Forced magnetic reconnection -: art. no. L06105

被引:92
作者
Birn, J [1 ]
Galsgaard, K
Hesse, M
Hoshino, M
Huba, J
Lapenta, G
Pritchett, PL
Schindler, K
Yin, L
Büchner, J
Neukirch, T
Priest, ER
机构
[1] Los Alamos Natl Lab, Space & Atmospher Sci Grp, Los Alamos, NM 87545 USA
[2] Niels Bohr Inst Astron Phys & Geophys, DK-2100 Copenhagen, Denmark
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[4] Univ Tokyo, Dept Earth & Planetary Phys, Bunkyo Ku, Tokyo 1130033, Japan
[5] USN, Res Lab, Washington, DC 20375 USA
[6] Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
[7] Ruhr Univ Bochum, Inst Theoret Phys, D-44780 Bochum, Germany
[8] Max Planck Inst Sonnensyst Forsch, D-37191 Katlenburg Lindau, Germany
[9] Univ St Andrews, Sch Math & Stat, St Andrews KY16 9SS, Fife, Scotland
关键词
D O I
10.1029/2004GL022058
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Using a multi-code approach, we investigate current sheet thinning and the onset and progress of fast magnetic reconnection, initiated by temporally limited, spatially varying, inflow of magnetic flux. The present study extends an earlier collaborative effort into the transition regime from thick to thin current sheets. Again we find that full particle, hybrid, and Hall-MHD simulations lead to the same fast reconnection rates, apparently independent of the dissipation mechanism. The reconnection rate in MHD simulations is considerably larger than in the earlier study, although still somewhat smaller than in the particle simulations. All simulations lead to surprisingly similar final states, despite differences in energy transfer and dissipation. These states are contrasted with equilibrium models derived for the same boundary perturbations. The similarity of the final states indicates that entropy conservation is satisfied similarly in fluid and kinetic approaches and that Joule dissipation plays only a minor role in the energy transfer.
引用
收藏
页码:1 / 5
页数:5
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