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- W2127777433 abstract "Aims. We consider the stability of simple hydrodynamic models of the solar tachocline. This study addresses only the non-magnetic instabilities. In our model there is a strong radial shear, which because of the rotation is coupled to a latitudinal temperature gradient. We also assume there is a strong stable stratification, appropriate for the slow tachocline." @default.
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- W2127777433 date "2008-07-09" @default.
- W2127777433 modified "2023-09-24" @default.
- W2127777433 title "Hydrodynamic instabilities in the solar tachocline" @default.
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- W2127777433 doi "https://doi.org/10.1051/0004-6361:200810039" @default.
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