On the thermodynamics of turbulent convection


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Abstract

The thermodynamic properties of a steady-state flow in the gravitational field have been determined by applying the entropy production equation and the Prigogine theorem to an ideal one-component turbulent gas under the assumption that fluctuations are polytropic. Applications to the problems of the surface layer dynamics and free convection are also considered.

About the authors

A. M. Krigel’

Editorial Board of Journal “Technical Physics,”

Author for correspondence.
Email: amkrigel@gmail.com
Russian Federation, ul. Mendeleevskaya 1, St. Petersburg, 199034


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