Numerical simulations of turbulent dynamos

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dc.creatorBrandenburg, Axel
dc.date2000-10-24
dc.date.accessioned2026-07-07T01:56:12Z
dc.date.available2026-07-07T01:56:12Z
dc.descriptionUsing a periodic box calculation it is shown that, owing to helicity conservation, a large scale field can only develop on a resistive timescale. This behaviour can be reproduced by a mean-field dynamo with alpha and eta_t quenchings that are equally strong and `catastrophic'.
dc.description3 Pages LaTex, to appear in proceedings of the 24th IAU General Assembly, Joint Discussion 14 "The Origins of Galactic Magnetic Fields"
dc.identifierhttps://arxiv.org/abs/astro-ph/0010495
dc.identifierhttp://arxiv.org/abs/astro-ph/0010495
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1911
dc.subjectAstrophysics
dc.titleNumerical simulations of turbulent dynamos
dc.typetext

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