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Mechanisms for Dynamo Mode Excitation

Published online by Cambridge University Press:  19 July 2016

P. Hoyng
P. Hoyng*
Affiliation:
Laboratory for Space Research Sorbonnelaan 2, 3584 CA Utrecht The Netherlands

Extract

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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 

References

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