Numerical Simulations of Magnetic Fields in Astrophysical Turbulence

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dc.creatorZweibel, Ellen G.
dc.creatorHeitsch, Fabian
dc.creatorFan, Yuhong
dc.date2002-02-28
dc.date.accessioned2026-07-25T11:43:27Z
dc.descriptionThe generation and evolution of astrophysical magnetic fields occurs largely through the action of turbulence. In many situations, the magnetic field is strong enough to influence many important properties of turbulence itself. Numerical simulation of magnetized turbulence is especially challenging in the astrophysical regime because of the high magnetic Reynolds numbers involved, but some aspects of this difficulty can be avoided in weakly ionized systems.
dc.description26 pages, 4 figures, accepted for "Simulations of magnetohydrodynamic turbulence in astrophysics" eds. T. Passot & E. Falgarone, Springer Lecture Notes in Physics
dc.identifierhttps://arxiv.org/abs/astro-ph/0202525
dc.identifierhttp://arxiv.org/abs/astro-ph/0202525
dc.identifierLect.Notes Phys. 614 (2003) 101-126
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/5087
dc.subjectAstrophysics
dc.titleNumerical Simulations of Magnetic Fields in Astrophysical Turbulence
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