The helicity constraint in spherical shell dynamos
classification
🌌 astro-ph
keywords
sphericalconstraintdimensionaldynamoshelicityshellsimulationsaccounts
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The motivation for considering distributed large scale dynamos in the solar context is reviewed in connection with the magnetic helicity constraint. Preliminary accounts of 3-dimensional direct numerical simulations (in spherical shell segments) and simulations of 2-dimensional mean field models (in spherical shells) are presented. Interesting similarities as well as some differences are noted.
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