Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2010-12-20
Advances in Plasma Astrophysics, ed. Proc. IAU, Vol. 6, IAU Symp. S274, pp. 473-475 (2011)
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
3 pages, 2 figures, proceedings of IAU Symp. 274, Advances in Plasma Astrophysics, ed. A. Bonanno, E. de Gouveia dal Pino and
Scientific paper
10.1017/S1743921311007538
A reduction of total mean turbulent pressure due to the presence of magnetic fields was previously shown to be a measurable effect in direct numerical simulations. However, in the studied parameter regime the formation of large-scale structures, as anticipated from earlier mean-field simulations, was not found. An analysis of the relevant mean-field parameter dependency and the parameter domain of interest is conducted in order to clarify this apparent discrepancy.
Brandenburg Axel
Kemel Koen
Kleeorin Nathan
Rogachevskii Igor
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