1987
DOI: 10.1103/physrevlett.59.285
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Intensity correlation functions and fluctuations in light scattered from a random medium

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Cited by 221 publications
(130 citation statements)
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“…1 Several authors have considered this contribution in a reflection geometry. 3,12,[27][28][29][30] The angular C (2) correlation is inversely proportional to the illumination area, and is expected to be negligibly small for the geometry of our experiment. In contrast, the near-field correlation in reflection is a local effect on a length scale of order , which does not vanish for plane-wave illumination.…”
Section: Discussionmentioning
confidence: 99%
“…1 Several authors have considered this contribution in a reflection geometry. 3,12,[27][28][29][30] The angular C (2) correlation is inversely proportional to the illumination area, and is expected to be negligibly small for the geometry of our experiment. In contrast, the near-field correlation in reflection is a local effect on a length scale of order , which does not vanish for plane-wave illumination.…”
Section: Discussionmentioning
confidence: 99%
“…Substituting eq. ( 17) in this expression leads after some algebra to the following result, assuming Bi = 0 and dS = 8:…”
Section: Enhanced Backscatteringmentioning
confidence: 99%
“…Defining a correlation length, δr, as the first zero of C 1 gives δr = π/k = λ/2. The intensity is correlated far beyond δr as a result of scattering within the medium [2,3,4,5,6,7] so that intensity values in remote speckle spots are not statistically independent. This gives rise to two additional contributions to C, which can therefore be expressed as, C = C 1 + C 2 + C 3 [3,8], and leads to greatly enhanced mesoscopic fluctuations [9].…”
mentioning
confidence: 99%