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A flexible Monte Carlo program has been developed to simulate imaging through a turbulent atmosphere. We have applied this to conventional stellar speckle imaging and to the situation where an object is coherently illuminated and viewed after double passage through a random phase screen. We show that the timeaveraged image contains diffraction-limited information on the Fourier modulus of the object.
Christopher J. Solomon,Theo Mavroidis, andChristopher Dainty
"Monte Carlo simulations of coherent and incoherent imaging through atmospheric turbulence", Proc. SPIE 1319, Optics in Complex Systems, (1 July 1990); https://doi.org/10.1117/12.34803
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Christopher J. Solomon, Theo Mavroidis, Christopher Dainty, "Monte Carlo simulations of coherent and incoherent imaging through atmospheric turbulence," Proc. SPIE 1319, Optics in Complex Systems, (1 July 1990); https://doi.org/10.1117/12.34803