. This effect could be detected by combining upcoming lensing surveys, e.g. the LSST and Euclid surveys with a low redshift galaxy survey or a 21cm intensity mapping survey which can map the neutrino flow field. The data obtained with LSST and Euclid should enable us to make positive detection if the three neutrino masses are Quasi-Degenerate, and a future high precision 21cm lensing survey would allow the normal hierarchy and inverted hierarchy cases to be distinguished, and even the right handed Dirac neutrinos may be detectable.

  6. Aquifer behavior with reinjection 

    E-Print Network [OSTI]

    Bonet, Euclides Jose

    1967-01-01T23:59:59.000Z

    AQUIFER BEHAVIOR WITH REINJECTION A Thesis By EUCLIDES JOSE BONET Submitted to the Graduate College of the Texas ARUM University in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE May, f967 Major Subject... Petroleum Engineering AQUIFER BEHAVIOR WITH REINJECTION A Thesis By E UC LI DES JOSE BONE T Approved as to style and content by: (Chairman of Committee) (Member) (Member) May, 1967 ACKNOWLEDGMENT Thanks are due to Petroleo Brasilerio S...

  7. An analysis of the market news and related information available to Arizona cattle producers

    E-Print Network [OSTI]

    Stubblefield, Thomas Mason

    1956-01-01T23:59:59.000Z

    Agricultural Experiment Station, Tucson, 1951* 8 RANCHING AREAS AREAS 1.- MOHAVE STRIP 2.- NAVAJO RESERVATION 3r SOUTHWESTERN DESERT 4.- SOUTHEASTERN AREA 5.? CENTRAL MOUNTAINS AND FOOTHILL AREA adjacent to the irrigated valleys in Maricopa, Pinal... (Maricopa County). The other two important areas are Tucson (Pina County) and Safford (Graham County). Table 6 presents the average per cent of total monthly slaughter for each of these areas, as well as that slaughtered in other counties of the state...

  8. Bedrock structure, lithology and ground water: influences on slope failure initiation in Davis County, Utah

    E-Print Network [OSTI]

    Ala, Souren Nariman

    1990-01-01T23:59:59.000Z

    , for his input. The Salt Lake City office of Dames and Moore generously provided for me to print the results of my Viii geophysical surveys. Mr. Roger Fallon of Salt Lake City did us a great service by flying us around the Wasatch Front canyons; much... Complex between Farmington and Stone Creeks. . . . . . . . . . . . pocket INTRODUCTION Rapid population growth in the urban area along the eastern border of the Great Salt Lake, Utah, has led to residential development in the western foothills...

  9. Panos D. Prevedouros, PhD, Asc. Professor of Transportation Engineering, Department of Civil and Environmental Engineering, UH-Manoa pdp@hawaii.edu January 2004 This is a comprehensive but not an exhaustive list of suggestions for easing traffic congest

    E-Print Network [OSTI]

    Prevedouros, Panos D.

    , these funds can be used to improve the City's extensive traffic signal system, the Traffic Control Center the Liliha St. on ramp and the Pali Hwy. off-ramp. o Control the inflow of the Vineyard Blvd. and Ward Ave for buses and HOV!HOT). o If the above viaduct can't be done, then re-design the Sand Island Access Road

  10. Evolution de la flore adventice du vignoble de Cte-d'Or sous la pression des techniques d'entretien des cultures

    E-Print Network [OSTI]

    Boyer, Edmond

    techniques d'entretien. En l'absence de désherbage chimique, comme c'était le cas en 1969, la flore adventice communautés. SUMMARY Changes in the weed flora of COte-d'Or vineyards in relation to weed control methods Strasbourg Cedex. (**) Adresse actuclle : Service de la Protection des Végétaux, « La Fenêtre Nord », Route

  11. A Life in Letters: Personal Essays

    E-Print Network [OSTI]

    Fangman, Ellen Mary

    2008-12-16T23:59:59.000Z

    on the battlefield, while I waged a different kind of warfare as I struggled with growing into a woman’s body. This essay is a sort of loving “slap in the face” at the men who knew nothing of what it meant to carry a tampon and bleed over miles of mountainous... these oft- feeble, oft-boisterous people we call our “selves.” In humorous tones, I write to Edna St. Vincent Millay, asking her to intercede for me with her favorite geometrician, Euclid, that I might be relieved of a recurring nightmare that involves...

  12. Beyond the plane-parallel and Newtonian approach: wide-angle redshift distortions and convergence in general relativity

    SciTech Connect (OSTI)

    Bertacca, Daniele; Maartens, Roy [Physics Department, University of the Western Cape, Cape Town 7535 (South Africa); Raccanelli, Alvise [Jet Propulsion Laboratory, California Institute of Technology, Pasadena CA 91109 (United States); Clarkson, Chris, E-mail: daniele.bertacca@pd.infn.it, E-mail: Roy.Maartens@port.ac.uk, E-mail: Alvise@caltech.edu, E-mail: Clarkson@maths.uct.ac.za [Centre for Astrophysics, Cosmology and Gravitation and Department of Mathematics and Applied Mathematics, University of Cape Town, Cape Town 7701 (South Africa)

    2012-10-01T23:59:59.000Z

    We extend previous analyses of wide-angle correlations in the galaxy power spectrum in redshift space to include all general relativistic effects. These general relativistic corrections to the standard approach become important on large scales and at high redshifts, and they lead to new terms in the wide-angle correlations. We show that in principle the new terms can produce corrections of nearly 10% on Gpc scales over the usual Newtonian approximation. General relativistic corrections will be important for future large-volume surveys such as SKA and Euclid, although the problem of cosmic variance will present a challenge in observing this.

  13. Skills as tribute: Phoenician sailors and shipwrights in the service of Neo-Assyria

    E-Print Network [OSTI]

    Trakadas, Athena Lynn

    1999-01-01T23:59:59.000Z

    ' skills as shipwrights and seafarers played in this socio-economic association with Assyria can be better reconstructed. . . . even the weariest river winds somewhere safe to sea. -Odysseus Elytis s ksv0s p io TABLE OF CONTENTS ABSTRACT. Page... farming, and to the east by the foothills of the Zagros Mountains (fig. 5)ae To the north of Assyria lay the fertile Habur region, once part of the Middle Assyrian kingdom, but separated by no natural geographical barriers. The topography of the region...

  14. Geographic variation and distribution of the genus Tomodactylus in Mexico

    E-Print Network [OSTI]

    Dixon, James Ray

    1957-01-01T23:59:59.000Z

    of the town on the accoapanying aap (Nap 9)~ (4) a statenent of the vegetation type that oocurs there. 8 INALOA Concordia. 108 04';33 17') 88 ft. ; Location 1, Troy- 0 ical Deciduous Forest. A saall village in the foothills of the 8 ierra Madre Oocidental..., NAYARIT ~Ah ~1. 104 SOB~31 03'; 3, 300 ft. ) Looation 5 ~ Scrub oah in the Pine-oak Forest, EJ QgJIIBL11II 104 38 ) 81 10 / 3 B 300 f t d ( Location 4 ~ Tropical Deciduous Forest. A snail village in a I, JO 'gCO O+~q 10 IIFO OF rZ~ag deep valley...

  15. An internship on the Beaverhead Ranch in Southwest Montana 

    E-Print Network [OSTI]

    Donnelly, George Arthur

    1997-01-01T23:59:59.000Z

    insight, his thorough inspections, and his evaluations to current and future situations in the ranching industry. Ranches and Feedyards The Spring Creek Ranch was the first ranch purchased. It operates today on 10, 000 acres in the Flint Hills... temperatures can be found. 12 Herds of elk can be seen grazing among the cattle in the foothills and benches, to the highest elevations. Some of the herds are 2, 000 to 3, 000 in number and therefor play an itnportant role in calculating stocking rates...

  16. Newsfront 31 December 2007 - 6 January 2008, Issue 47

    E-Print Network [OSTI]

    Ghimire, Yubaraj

    countability to parliament-- a role that Prachanda hopes to snatch any time now. Enviro6 31 Dec, 2007- 6 Jan, 20081 D 7 6 81 D 7 6 81 D 7 6 81 D 7 6 8 Lessons from Himalayan degradation The Hindu-Kush Himalaya (HKH) continues to inspire religious devotion... in increasingly congested, polluted and crime-infested hill and foot-hill towns. Their inhabitants may score higher than national averages on income and educational indicators, but they depend on very poor services from for example water authorities and police...

  17. Footville, Wisconsin: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdf Jump to:ar-80m.pdfFillmoreGabbs Valley Area(Sasada,Foothills Energy

  18. Foraker, Oklahoma: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdf Jump to:ar-80m.pdfFillmoreGabbs Valley Area(Sasada,Foothills EnergyForaker,

  19. Forbes Energy LLC | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdf Jump to:ar-80m.pdfFillmoreGabbs Valley Area(Sasada,Foothills

  20. Ford County, Illinois: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdf Jump to:ar-80m.pdfFillmoreGabbs Valley Area(Sasada,FoothillsFord County,

  1. Ford County, Kansas: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdf Jump to:ar-80m.pdfFillmoreGabbs Valley Area(Sasada,FoothillsFord

  2. Ford Heights, Illinois: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdf Jump to:ar-80m.pdfFillmoreGabbs Valley Area(Sasada,FoothillsFordFord Heights,

  3. Fords, New Jersey: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdf Jump to:ar-80m.pdfFillmoreGabbs Valley Area(Sasada,FoothillsFordFord

  4. Future cosmological sensitivity for hot dark matter axions

    E-Print Network [OSTI]

    Archidiacono, Maria; Hamann, Jan; Hannestad, Steen; Raffelt, Georg; Wong, Yvonne Y Y

    2015-01-01T23:59:59.000Z

    We study the potential of a future, large-volume photometric survey to constrain the axion mass $m_a$ in the hot dark matter limit. Future surveys such as Euclid will have significantly more constraining power than current observations for hot dark matter. Nonetheless, the lowest accessible axion masses are limited by the fact that axions lighter than $\\sim 0.15$ eV decouple before the QCD epoch, assumed here to occur at a temperature $T_{\\rm QCD} \\sim 170$ MeV; this leaves an axion population of such low density that its late-time cosmological impact is negligible. For larger axion masses, $m_a \\gtrsim 0.15$ eV, where axions remain in equilibrium until after the QCD phase transition, we find that a Euclid-like survey combined with Planck CMB data can detect $m_a$ at very high significance. Our conclusions are robust against assumptions about prior knowledge of the neutrino mass. Given that the proposed IAXO solar axion search is sensitive to $m_a\\lesssim 0.2$ eV, the axion mass range probed by cosmology is n...

  5. Bottling as a marketing strategy for the Aragon wine industry

    E-Print Network [OSTI]

    Dominguez, Jose Antonio

    1990-01-01T23:59:59.000Z

    is that the distribution of Aragon wine sales is inconsistent with the varietal distribution of Aragon wine production as reported by the Ministry of Agriculture of Spain. This thesis suggests the necessity for a change in the official view of the real structure... Equipment 17 18 22 CHAPTER II. C. Sales of Aragon Wine Industry II. C, 1. Sales According to Wine Type. II. C. 2. Wine Sales According to the Kind of Container II. C. 3. Wine Sales According to Legal Status of Vineyards II. D. Supply Concentration...

  6. Investigation and Improvement of American Grapes at the Munson Experiment Grounds near Denison, Texas, from 1876 to 1900.

    E-Print Network [OSTI]

    Munson, T. V. (Thomas Volney)

    1899-01-01T23:59:59.000Z

    TEXAS AGRICULTURAL EXPERIMENT STATIONS. I'OSTOFFICE: COLLEGE SrI'ATION, BKAZOS COUNTY, TEXAS. BULLETIN NO. 56. Specinl Se~/~icen.-Nov~~r~e~, 1 899..-IIo?.tic?,1d?rn. lNVESTlGATlON AND IMPROVEMENT 0 F AMERICAN GRAPES AT THE $TUNSON... full comprehension of such matters, so that they can derive full benefit therefrom. In order that each successlive generation of experimenters and vineyard- ists might take up the work where the last left off, and continue to progress all the time...

  7. Vinton Public Power Auth | Open Energy Information

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  9. Virender Dogra Power Projects P Ltd | Open Energy Information

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  12. Virginia Biodiesel Refinery | Open Energy Information

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  16. Virginia Mun Elec Assn No 1 | Open Energy Information

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  1. Viridis Africa 2013 - investment in cleantech | OpenEI Community

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  7. Recovery of fluctuation spectrum evolution from tomographic shear spectra

    SciTech Connect (OSTI)

    Bonometto, Silvio A.; Mezzetti, Marino, E-mail: bonometto@oats.inaf.it, E-mail: mezzetti@oats.inaf.it [Department of Physics, Astronomy Unit, Trieste University, Via Tiepolo 11, I 34143 Trieste (Italy)

    2013-05-01T23:59:59.000Z

    Forthcoming large angle surveys are planned to obtain high precision tomographic shear data. In principle, they will allow us to recover the spectra of matter density fluctuation, at various redshift, through the inversion of the expressions yielding shear spectra from fluctuation spectra. This was discussed in previous work, where SVD techniques for matrix inversion were also shown to be the optimal tool to this aim. Here we show the significant improvements obtainable by using a 7 bin tomography, as allowed by future Euclid data, and discuss error propagation from shear to fluctuation spectra. We find that the technique is a promising tool, namely for the analysis of baryon physics through high–l shear spectra and to test the consistency between expansion rate and fluctuation growth.

  8. Constraining primordial magnetic fields with future cosmic shear surveys

    SciTech Connect (OSTI)

    Fedeli, C. [Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611 (United States); Moscardini, L., E-mail: cosimo.fedeli@astro.ufl.edu, E-mail: lauro.moscardini@unibo.it [Dipartimento di Astronomia, Università di Bologna, Via Ranzani 1, 40127 Bologna (Italy)

    2012-11-01T23:59:59.000Z

    The origin of astrophysical magnetic fields observed in galaxies and clusters of galaxies is still unclear. One possibility is that primordial magnetic fields generated in the early Universe provide seeds that grow through compression and turbulence during structure formation. A cosmological magnetic field present prior to recombination would produce substantial matter clustering at intermediate/small scales, on top of the standard inflationary power spectrum. In this work we study the effect of this alteration on one particular cosmological observable, cosmic shear. We adopt the semi-analytic halo model in order to describe the non-linear clustering of matter, and feed it with the altered mass variance induced by primordial magnetic fields. We find that the convergence power spectrum is, as expected, substantially enhanced at intermediate/small angular scales, with the exact amplitude of the enhancement depending on the magnitude and power-law index of the magnetic field power spectrum. Specifically, for a fixed amplitude, the effect of magnetic fields is larger for larger spectral indices. We use the predicted statistical errors for a future wide-field cosmic shear survey, on the model of the ESA Cosmic Vision mission Euclid, in order to forecast constraints on the amplitude of primordial magnetic fields as a function of the spectral index. We find that the amplitude will be constrained at the level of ? 0.1 nG for n{sub B} ? ?3, and at the level of ? 10{sup ?7} nG for n{sub B} ? 3. The latter is at the same level of lower bounds coming from the secondary emission of gamma-ray sources, implying that for high spectral indices Euclid will certainly be able to detect primordial magnetic fields, if they exist. The present study shows how large-scale structure surveys can be used for both understanding the origins of astrophysical magnetic fields and shedding new light on the physics of the pre-recombination Universe.

  9. Systematic errors in the measurement of neutrino masses due to baryonic feedback processes: Prospects for stage IV lensing surveys

    E-Print Network [OSTI]

    Aravind Natarajan; Andrew R. Zentner; Nicholas Battaglia; Hy Trac

    2014-09-04T23:59:59.000Z

    We examine the importance of baryonic feedback effects on the matter power spectrum on small scales, and the implications for the precise measurement of neutrino masses through gravitational weak lensing. Planned large galaxy surveys such as the Large Synoptic Sky Telescope (LSST) and Euclid are expected to measure the sum of neutrino masses to extremely high precision, sufficient to detect non-zero neutrino masses even in the minimal mass normal hierarchy. We show that weak lensing of galaxies while being a very good probe of neutrino masses, is extremely sensitive to baryonic feedback processes. We use publicly available results from the Overwhelmingly Large Simulations (OWLS) project to investigate the effects of active galactic nuclei feedback, the nature of the stellar initial mass function, and gas cooling rates, on the measured weak lensing shear power spectrum. Using the Fisher matrix formalism and priors from CMB+BAO data, we show that when one does not account for feedback, the measured neutrino mass may be substantially larger or smaller than the true mass, depending on the dominant feedback mechanism, with the mass error |\\Delta m_nu| often exceeding the mass m_nu itself. We also consider gravitational lensing of the cosmic microwave background (CMB) and show that it is not sensitive to baryonic feedback on scales l < 2000, although CMB experiments that aim for sensitivities sigma(m_nu) < 0.02 eV will need to include baryonic effects in modeling the CMB lensing potential. A combination of CMB lensing and galaxy lensing can help break the degeneracy between neutrino masses and baryonic feedback processes. We conclude that future large galaxy lensing surveys such as LSST and Euclid can only measure neutrino masses accurately if the matter power spectrum can be measured to similar accuracy.

  10. Testing a phenomenologically extended DGP model with upcoming weak lensing surveys

    SciTech Connect (OSTI)

    Camera, Stefano; Diaferio, Antonaldo [Dipartimento di Fisica Generale ''A. Avogadro'', Università di Torino, via P. Giuria 1, 10125 Torino (Italy); Cardone, Vincenzo F., E-mail: camera@ph.unito.it, E-mail: diaferio@ph.unito.it, E-mail: winnyenodrac@gmail.com [Dipartimento di Scienze e Tecnologie per l'Ambiente e il Territorio, Università degli Studi del Molise, Contrada Fonte Lappone, 86090 Pesche (Italy)

    2011-01-01T23:59:59.000Z

    A phenomenological extension of the well-known brane-world cosmology of Dvali, Gabadadze and Porrati (eDGP) has recently been proposed. In this model, a cosmological-constant-like term is explicitly present as a non-vanishing tension ? on the brane, and an extra parameter ? tunes the cross-over scale r{sub c}, the scale at which higher dimensional gravity effects become non negligible. Since the Hubble parameter in this cosmology reproduces the same ?CDM expansion history, we study how upcoming weak lensing surveys, such as Euclid and DES (Dark Energy Survey), can confirm or rule out this class of models. We perform Monte Carlo Markov Chain simulations to determine the parameters of the model, using Type Ia Supernovæ, H(z) data, Gamma Ray Bursts and Baryon Acoustic Oscillations. We also fit the power spectrum of the temperature anisotropies of the Cosmic Microwave Background to obtain the correct normalisation for the density perturbation power spectrum. Then, we compute the matter and the cosmic shear power spectra, both in the linear and non-linear régimes. The latter is calculated with the two different approaches of Hu and Sawicki (2007) (HS) and Khoury and Wyman (2009) (KW). With the eDGP parameters coming from the Markov Chains, KW reproduces the ?CDM matter power spectrum at both linear and non-linear scales and the ?CDM and eDGP shear signals are degenerate. This result does not hold with the HS prescription. Indeed, Euclid can distinguish the eDGP model from ?CDM because their expected power spectra roughly differ by the 3? uncertainty in the angular scale range 700?

  11. Solid bitumen at Atigun Gorge, central Brooks Range front: Implications for oil exploration in the North Slope fold and thrust belt

    SciTech Connect (OSTI)

    Howell, D.G.; Johnsson, M.J.; Bird, K.J. (U.S. Geological Survey, Menlo Park, CA (United States))

    1991-03-01T23:59:59.000Z

    The Atigun Gorge area of the north-central Brooks range is a structurally complex region in which a sequence of north-verging duplex structures involving Paleozoic and Mesozoic Ellesmerian continental margin deposits are structurally overlain by a south-verging thrust of Brookian foreland basin deposits of Albian age. The resulting structural triangle zone is marked by numerous small-scale thrusts involving Permian and Triassic strata in which solid bitumen, occupying fissures up to 10 cm wide and several meters in length, has been found. The presence of aromatics in the odorless, black material was confirmed by ultraviolet fluorescence following extraction in dichloromethane. The occurrence of solid bitumen at Atigun Gorge adds to a growing inventory of hydrocarbon-filled fractures found mostly in Cretaceous rocks in the Brooks Range foothills. These occurrences are consistent with a model of hydrocarbon generation beneath the northern margin of the Brooks Range. The regional distribution of vitrinite reflectance isograds suggests that the northern margin of the Brooks Range and the adjoining foreland basin deposits of the North Slope have experienced similar thermal histories. The 0.6% vitrinite reflectance isograd intersects the land surface along the southern margin of the foreland and the 2.0% isograd lies within the northern part of the range. Although these relations suggest the possibility of petroleum resources at shallow depths beneath the Brooks Range foothills, they also indicate that a considerable amount of differential uplift has occurred, probably resulting in redistribution and some leakage of any oil and gas accumulations.

  12. Environmental Effects of Sediment Transport Alteration and Impacts on Protected Species: Edgartown Tidal Energy Project

    SciTech Connect (OSTI)

    Barrett, Stephen B.; Schlezinger, David, Ph.D; Cowles, Geoff, Ph.D; Hughes, Patricia; Samimy; Roland, I.; and Terray, E, Ph.D.

    2012-12-29T23:59:59.000Z

    The Islands of Martha�¢����s Vineyard and Nantucket are separated from the Massachusetts mainland by Vineyard and Nantucket Sounds; water between the two islands flows through Muskeget Channel. The towns of Edgartown (on Martha�¢����s Vineyard) and Nantucket recognize that they are vulnerable to power supply interruptions due to their position at the end of the power grid, and due to sea level rise and other consequences of climate change. The tidal energy flowing through Muskeget Channel has been identified by the Electric Power Research Institute as the strongest tidal resource in Massachusetts waters. The Town of Edgartown proposes to develop an initial 5 MW (nameplate) tidal energy project in Muskeget Channel. The project will consist of 14 tidal turbines with 13 providing electricity to Edgartown and one operated by the University of Massachusetts at Dartmouth for research and development. Each turbine will be 90 feet long and 50 feet high. The electricity will be brought to shore by a submarine cable buried 8 feet below the seabed surface which will landfall in Edgartown either on Chappaquiddack or at Katama. Muskeget Channel is located between Martha�¢����s Vineyard and Nantucket. Its depth ranges between 40 and 160 feet in the deepest portion. It has strong currents where water is transferred between Nantucket Sound and the Atlantic Ocean continental shelf to the south. This makes it a treacherous passage for navigation. Current users of the channel are commercial and recreational fishing, and cruising boats. The US Coast Guard has indicated that the largest vessel passing through the channel is a commercial scallop dragger with a draft of about 10 feet. The tidal resource in the channel has been measured by the University of Massachusetts-Dartmouth and the peak velocity flow is approximately 5 knots. The technology proposed is the helical Gorlov-type turbine positioned with a horizontal axis that is positively buoyant in the water column and held down by anchors. This is the same technology proposed by Ocean Renewable Power Company in the Western Passage and Cobscook Bay near Eastport Maine. The blades rotate in two directions capturing the tides energy both during flood and ebb tides. The turbines will be anchored to the bottom and suspended in the water column. Initial depth of the turbines is expected to be about 25 feet below the surface to avoid impacting navigation while also capturing the strongest currents. The Town of Edgartown was initially granted a Preliminary Permit by the Federal Energy Regulatory Commission (FERC) on March 1, 2008, and has recently received a second permit valid through August 2014. The Preliminary Permit gives Edgartown the exclusive right to apply for a power generation license for power generated from the hydrokinetic energy in the water flowing in this area. Edgartown filed a Draft Pilot License Application with FERC on February 1, 2010 and an Expanded Environmental Notification Form with the Massachusetts Environmental Policy Act (MEPA) Office at the same time. It expects to file a Final License Application in late 2013. Harris Miller Miller & Hanson (HMMH) of Burlington Massachusetts is acting as the Project Manager for the Town of Edgartown and collaborating with other partners of the project including the University of Massachusetts - Dartmouth's Marine Renewable Energy Center and the Massachusetts Clean Energy Center. HMMH was awarded a grant under the Department of Energy's Advanced Water Program to conduct marine science and hydrokinetic site-specific environmental studies for projects actively seeking a FERC License. HMMH, on behalf of the Town, is managing this comprehensive study of the marine environment in Muskeget Channel and potential impacts of the tidal project on indicator species and habitats. The University of Massachusetts School of Marine Science and Technology (SMAST) conducted oceanographic studies of tidal currents, tide level, benthic habit

  13. Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion

    SciTech Connect (OSTI)

    Fedeli, C. [Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611-2055 (United States); Bartelmann, M. [Zentrum für Astronomie, Universität Heidelberg, Albert-Überle-Straße 2, 69120 Heidelberg (Germany); Moscardini, L., E-mail: cosimo.fedeli@astro.ufl.edu, E-mail: bartelmann@uni-heidelberg.de, E-mail: lauro.moscardini@unibo.it [Dipartimento di Astronomia, Università di Bologna, Via Ranzani 1, 40127 Bologna (Italy)

    2012-10-01T23:59:59.000Z

    We examine the cosmological constraining power of future large-scale weak lensing surveys on the model of the ESA planned mission Euclid, with particular reference to primordial non-Gaussianity. Our analysis considers several different estimators of the projected matter power spectrum, based on both shear and flexion. We review the covariance and Fisher matrix for cosmic shear and evaluate those for cosmic flexion and for the cross-correlation between the two. The bounds provided by cosmic shear alone are looser than previously estimated, mainly due to the reduced sky coverage and background number density of sources for the latest Euclid specifications. New constraints for the local bispectrum shape, marginalized over ?{sub 8}, are at the level of ?f{sub NL} ? 100, with the precise value depending on the exact multipole range that is considered in the analysis. We consider three additional bispectrum shapes, for which the cosmic shear constraints range from ?f{sub NL} ? 340 (equilateral shape) up to ?f{sub NL} ? 500 (orthogonal shape). Also, constraints on the level of non-Gaussianity and on the amplitude of the matter power spectrum ?{sub 8} are almost perfectly anti-correlated, except for the orthogonal bispectrum shape for which they are correlated. The competitiveness of cosmic flexion constraints against cosmic shear ones depends by and large on the galaxy intrinsic flexion noise, that is still virtually unconstrained. Adopting the very high value that has been occasionally used in the literature results in the flexion contribution being basically negligible with respect to the shear one, and for realistic configurations the former does not improve significantly the constraining power of the latter. Since the shear shot noise is white, while the flexion one decreases with decreasing scale, by considering high enough multipoles the two contributions have to become comparable. Extending the analysis up to l{sub max} = 20,000 cosmic flexion, while being still subdominant, improves the shear constraints by ? 10% when added. However on such small scales the highly non-linear clustering of matter, the impact of baryonic physics, and the non-Gaussian part of the covariance matrix make any error estimation uncertain. By considering lower, and possibly more realistic, values of the flexion intrinsic shape noise results in flexion constraining power being a factor of ? 2 better than that of shear, and the bounds on ?{sub 8} and f{sub NL} being improved by a factor of ? 3 upon their combination.

  14. Accounting for baryonic effects in cosmic shear tomography: Determining a minimal set of nuisance parameters using PCA

    SciTech Connect (OSTI)

    Eifler, Tim; Krause, Elisabeth; Dodelson, Scott; Zentner, Andrew; Hearin, Andrew; Gnedin, Nickolay

    2014-05-28T23:59:59.000Z

    Systematic uncertainties that have been subdominant in past large-scale structure (LSS) surveys are likely to exceed statistical uncertainties of current and future LSS data sets, potentially limiting the extraction of cosmological information. Here we present a general framework (PCA marginalization) to consistently incorporate systematic effects into a likelihood analysis. This technique naturally accounts for degeneracies between nuisance parameters and can substantially reduce the dimension of the parameter space that needs to be sampled. As a practical application, we apply PCA marginalization to account for baryonic physics as an uncertainty in cosmic shear tomography. Specifically, we use CosmoLike to run simulated likelihood analyses on three independent sets of numerical simulations, each covering a wide range of baryonic scenarios differing in cooling, star formation, and feedback mechanisms. We simulate a Stage III (Dark Energy Survey) and Stage IV (Large Synoptic Survey Telescope/Euclid) survey and find a substantial bias in cosmological constraints if baryonic physics is not accounted for. We then show that PCA marginalization (employing at most 3 to 4 nuisance parameters) removes this bias. Our study demonstrates that it is possible to obtain robust, precise constraints on the dark energy equation of state even in the presence of large levels of systematic uncertainty in astrophysical processes. We conclude that the PCA marginalization technique is a powerful, general tool for addressing many of the challenges facing the precision cosmology program.

  15. 4MOST - 4-metre Multi-Object Spectroscopic Telescope

    E-Print Network [OSTI]

    de Jong, Roelof S; Chiappini, Cristina; Depagne, Éric; Haynes, Roger; Johl, Diane; Schnurr, Olivier; Schwope, Axel; Walcher, Jakob; Dionies, Frank; Haynes, Dionne; Kelz, Andreas; Kitaura, Francisco S; Lamer, Georg; Minchev, Ivan; Müller, Volker; Nuza, Sebastián E; Olaya, Jean-Christophe; Piffl, Tilmann; Popow, Emil; Steinmetz, Matthias; Ural, U?ur; Williams, Mary; Winkler, Roland; Wisotzki, Lutz; Ansorgb, Wolfgang R; Banerji, Manda; Solares, Eduardo Gonzalez; Irwin, Mike; Kennicutt, Robert C; King, David; McMahon, Richard; Koposov, Sergey; Parry, Ian R; Walton, Nicholas A; Finger, Gert; Iwert, Olaf; Krumpe, Mirko; Lizon, Jean-Louis; Vincenzo, Mainieri; Amans, Jean-Philippe; Bonifacio, Piercarlo; Cohen, Mathieu; Francois, Patrick; Jagourel, Pascal; Mignot, Shan B; Royer, Frédéric; Sartoretti, Paola; Bender, Ralf; Grupp, Frank; Hess, Hans-Joachim; Lang-Bardl, Florian; Muschielok, Bernard; Böhringer, Hans; Boller, Thomas; Bongiorno, Angela; Brusa, Marcella; Dwelly, Tom; Merloni, Andrea; Nandra, Kirpal; Salvato, Mara; Pragt, Johannes H; Navarro, Ramón; Gerlofsma, Gerrit; Roelfsema, Ronald; Dalton, Gavin B; Middleton, Kevin F; Tosh, Ian A; Boeche, Corrado; Caffau, Elisabetta; Christlieb, Norbert; Grebel, Eva K; Hansen, Camilla; Koch, Andreas; Ludwig, Hans-G; Quirrenbach, Andreas; Sbordone, Luca; Seifert, Walter; Thimm, Guido; Trifonov, Trifon; Helmi, Amina; Trager, Scott C; Feltzing, Sofia; Korn, Andreas; Boland, Wilfried

    2012-01-01T23:59:59.000Z

    The 4MOST consortium is currently halfway through a Conceptual Design study for ESO with the aim to develop a wide-field (>3 square degree, goal >5 square degree), high-multiplex (>1500 fibres, goal 3000 fibres) spectroscopic survey facility for an ESO 4m-class telescope (VISTA). 4MOST will run permanently on the telescope to perform a 5 year public survey yielding more than 20 million spectra at resolution R~5000 ({\\lambda}=390-1000 nm) and more than 2 million spectra at R~20,000 (395-456.5 nm & 587-673 nm). The 4MOST design is especially intended to complement three key all-sky, space-based observatories of prime European interest: Gaia, eROSITA and Euclid. Initial design and performance estimates for the wide-field corrector concepts are presented. We consider two fibre positioner concepts, a well-known Phi-Theta system and a new R-Theta concept with a large patrol area. The spectrographs are fixed configuration two-arm spectrographs, with dedicated spectrographs for the high- and low-resolution. A ful...

  16. Do we need model-dependent covariances when we test cosmological models with galaxy power spectra?

    E-Print Network [OSTI]

    Kalus, B; Samushia, L

    2015-01-01T23:59:59.000Z

    We consider the shape of the posterior distribution to be used when fitting cosmological models to power spectra measured from galaxy surveys. At very large scales, Gaussian posterior distributions in the power do not approximate the posterior distribution $\\mathcal P_R$ we expect for a Gaussian density field $\\delta_\\mathbf{k}$, even if we vary the covariance matrix according to the model to be tested. We compare alternative posterior distributions with $\\mathcal P_R$, both mode-by-mode and in terms of expected $f_\\mathrm{NL}$-measurements. Marginalising over a Gaussian posterior distribution $\\mathcal P_f$ with fixed covariance matrix yields a posterior mean value of $f_\\mathrm{NL}$ which, for a data set with the characteristics of Euclid, will be underestimated by $\\triangle f_\\mathrm{NL}=0.4$, while for the data release 9 (DR9) of the Sloan Digital Sky Survey (SDSS)-III Baryon Oscillation Spectroscopic Survey (BOSS) it will be underestimated by $\\triangle f_\\mathrm{NL}=19.1$. The inverse cubic normal dist...

  17. Cosmological tests of modified gravity: constraints on $F(R)$ theories from the galaxy clustering ratio

    E-Print Network [OSTI]

    Julien Bel; Philippe Brax; Christian Marinoni; Patrick Valageas

    2015-04-23T23:59:59.000Z

    The clustering ratio $\\eta$, a large-scale structure observable originally designed to constrain the shape of the power spectrum of matter density fluctuations, is shown to provide a sensitive probe of the nature of gravity in the cosmological regime. We apply this analysis to $F(R)$ theories of gravity using the luminous red galaxy (LRG) sample extracted from the spectroscopic Sloan Digital Sky Survey (SDSS) data release 7 and 10 catalogues. We find that General Relativity (GR), complemented with a Friedmann-Robertson-Walker (FRW) cosmological model with parameters fixed by the Planck satellite, describes extremely well the clustering of galaxies up to $z\\sim 0.6$. On large cosmic scales, the absolute amplitude of deviations from GR, $|f_{R_0 }|$, is constrained to be smaller than $4.6 \\times 10^{-5}$ at the $95\\%$ confidence level. This bound makes cosmological probes of gravity almost competitive with the sensitivity of Solar System tests, although still one order of magnitude less effective than astrophysical tests. We also extrapolate our results to future large surveys like Euclid and show that the astrophysical bound will certainly remain out of reach for such a class of modified-gravity models that only differ from $\\Lambda$CDM at low redshifts.

  18. I. Apples to apples $A^2$: photometric redshift predictions for next-generation surveys

    E-Print Network [OSTI]

    Ascaso, Begoña; Benítez, Narciso

    2015-01-01T23:59:59.000Z

    This is the first of a series of papers where we compare the expected performance of two of the largest stage IV next-generation surveys in the optical and infrared (LSST and Euclid), with a particular focus on cluster surveys. In this first paper, we introduce the mock catalogues we have utilized in this work, an N-body simulation+semi-analytical cone with a posterior modification with PhotReal, a technique which modifies the original photometry to make it more realistic by using an empirical library of spectral templates. We have confirmed the reliability of the mock catalogue by comparing the obtained color-magnitude relation, the luminosity and mass function and the angular correlation function with those of real data. We also analyze the behavior of the expected photometric redshifts for each different survey, in terms of photometric redshift resolution, photometric redshift bias and fraction of outliers. In addition, we discuss the benefits of using the BPZ \\emph{odds} photometric redshift quality param...

  19. Remarks on an attempted axiomatisation of Quantum Mechanics, due to Lucien Hardy, and Ten Theses on Hilbert's Sixth Problem and Quantum Measurement

    E-Print Network [OSTI]

    Joseph F. Johnson

    2006-06-15T23:59:59.000Z

    From the standpoint of Hilbert's Sixth Problem, which is the axiomatisation of Physics, the famous paper of Lucien Hardy's, Quantum Theory from Five Reasonable Axioms, is not relevant. The present paper argues that Hardy does not give a physical definition of `limit', and if we assume the usual mathematical definition of limit of a sequence, he fails to define a sequence in physical terms to which the usual definition is applicable. We argue that one should not, in fact, try to define probability in terms of the usual notion of limit of a sequence of results of a measurement because of seemingly insurmountable difficulties in axiomatising the notion of function or sequence in this context. Von Plato's and the authour's work (see http:arxiv.org/abs/quant-ph/0502124 and euclid.unh.edu/~jjohnson/axiomatics.html for larger context and further references) on the definition of physical probability needs to be used in this context. We conclude with ten theses on quantum measurement, from the standpoint of the Hilbert problem.

  20. Counting voids to probe dark energy

    E-Print Network [OSTI]

    Pisani, Alice; Hamaus, Nico; Alizadeh, Esfandiar; Biswas, Rahul; Wandelt, Benjamin D; Hirata, Christopher M

    2015-01-01T23:59:59.000Z

    We show that the number of observed voids in galaxy redshift surveys is a sensitive function of the equation of state of dark energy. Using the Fisher matrix formalism we find the error ellipses in the $w_0-w_a$ plane when the equation of state of dark energy is assumed to be of the form $w_{CPL}(z)=w_0 +w_a z/(1+z)$. We forecast the number of voids to be observed with the ESA Euclid satellite and the NASA WFIRST mission, taking into account updated details of the surveys to reach accurate estimates of their power. The theoretical model for the forecast of the number of voids is based on matches between abundances in simulations and the analytical prediction. To take into account the uncertainties within the model, we marginalize over its free parameters when calculating the Fisher matrices. The addition of the void abundance constraints to the data from Planck, HST and supernova survey data noticeably tighten the $w_0-w_a$ parameter space. We thus quantify the improvement in the constraints due to the use of...

  1. On geometry influence on the behavior of a quantum mechanical scalar particle with intrinsic structure in external magnetic and electric fields

    E-Print Network [OSTI]

    O. V. Veko; K. V. Kazmerchuk; E. M. Ovsiyuk; V. V. Kisel; V. M. Red'kov

    2014-11-07T23:59:59.000Z

    Relativistic theory of the Cox's scalar not point-like particle with intrinsic structure is developed on the background of arbitrary curved space-time. It is shown that in the most general form, the extended Proca-like tensor first order system of equations contains non minimal interaction terms through electromagnetic tensor F_{\\alpha \\beta} and Ricci tensor R_{\\alpha \\beta}. In relativistic Cox's theory, the limiting procedure to non-relativistic approximation is performed in a special class of curved space-time models. This theory is specified in simple geometrical backgrounds: Euclid's, Lobachevsky's, and Rie\\-mann's. Wave equation for the Cox's particle is solved exactly in presence of external uniform magnetic and electric fields in the case of Minkowski space. Non-trivial additional structure of the particle modifies the frequency of a quantum oscillator arising effectively in presence if external magnetic field. Extension of these problems to the case of the hyperbolic Lobachevsky space is examined. In presence of the magnetic field, the quantum problem in radial variable has been solved exactly; the quantum motion in z-direction is described by 1-dimensional Schr\\"{o}dinger-like equation in an effective potential which turns out to be too difficult for analytical treatment. In the presence of electric field, the situation is similar. The same analysis has been performed for spherical Riemann space model.

  2. Constraining inflation with future galaxy redshift surveys

    SciTech Connect (OSTI)

    Huang, Zhiqi; Vernizzi, Filippo [CEA, Institut de Physique Théorique, 91191 Gif-sur-Yvette cédex (France); Verde, Licia, E-mail: zhiqi.huang@cea.fr, E-mail: liciaverde@icc.ub.edu, E-mail: filippo.vernizzi@cea.fr [Institute of Sciences of the Cosmos (ICCUB), University of Barcelona, Marti i Franques 1, Barcelona 08024 (Spain)

    2012-04-01T23:59:59.000Z

    With future galaxy surveys, a huge number of Fourier modes of the distribution of the large scale structures in the Universe will become available. These modes are complementary to those of the CMB and can be used to set constraints on models of the early universe, such as inflation. Using a MCMC analysis, we compare the power of the CMB with that of the combination of CMB and galaxy survey data, to constrain the power spectrum of primordial fluctuations generated during inflation. We base our analysis on the Planck satellite and a spectroscopic redshift survey with configuration parameters close to those of the Euclid mission as examples. We first consider models of slow-roll inflation, and show that the inclusion of large scale structure data improves the constraints by nearly halving the error bars on the scalar spectral index and its running. If we attempt to reconstruct the inflationary single-field potential, a similar conclusion can be reached on the parameters characterizing the potential. We then study models with features in the power spectrum. In particular, we consider ringing features produced by a break in the potential and oscillations such as in axion monodromy. Adding large scale structures improves the constraints on features by more than a factor of two. In axion monodromy we show that there are oscillations with small amplitude and frequency in momentum space that are undetected by CMB alone but can be measured by including galaxy surveys in the analysis.

  3. Additive structure of Z(.) mod m_k (squarefree) and Goldbach's Conjecture

    E-Print Network [OSTI]

    N. F. Benschop

    2009-10-08T23:59:59.000Z

    The product m_k of the first k primes (2..p_k) has neighbours m_k +/- 1 with all prime divisors beyond p_k, implying there are infinitely many primes [Euclid]. All primes between p_k and m_k are in the group G_1 of units in semigroup Z_{m_k}(.) of mutiplication mod m_k. Due to the squarefree modulus Z_{m_k} is a disjoint union of 2^k groups, with as many idempotents - one per divisor of m_k, which form a Boolean lattice BL. The generators of Z_{m_k} and the additive properties of its lattice are studied. It is shown that each complementary pair in BL adds to 1 mod m_k and each even idempotent e in BL has successor e+1 in G_1. It follows that G_1+G_1 \\equiv E, the set of even residues in Z_{m_k}, so each even residue is the sum of two roots of unity, proving "Goldbach for Residues" mod m_k ("GR"). . . . Induction on k by extending residues mod m_k with "carry" a 1) successive 2n are in overlapping intervals, while the smallest composite unit in G_1 mod m_k is p_{k+1}^2, yielding "GC": Each 2n > 4 is the sum of two odd primes.

  4. Wide Angle Effects in Galaxy Surveys

    E-Print Network [OSTI]

    Yoo, Jaiyul

    2013-01-01T23:59:59.000Z

    Current and future galaxy surveys cover a large fraction of the entire sky with a significant redshift range, and the recent theoretical development shows that general relativistic effects are present in galaxy clustering on very large scales. This trend has renewed interest in the wide angle effect in galaxy clustering measurements, in which the distant-observer approximation is often adopted. Using the full wide-angle formula for computing the redshift-space correlation function, we show that compared to the sample variance, the deviation in the redshift-space correlation function from the simple Kaiser formula with the distant-observer approximation is negligible in the SDSS and is completely irrelevant in future galaxy surveys such as Euclid and the BigBOSS, if the theoretical prediction from the Kaiser formula is averaged over the survey volume and the non-uniform distribution of cosine angle between the line-of-sight and the pair separation directions is properly considered. We also find small correctio...

  5. Supermassive population III supernovae and the birth of the first quasars

    SciTech Connect (OSTI)

    Whalen, Daniel J.; Smidt, Joseph [T-2, Los Alamos National Laboratory, Los Alamos, NM 87545 (United States); Even, Wesley; Fryer, Chris L. [CCS-2, Los Alamos National Laboratory, Los Alamos, NM 87545 (United States); Heger, Alexander [Monash Centre for Astrophysics, Monash University, Victoria 3800 (Australia); Chen, K.-J. [School of Physics and Astronomy, University of Minnesota, Twin Cities, Minneapolis, MN 55455 (United States); Stiavelli, Massimo [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Xu, Hao [Center for Astrophysics and Space Sciences, UC San Diego, La Jolla, CA 92093 (United States); Joggerst, Candace C. [XTD-3, Los Alamos National Laboratory, Los Alamos, NM 87545 (United States)

    2013-11-20T23:59:59.000Z

    The existence of supermassive black holes as early as z ? 7 is one of the great, unsolved problems in cosmological structure formation. One leading theory argues that they are born during catastrophic baryon collapse in z ? 15 protogalaxies that form in strong Lyman-Werner UV backgrounds. Atomic line cooling in such galaxies fragments baryons into massive clumps that are thought to directly collapse to 10{sup 4}-10{sup 5} M {sub ?} black holes. We have now discovered that some of these fragments can instead become supermassive stars that eventually explode as thermonuclear supernovae (SNe) with energies of ?10{sup 55} erg, the most energetic explosions in the universe. We have calculated light curves and spectra for supermassive Pop III SNe with the Los Alamos RAGE and SPECTRUM codes. We find that they will be visible in near-infrared all-sky surveys by Euclid out to z ? 10-15 and by WFIRST and WISH out to z ? 15-20, perhaps revealing the birthplaces of the first quasars.

  6. Quintessence versus phantom dark energy: the arbitrating power of current and future observations

    SciTech Connect (OSTI)

    Novosyadlyj, B.; Sergijenko, O. [Astronomical Observatory of Ivan Franko National University of Lviv, Kyryla i Methodia str., 8, Lviv, 79005 (Ukraine); Durrer, R. [Université de Genève, Département de Physique Théorique and CAP, 24 quai Ernest-Ansermet, CH-1211 Genève 4 (Switzerland); Pelykh, V., E-mail: novos@astro.franko.lviv.ua, E-mail: olka@astro.franko.lviv.ua, E-mail: ruth.durrer@unige.ch, E-mail: pelykh@iapmm.lviv.ua [Ya. S. Pidstryhach Institute for Applied Problems of Mechanics and Mathematics, Naukova str., 3-b, Lviv, 79060 (Ukraine)

    2013-06-01T23:59:59.000Z

    We analyze the possibility to distinguish between quintessence and phantom scalar field models of dark energy using observations of luminosity distance moduli of SNe Ia, CMB anisotropies and polarization, matter density perturbations and baryon acoustic oscillations. Among the present observations only Planck data on CMB anisotropy and SDSS DR9 data on baryon acoustic oscillations may be able to decide between quintessence or phantom scalar field models, however for each model a set of best-fit parameters exists, which matches all data with similar goodness of fit. We compare the relative differences of best-fit model predictions with observational uncertainties for each type of data and we show that the accuracy of SNe Ia luminosity distance data is far from the one necessary to distinguish these types of dark energy models, while the CMB data (WMAP, ACT, SPT and especially Planck) are close to being able to reliably distinguish them. Also an improvement of the large-scale structure data (future releases of SDSS BOSS and e.g. Euclid or BigBOSS) will enable us to surely decide between quintessence and phantom dark energy.

  7. Measurements of Ammonia at Blodgett Forest

    SciTech Connect (OSTI)

    Fischer, Marc L.; Littlejohn, David

    2007-04-01T23:59:59.000Z

    Ammonia is a reactive trace gas that is emitted in large quantities by animal agriculture and other sources in California, which subsequently forms aerosol particulate matter, potentially affecting visibility, climate, and human health. We performed initial measurements of NH{sub 3} at the Blodgett Forest Research Station (BFRS) during a 3 week study in June, 2006. The site is used for ongoing air quality research and is a relatively low-background site in the foothills of the Sierra Nevada. Measured NH{sub 3} mixing ratios were quite low (< 1 to {approx}2 ppb), contrasting with typical conditions in many parts of the Central Valley. Eddy covariance measurements showed NH{sub 3} fluxes that scaled with measured NH{sub 3} mixing ratio and calculated aerodynamic deposition velocity, suggesting dry deposition is a significant loss mechanism for atmospheric NH{sub 3} at BFRS. A simple model of NH{sub 3} transport to the site supports the hypothesis that NH{sub 3} is transported from the Valley to BFRS, but deposits on vegetation during the summer. Further work is necessary to determine whether the results obtained in this study can be generalized to other seasons.

  8. Solar Energy Development Assistance for Fort Hunter Liggett

    SciTech Connect (OSTI)

    Russo, Bryan J.; Hoffman, Michael G.; Chvala, William D.

    2011-03-30T23:59:59.000Z

    Pacific Northwest National Laboratory provided assistance to Fort Hunter Liggett to determine the opportunities for solar energy development on the site. Increasing use of renewable energy is mandated by several executive orders and legislation. Fort Hunter Liggett has many attributes that enhance its suitability for renewable energy development. First, the site is located south of San Francisco in a remote portion of the costal foothills. Brush and forest fires are frequent and often result in power outages, which subsequently impacts the site’s training mission. In addition, the site’s blended electric rate during fiscal year (FY) 2010 was high at 12 ¢/kWh. Lastly, the solar resource is moderately high; the site receives nearly 5.7 kWh/m2/day on a south facing, latitude-tilted surface. In light of these factors, the site is a clear candidate for a solar photovoltaic array. Prior to Pacific Northwest National Laboratory’s (PNNL) involvement, the site secured funding for a 1 megawatt (MW) photovoltaic (PV) array that will also provide shading for site vehicles. To best implement this project, PNNL conducted a site visit and was tasked with providing the site technical guidance and support regarding module selection, array siting, and other ancillary issues.

  9. Superinsulation in refrigerators and freezers

    SciTech Connect (OSTI)

    Vineyard, E.; Stovall, T.K.; Wilkes, K.E.; Childs, K.W.

    1998-02-01T23:59:59.000Z

    The results presented here were obtained during Phase 4 of the first CRADA, which had the specific objective of determining the lifetime of superinsulations when installed in simulated refrigerator doors. The second CRADA was established to evaluate and test design concepts proposed to significantly reduce energy consumption in a refrigerator-freezer that is representative of approximately 60% of the US market. The stated goal of this CRADA is to demonstrate advanced technologies which reduce, by 50%, the 1993 National Appliance Energy Conservation Act (NAECA) standard energy consumption for a 20 ft{sup 3} (570 L) top-mount, automatic-defrost, refrigerator-freezer. For a unit this size, the goal translates to an energy consumption of 1.003 kWh/d. The general objective of the research is to facilitate the introduction of efficient appliances by demonstrating design changes that can be effectively incorporated into new products. In previous work on this project, a Phase 1 prototype refrigerator-freezer achieved an energy consumption of 1.413 kWh/d [Vineyard, et al., 1995]. Following discussions with an advisory group comprised of all the major refrigerator-freezer manufacturers, several options were considered for the Phase 2 effort, one of which was cabinet heat load reductions.

  10. BEST Winery Guidebook: Benchmarking and Energy and Water SavingsTool for the Wine Industry

    SciTech Connect (OSTI)

    Galitsky, Christina; Worrell, Ernst; Radspieler, Anthony; Healy,Patrick; Zechiel, Susanne

    2005-10-15T23:59:59.000Z

    Not all industrial facilities have the staff or the opportunity to perform a detailed audit of their operations. The lack of knowledge of energy efficiency opportunities provides an important barrier to improving efficiency. Benchmarking has demonstrated to help energy users understand energy use and the potential for energy efficiency improvement, reducing the information barrier. In California, the wine making industry is not only one of the economic pillars of the economy; it is also a large energy consumer, with a considerable potential for energy-efficiency improvement. Lawrence Berkeley National Laboratory and Fetzer Vineyards developed an integrated benchmarking and self-assessment tool for the California wine industry called ''BEST''(Benchmarking and Energy and water Savings Tool) Winery. BEST Winery enables a winery to compare its energy efficiency to a best practice winery, accounting for differences in product mix and other characteristics of the winery. The tool enables the user to evaluate the impact of implementing energy and water efficiency measures. The tool facilitates strategic planning of efficiency measures, based on the estimated impact of the measures, their costs and savings. BEST Winery is available as a software tool in an Excel environment. This report serves as background material, documenting assumptions and information on the included energy and water efficiency measures. It also serves as a user guide for the software package.

  11. Cosmological parameter constraints from SDSS luminous red galaxies: a new treatment of large-scale clustering

    E-Print Network [OSTI]

    Ariel G. Sanchez; M. Crocce; A. Cabre; C. M. Baugh; E. Gaztanaga

    2009-08-19T23:59:59.000Z

    We apply a new model for the spherically averaged correlation function at large pair separations to the measurement of the clustering of luminous red galaxies (LRGs) made from the SDSS by Cabre and Gaztanaga(2009). Our model takes into account the form of the BAO peak and the large scale shape of the correlation function. We perform a Monte Carlo Markov chain analysis for different combinations of datasets and for different parameter sets. When used in combination with a compilation of the latest CMB measurements, the LRG clustering and the latest supernovae results give constraints on cosmological parameters which are comparable and in remarkably good agreement, resolving the tension reported in some studies. The best fitting model in the context of a flat, Lambda-CDM cosmology is specified by Omega_m=0.261+-0.013, Omega_b=0.044+-0.001, n_s=0.96+-0.01, H_0=71.6+-1.2 km/s/Mpc and sigma_8=0.80+-0.02. If we allow the time-independent dark energy equation of state parameter to vary, we find results consistent with a cosmological constant at the 5% level using all data sets: w_DE=-0.97+-0.05. The large scale structure measurements by themselves can constrain the dark energy equation of state parameter to w_DE=-1.05+-0.15, independently of CMB or supernovae data. We do not find convincing evidence for an evolving equation of state. We provide a set of "extended distance priors" that contain the most relevant information from the CMB power spectrum and the shape of the LRG correlation function which can be used to constrain dark energy models and spatial curvature. Our model should provide an accurate description of the clustering even in much larger, forthcoming surveys, such as those planned with NASA's JDEM or ESA's Euclid mission.

  12. CLUSTER LENSING PROFILES DERIVED FROM A REDSHIFT ENHANCEMENT OF MAGNIFIED BOSS-SURVEY GALAXIES

    SciTech Connect (OSTI)

    Coupon, Jean; Umetsu, Keiichi [Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 10617, Taiwan (China); Broadhurst, Tom, E-mail: coupon@asiaa.sinica.edu.tw [Department of Theoretical Physics, University of Basque Country UPV/EHU, P.O. Box 644, E-48080 Bilbao (Spain)

    2013-07-20T23:59:59.000Z

    We report the first detection of a redshift-depth enhancement of background galaxies magnified by foreground clusters. Using 300,000 BOSS survey galaxies with accurate spectroscopic redshifts, we measure their mean redshift depth behind four large samples of optically selected clusters from the Sloan Digital Sky Survey (SDSS) surveys, totaling 5000-15,000 clusters. A clear trend of increasing mean redshift toward the cluster centers is found, averaged over each of the four cluster samples. In addition, we find similar but noisier behavior for an independent X-ray sample of 158 clusters lying in the foreground of the current BOSS sky area. By adopting the mass-richness relationships appropriate for each survey, we compare our results with theoretical predictions for each of the four SDSS cluster catalogs. The radial form of this redshift enhancement is well fitted by a richness-to-mass weighted composite Navarro-Frenk-White profile with an effective mass ranging between M{sub 200} {approx} 1.4-1.8 Multiplication-Sign 10{sup 14} M{sub Sun} for the optically detected cluster samples, and M{sub 200} {approx} 5.0 Multiplication-Sign 10{sup 14} M{sub Sun} for the X-ray sample. This lensing detection helps to establish the credibility of these SDSS cluster surveys, and provides a normalization for their respective mass-richness relations. In the context of the upcoming bigBOSS, Subaru Prime Focus Spectrograph, and EUCLID-NISP spectroscopic surveys, this method represents an independent means of deriving the masses of cluster samples for examining the cosmological evolution, and provides a relatively clean consistency check of weak-lensing measurements, free from the systematic limitations of shear calibration.

  13. WEAK LENSING MEASUREMENT OF GALAXY CLUSTERS IN THE CFHTLS-WIDE SURVEY

    SciTech Connect (OSTI)

    Shan Huanyuan; Tao Charling [Department of Physics and Tsinghua Center for Astrophysics, Tsinghua University, Beijing, 100084 (China); Kneib, Jean-Paul; Jauzac, Mathilde; Limousin, Marceau [Laboratoire d'Astrophysique de Marseille, CNRS-Universite de Provence, 38 rue Frederic Joliot-Curie, F-13388 Marseille Cedex 13 (France); Fan Zuhui [Department of Astronomy, Peking University, Beijing, 100871 (China); Massey, Richard [Institute for Astronomy, Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ (United Kingdom); Rhodes, Jason [California Institute of Technology, MC 350-17, 1200 East California Boulevard, Pasadena, CA 91125 (United States); Thanjavur, Karun [Canada France Hawaii Telescope, 65-1238 Mamalahoa Hwy, Kamuela, HI 96743 (United States); McCracken, Henry J., E-mail: shanhuany@gmail.com [Institude d'Astrophysique de Paris, UMR 7095, 98 bis Boulevard Arago, F-75014 Paris (France)

    2012-03-20T23:59:59.000Z

    We present the first weak gravitational lensing analysis of the completed Canada-France-Hawaii Telescope Legacy Survey (CFHTLS). We study the 64 deg{sup 2} W1 field, the largest of the CFHTLS-Wide survey fields, and present the largest contiguous weak lensing convergence 'mass map' yet made. 2.66 million galaxy shapes are measured, using the Kaiser Squires and Broadhurst Method (KSB) pipeline verified against high-resolution Hubble Space Telescope imaging that covers part of the CFHTLS. Our i'-band measurements are also consistent with an analysis of independent r'-band imaging. The reconstructed lensing convergence map contains 301 peaks with signal-to-noise ratio {nu} > 3.5, consistent with predictions of a {Lambda}CDM model. Of these peaks, 126 lie within 3.'0 of a brightest central galaxy identified from multicolor optical imaging in an independent, red sequence survey. We also identify seven counterparts for massive clusters previously seen in X-ray emission within 6 deg{sup 2} XMM-LSS survey. With photometric redshift estimates for the source galaxies, we use a tomographic lensing method to fit the redshift and mass of each convergence peak. Matching these to the optical observations, we confirm 85 groups/clusters with {chi}{sup 2}{sub reduced} < 3.0, at a mean redshift (z{sub c} ) = 0.36 and velocity dispersion ({sigma}{sub c}) = 658.8 km s{sup -1}. Future surveys, such as DES, LSST, KDUST, and EUCLID, will be able to apply these techniques to map clusters in much larger volumes and thus tightly constrain cosmological models.

  14. Polluting of Winter Convective Clouds upon Transition from Ocean Inland Over Central California: Contrasting Case Studies

    SciTech Connect (OSTI)

    Rosenfeld, Daniel; Chemke, Rei; Prather, Kimberly; Suski, Kaitlyn; Comstock, Jennifer M.; Schmid, Beat; Tomlinson, Jason M.; Jonsson, Haf

    2014-01-01T23:59:59.000Z

    In-situ aircraft measurements of aerosol chemical and cloud microphysical properties were conducted during the CalWater campaign in February and March 2011 over the Sierra Nevada Mountains and the coastal waters of central California. The main objective was to elucidate the impacts of aerosol properties on clouds and precipitation forming processes. In order to accomplish this, we compared contrasting cases of clouds that ingested aerosols from different sources. The results showed that clouds containing pristine oceanic air had low cloud drop concentrations and started to develop rain 500 m above their base. This occurred both over the ocean and over the Sierra Nevada, mainly in the early morning when the radiatively cooled stable continental boundary layer was decoupled from the cloud base. Supercooled rain dominated the precipitation that formed in growing convective clouds in the pristine air, up to the -21°C isotherm level. A contrasting situation was documented in the afternoon over the foothills of the Sierra Nevada, when the clouds ingested high pollution aerosol concentrations produced in the Central Valley. This led to slow growth of the cloud drop effective radius with height and suppressed and even prevented the initiation of warm rain while contributing to the development of ice hydrometeors in the form of graupel. Our results show that cloud condensation and ice nuclei were the limiting factors that controlled warm rain and ice processes, respectively, while the unpolluted clouds in the same air mass produced precipitation quite efficiently. These findings provide the motivation for deeper investigations into the nature of the aerosols seeding clouds.

  15. Report on surface geology and groundwater investigations of Mortons and Green Valley Well Fields. Final technical report, November 1980-May 1982. [Proposed WyCoalGas Project, Converse County, Wyoming; site evaluation

    SciTech Connect (OSTI)

    None

    1982-01-01T23:59:59.000Z

    The general region of investigation of this report is in the southern part of the Powder River Basin near the Town of Douglas, Wyoming. Two specific areas within this region were investigated to determine the groundwater potential with drilling and testing programs during the years 1973 to 1975. One area of investigation is located approximately 12 miles west of Douglas in T32 and 33N, R73 and 74W, and is known as the Green Valley Well Field. This area is situated in the foothills of the north end of the Laramie Range and encompasses approximately 25 square miles. In this area the Madison Formation limestone and the Flathead Formation sandstone are the aquifers of interest for groundwater production. The second area is located approximately 13 miles north of Douglas in T34 and 35N, R70 and 71W, and is known as the Mortons Well Field. This area encompasses about 30 square miles. In this area, the Lance Formation and Fox Hills Formation sandstones are the aquifers of interest. Contained within the body of this report are two geologic studies prepared by consulting geologists, Dr. Peter Huntoon and Henry Richter. These studies define the pertinent structural and groundwater geologic features in and in the vicinities of the Mortons and Green Valley Well Fields. A relatively complex structural geology was encountered in the Green Valley area. The study of the Mortons area suggests that the geology of this area is relatively uniform. Inventories of the water users in the vicinities of the two study areas are included at the back of this report in Appendix B. These inventories are comprised of water appropriations as recognized by the Wyoming State Engineer's Office. Both groundwater and surface water appropriations are inventoried within the Green Valley study area. Only groundwater appropriations are inventoried within the Mortons study area.

  16. Biological investigations of the Sandia National Laboratories Sol se Mete Aerial Cable Facility

    SciTech Connect (OSTI)

    Sullivan, R.M.

    1994-10-01T23:59:59.000Z

    This report provides results of a comprehensive biological field survey performed on the Sandia National Laboratories Aerial Cable Facility, at the east end of Kirtland Air Force Base (KAFB), Bernalillo County, New Mexico. This survey was conducted late September through October, 1991. ACF occupies a 440-acre tract of land withdrawn by the US Forest Service (USFS) for use by KAFB, and in turn placed under operational control of SNL by the Department of Energy (DOE). All land used by SNL for ACF is part of a 15,851-acre tract of land withdrawn by the US Forest Service. In addition, a number of different organizations use the 15,851-acre area. The project area used by SNL encompasses portions of approximately six sections (3,840 acres) of US Forest Service land located within the foothills of the west side of the Manzano Mountains (East Mesa). The biological study area is used by the KAFB, the US Department of Interior, and SNL. This area includes: (1) Sol se Mete Springs and Canyon, (2) East Anchor Access Road, (3) East Anchor Site, (4) Rocket Sled Track, (5) North Arena, (6) East Instrumentation Site and Access Road, (7) West Anchor Access Road, (8) West Anchor Site, (9) South Arena, (10) Winch Sites, (11) West Instrumentation Sites, (12) Explosive Assembly Building, (13) Control Building, (14) Lurance Canyon Road and vicinity. Although portions of approximately 960 acres of withdrawn US Forest Service land have been altered, only 700 acres have been disturbed by activities associated with ACF; approximately 2,880 acres consist of natural habitat. Absence of grazing by livestock and possibly native ungulates, and relative lack of human disturbance have allowed this area to remain in a more natural vegetative state relative to the condition of private range lands throughout New Mexico. This report evaluates threatened and endangered species found on ACF, as well as a comprehensive assessment of biological habitats.

  17. Role of performance measures in reengineering U.S. Department of Energy`s management of environmental management programs

    SciTech Connect (OSTI)

    Murthy, K.S.; Harroun, W.P.

    1996-06-01T23:59:59.000Z

    The Rocky Flats Environmental Technology Site (Rocky Flats) contributed to America`s defense up to the end of the Cold War. It is one of several large US Department of Energy (DOE) nuclear industrial facilities, currently undergoing cleanup and closure. The Site was constructed in a sparsely populated area along the Rocky Mountain Foothills, near Denver, in 1952. In the 45 years since, Denver has grown to a major metropolitan area. Over 2 million people live within the Site`s 50-mile radius. The Site is directly upstream of water supplies that serve over 300,000 people. As a result, accelerated cleanup, consolidation, reuse, and closure of the Site are the current essentials. The Site has had three management and operating (M and O) contractors since inception. In keeping with the shift in the Site`s paradigm from one of weapon-parts production program to cleanup and closure project, DOE changed its contracting philosophy for the Site from the M and O type of contract to a Performance-based Incentive Fee Integrating Management contract (PBIF IMC). Doe selected the Site`s fourth contractor as an IMC contractor in July 1995. Kaiser-Hill Company L.L.C. was awarded the contract and assumed IMC responsibility for the Site on July 1, 1995. Integral to this contract is the establishment and implementation of a performance measures system. Performance measures are the bases for incentives that motivate the IMC and the subcontractors working at Rocky Flats. This paper provides an overview of Performance Measures system practiced at Rocky Flats from July 1995 to December 1995. Also described are the developments in reengineering during the July 1995--March 1996 interval.

  18. Human Health and Ecological Risk Assessment for the Operation of the Explosives Waste Treatment Facility at Site 300 of the Lawrence Livermore National Laboratory

    SciTech Connect (OSTI)

    Gallegos, G; Daniels, J; Wegrecki, A

    2007-10-01T23:59:59.000Z

    This document contains the human health and ecological risk assessment for the Resource Recovery and Conservation Act (RCRA) permit renewal for the Explosives Waste Treatment Facility (EWTF). Volume 1 is the text of the risk assessment, and Volume 2 (provided on a compact disc) is the supporting modeling data. The EWTF is operated by the Lawrence Livermore National Laboratory (LLNL) at Site 300, which is located in the foothills between the cities of Livermore and Tracy, approximately 17 miles east of Livermore and 8 miles southwest of Tracy. Figure 1 is a map of the San Francisco Bay Area, showing the location of Site 300 and other points of reference. One of the principal activities of Site 300 is to test what are known as 'high explosives' for nuclear weapons. These are the highly energetic materials that provide the force to drive fissionable material to criticality. LLNL scientists develop and test the explosives and the integrated non-nuclear components in support of the United States nuclear stockpile stewardship program as well as in support of conventional weapons and the aircraft, mining, oil exploration, and construction industries. Many Site 300 facilities are used in support of high explosives research. Some facilities are used in the chemical formulation of explosives; others are locations where explosive charges are mechanically pressed; others are locations where the materials are inspected radiographically for such defects as cracks and voids. Finally, some facilities are locations where the machined charges are assembled before they are sent to the onsite test firing facilities, and additional facilities are locations where materials are stored. Wastes generated from high-explosives research are treated by open burning (OB) and open detonation (OD). OB and OD treatments are necessary because they are the safest methods for treating explosives wastes generated at these facilities, and they eliminate the requirement for further handling and transportation that would be required if the wastes were treated off site.

  19. Evolution of the Llanos Basin and the deformation of the Eastern Cordiller, Columbia

    SciTech Connect (OSTI)

    Addison, F.; Cooper, M.; Hayward, A.; Howe, S. O'Leary, J. (BP Exploration Co. Ltd., Santafe de Bogota (Colombia))

    1993-02-01T23:59:59.000Z

    The Llanos Basin is located on the flank of the Eastern Cordillera in northeast Colombia. Basin development commenced with the deposition of a synrift Triassic and Jurassic megasequence related to the separation of North and South America in the Caribbean. Basin development continued with the Cretaceous Back Arc Megasequence deposited in a back arc basin behind the Andean subduction zone. Three major sequences can be recognized corresponding to extensional pulses in the Tithonian, Albian, and the Santonian which control thickness and facies distributions. The primary reservoir in the basin is the Late Eocene Mirandor Formation which was deposited in a fluvial system which prograded from the Guyana Shield to the west-northwest. This was deposited as part of the Pre-Andean Foreland Basin Megasequence (Bartonian to Serravallian) which developed as a result of uplift onset and deformation in the Central Cordillera. This megasequence covered the Magdalena Valley the Eastern Cordillera ad the Llanos Basin. In the foothills of the Eastern Cordillera, the Mirador Formation begins to show evidence of marine influence and was probably deposited in a series of shoreface sands and offshore bar complexes in the Cordillera. The Pre-Andean Foreland Basin Megasequence includes the Eocene-Oligocene Carbonera Formation which was deposited in a low every fluvial system that was mud dominated. Within the Carbonera Formation, a series of major, grossly coarsening upward cycles can be seen which are separated by maximum flooding surfaces that approximate to time lines. These cycles correspond to the early phases of development of the Central Cordillera with each pulse being seen as an influx of coarser clastics to the basin. The deformation style in the Eastern Cordillera is a mixture of thin-skinned thrust structures and the inversion of the thick-skinned basement involved extension faults. The inversion structures include the Cuisana field, a giant oil and gas-condensate discovery.

  20. Non-linear evolution of the cosmic neutrino background

    SciTech Connect (OSTI)

    Villaescusa-Navarro, Francisco; Viel, Matteo [INAF/Osservatorio Astronomico di Trieste, Via Tiepolo 11, 34143, Trieste (Italy); Bird, Simeon [Institute for Advanced Study, 1 Einstein Drive, Princeton, NJ, 08540 (United States); Peña-Garay, Carlos, E-mail: villaescusa@oats.inaf.it, E-mail: spb@ias.edu, E-mail: penya@ific.uv.es, E-mail: viel@oats.inaf.it [Instituto de Física Corpuscular, CSIC-UVEG, E-46071, Paterna, Valencia (Spain)

    2013-03-01T23:59:59.000Z

    We investigate the non-linear evolution of the relic cosmic neutrino background by running large box-size, high resolution N-body simulations which incorporate cold dark matter (CDM) and neutrinos as independent particle species. Our set of simulations explore the properties of neutrinos in a reference ?CDM model with total neutrino masses between 0.05-0.60 eV in cold dark matter haloes of mass 10{sup 11}?10{sup 15} h{sup ?1}M{sub s}un, over a redshift range z = 0?2. We compute the halo mass function and show that it is reasonably well fitted by the Sheth-Tormen formula, once the neutrino contribution to the total matter is removed. More importantly, we focus on the CDM and neutrino properties of the density and peculiar velocity fields in the cosmological volume, inside and in the outskirts of virialized haloes. The dynamical state of the neutrino particles depends strongly on their momentum: whereas neutrinos in the low velocity tail behave similarly to CDM particles, neutrinos in the high velocity tail are not affected by the clustering of the underlying CDM component. We find that the neutrino (linear) unperturbed momentum distribution is modified and mass and redshift dependent deviations from the expected Fermi-Dirac distribution are in place both in the cosmological volume and inside haloes. The neutrino density profiles around virialized haloes have been carefully investigated and a simple fitting formula is provided. The neutrino profile, unlike the cold dark matter one, is found to be cored with core size and central density that depend on the neutrino mass, redshift and mass of the halo, for halos of masses larger than ? 10{sup 13.5}h{sup ?1}M{sub s}un. For lower masses the neutrino profile is best fitted by a simple power-law relation in the range probed by the simulations. The results we obtain are numerically converged in terms of neutrino profiles at the 10% level for scales above ? 200 h{sup ?1}kpc at z = 0, and are stable with respect to box-size and starting redshift of the simulation. Our findings are particularly important in view of upcoming large-scale structure surveys, like Euclid, that are expected to probe the non-linear regime at the percent level with lensing and clustering observations.

  1. Measuring the neutrino mass from future wide galaxy cluster catalogues

    SciTech Connect (OSTI)

    Carbone, Carmelita; Moscardini, Lauro; Cimatti, Andrea [Dipartimento di Astronomia, Alma Mater Studiorum-Università di Bologna, via Ranzani 1, I-40127 Bologna (Italy); Fedeli, Cosimo, E-mail: carmelita.carbone@unibo.it, E-mail: cosimo.fedeli@astro.ufl.edu, E-mail: lauro.moscardini@unibo.it, E-mail: a.cimatti@unibo.it [Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611 (United States)

    2012-03-01T23:59:59.000Z

    We present forecast errors on a wide range of cosmological parameters obtained from a photometric cluster catalogue of a future wide-field Euclid-like survey. We focus in particular on the total neutrino mass as constrained by a combination of the galaxy cluster number counts and correlation function. For the latter we consider only the shape information and the Baryon Acoustic Oscillations (BAO), while marginalising over the spectral amplitude and the redshift space distortions. In addition to the cosmological parameters of the standard ?CDM+? model we also consider a non-vanishing curvature, and two parameters describing a redshift evolution for the dark energy equation of state. For completeness, we also marginalise over a set of ''nuisance'' parameters, representing the uncertainties on the cluster mass determination. We find that combining cluster counts with power spectrum information greatly improves the constraining power of each probe taken individually, with errors on cosmological parameters being reduced by up to an order of magnitude. In particular, the best improvements are for the parameters defining the dynamical evolution of dark energy, where cluster counts break degeneracies. Moreover, the resulting error on neutrino mass is at the level of ?(M{sub ?}) ? 0.9 eV, comparable with that derived from present Ly? forest measurements and Cosmic Microwave background (CMB) data in the framework of a non-flat Universe. Further adopting Planck priors and reducing the number of free parameters to a ?CDM+? cosmology allows to place constraints on the total neutrino mass of ?(M{sub ?}) ? 0.08 eV, close to the lower bound enforced by neutrino oscillation experiments. Finally, in the optimistic case where uncertainties in the calibration of the mass-observable relation were so small to be neglected, the combination of Planck priors with cluster counts and power spectrum would constrain the total neutrino mass down to ?(M{sub ?}) ? 0.034 eV, i.e. the minimum neutrino mass predicted by oscillation experiments would be detected in a ?CDM framework. We thus show that galaxy clusters from future wide galaxy surveys will be an excellent tool for studying cosmology and fundamental physics.

  2. OPTICAL/NEAR-INFRARED SELECTION OF RED QUASI-STELLAR OBJECTS: EVIDENCE FOR STEEP EXTINCTION CURVES TOWARD GALACTIC CENTERS?

    SciTech Connect (OSTI)

    Fynbo, J. P. U.; Krogager, J.-K.; Vestergaard, M.; Geier, S. [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen O (Denmark); Venemans, B. [Max-Planck Institute for Astronomy, Koenigstuhl 17, D-69117 Heidelberg (Germany); Noterdaeme, P. [CNRS-UPMC, UMR7095, Institut d'Astrophysique de Paris, 98bis Bd. Arago, F-75014 Paris (France); Moller, P. [European Southern Observatory, Karl-Schwarzschildstrasse 2, D-85748 Garching bei Muenchen (Germany); Ledoux, C. [European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago 19 (Chile)

    2013-01-15T23:59:59.000Z

    We present the results of a search for red QSOs using a selection based on optical imaging from the Sloan Digital Sky Survey (SDSS) and near-infrared imaging from UKIDSS. Our main goal with the selection is to search for QSOs reddened by foreground dusty absorber galaxies. For a sample of 58 candidates (including 20 objects fulfilling our selection criteria that already have spectra in the SDSS), 46 (79%) are confirmed to be QSOs. The QSOs are predominantly dust-reddened except for a handful at redshifts z {approx}> 3.5. However, the dust is most likely located in the QSO host galaxies (and for two, the reddening is primarily caused by Galactic dust) rather than in the intervening absorbers. More than half of the QSOs show evidence of associated absorption (BAL absorption). Four (7%) of the candidates turned out to be late-type stars, and another four (7%) are compact galaxies. We could not identify the remaining four objects. In terms of their optical spectra, these QSOs are similar to the QSOs selected in the FIRST-2MASS Red Quasar Survey except they are on average fainter, more distant, and only two are detected in the FIRST survey. As per the usual procedure, we estimate the amount of extinction using the SDSS QSO template reddened by Small-Magellanic-Cloud-(SMC) like dust. It is possible to get a good match to the observed (rest-frame ultraviolet) spectra, but it is not possible to match the observed near-IR photometry from UKIDSS for nearly all the reddened QSOs. The most likely reasons are that the SDSS QSO template is too red at optical wavelengths due to contaminating host galaxy light and because the assumed SMC extinction curve is too shallow. Three of the compact galaxies display old stellar populations with ages of several Gyr and masses of about 10{sup 10} M{sub Sun} (based on spectral energy distribution modeling). The inferred stellar densities in these galaxies exceed 10{sup 10} M{sub Sun} kpc{sup -2}, which is among the highest measured for early-type galaxies. Our survey has demonstrated that selection of QSOs based on near-IR photometry is an efficient way to select QSOs, including reddened QSOs, with only small contamination from late-type stars and compact galaxies. This will be useful with ongoing and future wide-field near-IR surveys such as the VISTA and EUCLID surveys.

  3. Nuclear Emergency and the Atmospheric Dispersion of Nuclear Aerosols: Discussion of the Shared Nuclear Future - 13163

    SciTech Connect (OSTI)

    Rana, Mukhtar A. [Science-Admin Coherence Cell (SACC), PINSTECH Admin Blk, PAEC, Islamabad (Pakistan)] [Science-Admin Coherence Cell (SACC), PINSTECH Admin Blk, PAEC, Islamabad (Pakistan); Ali, Nawab [Physics Division, Directorate of Science, Pakistan Institute of Nuclear Science and Technology (PINSTECH), P.O. Nilore, Islamabad (Pakistan)] [Physics Division, Directorate of Science, Pakistan Institute of Nuclear Science and Technology (PINSTECH), P.O. Nilore, Islamabad (Pakistan); Akhter, Parveen [Pakistan Institute of Engineering and Applied Sciences (PIEAS), Islamabad (Pakistan)] [Pakistan Institute of Engineering and Applied Sciences (PIEAS), Islamabad (Pakistan); Khan, E.U. [Department of Physics, International Islamic University (IIU), Kettle Fields, Kashmir Highways, Islamabad (Pakistan)] [Department of Physics, International Islamic University (IIU), Kettle Fields, Kashmir Highways, Islamabad (Pakistan); Mathieson, John [International Relations, Nuclear Decommissioning Authority (NDA), Building 587, Curie Avenue, Harwell, Didcot, Oxon, OX11 0RH (United Kingdom)] [International Relations, Nuclear Decommissioning Authority (NDA), Building 587, Curie Avenue, Harwell, Didcot, Oxon, OX11 0RH (United Kingdom)

    2013-07-01T23:59:59.000Z

    This paper has a twofold objective. One is to analyze the current status of high-level nuclear waste disposal along with presentation of practical perspectives about the environmental issues involved. Present disposal designs and concepts are analyzed on a scientific basis and modifications to existing designs are proposed from the perspective of environmental safety. Other is to understand the aerosol formation in the atmosphere for the case of the leakage from the nuclear waste containers or a nuclear accident. Radio-nuclides released from the waste will attach themselves to the existing aerosols in the atmosphere along with formation of new aerosols. Anticipating the nuclear accident when a variety of radioactive aerosols will form and exist in the atmosphere, as a simple example, measurement of naturally existing radioactive aerosols are made in the atmosphere of Islamabad and Murree. A comparison with similar measurements in 3 cities of France is provided. Measurement of radionuclides in the atmosphere, their attachment to aerosols and follow up transport mechanisms are key issues in the nuclear safety. It is studied here how {sup 7}Be concentration in the atmospheric air varies in the capital city of Islamabad and a Himalaya foothill city of Murree (Pakistan). Present results are compared with recent related published results to produce a {sup 7}Be concentration versus altitude plot up to an altitude of 4000 m (a.s.l.). Origin and variance of {sup 7}Be concentration at different altitudes is discussed in detail. The relevance of results presented here with the evaluation of implications of Chernobyl and Fukushima nuclear disasters has been discussed in a conclusive manner. It is the first international report of a joint collaboration/project. The project is being generalized to investigate and formulate a smooth waste storage and disposal policy. The project will address the fission and fusion waste reduction, its storage, its recycling, air, water and soil quality monitoring, and the final disposal with the major foci of dealing with related chemical, biogical, physical, geophysical, engineering, management and administration aspects. (authors)

  4. The Common Occurrence of Highly Supercooled Drizzle and Rain near the Coastal Regions of the Western United States

    SciTech Connect (OSTI)

    Rosenfeld, Daniel; Chemke, Rei; DeMott, Paul J.; Sullivan, Ryan C.; Rasmussen, R M.; McDonough, Frank; Comstock, Jennifer M.; Schmid, Beat; Tomlinson, Jason M.; Jonsson, Haf; Suski, Kaitlyn; Cazorla, Alberto; Prather, Kimberly

    2013-09-05T23:59:59.000Z

    The formation of highly supercooled rain was documented by aircraft observations in clouds at a wide range of conditions near the coastal region of the western United States. Several case studies are described in detail using combined cloud and aerosol measurements to document both the highly super-cooled condition and the relatively pristine aerosol conditions under which it forms. The case studies include: (1) Marine convective clouds over the coastal waters of northern California, as measured by cloud physics probes flown on a Gulfstream-1 aircraft during the CALWATER campaign in February and early March 2011. The clouds had extensive drizzle in their tops, which extended downward to the 0°C isotherm as supercooled rain. Ice multiplication was observed only in mature parts of the clouds where cloud water was already depleted. (2) Orographically triggered convective clouds in marine air mass over the foothills of the Sierra Nevada to the east of Sacramento, as measured in CALWATER. Supercooled rain was observed down to -21°C. No indications for ice multiplication were evident. (3) Orographic layer clouds over Yosemite National Park, also measured in CALWATER. The clouds had extensive drizzle at -21°C, which intensified with little freezing lower in the cloud, and (4) Supercooled drizzle drops in layer clouds near Juneau, Alaska, as measured by the Wyoming King Air as part of a FAA project to study aircraft icing in this region. Low concentrations of CCN was a common observation in all these clouds, allowing for the formation of clouds with small concentration of large drops that coalesced into supercooled drizzle and raindrops. Another common observation was the absence of ice nuclei and/or ice crystals in measurable concentrations was associated with the persistent supercooled drizzle and rain. Average ice crystal concentrations were 0.007 l-1 at the top of convective clouds at -12°C and 0.03 l-1 in the case of layer clouds at -21°C. In combination these two conditions provide ideal conditions for the formation of highly supercooled drizzle and rain. These results help explain the anomalously high incidences of aircraft icing at cold temperatures in U.S. west coast clouds (Bernstein et al., 2004) and highlight the need to include aerosol effects when simulating aircraft icing with cloud models. These case studies can also serve as benchmarks for explicit cloud microphysics models attempting to simulate the formation of precipitation in these types of pristine conditions.

  5. Producing Light Oil from a Frozen Reservoir: Reservoir and Fluid Characterization of Umiat Field, National Petroleum Reserve, Alaska

    SciTech Connect (OSTI)

    Hanks, Catherine

    2012-12-31T23:59:59.000Z

    Umiat oil field is a light oil in a shallow, frozen reservoir in the Brooks Range foothills of northern Alaska with estimated oil-in-place of over 1 billion barrels. Umiat field was discovered in the 1940’s but was never considered viable because it is shallow, in the permafrost, and far from any transportation infrastructure. The advent of modern drilling and production techniques has made Umiat and similar fields in northern Alaska attractive exploration and production targets. Since 2008 UAF has been working with Renaissance Alaska Inc. and, more recently, Linc Energy, to develop a more robust reservoir model that can be combined with rock and fluid property data to simulate potential production techniques. This work will be used to by Linc Energy as they prepare to drill up to 5 horizontal wells during the 2012-2013 drilling season. This new work identified three potential reservoir horizons within the Cretaceous Nanushuk Formation: the Upper and Lower Grandstand sands, and the overlying Ninuluk sand, with the Lower Grandstand considered the primary target. Seals are provided by thick interlayered shales. Reserve estimates for the Lower Grandstand alone range from 739 million barrels to 2437 million barrels, with an average of 1527 million bbls. Reservoir simulations predict that cold gas injection from a wagon-wheel pattern of multilateral injectors and producers located on 5 drill sites on the crest of the structure will yield 12-15% recovery, with actual recovery depending upon the injection pressure used, the actual Kv/Kh encountered, and other geologic factors. Key to understanding the flow behavior of the Umiat reservoir is determining the permeability structure of the sands. Sandstones of the Cretaceous Nanushuk Formation consist of mixed shoreface and deltaic sandstones and mudstones. A core-based study of the sedimentary facies of these sands combined with outcrop observations identified six distinct facies associations with distinctive permeability trends. The Lower Grandstand sand consists of two coarsening-upward shoreface sands sequences while the Upper Grandstand consists of a single coarsening-upward shoreface sand. Each of the shoreface sands shows a distinctive permeability profile with high horizontal permeability at the top getting progressively poorer towards the base of the sand. In contrast, deltaic sandstones in the overlying Ninuluk are more permeable at the base of the sands, with decreasing permeability towards the sand top. These trends impart a strong permeability anisotropy to the reservoir and are being incorporated into the reservoir model. These observations also suggest that horizontal wells should target the upper part of the major sands. Natural fractures may superimpose another permeability pattern on the Umiat reservoir that need to be accounted for in both the simulation and in drilling. Examination of legacy core from Umiat field indicate that fractures are present in the subsurface, but don't provide information on their orientation and density. Nearby surface exposures of folds in similar stratigraphy indicate there are at least three possible fracture sets: an early, N/S striking set that may predate folding and two sets possibly related to folding: an EW striking set of extension fractures that are parallel to the fold axes and a set of conjugate shear fractures oriented NE and NW. Analysis of fracture spacing suggests that these natural fractures are fairly widely spaced (25-59 cm depending upon the fracture set), but could provide improved reservoir permeability in horizontal legs drilled perpendicular to the open fracture set. The phase behavior of the Umiat fluid needed to be well understood in order for the reservoir simulation to be accurate. However, only a small amount of Umiat oil was available; this oil was collected in the 1940’s and was severely weathered. The composition of this ‘dead’ Umiat fluid was characterized by gas chromatography. This analysis was then compared to theoretical Umiat composition derived using the Pedersen method with original Umiat

  6. Final Technical Report: Intensive Quenching Technology for Heat Treating and Forging Industries

    SciTech Connect (OSTI)

    Aronov, Michael A.

    2005-12-21T23:59:59.000Z

    Intensive quenching (IQ) process is an alternative way of hardening (quenching) steel parts through the use of highly agitated water and then still air. It was developed by IQ Technologies, Inc. (IQT) of Akron, Ohio. While conventional quenching is usually performed in environmentally unfriendly oil or water/polymer solutions, the IQ process uses highly agitated environmentally friendly water or low concentration water/mineral salt solutions. The IQ method is characterized by extremely high cooling rates of steel parts. In contrast to conventional quenching, where parts cool down to the quenchant temperature and usually have tensile or neutral residual surface stresses at the end of quenching. The IQ process is interrupted when the part core is still hot and when there are maximum compressive stresses deep into the parts, thereby providing hard, ductile, better wear resistant parts. The project goal was to advance the patented IQ process from feasibility to commercialization in the heat-treating and forging industries to reduce significantly energy consumption and environmental impact, to increase productivity and to enhance economic competitiveness of these industries as well as Steel, Metal Casting and Mining industries. To introduce successfully the IQ technology in the U.S. metal working industry, the project team has completed the following work over the course of this project: A total of 33 manufacturers of steel products provided steel parts for IQ trails. IQT conducted IQ demonstrations for 34 different steel parts. Our customers tested intensively quenched parts in actual field conditions to evaluate the product service life and performance improvement. The data obtained from the field showed the following: Service life (number of holes punched) of cold-work punches (provided by EHT customer and made of S5 shock-resisting steel) was improved by two to eight times. Aluminum extrusion dies provided by GAM and made of hot work H-13 steel outperformed the standard dies by at least 50%. Dies provided by an AST customer, made of plain carbon 1045 steel and used for pellet manufacturing outperformed the standard dies by more than 100%. Concrete crusher liner wear plates provided by an EHT customer and made of 1045 steel, had the same surface hardness as the plates made of more expensive, pre-hardened high alloy HARDOX-500 material supplied by a Swedish company and used currently by the EHT customer. The 1045 material intensively quenched wear plates are currently in the field. Concrete block molding machine wear plates provided by an IQT customer and made of 8620 steel were processed at the AST production IQ system using a 40% reduced carburization cycle. An effective case depth in the intensively quenched wear plates was the same as in the standard, oil quenched parts. Base keys provided by an EHT customer and made of 8620 steel were processed using a 40% reduced carburization cycle. The intensively quenched parts showed the same performance as standard parts. IQT introduced the IQ process in heat treat practices of three commercial heat-treating shops: Akron Steel Treating Co., Summit Heat Treating Co. and Euclid Heat Treating Co. CWRU conducted a material characterization study for a variety of steels to develop a database to support changing/modification of recognized standards for quenching steel parts. IQT conducted a series of IQ workshops, published seven technical papers and participated in ASM Heat Treating Society conference and exposition and in Furnace North America Show. IQT designed and built a fully automated new IQ system installed at the Center for Intensive Quenching. This system includes the following major components: a stand-alone 1,900-gallon IQ water system, a 24'' x 24'' atmosphere pit furnace, and an automated load transfer mechanism. IQT established a ''Center for Intensive Quenching'' at the AST facilities. The 4,000 square feet Center includes the following equipment: High-velocity single part quenching IQ unit developed and built previously under EMTEC CT-65 project. The unit is equipped w