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WFIRST coronagraph optical modelingEnd-to-end numerical optical modeling of the WFIRST coronagraph incorporating wavefront sensing and control is used to determine the performance of the coronagraph with realistic errors, including pointing jitter and polarization. We present the performance estimates of the current flight designs as predicted by modeling. We also describe the release of a new version of the PROPER optical propagation library, our primary modeling tool, which is now available for Python and Matlab in addition to IDL.
Document ID
20210007888
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Zhou, Hanying
Sidick, Erkin
Saini, Navtej
Nemati, Bijan
Marx, David
Marchen, Luis
Gutt, Gary
Amiri, Nikta
Tang, Hong
McGuire, James
Riggs, A. J.
Krist, John
Date Acquired
August 8, 2017
Publication Date
August 8, 2017
Publication Information
Publisher: Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2017
Distribution Limits
Public
Copyright
Other
Technical Review

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