JPL Technical Report Server

WFIRST coronagraph optical modeling

Show simple item record Krist, John Riggs, A. J. McGuire, James Tang, Hong Amiri, Nikta Gutt, Gary Marchen, Luis Marx, David Nemati, Bijan Saini, Navtej Sidick, Erkin Zhou, Hanying 2020-03-23T20:23:54Z 2020-03-23T20:23:54Z 2017-08-08
dc.identifier.citation 2017 SPIE Optics and Photonics, San Diego, California, August 6-10, 2017 en_US
dc.identifier.clearanceno CL#17-3883
dc.description.abstract End-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. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2017 en_US
dc.title WFIRST coronagraph optical modeling en_US
dc.type Preprint en_US

Files in this item

This item appears in the following Collection(s)

Show simple item record



My Account