The use of a holographic method in stellar interferometry

Details The use of a holographic method in stellar interferometry The use of a holographic method in stellar interferometry

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977opsp...43..324v&link_type=abstract

Optika i Spektroskopiia, vol. 43, Aug. 1977, p. 324-330. In Russian.

Physics

Atmospheric Turbulence, Holographic Interferometry, Michelson Interferometers, Stellar Radiation, Coherence Coefficient, Correlation, Fourier Transformation, Stellar Luminosity, Stellar Spectra

Scientific paper

A method of observing the interference of independent, weakly degenerate fields through the turbulent atmosphere using Michelson stellar interferometry is described. The accuracy of measurements of the mutual-coherence function is studied for systems with recording of the interference pattern of the initial fields and their Fourier transformations. This holographic system allows one to avoid difficulties associated with the formation of spatial spectra of interfering fields from sources of small angular dimensions.

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