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We perform direct numerical simulations of three-dimensional freely decaying magnetohydrodynamic turbulence. For helical magnetic fields, an inverse cascade effect is observed in which power is transferred from smaller scales to larger scales. The magnetic field reaches a scaling regime with self-similar evolution, and power-law behavior at high wave numbers. We also find power-law decay in the magnetic and kinematic energies, and power-law growth in the characteristic length scale of the magnetic field.
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Mattias Christensson
University of Sussex
Mark Hindmarsh
University of Helsinki
Axel Brandenburg
Stockholm University
Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics
Newcastle University
University of Sussex
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Christensson et al. (Mon,) studied this question.
synapsesocial.com/papers/6a15684cb2e0231f158271d1 — DOI: https://doi.org/10.1103/physreve.64.056405
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