• Infrared and Laser Engineering
  • Vol. 37, Issue 2, 343 (2008)
[in Chinese]1、*, [in Chinese]1, [in Chinese]1, [in Chinese]1, [in Chinese]1, [in Chinese]2, and [in Chinese]2
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    [in Chinese], [in Chinese], [in Chinese], [in Chinese], [in Chinese], [in Chinese], [in Chinese]. Method of solving the initial structure of two-mirror reflecting system[J]. Infrared and Laser Engineering, 2008, 37(2): 343 Copy Citation Text show less
    References

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    [2] SPILLER E,McCORKLE R A,WILCZYNSKI J S,et al.Normal-incidence soft χ-ray telescopes[J].Opt Eng,1991,30(81:1109-1115.

    [3] HOOVER R B,BAKER P C,HADAWAY J B,et al.Performance of the Multi-Spectral Solar Telescope Array Ⅲ:Optical characteristics of the Ritchey-Chrétien and Cassegrain telescopes[C]//Proceedings of SPIE,X-ray/EUV optics for astronomy,microscopy,polarimetry,and projection lithography,1990,1343:189-202.

    [4] HANNAN P G.General analysis of two-mirror relay systems[J].Appl Opt,1992,31(4):513-518.

    [5] STAVROUDIS O N.Two-Mirror Systems with Spherical Reflecting Surfaces[J].Opt Soc Ant,1967,57(6):741-748.

    [6] BOTTEMA M,WOODRUFF A.Third Order Aberrations in Cassegrain-Type Telescopes and Coma Correction in Servo Stabilized Images[J].Appl Opt,1971,10(2):300-303.

    [7] ROSIN S.Inverse Cassegrain Systems[J].Appl Opt,1968,7(8):1485-1498.

    [8] SCHROEDER D J.Selected Papers on Astronomical Optics[M].Bellingham:Optical Engineering Press,1993:81-96.

    [11] SMITH W J.Modern Optical Engineering[M].New York:McGraw Hill Book Company,2000:330.

    [12] CHEN Bo,GONG Yan,NI Qi 4iang.A complex solar X-ray and EUV imaging telescope design[J].Telescopes and Instrumentation for Solar Astrophysicsv,2004,5171:155-159.

    [in Chinese], [in Chinese], [in Chinese], [in Chinese], [in Chinese], [in Chinese], [in Chinese]. Method of solving the initial structure of two-mirror reflecting system[J]. Infrared and Laser Engineering, 2008, 37(2): 343
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