Computer simulation of a method for object reconstruction from stellar speckle interferometry data

Details Computer simulation of a method for object reconstruction from stellar speckle interferometry data Computer simulation of a method for object reconstruction from stellar speckle interferometry data

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apopt..21.3132w&link_type=abstract

Applied Optics, vol. 21, Sept. 1, 1982, p. 3132-3137.

Physics

Optics

24

Computerized Simulation, Image Reconstruction, Interferometry, Speckle Patterns, Stellar Atmospheres, Turbulence Effects, Angular Resolution, Atmospheric Turbulence, Fourier Transformation, High Resolution, Image Processing, Stellar Magnitude, Telescopes, Wave Diffraction

Scientific paper

A method for reconstructing a diffraction-limited image from data consisting of many short-exposure turbulence degraded images is described. The results of a computer simulation of the method are presented. The method should prove useful for obtaining high-angular resolution images from large earth bound telescopes. The simulation indicates that the method may be applicable to astronomical objects as faint as about the 11th magnitude.

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