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• W2017015981 abstract "The description of stellar turbulent convection requires a minimum of five coupled, time-dependent, nonlocal, differential equations for the five variables: turbulent kinetic energy, turbulent potential energy, turbulent pressure, convective flux, and energy dissipation. Any fewer number of equations makes the model local. In this paper, we present the following results:" @default.
• W2017015981 created "2016-06-24" @default.
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• W2017015981 date "1998-02-01" @default.
• W2017015981 modified "2023-09-23" @default.
• W2017015981 title "Stellar Turbulent Convection. I. Theory" @default.
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• W2017015981 doi "https://doi.org/10.1086/305141" @default.
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