“…This non-stationary nature of atmospheric turbulence has led to model optical scintillations as a conditional random process (Al-Habash et al, 2001;Churnside & Clifford, 1987;Churnside & Frehlich, 1989;Fante, 1975;Hill & Frehlich, 1997;Strohbehn, 1978;Wang & Strohbehn, 1974;de Wolf, 1974), in which the irradiance can be written as a product of one term that arises from large-scale turbulent eddy effects by a second term that represent the statistically independent small-scale eddy effects. One of the first attempts to gain wide acceptance for a variety of applications was the K distribution (Abdi & Kaveh, 1998;Jakerman, 1980) that provides excellent models for predicting irradiance statistics in a variety of experiments involving radiation scattered by turbulent media. The K distribution can be derived from a mixture of the conditional negative exponential distribution and a gamma distribution.…”