Acta Optica Sinica, Volume. 21, Issue 2, 186(2001)
A New Method for Astronomical Image Reconstruction in Spatial Region: Iterative Shift-and-Add Technique
[3] [3] Labeyrie A. Attainment of diffraction limited resolution in large telescopes by Fourier analyzing speckle patterns in star images. Asrton. Astrophys., 1970, 6(1):85~87
[5] [5] Fienup J R. Reconstruction of an object from the modulus of its Fourier transform. Opt. Lett., 1978, 3(1):27~29
[6] [6] Knox K T, Thompson B J. Becovery of images from atmospherically degraded short-exposure photographs. Astron. J., 1974, 193(1):L45~L48
[7] [7] Lohmann A W, Weigelt G P, Wirnitzer B. Speckle masking in astronomy trible correlation theory and application. Appl. Opt., 1983, 22(24):4028~4037
[9] [9] Bates R H T, Cady F M. Towards true imaging by wideband speckle interferometry. Opt. Commun., 1980, 32(3):365~369
[10] [10] Ribak E. Astronomical images by filtered weighted shift-and-add technique. J. Opt. Soc. Am. (A), 1986, 3(12):2069~2076
[12] [12] Hunt B R, Fright W R, Bates R H. Analysis of the shift-and-add method for imaging through turbulent media. J. Opt. Soc. Am. (A), 1983, 73(4):456~465
Get Citation
Copy Citation Text
[in Chinese], [in Chinese], [in Chinese], [in Chinese]. A New Method for Astronomical Image Reconstruction in Spatial Region: Iterative Shift-and-Add Technique[J]. Acta Optica Sinica, 2001, 21(2): 186