“…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].…”