On- and off-axis statistical behavior of adaptive-optics-corrected short-exposure Strehl ratio.

Statistical behavior of the adaptive-optics- (AO-) corrected short-exposure point-spread function (PSF) is derived assuming a perfect correction of the phase's low spatial frequencies. Analytical expressions of the Strehl ratio (SR) fluctuations of on- and off-axis short-exposure PSFs are obtained. A theoretical expression of the short SR angular correlation is proposed and used to derive a definition of an anisoplanatic angle for AO-corrected images. Several applications of the analytical expressions are proposed: AO performance characterization, postprocessing imaging, light coupling into fiber, and exoplanet detection from a ground-based telescope.

[1]  Darryl P. Greenwood,et al.  Bandwidth specification for adaptive optics systems , 1977 .

[2]  Gerard Rousset,et al.  First diffraction-limited astronomical images with adaptive optics , 1990, Astronomical Telescopes and Instrumentation.

[3]  J. Goodman Statistical Properties of Laser Speckle Patterns , 1963 .

[4]  Laurent M. Mugnier,et al.  Deconvolution of adaptive optics images: from theory to practice , 2000, Astronomical Telescopes and Instrumentation.

[5]  Jean-Marc Conan,et al.  Etude de la correction partielle en optique adaptative , 1994 .

[6]  M P Cagigal,et al.  Rician distribution to describe speckle statistics in adaptive optics. , 1999, Applied optics.

[7]  H. Maître,et al.  Estimation of the adaptive optics long-exposure point-spread function using control loop data , 1997 .

[8]  F Roddier,et al.  On the origin of speckle boiling and its effects in stellar speckle interferometry , 1982 .

[9]  Thierry Fusco,et al.  VLT-"Planet Finder": specifications for a ground-based high contrast imager , 2002 .

[10]  Francois Rigaut,et al.  Adaptive optics on a 3.6-m telescope : results and performance , 1991 .

[11]  J. Conan,et al.  Wave-front temporal spectra in high-resolution imaging through turbulence , 1995 .

[12]  D. Fried Anisoplanatism in adaptive optics , 1982 .

[13]  F Roddier,et al.  On the isoplanatic patch size in stellar speckle interferometry , 1982 .

[14]  Horace W. Babcock,et al.  THE POSSIBILITY OF COMPENSATING ASTRONOMICAL SEEING , 1953 .

[15]  M P Cagigal,et al.  Speckle statistics in partially corrected wave fronts. , 1998, Optics letters.

[16]  F Cassaing,et al.  Coupling of large telescopes and single-mode waveguides: application to stellar interferometry. , 2001, Journal of the Optical Society of America. A, Optics, image science, and vision.

[17]  Gerard Rousset,et al.  Evaluation of Image Quality Obtained with Adaptive Optics Partial Correction , 1992 .

[18]  David Mouillet,et al.  Deconvolution of astronomical images obtained from ground-based telescopes with adaptive optics , 2003, SPIE Astronomical Telescopes + Instrumentation.

[19]  J. C. Dainty,et al.  Stellar Speckle Interferometry , 1976 .

[20]  David G. Sandler,et al.  Optimization and Performance of Adaptive Optics for Imaging Extrasolar Planets , 1995 .

[21]  L M Mugnier,et al.  Myopic deconvolution of adaptive optics images by use of object and point-spread function power spectra. , 1998, Applied optics.

[22]  T. Fusco,et al.  Myopic deconvolution method for adaptive optics images of stellar fields , 1999 .

[23]  Gerard Rousset,et al.  Angular correlation of Zernike polynomials for a laser guide star in adaptive optics , 1997 .

[24]  F. Chassat,et al.  Theoretical evaluation of the isoplanatic patch of an adaptive optics system working through the atmospheric turbulence , 1989 .

[25]  R. Noll Zernike polynomials and atmospheric turbulence , 1976 .

[26]  M. Roggemann Limited degree-of-freedom adaptive optics and image reconstruction. , 1991, Applied Optics.

[27]  Nicolas A. Roddier Atmospheric wavefront simulation using Zernike polynomials , 1990 .