Study of a large optical/IR telescope scheme

Details Study of a large optical/IR telescope scheme Study of a large optical/IR telescope scheme

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acasn..33..212z&link_type=abstract

Acta Astronomica Sinica (ISSN 0001-5245), vol. 33, no. 2, p. 212-219.

Physics

Optics

Infrared Astronomy, Infrared Telescopes, Visible Spectrum, Cassegrain Optics, Delay Lines, Field Of View, Light Beams, Transmittance

Scientific paper

The general design and operation of a large telescope array consisting of six 2.16-m telescopes are examined. The telescope can be operated both in the visible and IR wavelength regions in three different modes: (1) as an individual 2.16-m telescope at the prime focus, Cassegrain focus, and Coude focus; (2) as an incoherent array for the visible wavelength region; and (3) as a phase array. The advantages and disadvantages of the telescope array proposed here are examined from the technological, performance, and cost effectiveness standpoints.

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