Fast flow pattern associated with the dipolarization region: THEMIS observation

Details Fast flow pattern associated with the dipolarization region: THEMIS observation Fast flow pattern associated with the dipolarization region: THEMIS observation

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsm41b1719t&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SM41B-1719

Physics

[2740] Magnetospheric Physics / Magnetospheric Configuration And Dynamics, [2744] Magnetospheric Physics / Magnetotail

Scientific paper

Dipolarization is one of the most dramatic and key phenomena in the course of substorms. Spacecraft often observes fast flow signatures followed by the dipolarization with turbulent magnetic fluctuations. However, it is not clear whether such fast flows are independent of the dipolarization (thus can be a contributor for dipolarization) or result by the dipolarization. THEMIS multi-spacecraft sometimes provide the observation of tailward flows and/or azimuthally dominant flows associated with the dipolarization around 10 RE. In this study, we examine such flow patterns associated with the dipolarization and discuss their relation to the dipolarization.

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