RENATER2 Computer, Information Sciences Bandwidth Challenge from the Low-Lands The Netherlands, USA, Canada, CERN, France, Italy, Japan, UK Participating remote sites each have one or more UNIX hosts running Iperf and BBFTP servers: Asia Pacific Advanced Network (APAN) consortium, KEK High Energy Accelerator Research Organization, The Institute of Physical and Chemical Research (RIKEN)/ RIKEN Accelerator Research Facility (RARF), Japan; Argonne National Laboratory (ANL), Brookhaven National Laboratory (BNL), California Institute of Technology (Caltech), ESnet, Fermi National Accelerator Lab (Fermilab), NASA Goddard Space Flight Center (GSFC), Internet2, Thomas Jefferson National Accelerator Facility (JLab), Los Alamos National Laboratory (LANL), Lawrence Berkeley National Laboratory (LBNL), LBNL National Energy Research Scientific Computing Center (NERSC), Oak Ridge National Laboratory (ORNL), Rice University, San Diego Supercomputer Center at the University of California San Diego, Stanford Linear Accelerator Center (SLAC), Stanford University, Sun Microsystems, University of Delaware, University of Florida, University of Michigan, University of Texas at Dallas, University of Wisconsin/Madison, USA; CERN, Switzerland; Daresbury Laboratory, Manchester University, Rutherford Appleton Laboratory (RAL)/Oxford, University College London, UK; Institut National de Physique Nucléaire et de Physique des Particules (IN2P3), France; Istituto Nazionale di Fisica Nucleare (INFN) Milan INFN, Rome, Italy; NIKHEF, The Netherlands; TRIUMF, Canada European DataGrid Lead: CERN, European Organization for Nuclear Research, five main, fifteen associated partners European research agencies: European Space Agency (ESA); Centre National de la Recherche Scientifique (CNRS), France; Istituto Nazionale di Fisica Nucleare (INFN), Italy; National Institute for Nuclear Physics and High Energy Physics (NIKHEF), Holland; Particle Physics and Astronomy Research Council (PPARC), UK Associated partners: Czech Republic, Finland, France, Germany, Hungary, Italy, the Netherlands, Spain, Sweden and the United Kingdom iMAGIS--Models, Algorithms, Geometry for Graphics and Image Synthesis INRIA (Grenoble), France; Massachusetts Institute of Technology, USA; Cornell University, USA; Stanford University, USA; University of Toronto, Canada; Université de Montréal, Canada; Universitat de Girona, Spain; Erlangen-Nürnberg Universität, Germany Image/Video Transmission, Storage and Manipulation of 3D images LIMSI-CNRS, France; Beckman Institute for Advanced Science and Technology, University of Illinois at Urbana-Champaign, USA Kites Flying In and Out of Space USA, Canada, France, Japan, The Netherlands and Singapore Independent artist of France, visiting artist at Mountain Lake Workshop, Virginia Tech Foundation, National Center for Supercomputing Applications University of Illinoia at Urbana-Champaign (NCSA/UIUC), Virginia Tech, School of the Arts, Virginia Polytechnic Institute & State University, Electronic Visualization Laboratory (EVL) at the University of Illinois at Chicago (UIC), USA; SARA Computing and Networking Services, The Netherlands; Sorbonne and La Cite Museum de Musique Paris, France; Virtual Reality Development and Research Laboratory, Tohwa University, Japan; Institute of High Performance Computing, Singapore; New Media Innovation Center, Vancouver, British Columbia, Canada ReMaP--Regularity and Massive Parallelism Ecole Normale Superieure de Lyon (LIP), France; Innovative Computing Laboratory, University of Tennessee, USA Video IBPster USA, France, Germany and Italy Logistical Computing and Internetworking (LoCI) Lab at the University of Tennessee (UTENN), Innovative Computing Lab (UTENN), University of California Santa Barbara, University of California San Diego, USA; ENS Lyon, France; Università del Piemonte Orientale Alessandria, Italy; High Performance Computing Center Rechenzentrum Universität Stuttgart, Germany Geosciences Earth Observing System (EOS) NASA, USA; worldwide collaborators; Euro-Link NRN-linked institutions in Denmark, Finland, France, Norway, Sweden Indian Ocean Experiment (INDOEX) LMD (IPSL, Ecole Polytechnqiue-Palaiseau), France; Center for Clouds, Chemistry and Climate, SCRIPPS Institution for Oceanography, University of California, San Diego, USA The SEAWIFS Project Worldwide collaborators: based at NASA's Goddard Space Flight Center, USA US/France collaborators: LSCE (Laboratoire des Sciences du Climat et de l'Environnement, CEA Saclay), France; Rosenstiel School of Marine and Atmospheric Science (RSMAS), University of Miami, USA Math, Physical Sciences Accélération de Particules par Ondes de Choc Institut Astrophysique de Paris (IAP), France; North Carolina State University (Raleigh), USA Development of hydrodynamic models for the acceleration of particles in Supernovae remains CASSINI-HUYGENS Cluster II WBD (The Wide-band Plasma Wave Investigation) University of Iowa (Iowa City), USA; University of Minnesota, USA; Goddard Space Flight Center, USA; Observatoire de Paris, France; Centre de Recherches en Physique de L'Environnement Terrestre et Planetaire (CETP), France; University of Sheffield, UK; Austrian Academy of Science Space Research Institute, Austria; Swedish Institute of Space Physics, Sweden; European Space Research and Technology Centre (ESTEC), Netherlands CASSINI-HUYGENS Cluster II WEC (The Wave Experiment Consortium) Consortium of numerous institutions worldwide French-USA members collaborating via STAR TAP: Centre de Recherches en Physique de L'Environnement Terrestre et Planetaire (CETP), France; University of Berkeley Space Science Laboratory, USA; University of Iowa (Iowa City), USA CASSINI-HUYGENS Descent Imager/Spectral Radiometer (DISR) University of Arizona Lunar and Planetary Laboratory, USA; U.S. Geological Survey, USA; NASA Jet Propulsion Laboratory, USA; Observatoire de Paris Meudon, France; Laboratory of Glaciology and Geophysics of Grenoble, France; Technical University of Bruanschweig, Germany; Max Planck Institute for Aeronomy in Lindau, Germany CASSINI-VIMS (Visual and Infrared Mapping Spectrometer) Lunar and Planetary Lab, University of Arizona, USA; NASA Ames Research Center, USA; Jet Propulsion Laboratory (NASA), CalTech, USA; Cornell University, USA; US Geological Survey, Denver, USA; University of Arizona (Tucson), USA; SOEST, University of Hawaii, USA; Institut d'Astrophysique Spatiale, France; CNRS, France; DESPA/Observatoire de Meudon, France; Observatoire de Paris, Meudon, France; Instituto di Astrophysica Spaziale, CNR/IRSI, Italy; Instituto di Fisica, Italy; Agenzia Spatiale Italiana, Italy; Institut fur Planetenerkundung, DLR, Germany Catalog of Beryllium Stars Institut Astrophysique de Paris (IAP), France; Limber Observatory (Pipe Creek, Texas), USA CLIMSERV-CDC (une activité de service effectuée par l'IPSL) LMD (IPSL, Ecole Polytechnqiue-Palaiseau), France; EOSDIS/LARC, NASA Langley Atmospheric Sciences Data Center (Virginia), USA Data transfers from the EOSDIS database to the French database CLIMSERV Détection des Etoiles Doubles par Haute Résolution Angulaire Institut Astrophysique de Paris (IAP), France; Center for High Angular Resolution Astronomy, Georgia State University, USA Detection of binary stars Detection of Internally Reflected Cherenov light (DIRC), Particle Identification for BaBar Based at Stanford Linear Accelerator Center (SLAC), University of Stanford, USA Participating French institutions: Commissariat a l'Energie Atomic (CEA); DAPNIA-Saclay; Laboratoire de L'Accelerateur Lineaire (LAL), Orsay; LPNHE Paris VI et Paris VII; LPNHE de l'Ecole Polytechnique Participating US institutions: Lawrence Berkeley National Laboratory, University of California at Berkeley; Rutgers University; University of California at Santa Barbara; University of Cincinnati The DØ Experiment Worldwide collaborators: based at Fermilab, USA: US collaborators: Brookhaven National Laboratory; USA; Cornell University, USA; Lawrence Berkeley Laboratory, USA; Stanford Linear Accelerator Center, USA French collaborators: DAPNIA/SPP, Saclay; Centre de Physique des Particules, Marseille; Institut des Sciences Nucleaires, Grenoble; LPNHE, Universites Paris VI and VII; Laboratoire de L'Accelerateur Lineaire (LAL), Orsay Other collaborators: CERN, Switzerland; DESY, Germany; KEK, Japan ELDORA (ELectra DOppler RAdar) National Center for Atmospheric Research (NCAR), USA; Centre de Recherches en Physique de L'Environnement Terrestre et Planetaire (CETP), France Etude d'Amas de Galaxies en Ultraviolet Institut Astrophysique de Paris (IAP), France; University of Alabama (Huntsville), USA Analysis of observations of galaxy clusters with the EUVE satellite Etude de l'Amas ZWICKY 3146 Institut Astrophysique de Paris (IAP), France; Harvard-Smithsonian Center for Astrophysics (CfA), USA Studies of properties of clusters observed with X telescopes Etude des Disques de Gaz Institut Astrophysique de Paris (IAP), France; Yerkes Observatory, University of Chicago, USA Study of gaz disks around young planetary systems such as Beta Pictoris Etude des Effets de la Poussière dans les Galaxies Institut Astrophysique de Paris (IAP), France; Space Telescope Science Institute (STSCI), Baltimore, USA Theoretical prediction of observations with new telescopes in the infrared Etude Théorique et Expérimentale des Profils de Raies Institut Astrophysique de Paris (IAP), France; University of Louisville, USA Theoretical computation of ray profiles and comparison with experimental spectra Fluctuations de Brillance de Surface Institut Astrophysique de Paris (IAP), France; University of California at Berkeley, USA Theoretical predictions and observations of signal fluctuations in infrared imaging of galaxies FUSE (Far Ultraviolet Spectroscopic Explorer) The Johns Hopkins University, USA; The University of Colorado at Boulder, USA; The University of California at Berkeley, USA; Goddard Space Flight Center (NASA), USA; Canadian Space Agency (CSA), Canada; French Space Agency (Centre National d'Etudes Spatiales), France; Institut Astrophysique de Paris (IAP), France GALILEO Galileo worldwide collaborators US/France collaborators CETP (IPSL, Vélizy), France; University of Iowa (Iowa City), US GALILEO/NIMS Department of Space Research (DESPA)/Observatoire de Paris Meudon, France; NASA Jet Propulsion Laboratory (Pasadena), USA< Infrared spectro-imagery of Jupiter with the GALILEO spacecraft HESSI The High Energy Solar Spectroscopic Imager Goddard Space Flight Center (NASA), USA; University of Berkeley Space Science Laboratory, USA; Montana State University, USA; University of Alabama at Huntsville, USA; Lawrence Berkeley National Laboratory, USA; National Oceanic and Atmospheric Administration (NOAA), USA; Observatoire de Paris Meudon, France; ETHZ, Switzerland; Paul Scherrer Institute, Switzerland; University of Glasgow, Scotland;University of Tokyo, Japan; DelftU, The Netherlands Hubble Space Telescope Worldwide collaborators US/France collaborators: Institut Astrophysique de Paris (IAP), France; Space Telescope Science Institute (STSCI), Baltimore, USA IRON Worldwide Collaborators French-US collaborators: Observatoire de Paris Meudon, France; Ohio State University, USA Large Scale Structure and Cluster Formation Institut Astrophysique de Paris (IAP), France; Harvard-Smithsonian Center for Astrophysics (CfA), USA Long-term NASA project: Combined analysis in optical, X-ray and radio LIC (Local Interstellar Cloud) Study Institut Astrophysique de Paris (IAP), France; LPL-WEST (Tucson, Arizona), USA Minor Planet Ephemeris Service Institut Astrophysique de Paris (IAP), France; Smithsonian Astrophysical Observatory (Massachusetts), USA Modèles de Formation d'Etoiles avec Vent Galactique Institut Astrophysique de Paris (IAP), France; University of Illinois at Urbana-Champaign, USA Models for formation and evolution of galaxies with loss of mass. Consequences for the chemical evolution of elements D, He, O, Fe and others Nucléosynthèse du Big Bang dans le Modèle Cosmologique Standard Institut Astrophysique de Paris (IAP), France; Theoretical Physics Institute School of Physics and Astronomy, University of Minnesota, USA Development of a model for the primordial nucleosynthesis. Study of cosmologic parameters and comparison with observational constraints Observation of Lithium, Beryllium and Bore elements in Halo Stars, and Development of Astrophysical Models Detailing their Chemical Evolution in the Galaxy Institut Astrophysique de Paris (IAP), France; University of Chicago, USA SLOAN Digital Sky Survey Institut Astrophysique de Paris (IAP), France; Johns Hopkins University, USA Surveys Radio Institut Astrophysique de Paris (IAP); National Radio Astronomy Organization (NRAO), Virginia, USA Properties of deep radio surveys TERAPIX (Traitement Elementaire Reduction et Analyse des PIXels) Centre National de la Recherche Scientifique (CNRS), France; University of Hawaii, USA; National Research Council Canada, Canada Theoretical Computation Dealing with Distribution of Gaseous Components of Circumstellar Shells Institut Astrophysique de Paris (IAP), France; University of Chicago, USA
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