Processing of N-speckle images of astronomical objects

Details Processing of N-speckle images of astronomical objects Processing of N-speckle images of astronomical objects

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981svjqe...8..189b&link_type=abstract

Kvantovaia Elektronika (Moscow), vol. 8, Jan. 1981, p. 189, 190. In Russian.

Physics

Optics

1

Astronomical Photometry, Atmospheric Turbulence, Image Processing, Optical Correction Procedure, Speckle Patterns, Atmospheric Optics, Fourier Transformation, Turbulence Effects

Scientific paper

An approach to 'seeing' through a turbulent atmosphere is suggested which is based on the recording and processing of speckle images of an extended astronomical object. A modification of the Labeyrie speckle interferometry method is proposed which makes it possible to restore the image of the extended object, undistorted by the atmosphere, from its N-speckle images.

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