Title of article
Energy balance during bursty reconnection Original Research Article
Author/Authors
V.S. Semenov، نويسنده , , N.N. Volkonskaya، نويسنده , , H.K Biernat، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2000
Pages
4
From page
561
To page
564
Abstract
In this paper we study the energy budget during magnetic reconnection. To this end, we concentrate on time-varying reconnection. Our considerations are based on the generalization of the Petschek model for a time varying reconnection rate. For the sake of simplicity, we consider a 2D asymmetric current sheet configuration with an incompressible plasma. Under these circumstances, the reconnection problem can be formulated in an analytical way, and a particularly clear insight can be gained. It turns out that as a result of the fast motion of the outflow region, magnetic energy is accumulated external to its leading front, whereas it is rarefied in the wake region.
Journal title
Advances in Space Research
Serial Year
2000
Journal title
Advances in Space Research
Record number
1127029
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