Compression of the current sheet and its impact into the reconnection rate

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dc.creatorVainshtein, S. I.
dc.creatorMikić, Z.
dc.creatorSagdeev, R.
dc.date2007-11-11
dc.date2007-11-14
dc.date.accessioned2026-07-07T08:42:32Z
dc.date.available2026-07-07T08:42:32Z
dc.descriptionNumerical simulations of strongly compressible MHD corresponding to a stellar atmosphere with substantial gravity and near force-free magnetic fields show that the current sheet collapses (its width decreasing substantially). As a result, the reconnection rate increases dramatically.
dc.description24 pages 10 figures, typos corrected
dc.identifierhttps://arxiv.org/abs/0711.1666
dc.identifierhttp://arxiv.org/abs/0711.1666
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/141991
dc.subjectAstrophysics
dc.titleCompression of the current sheet and its impact into the reconnection rate
dc.typetext

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