Optics and Precision Engineering, Volume. 30, Issue 23, 3031(2022)
Dome design of large ground-based telescope
[1] [1] 1张景旭. 地基大口径望远镜系统结构技术综述[J]. 中国光学, 2012, 5(4): 327-336. doi: 10.3788/CO.20120504.0327ZHANGJ X. Overview of structure technologies of large aperture ground-based telescopes[J]. Chinese Optics, 2012, 5(4): 327-336.(in Chinese). doi: 10.3788/CO.20120504.0327
[2] [2] 2程景全. 天文望远镜原理和设计射电、红外、光学、X射线和γ射线望远镜[M]. 北京: 中国科学技术出版社, 2003.CHENGJ Q. Principles of Astronomical Telescope Design[M]. Beijing: China Science and Technology Press, 2003.(in Chinese)
[3] C DENKER, A LAGG, K G PUSCHMANN et al. The GREGOR Solar Telescope. IAU Special Session, 6(2012).
[4] L C ROBERTS, P D FIGGIS. Thermal conditioning of the AEOS telescope. Waikoloa, 4837, 264-271(2003).
[5] D R BLANCO, M W JOHNS. Thermal design of the WIYN. Kailua, 2199, 743-753(3).
[6] J TERAN, D S PORTER, E A HILEMAN et al. Unique dome design for the SOAR telescope project, 4004, 155-163(2000).
[7] [7] 7胡海飞, 赵宏伟, 刘振宇, 等. 4 m口径SiC反射镜原位检测用静压支撑系统[J]. 光学 精密工程, 2017, 25(10): 2607-2613. doi: 10.3788/OPE.20172510.2607HUH F, ZHAOH W, LIUZH Y, et al. Hydrostatic support system for in situ optical testing of a 4 m aperture SiC mirror[J]. Opt. Precision Eng., 2017, 25(10): 2607-2613.(in Chinese). doi: 10.3788/OPE.20172510.2607
[8] [8] 8吴小霞, 李剑锋, 宋淑梅, 等. 4 m SiC轻量化主镜的主动支撑系统[J]. 光学 精密工程, 2014, 22(9): 2451-2457. doi: 10.3788/OPE.20142209.2451WUX X, LIJ F, SONGS M, et al. Active support system for 4 m SiC lightweight primary mirror[J]. Optics and Precision Engineering, 2014, 22(9): 2451-2457.(in Chinese). doi: 10.3788/OPE.20142209.2451
[9] [9] 9吴小霞, 王鸣浩, 明名, 等. 大口径SiC轻量化主镜热变形的定标[J]. 光学 精密工程, 2012, 20(6): 1243-1249. doi: 10.3788/OPE.20122006.1243WUX X, WANGM H, MINGM, et al. Calibration of thermal distortion for large aperture SiC lightweight mirror[J]. Optics and Precision Engineering, 2012, 20(6): 1243-1249.(in Chinese). doi: 10.3788/OPE.20122006.1243
[10] M BOCCAS. Protected-silver coatings for the 8-m Gemini telescope mirrors. Thin Solid Films, 502, 275-280(2006).
[11] J SEBAG, K VOGIATZIS. Estimating dome seeing for LSST, 9150, 268-277(2014).
[12] O LAI, J K WITHINGTON, R LAUGIER et al. Direct measure of dome seeing with a localized optical turbulence sensor. Monthly Notices of the Royal Astronomical Society, 484, 5568-5577(2019).
[13] L ZAGO. Engineering handbook for local and dome seeing, 2871, 726-736(1997).
[14] J C WYNGAARD, Y IZUMI, S A COLLINS. Behavior of the refractive-index-structure parameter near the ground. JOSA, 61, 1646-1650(1971).
[15] T A BIDA, E W DUNHAM, L P BRIGHT et al. Site testing for the discovery channel telescope, 5489, 196-206(2004).
[16] V L KRABBENDAM, G P RUTHVEN, V P BENNETT et al. Active optical system design for the, 4003, 122-135(4).
[17] R SAGAR, M NAJA, G MAHESWAR et al. Science at high-altitude sites of ARIES - astrophysics and atmospheric sciences. Proceedings of the Indian National Science Academy, 80, 759(2014).
[18] J COZAR-CASTELLANO, M N CAGIGAL, N VEGA et al. Overview of telescope structure, enclosure, and pier preliminary design of the European Solar Telescope, 12187, 693-703(2022).
[19] N E DALRYMPLE, J M OSCHMANN, R P HUBBARD. ATST enclosure: seeing performance, thermal modeling, and error budgets, 5497, 497-507(2004).
Get Citation
Copy Citation Text
Xiangyi LIU, Zhichen WANG, Zhi WANG. Dome design of large ground-based telescope[J]. Optics and Precision Engineering, 2022, 30(23): 3031
Received: Nov. 8, 2022
Accepted: --
Published Online: Jan. 10, 2023
The Author Email: WANG Zhichen (zcwang911@163.com)