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The Málaga distribution fading design is employed to model the statistical distribution of a spherical revolution propagating through anisotropic oceanic turbulence, which will be a versatile style of weak-to-strong turbulence. Initially, the scintillation index for a spherical wave propagating in oceanic turbulence is created, and closed-form expressions for the outage probability and average station capability associated with UWOC methods are then proposed when it comes to Mei

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