Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003padeu..13...89s&link_type=abstract
In: Contributions to NATO Advanced Research Workshop Turbulence, Waves, and Instabilities in the Solar Plasma; Hungary, 16-20 Se
Astronomy and Astrophysics
Astronomy
Scientific paper
The dynamo action of unstable magnetic flux tubes due to magnetic
buoyancy in a rotating stellar convection zone is summarized and the
implications of a flux tube dynamo with a threshold in field strength
for dynamo action is discussed in connection with the observed
variability of solar and stellar magnetic activity.
Ferriz-Mas Antonio
Schmitt Denis
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