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- W4255115280 abstract "The problem of the existence, evolution, and stability of spatial structures in convection is of considerable importance to astrophysics as well as to geophysical hydrodynamics. The Boussinesq approximation will be used because the considered motions in stars are sufficiently slow. The system of hydrodynamic equations describing convection in a rotating inhomogeneous medium has the form: Here D t is the total time derivative, U the velocity, P, T , and C the deviations of the pressure, temperature, and helium abundance (by mass) from the basic equilibrium values, ρ m , ν m , χ m , and D m the values averaged over the considered layer of the density, viscosity, thermal and helium diffusivities, β T and β c the averaged coefficients of the thermal and helium expansions, g and Ω the gravitational acceleration and angular velocity, ∇ T b , and ∇ C b the values of the basic equilibrium temperature and helium gradients, and ñ T ad the adiabatic temperature gradient." @default.
- W4255115280 created "2022-05-12" @default.
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- W4255115280 date "1990-01-01" @default.
- W4255115280 modified "2023-09-25" @default.
- W4255115280 title "Convection and its Stability in the Equatorial Regions of the Convection Zone" @default.
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- W4255115280 doi "https://doi.org/10.1017/s0074180900044296" @default.
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