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The Terrestrial Planet Finder coronagraph dynamics error budget

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dc.contributor.author Shaklan, Stuart B.
dc.contributor.author Marchen, Luis
dc.contributor.author Green, Joseph J.
dc.contributor.author Lay, Oliver P.
dc.date.accessioned 2005-10-13T19:49:03Z
dc.date.available 2005-10-13T19:49:03Z
dc.date.issued 2005-07
dc.identifier.citation Optics and Photonics, SPIE Annual Meeting, San Diego, CA, July 31, 2005 en
dc.identifier.clearanceno 05-1799
dc.identifier.uri http://hdl.handle.net/2014/37766
dc.description.abstract The Terrestrial Planet Finder Coronagraph (TPF-C) demands extreme wave front control and stability to achieve its goal of detecting earth-like planets around nearby stars. We describe the performance models and error budget used to evaluate image plane contrast and derive engineering requirements for this challenging optical system. en
dc.description.sponsorship NASA en
dc.format.extent 993067 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US en
dc.publisher Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2005. en
dc.subject coronagraph en
dc.subject telescope en
dc.subject extra-solar planets en
dc.title The Terrestrial Planet Finder coronagraph dynamics error budget en
dc.type Preprint en


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