Two-dimensional disk dynamos with vertical outflows into a halo

dc.creatorvon Rekowski, B.
dc.creatorDobler, W.
dc.creatorShukurov, A.
dc.creatorBrandenburg, A.
dc.date2000-12-01
dc.date.accessioned2026-07-07T01:56:47Z
dc.date.available2026-07-07T01:56:47Z
dc.descriptionWe study the effects of vertical outflows on mean-field dynamos in disks. These outflows could be due to thermal winds or magnetic buoyancy. We analyse numerical solutions of the nonlinear mean-field dynamo equations using a two-dimensional finite-difference model. Contrary to expectations, a modest vertical velocity can enhance dynamo action. This can lead to super-exponential growth of the magnetic field and to higher magnetic energies at saturation in the nonlinear regime.
dc.description8 pages, 13 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0012013
dc.identifierhttp://arxiv.org/abs/astro-ph/0012013
dc.identifierin: Dynamo and Dynamics, a Mathematical Challenge (eds. P. Chossat, D. Armbruster and I.Oprea), NATO Science Series II/26, Kluwer Academic Publishers, p. 305 (2001)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2128
dc.subjectAstrophysics
dc.titleTwo-dimensional disk dynamos with vertical outflows into a halo
dc.typetext

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