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Direct numerical simulation of dynamo transition for nonhelical MHD

Abstract:
Pseudospectral Direct Numerical Simulation (DNS) has been performed to simulate dynamo transition for nonhelical magnetohydrodynamics turbulence. The numerical results are compared with a recent low-dimensional model [Verma et al. [13]]. The forcing in DNS is the same as that used in the low-dimensional model. Dynamo transition is observed in DNS, but the forcing required for the transition is higher than that for the model. A qualitative similarity is observed between DNS and model results. The difference is due to the presence of large number of modes present in the DNS. © 2010 IOP Publishing Ltd.

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Publisher copy:
10.1088/1742-6596/208/1/012039

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Journal:
Journal of Physics: Conference Series More from this journal
Volume:
208
Pages:
012039-012039
Publication date:
2010-01-01
DOI:
EISSN:
1742-6596
ISSN:
1742-6588


Language:
English
Pubs id:
pubs:367580
UUID:
uuid:193c2396-641c-4032-94f2-bfa741456919
Local pid:
pubs:367580
Source identifiers:
367580
Deposit date:
2013-11-16
ARK identifier:

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