Seeing effects removal in a Michelson stellar interferometer

Details Seeing effects removal in a Michelson stellar interferometer Seeing effects removal in a Michelson stellar interferometer

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976josa...66.1347r&link_type=abstract

Optical Society of America, Journal, vol. 66, Dec. 1976, p. 1347-1350.

Computer Science

5

Atmospheric Turbulence, Diffraction Patterns, Michelson Interferometers, Optical Correction Procedure, Speckle Patterns, Stellar Spectrophotometry, Normal Density Functions, Optical Transfer Function, Power Spectra, Random Signals, Turbulence Effects

Scientific paper

There is no unique definition of the fringe contrast in a random structure such as the image given by a Michelson stellar interferometer. A definition is given which leads to a contrast value independent of the seeing conditions provided the wave-front perturbations on the two apertures are uncorrelated. Moreover, if simultaneous observations through a single aperture are available, the seeing effects can be completely removed.

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