Image formation in coronagraphs due to mirror polarization aberrations

Image formation in coronagraphs due to mirror polarization aberrations

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 PS...

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Bibliographic Details
Main Author: Chipman, Russell A.
Other Authors: Univ Arizona, Coll Opt Sci
Language:en
Published: SPIE-INT SOC OPTICAL ENGINEERING 2017
Subjects:
Polarization aberration
Online Access:Russell A. Chipman, "Image formation in coronagraphs due to mirror polarization aberrations", Proc. SPIE 10590, International Optical Design Conference 2017, 105901V (27 November 2017); doi: 10.1117/12.2291913; https://doi.org/10.1117/12.2291913
http://hdl.handle.net/10150/627180
http://arizona.openrepository.com/arizona/handle/10150/627180

Internet

Russell A. Chipman, "Image formation in coronagraphs due to mirror polarization aberrations", Proc. SPIE 10590, International Optical Design Conference 2017, 105901V (27 November 2017); doi: 10.1117/12.2291913; https://doi.org/10.1117/12.2291913
http://hdl.handle.net/10150/627180
http://arizona.openrepository.com/arizona/handle/10150/627180

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