A precise method of monitoring the alignment of two-mirror telescopes, based on a system of synthesized annular holograms

A precise method of monitoring the alignment of two-mirror telescopes, based on a system of synthesized annular holograms
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DOI:
10.1364/jot.79.000167
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发表时间:
2012-03
影响因子:
0.4
通讯作者:
V. A. Baloev;V. Ivanov;N. P. Larionov;A. V. Lukin;A. N. Mel’nikov;A. .. Skochilov;A. M. Uraskin;Yu. P. Chugunov
V. A. Baloev;V. Ivanov;N. P. Larionov;A. V. Lukin;A. N. Mel’nikov;A. .. Skochilov;A. M. Uraskin;Yu. P. Chugunov
中科院分区:
物理与天体物理4区
文献类型:
--
作者:
V. A. Baloev;V. Ivanov;N. P. Larionov;A. V. Lukin;A. N. Mel’nikov;A. .. Skochilov;A. M. Uraskin;Yu. P. Chugunov

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本文介绍了在天文台条件下以及在空间中制造和运行期间监测双镜卡塞格伦和里奇-克雷蒂恩望远镜对准的可能性的研究结果。该方法是基于一个系统的同轴合成环形全息作为光学补偿器和参考光学元件。
This paper presents the results of a study of the possibility of monitoring the alignment of two-mirror Cassegrain and Ritchey–Cretien 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.