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dc.contributor.authorOh, Se Baeken_US
dc.contributor.authorBarbastathis, Georgeen_US
dc.date.accessioned2009-10-19T13:22:39Z
dc.date.available2009-10-19T13:22:39Z
dc.date.issued2009-08en_US
dc.date.submitted2009-04en_US
dc.identifier.issn0146-9592en_US
dc.identifier.urihttp://hdl.handle.net/1721.1/49444
dc.description.abstractBased on a linear systems approach, we derive the Wigner distribution function (WDF) of a 4f imager with a volume holographic three-dimensional pupil; then we obtain the WDF of the volume hologram itself by using the shearing properties of the WDF. Two common configurations, plane and spherical wave reference volume holograms, are examined in detail. The WDF elucidates the shift variant nature of the volume holographic element in both cases.en_US
dc.language.isoen_USen_US
dc.publisherOptical Society of Americaen_US
dc.relation.isversionofhttp://dx.doi.org/10.1364/OL.34.002584en_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alikeen_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/en_US
dc.sourceSe Baek Ohen_US
dc.titleWigner distribution function of volume hologramsen_US
dc.typeArticleen_US
dc.identifier.citationS. Oh and G. Barbastathis, "Wigner distribution function of volume holograms," Opt. Lett. 34, 2584-2586 (2009).en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Mechanical Engineeringen_US
dc.contributor.approverOh, Se Baeken_US
dc.contributor.mitauthorBarbastathis, Georgeen_US
dc.contributor.mitauthorOh, Se Baeken_US
dc.relation.journalOptics Lettersen_US
dc.eprint.versionAuthor's final manuscript
dc.type.urihttp://purl.org/eprint/type/SubmittedJournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsOh, Se Baek; Barbastathis, Georgeen
dc.identifier.orcidhttps://orcid.org/0000-0002-4140-1404
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


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