Aperture synthesis of astronomical telescopes

Details Aperture synthesis of astronomical telescopes Aperture synthesis of astronomical telescopes

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985opmep..52...32d&link_type=abstract

(Optiko-Mekhanicheskaia Promyshlennost', vol. 52, Dec. 1985, p. 32-38) Soviet Journal of Optical Technology (ISSN 0038-5514), vo

Astronomy and Astrophysics

Astronomy

Synthetic Apertures, Telescopes, Antenna Design, Atmospheric Attenuation, Mirrors, Optical Transfer Function, Phased Arrays, Redundancy, Synthetic Arrays

Scientific paper

The problem of building large-diameter astronomical telescopes using aperture synthesis methods is examined. Telescopes having a sectional main mirror, the synthesis of partially filled apertures, and methods for adjusting and phasing them are described. The limitations associated with atmospheric turbulence and possible ways of reducing their influence through the use of nonredundant aperture synthesis systems are indicated.

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