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Detailed Reference Information |
Fu, S.Y., Pu, Z.Y. and Liu, Z.X. (1995). Vortex-induced magnetic reconnection and single X line reconnection at the magnetopause. Journal of Geophysical Research 100: doi: 10.1029/94JA02898. issn: 0148-0227. |
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Vortex-induced magnetic reconnection (VIMR) and bursty single X line reconnection (BSXR) at the magnetopause are studied using two-dimensional MHD simulation. The VIMR and BSXR occur when the flow-aligned Alfv¿n Mach number is greater or less, respectively, than a critical value which typically ranges from 0.3 to 0.6 for different anomalous resistance conditions. In the former case, the streamlines and magnetic field lines are in alignment and construct a concentric vortical pattern, whereas in the latter case, magnetic field lines do not form closed loops, and vortices occur around the X line. The topological structure of the asymptotic quasi-steady state of 2-D reconnection depends strongly upon the topological invariants such as the cross helicity. The different sites where VIMR and BSXR work at the magnetopause to form flux transfer events are discussed. ¿ American Geophysical Union 1995 |
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Abstract |
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Keywords
Space Plasma Physics, Magnetic reconnection, Magnetospheric Physics, Solar wind/magnetosphere interactions, Magnetospheric Physics, Magnetopause, cusp, and boundary layers, Space Plasma Physics, Numerical simulation studies |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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