Berkeley heterodyne interferometer

Details Berkeley heterodyne interferometer Berkeley heterodyne interferometer

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ssrv...17..677b&link_type=abstract

(Workshop on Coherent Detection in Astronomy, Rhenen, Netherlands, Apr. 25, 26, 1974.) Space Science Reviews, vol. 17, July 1975

Astronomy and Astrophysics

Astronomy

Infrared Astronomy, Infrared Interferometers, Optical Heterodyning, Stellar Radiation, Cosmic Dust, Infrared Stars, Interferometry, Optical Paths, Solar Instruments, Stellar Envelopes

Scientific paper

A prototype heterodyne stellar interferometer has been built in order to demonstrate the feasibility of heterodyne techniques in measuring angular diameters of bright infrared stars. The first system tests were performed in December 1972. Attention is given to investigations concerning the possibility that optical air turbulence within the structure of the solar telescope employed can possibly destroy the phase coherence of the fringe signals.

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