Development of a space soft X-ray and EUV normal incidence telescope

CHEN Bo; NI Qi-liang; CAO Ji-hong; GONG Yan; CAO Jian-lin

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Development of a space soft X-ray and EUV normal incidence telescope

更新时间：2020-08-12

- Development of a space soft X-ray and EUV normal incidence telescope
- Optics and Precision Engineering Vol. 11, Issue 4, Pages: 315-319(2003)
- 作者机构：
  
  中国科学院, 长春光学精密机械与物理研究所, 应用光学国家重点实验室,吉林长春,130022
- 作者简介：
- 基金信息：
- DOI：
  CLC： TN305.7
- Received：16 January 2003，
  
  Revised：19 June 2003，
  
  Published Online：15 August 2003，
  
  Published：15 August 2003
- 稿件说明：
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陈波, 尼启良, 曹继红, 巩岩, 曹健林. 空间软X射线/极紫外波段正入射望远镜研究[J]. 光学精密工程, 2003,(4): 315-319

CHEN Bo, NI Qi-liang, CAO Ji-hong, GONG Yan, CAO Jian-lin. Development of a space soft X-ray and EUV normal incidence telescope[J]. Editorial Office of Optics and Precision Engineering, 2003,(4): 315-319
陈波, 尼启良, 曹继红, 巩岩, 曹健林. 空间软X射线/极紫外波段正入射望远镜研究[J]. 光学精密工程, 2003,(4): 315-319 DOI：

CHEN Bo, NI Qi-liang, CAO Ji-hong, GONG Yan, CAO Jian-lin. Development of a space soft X-ray and EUV normal incidence telescope[J]. Editorial Office of Optics and Precision Engineering, 2003,(4): 315-319 DOI：

摘要

介绍国际上空间软X射线/极紫外波段正入射望远镜研究进展情况。着重介绍了长春光机所设计的四波段同时成像空间极紫外太阳望远镜。该望远镜由四个不同波长的多层膜正入射望远镜组成

工作波长分别为12.9nm、17.1nm、19.5nm和30.4nm

视场角为8.5′×8.5′

设计角分辨率为0.5″。为了验证设计方案可行性及关键技术水平

集成出一套17.1nm极紫外望远镜演示样机。

Abstract

While the progress in researches on space soft X-ray and EUV normal incidence telescopes world wide is reviewed

the space EUV normal incidence telescope designed and developed by Changchun institute of optics

fine mechanics and physics (CIOMP)

is emphatically detailed. The telescope has four individual channels of multilayer coating normal incident optics with working wavelengths of 12.9 nm

17.1 nm

19.5 nm and 30.4 nm. The field of view and angular resolution are 0.2° and 0.5″

respectively. The telescope is capable of simultaneously imaging the sun at the four wavelengths.

关键词

Keywords

references

ARTHUR B C, WALKER J R, JOAKIN F, et al. High resolution imaging with multilayer soft X-ray, EUV and FUV telescopes of modest aperture and cost[J].SPIE, 1991,1494:320.

HOOVER R B, BAKER P H, HADAWAY J B, et al.Performance of the multi-spectral solar telescope array[J]. SPIE,1990,1343:189.

HADAWAU J B,JOHNSON R B. Design and analysis of optical systems for the Stanford/MSFC multi-special solar telescope array[J].SPIE,1989,1160:195.

HARVEY J E, ZMEK W P,FTACLAS C. Imaging capabilities of normal-incidence X-ray telescope[J].Optical Engineering,1990,29(6):603-608.

空间极紫外太阳望远镜系列报告[R].中国科学院长春光学精密机械与物理研究所,1999.Space extreme ultra-violet telescope document[R].Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences.1999.

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CHEN Bo

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WANG Zhichen

LI Hongwen

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Related Institution

State Key Laboratory of Applied Optics,Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033,China

University of Chinese Academy of Sciences

Changchun Institute of Optics，Fine Mechanics and Physics，Chinese Academy of Sciences

Advanced Laser Technology Laboratory of Anhui Province

University of Science and Technology of China

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