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Numerical simulation of the \(\alpha\)-effect and turbulent magnetic diffusion with molecular diffusivity. (English) Zbl 0601.76043

Summary: We extend the numerical methods of a previous paper [the first author, S. Duane and the second author, ibid. 138, 75-91 (1984; Zbl 0536.76084)] to the study of the \(\alpha\)-effect in a turbulent plasma. In the frozen-turbulence case the \(\alpha\)-effect vanishes for zero molecular diffusivity. The values of \(\alpha\) is, however, found to depend very sensitively on the molecular diffusivity. The same is true for the turbulent magnetic diffusivity \(\beta\). The theoretical predictions of the first-order smoothing and the Markovian approximations are well satisfied in the appropriate limits, for both \(\alpha\) and \(\beta\).

MSC:

76E25 Stability and instability of magnetohydrodynamic and electrohydrodynamic flows
76F99 Turbulence
76M99 Basic methods in fluid mechanics

Citations:

Zbl 0536.76084
Full Text: DOI

References:

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[2] Molchanov, Geophys. Astrophys. Fluid Dyn. 30 pp 242– (1984)
[3] Moffatt, Geophys. Astrophys. Fluid Dyn. 14 pp 147– (1979)
[4] DOI: 10.1017/S0022112076002875 · Zbl 0366.76042 · doi:10.1017/S0022112076002875
[5] Helfand, Bell. Syst. Tech. J. 58 pp 2289– (1979) · Zbl 0432.65073 · doi:10.1002/j.1538-7305.1979.tb02967.x
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[7] Drummond, J. Fluid Mech. 138 pp 75– (1984)
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