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Showing 1 to 1 of 1 for “"Tachokline"”.
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Formation and stability of the solar tachocline in MHD simulations
The solar tachocline is a thin transition layer between the solar radiative zone rotating uniformly and the solar convection zone, which has a mainly latitudinal differential rotation profile. This layer has a thickness of less than $0.05R_{\sun}$ and is subject to extreme radial as well as …