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环境对大口径SiC轻量化主镜视宁度的影响 被引量:5

Affect of environment on mirror seeing of large-aperture SiC lightweight primary mirror
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摘要 由于地基大口径望远镜主镜视宁度与望远镜系统成像质量相关,本文研究了环境对主镜视宁度的影响。理论分析了影响主镜视宁度大小的因素,得出主镜视宁度会随主镜表面和环境之间温差的增大而增大的结论。利用有限元法分析了自然对流和吹风条件下主镜的温度变化和温度分布;最后通过相应工况条件下2mSiC轻量化主镜的温度测试实验对仿真分析结果进行了验证。实验结果显示:在初始温差为6℃的无风自然对流情况下,主镜与环境达到温度平衡约需4h;而在初始温差为8℃的吹风情况下,主镜与环境达到热平衡仅需1.5h。分析和实验结果表明:采用强迫对流热控措施可快速而有效地将主镜视宁度控制在合理的范围内,可获得更多的望远镜观测时间,同时保证大口径望远镜系统的成像质量。 As the primary mirror seeing of a ground based large aperture telescope is directly related to its image quality,this paper researches the effect of environments on the primary mirror seeing.Through theoretical analysis,it points out that the size of the primary mirror seeing will increase with the temperature change between the primary mirror surface and the environments.Then using thermal analysis software Radtherm,the temperature changes and temperature distributions of a 2m SiC lightweight primary mirror were analyzed under two different conditions of natural convection and natural flowing.Finally,the some temperature experiments on the 2 m SiC lightweight primary mirror under the working conditions mentioned above were performed to verify simulation results.The experiment results indicate that it takes about 4hours to reach temperature equilibrium with the environment for the primary mirror in case of natural convection with initial 6 ℃ temperaturedifference;however,it takes only about 1.5 hours in case of natural flowing with initial 8 ℃temperature difference.It shows the greater temperature difference but much less consumed time.These means that when the thermal control system and control method are forced to the large-aperture telescope system to perform the convective heat control,the mirror seeing will be controlled in a reasonable range more quickly and more effectively,and more telescope observation time can be obtained meanwhile maintaining much better image quality.
出处 《光学精密工程》 EI CAS CSCD 北大核心 2015年第3期776-783,共8页 Optics and Precision Engineering
基金 中科院三期创新工程专项基金资助项目(No.O65X32C060)
关键词 大口径望远镜 SiC轻量化主镜 视宁度 温度梯度 large aperture telescopy lightweight SiC primary mirror mirror seeing temperature gradient
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参考文献18

  • 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. 被引量:76
  • 2胡君,王栋,孙天宇.现代航天光学成像遥感器的应用与发展[J].中国光学与应用光学,2010,3(6):519-533. 被引量:28
  • 3王红,田铁印.轴向温差对空间遥感器光学系统成像质量的影响[J].光学精密工程,2007,15(10):1489-1494. 被引量:19
  • 4吴清文,卢锷,王家骐,牛晓明.主镜稳定温度场特性分析[J].光学精密工程,1996,4(6):47-53. 被引量:11
  • 5STEPP L, HANSEN E. The Gemini primary mir- ror thermal management I-J~. SPIE, 1994, 2911: 911-913.
  • 6RACINE R, SALMON D, COWLEY D, et al.. Mirror, dome and natural seeing at CFHT [J]. Publications of the Astronomical Society of the Pacific, 1991, 103:1020-1032.
  • 7WOOD P Y, RYAN S G. Effects on seeing at the Anglo-Australian telescope of temperature differ- ences between outside air, dome air and mirror [J]. Proceedings of the Astronomical Society of Aus- tralia, 1995,12: 95-96.
  • 8LARRY W GOBLE. Temperature control of the 3. 5-Meter WIYN telescope primary mirror [J]. SPIE, 1991, 1532~161-163.
  • 9BRIAN CUERDENA. Jacques sebagb and etc. LSST mirror thermal performance [J]. SPIE, 2004, 5495: 189-191.
  • 10DOUGLAS R. Neill. LSST primary/tertiary mir- ror thermal controlsystem [J]. SPIE,2010,7733.. 77331E-2.

二级参考文献101

共引文献177

同被引文献45

  • 1ZHANG H Y, LIXN, MENGX H, etal.. Mir- ror seeing control of large infrared solar telescope [J]. SPIE,2010,7733, doi.. 10. 1117/12. 856099.
  • 2CHAFFEE H F, CROMWELL R H. Seeing meas- urements at the multiple mirror telescope obtained with a very high quality 1.8-m primary mirror [J]. SPIE, 1990,1236 : 13-17.
  • 3LAWRENCE D B, JOHN F, GARY A, et al.. Seeing studies on a 1.8 m mirror [J]. SPIE, 1990, 1236:492 506.
  • 4AKIHIKO M, RYUSUKE O, NARUHISA T, etal.. Temperature control for the primary mirror and seeing statistics of Subaru Telescope [J]. SPIE, 2003,4837 : 255-263.
  • 5TIMOTHY G H, ANDREW J A, TIMOTHY C C, et al.. Thermal performance and facility seeing at the upgraded 3.8 m UK Infrared Telescope (UKIRT) [J]. SPIE, 2000,4004 : 104-114.
  • 6FRANK G D, DAVID K, GARY A C, et al.. High-speed seeing measurements at the Keck Tele- scope [J]. SPIE,1994,2201,310-313.
  • 7CARL N, BYOUNG J S, MITCHELL T, etal.. Wavefront sensing and control performance modeling o the Thirty Meter Telescopes {or systematic trade analyses [J]. SPIE,2014,9150:91500S(1-10).
  • 8BYOUNG J S, CARL N, GEORGE A, etal.. A- nalysis for Normalized Point Source Sensitivity as a performance metric for the Thirty Meter Telescope [J]. SPIE,2008,7071 70170T.
  • 9GEORGE Z A, BYOUNG J S, CARL N, et al.. A convenient telescope performance metric for ima-ging through turbulence [ J ]. SPIE, 2011, 8127:812709.
  • 10POYNEER L A, DAM M V, VIRAN J P. Ex- perimental verification of the frozen flow atmos- pheric turbulence assumption with use of astro- nomical adaptive optics telemetry [J]. J. Opt. Soc. Am. A,2009,26(4)..833-846.

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