2002•Geophysical Research LettersOpen access

Fast flow during current sheet thinning

Rumi Nakamura, W. Baumjohann, A. Runov, M. Volwerk, Tao Zhang, Berndt Klecker, Yulia V. Bogdanova, Antoine Roux, A. Balogh, Henri Rème, J. A. Sauvaud, H. U. Frey

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Abstract

In this paper we report Cluster observation of a fast flow event in the plasma sheet associated with a small auroral substorm intensification at 1838 UT on August 12, 2001. Cluster, located in the plasma sheet, experienced significant thinning of the current sheet associated with a high‐speed Earthward flow of 900 km/s. By using the four spacecraft magnetic field data and a Harris‐type current sheet model, it was estimated that the thickness of the current sheet changes from about 1 RE before the flow observation down to 400 km, i.e., close to the ion inertia length. In the vicinity of this thin current sheet there were also signatures of enhanced current density off the center of the neutral sheet, consistent with recent Geotail results.

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In this paper we report Cluster observation of a fast flow event in the plasma sheet associated with a small auroral substorm intensification at 1838 UT on August 12, 2001. Cluster, located in the plasma sheet, experienced significant thinning of the current sheet associated with a high‐speed Earthward flow of 900 km/s. By using the four spacecraft magnetic field data and a Harris‐type current sheet model, it was estimated that the thickness of the current sheet changes from about 1 RE before the flow observation down to 400 km, i.e., close to the ion inertia length. In the vicinity of this thin current sheet there were also signatures of enhanced current density off the center of the neutral sheet, consistent with recent Geotail results.

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Available abstract

In this paper we report Cluster observation of a fast flow event in the plasma sheet associated with a small auroral substorm intensification at 1838 UT on August 12, 2001. Cluster, located in the plasma sheet, experienced significant thinning of the current sheet associated with a high‐speed Earthward flow of 900 km/s. By using the four spacecraft magnetic field data and a Harris‐type current sheet model, it was estimated that the thickness of the current sheet changes from about 1 RE before the flow observation down to 400 km, i.e., close to the ion inertia length. In the vicinity of this thin current sheet there were also signatures of enhanced current density off the center of the neutral sheet, consistent with recent Geotail results.

Key concepts: Current sheet, Substorm, Plasma sheet, Current (fluid), Heliospheric current sheet, Physics, Flow (mathematics), Current density

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