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Cross-tail Current Evolution During Substorm Dipolarization : Volume 31, Issue 6 (27/06/2013)

By Lui, A. T. Y.

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Book Id: WPLBN0004002199
Format Type: PDF Article :
File Size: Pages 12
Reproduction Date: 2015

Title: Cross-tail Current Evolution During Substorm Dipolarization : Volume 31, Issue 6 (27/06/2013)  
Author: Lui, A. T. Y.
Volume: Vol. 31, Issue 6
Language: English
Subject: Science, Annales, Geophysicae
Collections: Periodicals: Journal and Magazine Collection (Contemporary), Copernicus GmbH
Historic
Publication Date:
2013
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications

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Y. Lu, A. T. (2013). Cross-tail Current Evolution During Substorm Dipolarization : Volume 31, Issue 6 (27/06/2013). Retrieved from http://members.worldlibrary.net/


Description
Description: Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723-6099, USA. We examine evolution of the cross-tail current during substorm current disruption/dipolarization using observations from two satellites in the near-Earth magnetotail at the downtail distances of 8–9 RE. By choosing times when these two satellites are separated, mainly in the north–south distance in the tail current sheet, precise determination of current density in the layer embedded between these satellites can be obtained with Ampère's law. Two such events are examined and several common features are found. The current densities in the layer embedded by the two satellites were reduced by ~ 40–70% during substorm dipolarization. The changes in current densities have the fast kinetic timescale, i.e., in seconds, implying a kinetic process for current disruption/dipolarization. The estimated power within the current layer was mainly dissipative in the dawn–dusk direction and mainly dynamo in the Sun–tail direction that is needed to drive the north–south substorm current system in the ionosphere. Remote sensing of the energization site with the ion sounding technique shows that the energization site was initially earthward of the satellite and moved down the tail at later times. Breakdown of the frozen-in condition occurred intermittently during the disturbance interval. These features provide important clues to the substorm onset process.

Summary
Cross-tail current evolution during substorm dipolarization

Excerpt
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