Paper
29 January 1988 Application Of Bispectrum Analysis To Infrared Speckle Data
Julian C. Christou, Jonathan D. Freeman, Francois Roddier, Donald W. McCarthy Jr., Michael L. Cobb, Stuart B. Shaklan
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Abstract
We have applied the bispectrum algorithm to one-dimensional infrared speckle data for retrieval of diffraction limited phases. We use a standard weighting averaging technique to combine the multiple phase estimates contained in the bispectrum. We have also used the bispectrum modulus to obtain visibility amplitudes. Results, including images, are presented for three different binary stars. Simulated data has also been used to study the behaviour of the algorithm under different signal-to-noise conditions as well as a study of phase recovery for different defocus conditions. We find that the algorithm is sensitive, at a low level, to focus changes especially for noisy data. Comparison of the bispectrum phases is made with those obtained from Knox-Thompson cross-spectra for all cases.
© (1988) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Julian C. Christou, Jonathan D. Freeman, Francois Roddier, Donald W. McCarthy Jr., Michael L. Cobb, and Stuart B. Shaklan "Application Of Bispectrum Analysis To Infrared Speckle Data", Proc. SPIE 0828, Digital Image Recovery and Synthesis, (29 January 1988); https://doi.org/10.1117/12.942076
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Cited by 6 scholarly publications.
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KEYWORDS
Visibility

Spatial frequencies

Signal to noise ratio

Image restoration

Modulation transfer functions

Speckle

Stars

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