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Solar Magnetic Fields and Dynamo Process

Published online by Cambridge University Press:  27 September 2017

A. Brandenburg and
I. Tuominen
A. Brandenburg
Affiliation:
Observatory and Astrophysics Laboratory, University of Helsinki, Tahtitorninmäki, SF-00130 Helsinki, Finland
I. Tuominen
Affiliation:
Observatory and Astrophysics Laboratory, University of Helsinki, Tahtitorninmäki, SF-00130 Helsinki, Finland

Abstract

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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.

Information

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

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