Multiframe phase-diversity algorithm for active imaging.
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A multiframe phase-diversity algorithm for imaging through the turbulent atmosphere tailored to the statistics of coherent light is developed and presented. The problem is posed as a maximum likelihood estimation where pupil-plane intensity data and atmospheric statistics are used to regularize the inverse problem. Reconstruction results characterized by residual mean square error are presented for varying detection parameters. The resulting algorithm appears to be robust under detection noise processes and results in significant improvement of processed images.
[1] R. Noll. Zernike polynomials and atmospheric turbulence , 1976 .
[2] Brian J. Thelen,et al. MAXIMUM A POSTERIORI ESTIMATION OF FIXED ABERRATIONS, DYNAMIC ABERRATIONS,AND THE OBJECT FROM PHASE-DIVERSE SPECKLE DATA , 1999 .
[3] James R. Fienup,et al. Joint estimation of object and aberrations by using phase diversity , 1992 .
[4] Steven G. Johnson,et al. The Design and Implementation of FFTW3 , 2005, Proceedings of the IEEE.