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On the Stability of Magnetic Flux Tubes in the Equator of a Star
Published online by Cambridge University Press: 19 July 2016
Abstract
We consider the linear stability of a toroidal flux tube lying in the equatorial plane of a differentially rotating star and investigate its dependence on superadiabaticity, magnetic field strength, and gradient of angular velocity.
- Type
- 1. The Solar Dynamo
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- Copyright © Kluwer 1993