@inproceedings{ee61c7e9b35b40e595042fc06cb57daa,
title = "Image formation in coronagraphs due to mirror polarization aberrations",
abstract = "The PSF for astronomical telescopes and instruments depends not only on geometric wavefront aberrations, but also on those polarization aberrations from the polarization properties of reflecting and transmitting surfaces. The image plane irradiance distribution is the linear superposition of four PSF images: One for each of the two orthogonal polarizations and one for each of two cross-coupled polarization terms.",
keywords = "Aberration, Polarization",
author = "Chipman, \{Russell A.\}",
note = "Publisher Copyright: {\textcopyright} 2017 SPIE.; International Optical Design Conference 2017, IODC 2017 ; Conference date: 09-07-2017 Through 13-07-2017",
year = "2017",
doi = "10.1117/12.2291913",
language = "English (US)",
series = "Proceedings of SPIE - The International Society for Optical Engineering",
publisher = "SPIE",
editor = "Muschaweck, \{Julius A.\} and Rogers, \{John R.\} and Clark, \{Peter P.\} and Pfisterer, \{Richard N.\}",
booktitle = "International Optical Design Conference 2017",
}