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Solar Magnetic Fields and Dynamo Process
Published online by Cambridge University Press: 27 September 2017
Abstract
We have computed kineamtic dynamo models for the Sun making realistic assumptions about the different induction effects. Recent results of helioseismology are used to infer the differential rotation. By changing the value of the angular velocity at the bottom of the convection zone in the models we find more or less agreement with the observations.
- Type
- Session III: Theory
- Information
- International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 369 - 372
- Copyright
- Copyright © Kluwer 1989