[1] HOLMES R B,MA S,BHOWMIK A,et al.. Aperture-synthesis techniques that use very-low-power illumination[J]. SPIE,1995,2566:177-185. [2] HOLMES R B,MA S,BHOWMIK A,et al.. Analysis and simulation of a synthetic-aperture technique for imaging through a turbulent medium[J]. JOSA A,1996,13(2):351-364. [3] FORD S D,VOELZ D G, GEO V L. Light Imaging National Testbed(GLINT)past, present, and future[J]. SPIE,1999,3815:2-10. [4] BELEN'KII M S. Coherence degradation of a speckle field and turbulence effects on Fourier telescopy imaging system[J]. SPIE,2002,4489:48-59. [5] BELEN'KII M S,HUGHES K,BRINKLEY T,et al.. Effect of turbulence on downlink and horizontal path on high-order coherence moments in Fourier telescopy system[J]. SPIE,2002,4821:62-73. [6] CUELLAR E L,STAPP J,COOPER J. Laboratory and field experimental demonstration of a fourier telescopy imaging system[J]. SPIE,2005,5896:58960D/1-58960D/15. [7] 董磊,刘欣悦,王建立. 实验室环境内傅里叶望远镜技术的实现[J]. 光学 精密工程 ,2008,16(6):999-1002. DONG L,LIU X Y,WANG J L. The realization of Fourier telescope technology in laboratory[J]. Opt. Precision Eng.,2008,16(6):999-1002 [8] SPIVEY B,STAPP J,SANDLER D. Phase closure and object reconstruction algorithm for Fourier telescopy applied to fast-moving targets[J]. SPIE,2006,630702/1-630702/16. [9] STAPP J,SPIVEY B,CHEN L. Simulation of a Fourier telescopy imaging system for objects in low earth orbit[J]. SPIE,2006,6307:630701/1-630701/11. [10] CUELLAR E L,COOPER J,MATHIS J. Laboratory demonstration of a multiple beam Fourier telescopy imaging system[J]. SPIE,2008,7094:70940G/1-70940G/12.