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arxiv: 1011.5214 · v1 · pith:HLCIORQMnew · submitted 2010-11-23 · 🌌 astro-ph.SR · astro-ph.IM

Stellar Imager (SI): developing and testing a predictive dynamo model for the Sun by imaging other stars

Kenneth G. Carpenter (GSFC) , Carolus J. Schrijver (LMATC) , Margarita Karovska (CfA) , Steve Kraemer (CUA) , Richard Lyon (GSFC) , David Mozurkewich (Seabrook Eng.) , Vladimir Airapetian (GMU) , John C. Adams (GSFC)
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Ronald J. Allen (STScI) Alex Brown (UCO/Boulder) Fred Bruhweiler (CUA) Alberto Conti (STScI) Joergen Christensen-Dalsgaard (U. Aarhus) Steve Cranmer (CfA) Manfred Cuntz (U. Texas/Arlington) William Danchi (GSFC) Andrea Dupree (CfA) Martin Elvis (CfA) Nancy Evans (CfA) Mark Giampapa (NSO/NOAO) Graham Harper (UCO/Boulder) Kathy Hartman (GSFC) Antoine Labeyrie (College de France) Jesse Leitner (GSFC) Chuck Lillie (NGST) Jeffrey L. Linsky (UCO/Boulder) Amy Lo (NGST) Ken Mighell (NOAO) David Miller (MIT) Charlie Noecker (BATC) Joe Parrish (Aurora Flight Systems) Jim Phillips (CfA) Thomas Rimmele (NSO) Steve Saar (CfA) Dimitar Sasselov (CfA/Harvard) H. Philip Stahl (MSFC) Eric Stoneking (GSFC) Klaus Strassmeier (AI-Potsdam) Frederick Walter (SUNY) Rogier Windhorst (ASU) Bruce Woodgate (GSFC) Robert Woodruff (LMSSC)
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classification 🌌 astro-ph.SR astro-ph.IM
keywords stellaractivitydynamoimagermagneticmodelpredictivestars
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The Stellar Imager mission concept is a space-based UV/Optical interferometer designed to resolve surface magnetic activity and subsurface structure and flows of a population of Sun-like stars, in order to accelerate the development and validation of a predictive dynamo model for the Sun and enable accurate long-term forecasting of solar/stellar magnetic activity.

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