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- W1613751581 abstract "The evidence for convective penetration exhibited by geophysical fluids, laboratory experiments and computer simulations is recalled. A simple model is deduced from these observations, which serves to establish a relation between the subadiabatic extend L of a convective region and the velocity W of the penetrating motions: L ∞ W 3/2 . Assuming that this velocity obeys the usual scaling of thermal convection, it is found that the subadiabatic penetation at the bottom of a convective envelope is of the order of a pressure scale-height, and that above a convective core it amounts to a substantial fraction of the core radius" @default.
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- W1613751581 date "1991-12-01" @default.
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- W1613751581 title "Convective penetration in stellar interiors" @default.
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