Sequential diversity imaging of extended sources

Sequential diversity imaging uses images from a video camera outfitted with an adaptive optic (AO) to improve the images of an extended object. Phase changes introduced by the AO provide the diversity. The technique estimates both the object and the time-varying wavefront introduced by the optical medium, including atmospheric distortion and changes in the camera. The wavefront estimate is used to control the AO and no other wavefront sensing mechanism is needed. We show computer simulations in which the imagery is improved by about a factor of three, provided that the AO changes are made about ten times faster than changes in the medium. Any camera with adaptive focus and digital processing could use the method.

[1]  Michael Lloyd-Hart,et al.  Sensing wave-front amplitude and phase with phase diversity. , 2002, Applied optics.

[2]  N. C. Gallagher,et al.  Method for Computing Kinoforms that Reduces Image Reconstruction Error. , 1973, Applied optics.

[3]  J. Dorband,et al.  Hubble Space Telescope Faint Object Camera calculated point-spread functions. , 1997, Applied optics.

[4]  R G Paxman,et al.  Phase-diversity correction of turbulence-induced space-variant blur. , 1994, Optics letters.

[5]  Robert A. Gonsalves,et al.  On Optimal Holographic Filters , 1974, Other Conferences.

[6]  Nicolas A. Roddier,et al.  Curvature Sensing: A New Wavefront Sensing Method , 1988, Optics & Photonics.

[7]  J R Fienup,et al.  Reconstruction of an object from the modulus of its Fourier transform. , 1978, Optics letters.

[8]  J. Elon Graves,et al.  University of Hawaii adaptive optics system: III. Wavefront curvature sensor , 1991, Optics & Photonics.

[9]  M. Teague Deterministic phase retrieval: a Green’s function solution , 1983 .

[10]  James R. Fienup,et al.  Optical misalignment sensing and image reconstruction using phase diversity , 1988 .

[11]  K. Mutoh,et al.  Measurement of telescope aberrations through atmospheric turbulence by use of phase diversity. , 2001, Applied optics.

[12]  F. Roddier,et al.  Wave-front reconstruction from defocused images and the testing of ground-based optical telescopes , 1993 .

[13]  Alan M. Title,et al.  Preparation of a Dual Wavelength Sequence of High-Resolution Solar Photospheric Images Using Phase Diversity , 1998 .

[14]  D. S. Acton,et al.  Phase-diversity wave-front sensor for imaging systems. , 1994, Applied optics.

[15]  Juan Antonio Quiroga Mellado,et al.  Wavefront measurement by solving the irradiance transport equation for multifocal systems , 2001 .

[16]  Piotr Kiedron Phase Retrieval Method Using Differential Filters , 1983, Other Conferences.

[17]  J. Krist,et al.  Phase-retrieval analysis of pre- and post-repair Hubble Space Telescope images. , 1995, Applied optics.

[18]  M C Roggemann,et al.  Diagnosing unknown aberrations in an adaptive optics system by use of phase diversity. , 1997, Optics letters.

[19]  Robert A. Gonsalves,et al.  Phase retrieval by differential intensity measurements , 1987 .

[20]  W. Southwell,et al.  Wave-front analyzer using a maximum likelihood algorithm , 1977 .

[21]  R. Gonsalves Phase retrieval from modulus data , 1976 .

[22]  Robert A. Gonsalves,et al.  Phase Retrieval And Diversity In Adaptive Optics , 1982 .

[23]  Gordon D. Love,et al.  Phase diversity experimental results : deconvolution of ν Scorpii , 1996 .

[24]  J. H. Seldin,et al.  Hubble Space Telescope characterized by using phase-retrieval algorithms. , 1993, Applied optics.

[25]  A. Papoulis Systems and transforms with applications in optics , 1981 .

[26]  Robert A. Gonsalves,et al.  Wavefront Sensing By Phase Retrieval , 1979, Optics & Photonics.

[27]  R A Gonsalves,et al.  Nonisoplanatic imaging by phase diversity. , 1994, Optics letters.

[28]  James R. Fienup,et al.  Phase retrieval for undersampled broadband images , 1999 .

[29]  Robert A. Gonsalves Adaptive Optics by Sequential Diversity Imaging , 2002 .