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• W3105330113 startingPage "70" @default.
• W3105330113 abstract "We consider the generation of magnetic activity --- dynamo waves --- in the astrophysical limit of very large magnetic Reynolds number. We consider kinematic dynamo action for a system consisting of helical flow and large-scale shear. We demonstrate that large-scale dynamo waves persist at high $Rm$ if the helical flow is characterised by a narrow band of spatial scales and the shear is large enough. However for a wide band of scales the dynamo becomes small-scale with a further increase of $Rm$, with dynamo waves re-emerging only if the shear is then increased. We show that at high $Rm$ the key effect of the shear is to suppress small-scale dynamo action, allowing large-scale dynamo action to be observed. We conjecture that this supports a general suppression principle --- large-scale dynamo action can only be observed if there is a mechanism that suppresses the small-scale fluctuations." @default.
• W3105330113 created "2020-11-23" @default.
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• W3105330113 date "2014-06-17" @default.
• W3105330113 modified "2023-09-26" @default.
• W3105330113 title "ON LARGE-SCALE DYNAMO ACTION AT HIGH MAGNETIC REYNOLDS NUMBER" @default.
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• W3105330113 doi "https://doi.org/10.1088/0004-637x/789/1/70" @default.
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