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Research Articles
Submitted on May 14, 2008 Tail Reconnection Triggering Substorm Onset
1 IGPP/ESS, UCLA, Los Angeles, CA, USA. * To whom correspondence should be addressed.
Magnetospheric substorms explosively release solar wind energy previously stored in Earths magnetotail, encompassing the entire magnetosphere and producing spectacular auroral displays. It has been unclear whether a substorm is triggered by a disruption of the electrical current flowing across the near-Earth magnetotail, at ~10 RE (RE = Earth Radius, or 6374 km), or by the process of magnetic reconnection typically seen farther out in the magnetotail, at ~20 to 30 RE. We report on simultaneous measurements in the magnetotail at multiple distances, at the time of substorm onset. Reconnection was observed at 20 RE, at least 1.5 min before auroral intensification, at least 2 min before near-Earth current disruption, and about 3 min before substorm expansion. These results demonstrate that substorms are likely initiated by tail reconnection.
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Science. ISSN 0036-8075 (print), 1095-9203 (online)