The phase problem in astronomy

Details The phase problem in astronomy The phase problem in astronomy

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jopt...10..308g&link_type=abstract

Journal of Optics, vol. 10, Nov.-Dec. 1979, p. 308-310.

Physics

Optics

Astronomy, Atmospheric Optics, Phase Error, Sky Brightness, Interferometers, Luminous Intensity, Wave Front Reconstruction

Scientific paper

The sky brightness distribution is the inverse Fourier transform of the
complex degree of coherence, i.e., a complete noiseless set of complex
correlation measurements. In practice these measurements are incomplete
and subject to error. The present paper reviews direct and indirect
methods for dealing with this problem.

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