[1] DOMINGO V.Soho,Yohkoh,UIysses and trace:the four solar missions in perspective and available resources[J].Astrophysics and Space Science,2002,282:171-188

[2] HANDY B N.ACTON L W,KANKELBORG C C,et al..The transition region and coronal explorer[J].Solar Physics,1999,187:229-260

[3] DEFISE J M,MOSES J D,CATURA R C,et al..Calibration of EIT instrument for the SOHO mission[J].SPIE,1995,2517:29-39

[5] CHEN B,NI Q L,WANG J L.Soft X-ray and extreme ultraviolet optics in CIOMP[J].Opt.Precision Eng.,2007,15(12):1862-1868

[6] COLLETTE J P,STOCKMAN Y,TOCK J P,et al..Performance of the XMM optical vertical test facility[J].SPIE,1996,2808:350-361

[7] BRAEUNINGER H,BURKERT W,HARTNER G D,et al..Calibration of hard X-ray(15～50keV)optics at the MPE test facility PANTER[J].SPIE,2004,5168:283-293

[8] KIM E D,CHIO Y W,KNAG M S,et al..Lessons learned from the optics and focal plane alignment of a wide field of view RC telescope[J].SPIE,2005,5877:1

[10] GORE D B,HADAWAY J B,HOOVER R B,et al..Optical focusing and alignment of the multi-spectral solar telescope array Ⅱ payload[J].SPIE,1995,2515:532-542