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dc.contributor.authorShack, R. V.
dc.date.accessioned2016-12-13T22:25:45Z
dc.date.available2016-12-13T22:25:45Z
dc.date.issued1967-08-28
dc.identifier.urihttp://hdl.handle.net/10150/621612
dc.descriptionQC 351 A7 no. 19en
dc.description.abstractABSTRACT The classical properties of an image formed by an optical system looking through a turbulent medium are scintillation, agitation, and blur. A simple but adequate statistical model is obtained describing the pupil function in the presence of random wavefront disturbances in both amplitude and phase. A measure of scintillation is then obtained in the form of a normalized, weighted integral in frequency space containing all the pertinent properties of the optical system. A similar measure of agitation is then developed, and finally a description of the blur is obtained in the form of an equivalent transfer function for the turbulent medium in which the contribution from amplitude variations and the contribution from phase variations are independent.
dc.language.isoen_USen
dc.publisherOptical Sciences Center, University of Arizona (Tucson, Arizona)en
dc.relation.ispartofseriesOptical Sciences Technical Report 19en
dc.rightsCopyright © Arizona Board of Regents
dc.subjectOptics.en
dc.subjectAtmospheric turbulence -- Scattering (Physics)en
dc.subjectMeteorological optics -- statistics.en
dc.titleInteraction of an Optical System with the Incoming Wavefront in the Presence of Atmospheric Turbulenceen_US
dc.typeTechnical Reporten
dc.description.collectioninformationThis title from the Optical Sciences Technical Reports collection is made available by the College of Optical Sciences and the University Libraries, The University of Arizona. If you have questions about titles in this collection, please contact repository@u.library.arizona.edu.
refterms.dateFOA2018-06-25T11:28:14Z
html.description.abstractABSTRACT The classical properties of an image formed by an optical system looking through a turbulent medium are scintillation, agitation, and blur. A simple but adequate statistical model is obtained describing the pupil function in the presence of random wavefront disturbances in both amplitude and phase. A measure of scintillation is then obtained in the form of a normalized, weighted integral in frequency space containing all the pertinent properties of the optical system. A similar measure of agitation is then developed, and finally a description of the blur is obtained in the form of an equivalent transfer function for the turbulent medium in which the contribution from amplitude variations and the contribution from phase variations are independent.


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