Flux transport solar dynamo models, current problems and possible solutions

Details Flux transport solar dynamo models, current problems and possible solutions Flux transport solar dynamo models, current problems and possible solutions

2008-12-05

arxiv.org/abs/0812.1169v1

Astronomy and Astrophysics

Astrophysics

To appear in the proceedings of the Magnetic Field in the Universe 2 conference, Cozumel, Mexico, January 28th to February 1st

Scientific paper

The sunspot solar cycle has been usually explained as the result of a dynamo process operating in the sun. This is a classical problem in Astrophysics that until the present is not fully solved. Here we discuss current problems and limitations with the solar dynamo modeling and their possible solutions using a kinematic dynamo model within the Babcock-Leighton approximation as a tool. In particular, we discuss the importance of the turbulent magnetic pumping versus the meridional flow circulation in the dynamo operation.

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