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Dynamos of the Sun and Stars, and Associated Convection Zone Dynamics
1983
Symposium - International astronomical union
I see my assignment in this talk as being to focus on the interaction between the magnetic fields produced by dynamo action and the dynamics of the fluid flow which drives this dynamo, and to make some connections to the solar and stellar dynamo problems. To do this really requires we start with a fluid dynamical model that satisfies relevant laws of fluid dynamics, and in which the flow can actually respond to the induced magnetic field. Thus the so-called kinematic dynamo models are not
doi:10.1017/s0074180900029910
fatcat:n7e6rg6ztne57ej44cbaqpx4me