A THEMIS multicase study of dipolarization fronts in the magnetotail plasma sheet

被引:303
作者
Runov, A. [1 ]
Angelopoulos, V. [1 ]
Zhou, X-Z. [1 ]
Zhang, X. -J. [1 ]
Li, S. [1 ]
Plaschke, F. [3 ]
Bonnell, J. [2 ]
机构
[1] Univ Calif Los Angeles, Inst Geophys & Planetary Sci, Los Angeles, CA 90095 USA
[2] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[3] Tech Univ Carolo Wilhelmina Braunschweig, Inst Geophys & Extraterrestr Phys, D-38106 Braunschweig, Germany
关键词
TEST PARTICLE ORBITS; SUBSTORM; SIMULATION; FLOW; INJECTIONS; CLUSTER; FIELDS; INSTRUMENT; EVENTS; TAIL;
D O I
10.1029/2010JA016316
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss results of a superposed epoch analysis of dipolarization fronts, rapid (delta t < 30 s), high-amplitude (delta B-z > 10 nT) increases in the northward magnetic field component, observed during six Time History of Events and Macroscale Interactions during Substorms (THEMIS) conjunction events. All six fronts propagated earthward; time delays at multiple probes were used to determine their propagation velocity. We define typical magnetic and electric field and plasma parameter variations during dipolarization front crossings and estimate their characteristic gradient scales. The study reveals (1) a rapid 50% decrease in plasma density and ion pressure, (2) a factor of 2-3 increase in high-energy (30-200 keV) electron flux and electron temperature, and (3) transient enhancements of similar to 5 mV/m in duskward and earthward electric field components. Gradient scales of magnetic field, plasma density, and particle flux were found to be comparable to the ion thermal gyroradius. Current densities associated with the B-z increase are, on average, 20 nA/m(2), 5-7 times larger than the current density in the cross-tail current sheet. Because j . E > 0, the dipolarization fronts are kinetic-scale dissipative regions with Joule heating rates of 10% of the total bursty bulk flow energy.
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页数:15
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