2001
DOI: 10.1117/1.1386641
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Mathematical model for the irradiance probability density function of a laser beam propagating through turbulent media

Abstract: We develop a model for the probability density function (pdf) of the irradiance fluctuations of an optical wave propagating through a turbulent medium. The model is a two-parameter distribution that is based on a doubly stochastic theory of scintillation that assumes that small-scale irradiance fluctuations are modulated by large-scale irradiance fluctuations of the propagating wave, both governed by independent gamma distributions. The resulting irradiance pdf takes the form of a generalized K distribution th… Show more

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Cited by 1,035 publications
(668 citation statements)
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“…Other turbulence models such as the I-K [15] and the gamma-gamma [16] are all included in the negative exponential distribution in the limit of strong turbulence.…”
Section: B the Negative Exponential Modelmentioning
confidence: 99%
“…Other turbulence models such as the I-K [15] and the gamma-gamma [16] are all included in the negative exponential distribution in the limit of strong turbulence.…”
Section: B the Negative Exponential Modelmentioning
confidence: 99%
“…As such, it is an interesting problem to analyze the degradation of signal strength due to scintillation of the optical signal as well as link performance against atmospheric turbulence channels. In atmospheric turbulence channels, the coherence time of the channels is on the order of milliseconds, which is typically much larger than the one-bit time interval of gigabit-per-second (Gbps) FSO signals [6][7][8][9][10][11]. Hence, for a one-bit time interval, the FSO channels are modeled as a constant and random variable that is governed by a log-normal, K, or gamma-gamma distribution.…”
Section: Introductionmentioning
confidence: 99%
“…Hence, for a one-bit time interval, the FSO channels are modeled as a constant and random variable that is governed by a log-normal, K, or gamma-gamma distribution. The gamma-gamma distribution is a tractable mathematical model with a multiplication of two parameters of small-scale and large-scale irradiance fluctuations, the probability density functions (PDFs) of which are independent gamma distributions, and it provides excellent agreement between theoretical and simulation results [6][7][8].…”
Section: Introductionmentioning
confidence: 99%
“…As derived in Ref. [8], the Gamma-Gamma probability density function (PDF) of the irradiance I is given by…”
mentioning
confidence: 99%
“…In Eq. (9), the positive parameters α and β represent the effective number of large-scale and small-scale cells of the scattering process, respectively [8] . From Ref.…”
mentioning
confidence: 99%