Automatic design of corrector systems for Cassegrain telescopes

Details Automatic design of corrector systems for Cassegrain telescopes Automatic design of corrector systems for Cassegrain telescopes

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976acasn..17....9s&link_type=abstract

Acta Astronomica Sinica, vol. 17, June 1976, p. 9-26. In Chinese, with abstract in English.

Physics

Optics

1

Cassegrain Optics, Computer Aided Design, Optical Correction Procedure, Telescopes, Aberration, Conical Bodies, Mirrors, Surface Geometry

Scientific paper

A series of correcting systems for Cassegrain telescopes was designed with the aid of a computer. During performance of calculations, it was assumed that the primary and secondary mirrors had strictly conical surfaces and that the telescope was completely free of third-order spherical aberration when the correcting systems are removed. The results can be transferred with the aid of scale calculations to real telescopes of any aperture size, but the aberrations expressed in seconds of arc remain unchanged.

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