Laser interferometric control problems in adaptive astronomical telescope

Details Laser interferometric control problems in adaptive astronomical telescope Laser interferometric control problems in adaptive astronomical telescope

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2200..581a&link_type=abstract

Proc. SPIE Vol. 2200, p. 581-592, Amplitude and Intensity Spatial Interferometry II, James B. Breckinridge; Ed.

Physics

Scientific paper

The paper deals with the problem of choosing proper wavelength for a wavefront sensor involving an internal laser source and a hologram on the surface of the primary mirror of a telescope. Some results of dimensional calculations for the optical arrangement for recording the hologram structure are presented. As a result a conclusion is drawn on the possibility of reducing the size of an optical stand for making this structure by increasing the operation wavelength of the control channel of a telescope.

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