Abstract
Magnetic reconnection is one of the fundamental macro processes in space and laboratory plasma systems. However, so far applications to large scale astrophysical plasmas are relatively few. This work attempts to shed some light on problems with respect to such applications. This particularly involves three-dimensional and turbulent or random occurrence of magnetic reconnection. A crucial question for reconnection in a very large scale system is the following. If reconnection is triggered in a single small region in a very extended current layer, how does it evolve in time? Does this region remain localized or does the reconnection region expand and if so, in what manner? To examine this problem we present results where reconnection is triggert in a single spot in an initially one-dimensional current layer.
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Otto, A. (1999). Three-Dimensional Magnetic Reconnection In Astrophysical Plasmas — Mhd Approach. In: Büchner, J., Axford, I., Marsch, E., Vasyliūnas, V. (eds) Plasma Astrophysics And Space Physics. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4203-8_3
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DOI: https://doi.org/10.1007/978-94-011-4203-8_3
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