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大口径轻量化主镜的温度场等效模型理论计算

谭玉凤 王继红 任戈 朱福音

强激光与粒子束2017,Vol.29Issue(6):5-11,7.
强激光与粒子束2017,Vol.29Issue(6):5-11,7.DOI:10.11884/HPLPB201729.160555

大口径轻量化主镜的温度场等效模型理论计算

Equivalent analytical calculation of the temperature field of the lightweighted primary mirror for large-aperture telescope

谭玉凤 1王继红 2任戈 3朱福音1

作者信息

  • 1. 中国科学院光电技术研究所,成都610209
  • 2. 中国科学院光束控制重点实验室,成都610209
  • 3. 中国科学院大学,北京100039
  • 折叠

摘要

Abstract

The thermal loads of ambient temperature and solar radiation around the telescope directly influence the temperature distribution within the primary mirror for a large-aperture telescope.Based on the unsteady heat conduction and boundary condition in the cylindrical coordinate system,the analytical temperature field for the primary mirror is calculated by separation of variables and Green's function method.To verify the theoretical model,the temperature distribution of a 2.8 m aperture solid mirror is calculated by the analytical solution.The calculated radial temperature distribution at the optical surface is in good agreement with those of FEA method,which reveal that the analytical solution can well reflect temperature distribution at the optical surface.A lightweighted mirror is equivalent to a thin mirror without ribs in the thermal analysis.The FEA analysis is conducted with both the mirror models,which verifies the validity of the equivalent model.The equivalent analytical calculation results of the temperature field for the lightweighted primary mirror have a significant reference value in the early design of the primary mirror for a large-aperture telescope.

关键词

大口径望远镜/轻量化主镜/非稳态导热/温度场

Key words

large-aperture telescope/lightweigbted mirror/unsteady heat conduction/temperature distribution

分类

能源科技

引用本文复制引用

谭玉凤,王继红,任戈,朱福音..大口径轻量化主镜的温度场等效模型理论计算[J].强激光与粒子束,2017,29(6):5-11,7.

基金项目

国家高技术发展计划项目 ()

强激光与粒子束

OA北大核心CSCDCSTPCD

1001-4322

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