[1] [1] FIGOSKI J W.The QuickBird telescope:the reality of large,high-quality,commercial space optics[C].Proc of SPIE,3779:22～30.

[2] [2] RUBEN P L.Aberrations arising from decenterations and tilts[J].J Opt Soc Am,1964,54(1):45～52.

[3] [3] ROGERS J R.Vector aberration theory and the design of off-axis systems[C].Proc of SPIE,1985,554:76-81.

[4] [4] SASIAN J M,DESCOUR M R.Power distribution and symmetry in lens systems[J].Optical Engineering,1998,37(3):1001～1004.

[5] [5] EGDALL I M.Manufacture of a three-mirror wide-field optical system[J].Optical Engineering,1985,24(2):285～289.

[6] [6] FIGOSKI J W.Development of a three-mirror,wide-field sensor,from paper design to hardware[C].Proc of SPIE,1989,1113:126～131.

[7] [7] COOK L G.Wide field of view three-mirror anastigmat (TMA) employing spherical secondary and tertiary mirrors[C].Proc of SPIE,1987,766:158～162.

[8] [8] FIGOSKI J W.Aberration characteristics of nonsymmetric systems[C].Proc of SPIE,1985,554:104～111.

[9] [9] THOMPSON K.A graphic approach to the analysis of perturbed optical systems[C].Proc of SPIE,1980,237:127～134.

[10] [10] SHACK R V,Thompson K.Influence of alignment errors of a telescope system on its aberration field[C].Proc of SPIE,1980,251:146～153.

[11] [11] ROGERS J R.Design techniques for systems containing tilted components[C].Proc of SPIE,1999,3737:286～299.