[1] [1] STOVER J C. Optical Scattering-measurement and Analysis［M］. SPIE Press,1995.

[2] [2] HARVEY J E, KRYWONONS A, STOVER J C. Unified scatter model for rough surface at large incident and scattered angles［J］. SPIE, 2007, 6672: 66720C1-C8.

[3] [3] MARTINEZ-GALARCE D S, BOERNER P, SOUFLI R, et al..The high-resolution lightweight telescope for the EUV (HiLiTE)［J］. SPIE, 2008,7011:70113k-1-12.

[4] [4] MARTINEZ-GALARCE D S, WALKER A B C, GORE D B, et al.. High resolution imaging with multilayer telescope: resolution performance of the MSSTAⅡ telescopes［J］.Opt. Precision Eng., 2000,39(4): 1063-1079.

[5] [5] DEFISE J M, MOSES J D,CATURA R C. Calibration of EIT instrument for the SOHO mission［J］.SPIE,1995,2517: 29-39.

[6] [6] CHEN B, NI Q L, CAO J H, et al.. Development of a space soft X-ray and EUV normal incidence telescope［J］. Opt. Precision Eng., 1999,7(5):89-94.(in Chinese)

[7] [7] 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.

[8] [8] GAO L. Study on the technique of alignment and imaging performance test of EUV solar telescope［D］. Beijing：Chinese Academy of Sciences, 2009:24-34.(in Chinese)

[9] [9] THOMPSON P L, HARVEY J E. System engineering analysis of aplanatic Wolter typeⅠX-ray telescopes［J］.Opt. Precision Eng.,2000,39:1677-1691.

[10] [10] LCHURCH E，TAKACS P Z. Light scatteringfrom non-Gaussian surface［J］. SPIE, 1995,2541：91-107.

[11] [11] NICODEMUS F E. Reflectance nomenclature and directional reflectance and emissivity［J］. Applied Optics, 1970,9：1474-1475.

[12] [12] GULLIKSON E M. Scattering from normal incidence EUV optics［J］. SPIE, 1998,3331：72-80.

[13] [13] CHURCH E L. Fractal surface finishparameters［J］. Applied Optics, 1988,27:1518-1526.

[14] [14] HARVEY J E, CHOI N, KRYWONONS A. Calculation BRDFs from surface PSDs for moderately rough optical surface［J］. SPIE, 2010, 7426：7426011-7426019.

[15] [15] DITTMAN M G. K-correlation power spectral density & surface scatter model［J］. SPIE, 2010, 6291：62910R1-R12.

[16] [16] GANGADHARA S. How to model surface scattering via the K-correlation distribution［R］. http://www.Zemax.com/KB

[17] [17] HARVERY J E, ZMEK W P, FTACLAS C. Imaging capabilities of normal-incidence X-ray telescope［J］. Opt. Precision Eng., 1990, 29: 603-608.

[18] [18] WALKER B C, LINDBLOM J F, ONEAL R H, et al.. Multi-spectral solar telescope array［J］. Optical Engineering, 1990, 29: 581-591.

[19] [19] PODGORSKI W A, CHEIMETS P N, BOERNER P. et al.. SDO-AIA mirror performance［J］. SPIE, 2009, 7438：74380F1-F13.