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Mechanisms for Dynamo Mode Excitation
Published online by Cambridge University Press: 19 July 2016
Extract
Dynamo theory of the solar magnetic field finds itself in a period of reappraisal since about 1980. There are two reasons for this: (1) The required increase of the angular speed Ω, with decreasing r is neither found in numerical simulations nor measured by helioseismology. (2) Mean field modeling shows often little regard for inherent physical restrictions and selfconsistency.
- Type
- II. The Solar Interior
- Information
- Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 45 - 49
- Copyright
- Copyright © Kluwer 1990