[1] PRIMOT J,ROUSSET G,FOUNTANELLA J.Deconvolution from wave-front sensing:a new technique for compensating turbulence-degraded images[J].J Opt Soc Am A,1990,7:1598-1609.
[2] HAGERTY S P,YOUNG J M,PECK C S,et al.Analytical comparison of pre-detection,post-detection,and hybrid image compensation techniques in the presence of atmospheric turbulence[C]//Proceedings of SPIE,Hybrid Image and Signal ProcessingⅣ,1994,2238:31-41.
[3] ROGGEMANN M C,WELSH B M.Signal-to-noise ratio for astronomical imaging by deconvolution from wave-front sensing[J].Appl Opt,1994,33:5400-5414.
[4] ROGGEMANN M C,WELSH B M.Biased estimators and objectspectrum estimation in the method of deconvolution from wavefront sensing[J].Appl Opt,1994,33:5754-5763.
[5] ROGGEMANN M C,WELSH B M.Signal-to-noise ratio for astronomical imaging by deconvolution from wave-front sensing[J].Appl Opt,1994,33:5400-5414.
[6] WELSH B M,ROGGEMANN M C.Signal-to-noise comparison of deconvolution from wave-front sensing with traditional linear and speckle image reconstruction[J].Appl Opt,1995,34:2111-2118.
[7] DAYTON D,GONGLEWSKI J,ROGERS S.Experimental measurements of estimator bias and the signal-to-noise ratio for deconvolution from wave-front sensing[J].Appl Opt,1997,36:3895-3903.
[8] FORD S D,WELSH B M,ROGGEMANN M C.Constrained least-squares estimation in deconvolution from wave-front sensing[J].Opt Commun,1998,151:93-100.
[9] RIMMELE T R,RADICK R R.Deconvolution solar images using a Shack-Hartmann wavefront sensor[C]// Proceedings of SPIE,Adaptive Optical System Technologies,1998,3353:1014-1021.
[10] LAURENT M M,CLELIA R,JEAN-MARC C,et al.Myopic deconvolution from wave-front sensing[J].J Opt Soc Am A,2001,18:862-872.
[11] PRIMOT J.Theoretical description of Shark-Hartmann wavefront sensor[J].Opt Commun,2003,222:81-92.
