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dc.contributor.authorChipman, Russell A.*
dc.date.accessioned2018-04-02T16:00:12Z
dc.date.available2018-04-02T16:00:12Z
dc.date.issued2017-11-27
dc.identifier.citationRussell 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/10.1117/12.2291913en
dc.identifier.issn0277-786X
dc.identifier.doi10.1117/12.2291913
dc.identifier.urihttp://hdl.handle.net/10150/627180
dc.description.abstractThe 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.
dc.language.isoenen
dc.publisherSPIE-INT SOC OPTICAL ENGINEERINGen
dc.relation.urlhttps://www.spiedigitallibrary.org/conference-proceedings-of-spie/10590/2291913/Image-formation-in-coronagraphs-due-to-mirror-polarization-aberrations/10.1117/12.2291913.fullen
dc.rights© (2017) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE).en
dc.subjectPolarization aberrationen
dc.titleImage formation in coronagraphs due to mirror polarization aberrationsen
dc.typeArticleen
dc.identifier.eissn1996-756X
dc.contributor.departmentUniv Arizona, Coll Opt Scien
dc.identifier.journalINTERNATIONAL OPTICAL DESIGN CONFERENCE 2017en
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en
dc.eprint.versionFinal published versionen
refterms.dateFOA2018-09-12T07:10:16Z
html.description.abstractThe 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.


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