'Science drivers' diaporamas de présentation

NIFS Science Drivers

NIFS Science Drivers. Science Drivers. Massive black holes. R ~ 3000-5000 AGN in nearby galaxies. R ~ 3000 Low mass stars. R ~ 1000 Compact star clusters. R ~ 2000 YSO jet mechanisms. R ~ 3000-6000 YSO/cloud interactions. R ~ 6000 Proto/planetary nebulae. R ~ 6000

907 views • 78 slides

Next Generation Adaptive Optics (NGAO) System Design Phase Update

Next Generation Adaptive Optics (NGAO) System Design Phase Update. Peter Wizinowich, Rich Dekany, Don Gavel, Claire Max Science Case Presenters: Brian Cameron, David Law, Jessica Lu, Phil Marshall, Chuck Steidel, Tommaso Treu Technical Team: Sean Adkins, Brian Bauman, Jim Bell,

539 views • 37 slides

Giant Magellan Telescope Project Science Drivers & AO Requirements

Giant Magellan Telescope Project Science Drivers & AO Requirements. Patrick McCarthy - GMT Director Phil Hinz & Michael Hart - GMT AO Team. AO4ELT - June 22, 2009. The GMT Partners. US Institutions Carnegie Institution Harvard University Smithsonian Institution Texas A&M University

525 views • 37 slides

NEON: Where We Are Today (And How We Got There) Jeffrey Goldman Science Office Director,

NEON: Where We Are Today (And How We Got There) Jeffrey Goldman Science Office Director, American Institute of Biological Sciences. Interacting Drivers of Biological Change. Evolution of infectious disease. Land use & habitat alteration. Biodiversity Species composition

415 views • 33 slides

Status of design requirements for the European ELT

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Institute for Sustainable Earth and Environmental Software ISEES

Institute for Sustainable Earth and Environmental Software ISEES. Matthew B. Jones National Center for Ecological Analysis and Synthesis (NCEAS) University of California Santa Barbara ISEES Science Drivers Workshop March 11-12, 2013. Science and Synthesis.

248 views • 17 slides

The Fusion Simulation Program

The Fusion Simulation Program. presented at the SWIM meeting on October 28, 2010 JR Cary Tech-X on behalf of the FSP Team Terminology The Fusion Simulation Program is expected to start in FY12 We are currently in the FSP Definition Project What will FSP be? How will it be run?.

297 views • 16 slides

The Millimetre-Wave Astronomy White Paper

The Millimetre-Wave Astronomy White Paper. Michael Burton UNSW. What place for millimetre-wave in Australian radio astronomy for the next decade?. ALMA 2012? SKA 2020?. Maintaining the vitality of the astronomical community till SKA. Australian MM-Wave Facilities.

302 views • 16 slides

Europlanet RI A network for all planetary scientists A service to the community

Europlanet RI A network for all planetary scientists A service to the community. Manuel Grande Scientific Dissemination Coordinator. A unique opportunity!. Provide support to the optimal use of data from past and present space missions by the broadest possible science community

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The Future of AO at Keck

The Future of AO at Keck. Sept 2004 Mike Brown, for the AOWG and Keck AO team. Your friendly AOWG. Mike Brown, Mark Colavita, Rich Dekany, Andrea Ghez, James Larkin, Mike Liu, Bruce MacIntosh, Keith Matthews, Claire Max, Mitch Troy

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Welcome to the WATER HM Barcelona Meeting

Welcome to the WATER HM Barcelona Meeting. Attending Today: Doug Alsdorf (OSU) Shannon Brown (JPL) Anny Cazenave (CNES) Diane Evans (JPL) Daniel Fernandez (JPL) Lee Fu (JPL) Juliette Lambin (CNES) Yves Menard (CNES) Nelly Mognard (CNES) Baptiste Mourre (ICM) Ernesto Rodriguez (JPL)

257 views • 13 slides

Summary of the Paris SKA Meeting 4-8 September 2006 R. T. Schilizzi

Summary of the Paris SKA Meeting 4-8 September 2006 R. T. Schilizzi. Main issues for the SKA project. science drivers engineering solutions cost (area, frequency range, FoV, baseline length) funding timeline governance operations impact on the community.

234 views • 12 slides

192 views • 11 slides

The Future of Geo

The Future of Geo. Hugh Barron. GOCAD bedrock model. acquire & enhance UK geoscience knowledge base. improve geoscience communication. enhance external partnerships. whole-systems science approach. 8 km. increase economic impact. zone of human interaction.

213 views • 11 slides

Rob Roser

83 views • 8 slides