Application of two step sensitivity matrix method in Cassegrain telescope alignment

Cao Yuze; Ma Wenli

doi:10.12086/oee.2020.180536

Journals >Opto-Electronic Engineering >Volume 47 >Issue 2 >Page 180536 > Article

Opto-Electronic Engineering
Vol. 47, Issue 2, 180536 (2020)

Application of two step sensitivity matrix method in Cassegrain telescope alignment

Cao Yuze^1、2、* and Ma Wenli¹

Author Affiliations

¹[in Chinese]

²[in Chinese]

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DOI: 10.12086/oee.2020.180536 Cite this Article

Cao Yuze, Ma Wenli. Application of two step sensitivity matrix method in Cassegrain telescope alignment[J]. Opto-Electronic Engineering, 2020, 47(2): 180536 Copy Citation Text

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References

[2] Figoski J W, Shrode T E, Moore G F. Computer-aided alignment of a wide-field, three-mirror, unobscured, high-resolution sen-sor[J]. Proceedings of SPIE, 1989, 1049: 166.

[3] Egdall I M. Manufacture of a three-mirror wide-field optical sys-tem[J]. Optical Engineering, 1985, 24(2): 242285.

[6] Kim S, Yang H S, Lee YW, et al. Merit function regression me-thod for efficient alignment control of two-mirror optical systems. [J]. Optics Express, 2007, 15(8): 5059–5068.

Cao Yuze, Ma Wenli. Application of two step sensitivity matrix method in Cassegrain telescope alignment[J]. Opto-Electronic Engineering, 2020, 47(2): 180536

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