Titlebook: Supernova Shells and Their Birth Events; Proceedings of a Wor Wolfgang Kundt Conference proceedings 1988 Springer-Verlag Berlin Heidelberg

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Richard G. Stromon-linear dynamo . The loss of magnetic energy is supposed to be due to buoyancy taking place in the neighborhood of the bottom of the convective zone. It is then assumed that the motion upwards of the flux tubes is taking place in a fluid having a high turbulent viscosity; (2) spin down. When carri

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D. K. Milne,J. L. Caswell,M. J. Kesteven,R. F. Haynes,R. S. Rogery occur on a resistive time-scale (i.e. with a growth rate that tends to zero as the magnetic resistivity of the medium tends to zero) in which case the dynamo is described as “slow”; or it may occur on the convective time-scale, in which case the dynamo is described as “fast”. The conventional desc

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D. A. Greenon-linear dynamo . The loss of magnetic energy is supposed to be due to buoyancy taking place in the neighborhood of the bottom of the convective zone. It is then assumed that the motion upwards of the flux tubes is taking place in a fluid having a high turbulent viscosity; (2) spin down. When carri

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M. de Muizon,R. G. Strom,M. J. A. Oort,J. J. Claas,R. Brauny occur on a resistive time-scale (i.e. with a growth rate that tends to zero as the magnetic resistivity of the medium tends to zero) in which case the dynamo is described as “slow”; or it may occur on the convective time-scale, in which case the dynamo is described as “fast”. The conventional desc

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W. Reich,N. Junkes,E. Fürsty occur on a resistive time-scale (i.e. with a growth rate that tends to zero as the magnetic resistivity of the medium tends to zero) in which case the dynamo is described as “slow”; or it may occur on the convective time-scale, in which case the dynamo is described as “fast”. The conventional desc

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