Signal-to-Noise in Photon Counting Speckle Interferometry with Real Detectors

Steven Ebstein

doi:10.1364/QLIP.1986.MC3

Topical Meeting on Quantum-Limited Imaging and Image Processing
Technical Digest Series (Optica Publishing Group, 1986),
paper MC3
•https://doi.org/10.1364/QLIP.1986.MC3

Signal-to-Noise in Photon Counting Speckle Interferometry with Real Detectors

Steven Ebstein

Quantum-Limited Imaging and Image Processing 1986

Honolulu, Hawaii United States
31 March–2 April 1986
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Astronomical Imaging: 1 (MC)

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S. Ebstein, "Signal-to-Noise in Photon Counting Speckle Interferometry with Real Detectors," in Topical Meeting on Quantum-Limited Imaging and Image Processing, Technical Digest Series (Optica Publishing Group, 1986), paper MC3.

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Abstract

In speckle interferometry, one estimates the angular power spectrum of short-exposure images degraded by atmospheric turbulence. The power spectrum is a random process due to the variability of atmospheric conditions and due to the stochastic nature of photodetection.

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