Segmented primary mirror telescope image quality estimation

Details Segmented primary mirror telescope image quality estimation Segmented primary mirror telescope image quality estimation

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spie.4003..262s&link_type=abstract

Proc. SPIE Vol. 4003, p. 262-269, Optical Design, Materials, Fabrication, and Maintenance, Philippe Dierickx; Ed.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The model of distortions caused by mistakes in installation of mirrors of a compound telescope of the large diameter is offered. The results, received on the basis of model, calculated according to the formulas for average image in a plane of its formation, it variance and characteristic of speckle structure of the image are resulted. It is shown, that the researched distortions should be taken into account at a choice of an installation site of a telescope, at processing the information in a service of meteoric and asteroid safety and fundamental astrophysical researches.

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