Physics
Scientific paper
Dec 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsm32b..04k&link_type=abstract
American Geophysical Union, Fall Meeting 2001, abstract #SM32B-04
Physics
2740 Magnetospheric Configuration And Dynamics, 2788 Storms And Substorms, 3220 Nonlinear Dynamics, 3230 Numerical Solutions
Scientific paper
Our recent analyses of electrojet index and Polar UVI image data have added to the evidence for self-organized criticality (SOC) in the magnetospheric dynamics. These analyses will be reviewed. The results support our earlier suggestion that this SOC component of the dynamics is centered in the plasma sheet and that it is related to the flow bursts and associated localized reconnections that have been observed there. It is necessary now to develop an interpretation of SOC in a plasma physical context. A plasma sheet model that may evolve into SOC will be discussed. The model contains a two-dimensional resistive MHD component coupled to a current driven instability that generates anomalous resistivity when and wherever the current density exceeds a critical threshold. In general terms, the model strongly couples fluid phenomena at MHD scales with kinetic phenomena at ion scales in an idealized manner. This strong coupling between such divergent scales introduces the possibility of multi-scale behavior in the intervening range of scales, and thus to the possibility of scale-free self-organized criticality. Numerical simulations of the plasma sheet model will be presented. The model exhibits quiet loading intervals interspersed with extremely dynamic unloading intervals during which magnetic flux is both annihilated and lost through plasmoid ejection. Based on the simulation results, a possible mechanism for the transition in the plasma sheet from sporadic localized reconnection to global organized reconnection at or near substorm onset will be discussed.
Baker Daniel N.
Klimas Alex J.
Uritsky Vadim
Vassiliadis Dimitris
Weigel Robert S.
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