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A shell model for turbulent dynamos.

Authors :
Nigro, G.
Perrone, D.
Veltri, P.
Source :
Proceedings of the International Astronomical Union; Sep2010 Supplement 274, Vol. 6 Issue S274, p159-161, 3p
Publication Year :
2010

Abstract

A self-consistent nonlinear dynamo model is presented. The nonlinear behavior of the plasma at small scale is described by using a MHD shell model for fields fluctuations; this allow us to study the dynamo problem in a large parameter regime which characterizes the dynamo phenomenon in many natural systems and which is beyond the power of supercomputers at today. The model is able to reproduce dynamical situations in which the system can undergo transactions to different dynamo regimes. In one of these the large-scale magnetic field jumps between two states reproducing the magnetic polarity reversals. From the analysis of long time series of reversals we infer results about the statistics of persistence times, revealing the presence of hidden long-time correlations in the chaotic dynamo process. [ABSTRACT FROM PUBLISHER]

Details

Language :
English
ISSN :
17439213
Volume :
6
Issue :
S274
Database :
Complementary Index
Journal :
Proceedings of the International Astronomical Union
Publication Type :
Academic Journal
Accession number :
61123117
Full Text :
https://doi.org/10.1017/S1743921311006818