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Turbulence belongs to the most widespread and, at the same time, the most complicated natural phenomena, related to the origin and development of organized structures (- dies of different scale) at a definite flow regime of fluids in essentially non-linear - drodynamic systems.
This book covers the development of continual models of turbulent natural media. Processes of self-organization are addressed in detail using irreversible thermodynamics and stochastic dynamics, and focusing on formation and evolution of protoplanetary discs.
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