Scheme of optical synthetic aperture telescope

Details Scheme of optical synthetic aperture telescope Scheme of optical synthetic aperture telescope

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991spie.1540..163m&link_type=abstract

In: Optomechanics and dimensional stability; Proceedings of the Meeting, San Diego, CA, July 25, 26, 1991 (A93-39433 15-74), p.

Physics

Optics

Charge Coupled Devices, Electromagnetic Interference, Fiber Optics, Infrared Telescopes, Optical Tracking, Synthetic Apertures, Astronomical Observatories, Image Processing, Image Resolution, Technological Forecasting

Scientific paper

An optical synthetic aperture telescope being presently designed for the Xinglong (China) station of the Beijing Astronomical Observatory, to be used by the international as well as national communities is described. The main body of the synthetic aperture telescope is the 4.3-m optical IR telescope, which will be positioned between the 2.16-m, 1.26-m, and 0.9-m telescopes at the Xinglong station. Through the fiber combination of the 4.3-m telescope and some of these optical telescopes, the Xinglong station will enhance its concentrating light power up to that of a 5.1-m telescope.

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