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Dynamo Action in Accretion Disks

Published online by Cambridge University Press:  19 July 2016

Ulf Torkelsson*
Affiliation:
Lund Observatory, Box 43, S-221 00 Lund, Sweden

Abstract

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Employing the standard theory for thin accretion disks I estimate the relevant parameters for a dynamo in an accretion disk. These estimates could then be compared to the results of numerical simulations. Some preliminary results of such simulations (Torkelsson & Brandenburg 1992) are presented too.

Type
5. Magnetic Field Generation in Accretion Disks
Copyright
Copyright © Kluwer 1993 

References

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