Simulation of stellar speckle imaging

Details Simulation of stellar speckle imaging Simulation of stellar speckle imaging

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2200..372j&link_type=abstract

Proc. SPIE Vol. 2200, p. 372-383, Amplitude and Intensity Spatial Interferometry II, James B. Breckinridge; Ed.

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Scientific paper

Standard FFT-based phase screen generation methods do not accurately model low-frequency turbulence characteristics. This paper introduces a new phase screen generation technique which uses low frequency subharmonic information to correct the problem. We compare our technique to two other subharmonic methods. The structure functions for this new method match very closely the structure functions of Kolmogorov turbulence theory.

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