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The atmospheric temperature inhomogeneities are the main cause of the indexof refraction variations resulting in strong fluctuations of intensity of thelaser beams propagating through the atmosphere. It is shown that theKolmogorov-Bolgiano-Obukhov phenomenology of the thermal (buoyancy driven)convection can effectively describe this process in the frames of thedistributed chaos approach. Results of the direct numerical simulations andmeasurements in the urban atmosphere (based on the laser beams with thewavelengths of 532nm and 690nm) have been used in order to support thetheoretical considerations.

Strong chaotic fluctuations of laser beams propagating through temperature inhomogeneities in the atmosphere