1975
DOI: 10.1007/bfb0111441
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Stellar speckle interferometry

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Cited by 96 publications
(127 citation statements)
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“…A much more useful prediction can be obtained from Berry's idea that a wavefunction of a chaotic system can be described as a random superposition of plane waves of the same wavenumber but different propagating direction. 36,37 Random plane wave (RPW) modeling gives predictions for both correlation functions above 36,38,39 which agree with the perturbation theory results for the diffusive regime: 35,40 ψ =⇒ e −|r The ψ correlation should thus approach 0, and the ψ 2 correlation should approach 1 for large r ′ . Figures 4 and 5 display our results for the diffusive regime, and show good agreement with the RPW predictions, especially in the ψ correlation.…”
Section: Simple Statistics: Agreement With Rmt/rpwsupporting
confidence: 66%
“…A much more useful prediction can be obtained from Berry's idea that a wavefunction of a chaotic system can be described as a random superposition of plane waves of the same wavenumber but different propagating direction. 36,37 Random plane wave (RPW) modeling gives predictions for both correlation functions above 36,38,39 which agree with the perturbation theory results for the diffusive regime: 35,40 ψ =⇒ e −|r The ψ correlation should thus approach 0, and the ψ 2 correlation should approach 1 for large r ′ . Figures 4 and 5 display our results for the diffusive regime, and show good agreement with the RPW predictions, especially in the ψ correlation.…”
Section: Simple Statistics: Agreement With Rmt/rpwsupporting
confidence: 66%
“…In the absence of movement (or for very short exposure time) there is no detectable fluctuation and the typical granular interference pattern, called speckle, has the same properties in the entire field of view. In the classical picture, summarized by Goodman in [9], the scattered field amplitudes are randomly distributed and consequently the intensity values follow a negative exponential distribution ( )…”
Section: Introductionmentioning
confidence: 99%
“…2). As shown in [12], the coherence function J J J(x 1 , x 2 ) is a weighted integral of a function M(η) that describes the illuminated area's shape at the scattering surface:…”
Section: Speckle Field Covariance and The Attenuation Maskmentioning
confidence: 99%