Thesis Detail
Abstract The optical signal propagating through an atmospheric optical channel is affected by fluctuations in both intensity and phase due to variations in the refractive index. The fluctuations in the received optical intensity is called scintillation. At this point, the main research effort is specially based on avoiding the harmful effects of the scintillation which can produce severe link performance degradation. In this sense, different mathematical models have been proposed to describe the model of the probability density function (PDF) of the received irradiance. A unifying statistical distribution, the Málaga or M model was proposed some years ago including the previous distributions as particular cases of the M model. The performance of the M distribution are all obtained assuming that the smallscale parameter is a natural number, due to the involvement of using an infinite summation in the generalized case. This thesis is presents a reformulation of the Malaga distribution. The behavior of the atmospheric optical channel is formed here as a superposition of the finite number of generalized-K distributed sub-channels, controlled by a discrete negative-binomial distribution dependent on the turbulence parameters. Also including a novel method to truncate the infinite sum into a finite one, letting the analysis of the AOC channel with real values of the small-scale parameter, thus providing a wider adaptability. In any case, new completely accurate expressions for the ergodic capacity, the outage probability and the outage rate of the system are obtained here as system parameters, and conditional BER, and average BER as channels parameters. Furthermore, numerical results show a perfect alignment with our derived analytical expressions. Contact Us
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