On Generation of magnetic field in astrophysical bodies

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dc.creatorVerma, Mahendra K.
dc.date2001-12-09
dc.date.accessioned2026-07-07T06:22:43Z
dc.date.available2026-07-07T06:22:43Z
dc.descriptionIn this letter we compute energy transfer rates from velocity field to magnetic field in MHD turbulence using field-theoretic method. The striking result of our field theoretic calculation is that there is a large energy transfer rate from the large-scale velocity field to the large-scale magnetic field. We claim that the growth of large-scale magnetic energy is primarily due to this transfer. We reached the above conclusion without any linear approximation like that in $α$-dynamo.
dc.description4 pages, Revtex, 1 figure
dc.identifierhttps://arxiv.org/abs/nlin/0112013
dc.identifierhttp://arxiv.org/abs/nlin/0112013
dc.identifierCurr.Sci. 85 (2002) 620
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/95995
dc.subjectChaotic Dynamics
dc.subjectAstrophysics
dc.subjectCondensed Matter
dc.titleOn Generation of magnetic field in astrophysical bodies
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