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Detailed Reference Information |
Scholer, M. and Lottermoser, R.-F. (1998). On the kinetic structure of the magnetotail reconnection layer. Geophysical Research Letters 25: doi: 10.1029/98GL52510. issn: 0094-8276. |
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The structure of the reconnection layer in the magnetotail is studied by solving the Riemann problem of the decay of a current sheet with a normal magnetic field component using 2-D hybrid and Hall MHD simulations. In the first run a segment of the reconnection layer obtained from a hybrid simulation of reconnection is used as initial state in a periodic system. The thin central current sheet becomes instable in the direction parallel to the current sheet: the electrical current becomes filamentary and a warped magnetic field structure develops. In a second run, where the initial state is a Harris sheet with a superposed normal magnetic field component, a similar behavior is found. In both cases the boundary of the layer is not bounded by slow mode switch-off shocks and no large-amplitude rotational wave train develops within the layer, in contrast to 1-D hybrid simulations of the same Riemann problem. The corresponding 2-D Hall MHD simulation results in a stable layer bounded by slow-mode switch-off shocks. ¿ 1998 American Geophysical Union |
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Abstract |
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Keywords
Space Plasma Physics, Magnetic reconnection, Space Plasma Physics, Numerical simulation studies, Magnetospheric Physics, Numerical modeling, Magnetospheric Physics, Magnetotail |
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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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