[2] [2] Pierre Cruzalebes. Optical Simulation of a 5 Apertures Spectro-interferometer for IMAOINO[A]. Proc. ESO/NOAO[C], 1988,757-767.

[3] [3] Mozurkewich D. Array layout and Beam Combination Considerations Necessary For Imaging with a Long Baseline Optical Interferometer[A]. Proc. ESO/NOAO[C]1988,801-804.

[4] [4] Jennison R C. A phase Sensitive interferometer technique for the measurement of the fourier transforms of spatial brightness distributions of small angular extent[J]. MNRAS, 1958, 118(3):276-284.

[5] [5] Rogstad D H. A Technique for Measuring Visibility Phase with an Optical Interferometer in the Presence of Atmospheric Seeing[J]. Appl Opt,1968,7(4):585-588.

[6] [6] Rhodes W T, Goodman J W. Interferometric technique for recording and restoring images degraded by unknown aberrations[J]. J. OPT. Soc. Am. A, 1973,63(6):647-657.

[7] [7] Baldwin J E, Haniff C A, Mackay C D. Close phase in high resolution optical imaging[J]. Nature,1986,320(17):595-597.

[8] [8] Baldwin J E, Beckett M G, Boysen R C, et al. The first images from an opticalaperture synthesis array: mapping of Capella with COAST at two epochs[J].A and A,1996,306,13-16.

[9] [9] Monnier J D. An introduction to Closure phases[A].Principle of Long Baseline Stellar Interferometry. NASA Report. 2000[C]. Edited by P.R. Lawson,2000,203-230.

[10] [10] Cornwell T J. A novel principle for optimization of the instantaneous Fourier plane coverage of correlation arrays[J]. IEEE transaction on antennas and propagation, 1988,36(8):1165-1167.

[12] [12] Monnier J D. Infrared interferomtry and spectroscpy of circumstellar envelope[D], Ph.D thesis, University of California at Berkeley, 1999.