A large multipurpose solar telescope complex - Requirements and means of realization

Details A large multipurpose solar telescope complex - Requirements and means of realization A large multipurpose solar telescope complex - Requirements and means of realization

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kfnt....3...80k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 3, July-Aug. 1987, p. 80-84. In Russian.

Physics

Optics

Chromosphere, Photosphere, Solar Instruments, Telescopes, Cassegrain Optics, Equipment Specifications, Mirrors, Polarization Characteristics, Resolution

Scientific paper

Preliminary results on the problem of creating a large multipurpose solar telescope are presented. A large photospheric-chromospheric telescope must have a resolution of 0.5-0.25 arcsec (potentially reaching 0.1 arcsec), a tracking power of at least 1 arcsec, and a small instrumental polarization (0.001-0.00001). A 2-m telescope is proposed which is pointed toward the sun and operates with an open short path of large-aperture rays according to a three-mirror Cassegrain-Gregory scheme. Image stability is achieved by using the coelostat system at the exit after the elliptical mirror.

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