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1989•International Astronomical Union ColloquiumOpen access

Solar Magnetic Fields and Dynamo Process

Axel Brandenburg, I. Tuominen

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Abstract

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.

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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.

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Available abstract

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.

Key concepts: Dynamo, Helioseismology, Differential rotation, Solar dynamo, Dynamo theory, Physics, Convection zone, Rotation (mathematics)

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