[1] Zhang Y, Liu H, Wu J, et al. Analysis and simulation of GIMS observation on dynamic targets[C]. Geoscience and Remote Sensing Symposium. IEEE, 2016:426-429.
[3] Chen L, Li Q, Yi G, and Zhu Y. 1-D mirrored interferometric aperture synthesis: performances, simulation, and experiments[J]. IEEE Tran. Geosci. Remote Sens., 2013, 51(5): 2960-2968.
[4] Chen L and Zhang X. 2-D mirrored interferometric aperture synthesis[C]. ISAPE2012,2012: 482-485.
[5] Zhu D, Hu F, Wu L, Li J, and Lang L. Low-redundancy linear arrays in mirrored interferometric aperture synthesis[J]. Optics Letters, 2015, 41(2):368-371.
[6] Li Y, Li Q, Jin R, et al. Array configuration optimization for Rotating mirrored aperture synthesis (RMAS)[C]. IEEE International Geoscience and Remote Sensing Symposium (IGARSS), 2016: 853-856.
[7] Li Q, Chen K, Guo W, et al. ESMAS: experiment system of mirrored aperture synthesis[C].IEEE International Geoscience and Remote Sensing Symposium (IGARSS),2016:2028-2031.
[8] Bertero M and Boccacci P. Introduction to Inverse Problems in Imaging[M]. London, U.K.: Inst. Physics, 1998.
[9] Butora R and Camps A, Noise maps in aperture synthesis radiometric images due to cross-correlation of visibility noise[J]. Radio Science, 2003, 38(4): 1067-1074.
[10] Dong J, Li Q, Zhu Y, et al. A method for seeking low-redundancy large linear arrays in aperture synthesis microwave radiometers[J]. IEEE Tran. Antennas. Propagat., 2010, 58(6):1913-1921.