Convection And Its Stability In The Equatorial Regions Of The Convection Zone
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.
KeywordsRayleigh Number Spherical Shell Amplitude Equation Chemical Inhomogeneity Helium Abundance
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