How far can minimal models explain the solar cycle?

Autor:	Simitev, R. D., Busse, F. H.
Rok vydání:	2012
Předmět:	Astrophysics - Solar and Stellar Astrophysics Physics - Fluid Dynamics
Druh dokumentu:	Working Paper
DOI:	10.1088/0004-637X/749/1/9
Popis:	A physically consistent model of magnetic field generation by convection in a rotating spherical shell with a minimum of parameters is applied to the Sun. Despite its unrealistic features the model exhibits a number of properties resembling those observed on the Sun. The model suggests that the large scale solar dynamo is dominated by a non-axisymmetric $m=1$ component of the magnetic field. Comment: Accepted for publication in the Astrophysical Journal on 2012/01/30
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/1201.6227 Zobrazit plný text záznamu View this record from Arxiv