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    U

    Universities Research Association

    院校EST. 1965
    62论文总数
    1,341引用总数

    The Universities Research Association is a non-profit association of more than 90 research universities, primarily but not exclusively in the United States. It was founded in 1965 at the behest of the President's Science Advisory Committee and the National Academy of Sciences to build and operate Fermilab, a National Accelerator Laboratory. Today, the mission of URA is "[t]o establish and operate in the national interest unique laboratories and facilities for research, development, and education in the physical and biological sciences to expand the frontiers of knowledge, foster innovation, and promote the education of future generations of scientists.

    论文量&引用量时间轴

    机构学者

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    Gilles Tran
    Gilles Tran
    Association Francaise de Zootechnie
    论文:8引用:0H-index:0
    Valerie Heuze
    Valerie Heuze
    AgroParisTech
    论文:8引用:0H-index:0
    Francois Lebas
    Francois Lebas
    French National Institute for Agriculture, Food, and Environment (INRAE)
    论文:8引用:0H-index:0
    R. Delagarde
    R. Delagarde
    Institut Agro, INRAE
    论文:6引用:0H-index:0
    Michel Lessire
    Michel Lessire
    ITAVI
    论文:4引用:0H-index:0
    Ira Harkavy
    Ira Harkavy
    Center for Community Partnerships, University of Pennsylvania
    论文:2引用:0H-index:0
    A.J. Elwyn
    A.J. Elwyn
    Fermi National Accelerator Laboratory, Universities Research Association
    论文:2引用:0H-index:0
    F. T. Cole
    F. T. Cole
    FERMI NATL ACCELERATOR LAB
    论文:2引用:0H-index:0
    J. D. Cossairt
    J. D. Cossairt
    Fermi National Accelerator Laboratory
    论文:2引用:0H-index:0

    论文(62)

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    排序
    1Kampung Warna Warni in Kuala Perlis: Empowering the Concept of Community-Based Tourism (CBT) in Rural Area, Perlis, Malaysia
    Mohd Hasfarisham Abd Halim,Mokhtar Saidin
    2025Local Development &amp Society(2025)
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    2Higher Education's Response to the Covid-19 Pandemic - Building a More Sustainable and Democratic Future
    Tony Gallagher, Sjur Bergan,Ira Harkavy,Ronaldo Munck, Hilligje van’t Land
    2021引用:11
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    3MID 2021 Congress Committee
    Christian Göth, Mechatronic Gmbh, Ger Kg, S Landvogt, Martin Barth
    2021
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    4HE Must Help Build a More Sustainable, Democratic Future
    Tony Gallagher, Sjur Bergen,Ira Harkavy,Ronaldo Munck, Hilligje van’t Land
    2021
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    5A Database of Geometric Albedo Spectra for Rocky Exoplanets
    Adam J. R. W. Smith,Avi M. Mandell,Gerónimo Villanueva

    Here we present a database of albedo spectra for rocky, Earth-sized and Earth-mass exoplanets, as computed with the NASA Planetary Spectrum Generator tool (psg.gsfc.nasa.gov; Villanueva et al. 2018). The database is presented in two Python .pickle files containing pandas DataFrame objects. The DataFrame index values are wavelength, in micrometers; while the column name values contain the encoded parameters represented in the model object's albedo spectra contained with in that column. Each cell then gives the calculated geometric albedo value for the column-named model planet at the row-indicated wavelength. Two files are presented. One contains models with clouds; one contains models without clouds. To decode the column names, using a Python string.format function. For cloudy models, the format is: ColName='{}{}H2{}_R1.0g9.8P{}A{}r10l{}ct{}f0.1'.format(Cdom,Cmix,H2mix,P0,As,Mcld,Ctop) For cloud-free models, the final two parameters are not used. Thus, the correct format is: ColName='{}{}H2{}_R1.0g9.8P{}A{}'.format(Cdom,Cmix,H2mix,P0,As) Here, the parameters are as follows: Cdom: The name of the dominant absorbing chemical in the atmosphere. Accepted values are H2O, CH4, CO2, SO2, and O2. Cmix: The log10 of the mixing value of the dominant chemical in the atmosphere. Accepted values are [-7.0,-6.0,-5.0,-4.0,-3.0,-2.0,-1.0,-0.01]. H2mix: The mixing ratio of molecular hydrogen in the (otherwise) N2 background gas. Expressed as H2/(H2+N2). Accepted values are [0.0,0.02,0.05,0.15,0.5]. P0: The surface pressure of the planet, in log10(bars). Accepted values are [-1.0,-0.5,0.0,0.5,1.0,1.5,2.0] As: The grey, geometric albedo value of the surface of the planet. Accepted values are [0.05,0.2,0.35,0.5] Mcld: The linear cloud mass of cloud matter in the atmosphere, in log10(kg/m^2). Accepted values are [-3.0,-2.5,-2.0,-1.5,-1.0]. Ctop: The pressure at the top layer of the clouds. Acceptable values are [-2.0,-1.5,-1.0,-0.5,0.0,0.5,1.0]. Note that Ctop<P0 for all models. Thus, an atmosphere with a pure N2 background gas and a 0.3% H2O mixing ratio, with 1 bar of surface pressure, 0.05 surface albedo, and 1 gram of cloud matter topping at 0.316 bars altitude would be named: H2O-3.0H20.0_R1.0g9.8P0.0A0.05r10l-3.0ct-0.5f0.1 The database is described in Smith et al. (in review).

    2020
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    合作机构(35)

    美国能源部合作论文 10
    Association Française de Chirurgie合作论文 8
    European Council,European Union合作论文 2
    宾夕法尼亚大学合作论文 2
    都柏林城市大学合作论文 2
    欧洲同步辐射设施合作论文 1
    European Southern Observatory合作论文 1
    爱荷华州立大学合作论文 1
    Unité de Virologie et Immunologie Moléculaires,Centre Île-de-France - Jouy-en-Josas - Antony,National Research Institute for Agriculture, Food and Environment合作论文 1
    Nordic Optical Telescope Scientific Association合作论文 1

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