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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.
Original language | English |
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Pages (from-to) | 561-564 |
Number of pages | 4 |
Journal | Advances in Space Research |
Volume | 26 |
Issue number | 3 |
DOIs | |
State | Published - 9 Mar 2000 |
ID: 53087225