Instrumental factors affecting the fringe contrast in optical interferometers

Details Instrumental factors affecting the fringe contrast in optical interferometers Instrumental factors affecting the fringe contrast in optical interferometers

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.171..333b&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

1

Diffraction Patterns, Radio Interferometers, Astronomical Observatories, Polarization Characteristics, Signal To Noise Ratios

Scientific paper

Interference fringes are the prime observable quantity in astronomical
optical and radio interferometers. To maximize the signal-to-noise
ratio, it is important to keep instrumental causes of fringe contrast
decrease to a minimum. These causes are discussed, and the tolerances to
be placed on them are derived.

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