Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-11-29
Astronomy and Astrophysics
Astrophysics
31 pages, 5 figures, submitted to ApJ
Scientific paper
Dynamical studies of MHD turbulence on the one hand, and arguments based upon magnetic helicity on the other, have yielded seemingly contradictory estimates for the $\alpha$ parameter in turbulent dynamo theory. Here we show, with direct numerical simulation of three-dimensional magnetohydrodynamic turbulence with a mean magnetic field, $\OB$, that the constraint on the dynamo $\alpha$-effect set by the magnetic helicity is time-dependent. A time-scale $t_c$ is introduced such that for $t
Chou Hongsong
Field George B.
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