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Effects of a moving X-line in a time-dependent reconnection model
2007
Annales Geophysicae
<p><strong>Abstract.</strong> In the frame of magnetized plasmas, reconnection appears as an essential process for the description of plasma acceleration and changing magnetic field topology. Under the variety of reconnection regions in our solar system, we focus our research onto the Earth's magnetotail. Under certain conditions a Near Earth Neutral Line (NENL) is free to evolve in the current sheet of the magnetotail. Reconnection in this region leads to the formation of Earth- and tailward
doi:10.5194/angeo-25-293-2007
fatcat:x4bnbzamkzad5nwro5jafo27gm