Abstract
This paper presents the results of a study of the possibility of monitoring the alignment of two-mirror Cassegrain and Ritchey–Crétien telescopes during both fabrication and operation under observatory conditions, as well as in space. The method is based on a system of coaxial synthesized annular holograms as optical compensators and reference optical elements.
© 2012 OSA
PDF Article
More Like This
Development of a two-channel system for monitoring the mirror elements of the Millimetron space observatory
P. S. Zavyalov, S. N. Makarov, A. V. Smirnov, S. D. Fedorchuk, M. F. Stupak, A. G. Verhoglyad, A. G. Elesin, M. A. Zavyalova, M. S. Kravchenko, D. V. Skokov, E. V. Vlasov, and A. V. Ermolenko
Appl. Opt. 61(2) 588-596 (2022)
Cited By
You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an Optica member, or as an authorized user of your institution.
Contact your librarian or system administrator
or
Login to access Optica Member Subscription