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Signal-to-noise limitations in white light holographyA simple derivation is given for the SNR in images reconstructed from incoherent holograms. Dependence is shown to be on the hologram SNR, object complexity, and the number of pixels in the detector. Reconstruction of involved objects becomes possible with high-dynamic-range detectors such as CCDs. White-light holograms have been produced by means of a rotational shear interferometer combined with a chromatic corrector. A digital inverse transform recreated the object.
Document ID
19880046347
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ribak, Erez (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Breckinridge, James B. (California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Roddier, Claude (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Roddier, Francois (National Optical Astronomy Observatories Tucson, AZ, United States)
Date Acquired
August 13, 2013
Publication Date
March 15, 1988
Publication Information
Publication: Applied Optics
Volume: 27
ISSN: 0003-6935
Subject Category
Optics
Accession Number
88A33574
Distribution Limits
Public
Copyright
Other

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