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• W2967800110 abstract "Solar magnetism is believed to originate through dynamo action in the tachocline. Statistical mechanics, in turn, tells us that dynamo action is an inherent property of magnetohydrodynamic (MHD) turbulence, depending essentially on magnetic helicity. Here, we model the tachocline as a rotating, thin spherical shell containing MHD turbulence. Using this model, we find an expression for the entropy and from this develop the thermodynamics of MHD turbulence. This allows us to introduce the macroscopic parameters that affect magnetic self-organization and dynamo action, parameters that include magnetic helicity, as well as tachocline thickness and turbulent energy." @default.
• W2967800110 created "2019-08-22" @default.
• W2967800110 creator A5010977470 @default.
• W2967800110 date "2019-08-19" @default.
• W2967800110 modified "2023-09-28" @default.
• W2967800110 title "Magnetic Helicity and the Solar Dynamo" @default.
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• W2967800110 doi "https://doi.org/10.3390/e21080811" @default.
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