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9 June 1994 Laser interferometric control problems in adaptive astronomical telescope
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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.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Vyatcheslav V. Anistchenko, Sergey N. Koreshev, Vadim A. Parfenov, Vladimir I. Podoba, Alexander G. Seregin, and Victor I. Sidorov "Laser interferometric control problems in adaptive astronomical telescope", Proc. SPIE 2200, Amplitude and Intensity Spatial Interferometry II, (9 June 1994);

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