2014
DOI: 10.1080/17455030.2013.874055
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The dependence of the intensity PDF of a random beam propagating in the maritime atmosphere on source coherence

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Cited by 16 publications
(8 citation statements)
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“…1 In our experiment, we generated the pseudo MGSM beams with phase screen realizations on an SLM with resolution of 256 x 256 pixels. Reference [9] describes the general process that we used for generating the SLM phase screens. To summarize the method: a 256 x 256 random matrix with Gaussian statistics and zero mean is convolved with a Multi-Gaussian window function of the form of Eq.…”
Section: Generation Of Pseudo Multi-gaussian Schell Model Beamsmentioning
confidence: 99%
“…1 In our experiment, we generated the pseudo MGSM beams with phase screen realizations on an SLM with resolution of 256 x 256 pixels. Reference [9] describes the general process that we used for generating the SLM phase screens. To summarize the method: a 256 x 256 random matrix with Gaussian statistics and zero mean is convolved with a Multi-Gaussian window function of the form of Eq.…”
Section: Generation Of Pseudo Multi-gaussian Schell Model Beamsmentioning
confidence: 99%
“…where factor B is introduced to meet the first of conditions (11), n μ are of the form (13) or (21) starting summation, say, from the most inner frame, n a are the weights. Figure 7 shows some combinations of frames with different symmetries.…”
Section: Frame Combinationsmentioning
confidence: 99%
“…We note that for our modeling of the frames the specification of the source intensity distribution is not necessary, since the far-zone intensity distribution is independent from it. There are at least two general methods for practical realization of the random sources with prescribed correlations, one based on the field modulation by a spatial light modulator [11] and the other on the modulation of the intensity in the Fourier plane [12].…”
Section: Introductionmentioning
confidence: 99%
“…The ability of beams radiated by random sources to mitigate scintillations (intensity fluctuations) on their propagation in turbulent atmosphere has been known for several decades via theoretical results and computer simulations 1-5 and mesuarements [6][7] . In all the aforementioned references the tested beams are supposed to be produced by Gaussian Schellmodel sources, i.e.…”
Section: Introductionmentioning
confidence: 99%