Image deconvolution from wavefront sensing: atmospheric turbulence simulation cell results.

Details Image deconvolution from wavefront sensing: atmospheric turbulence simulation cell results. Image deconvolution from wavefront sensing: atmospheric turbulence simulation cell results.

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988vlti....2..683p&link_type=abstract

ESO Conference on Very Large Telescopes and their Instrumentation, Vol. 2, p. 683 - 692

Computer Science

Methods Of Observation: Imaging

Scientific paper

A new technique is described for high resolution imaging through the atmospheric turbulence. As in speckle interferometry, short-exposure images are recorded, but in addition the associated wavefronts are measured by a Hartmann-Shack wavefront sensor. The knowledge of the wavefront allows the calculation of the point spread function. An estimate of the object can be computed from the correlation of image and point spread function.

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