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astro-ph2002★ 190 cited
Coronal heating distribution due to low-frequency wave-driven turbulence
P. Dmitruk, W. H. Matthaeus, L. J. Milano +3
The heating of the lower solar corona is examined using numerical simulations and theoretical models of magnetohydrodynamic turbulence in open magnetic regions. A turbulent energy…
astro-ph2000★ 6 cited
What can we infer about the underlying physics from burst distributions observed in an RMHD simulation ?
N. W. Watkins, S. Oughton, M. P. Freeman
We determine that the sizes of bursts in mean-square current density in a reduced magnetohydrodynamic (RMHD)simulation follow power-law probability density function (PDF). The PDFs…