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The THEMIS Mission

The THEMIS mission aims to determine the trigger and large-scale evolution of substorms by employing five identical micro-satellites which line up along the Earth's magnetotail to track the motion of particles, plasma, and waves from one point to another and for the first time, resolve space-ti...

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Detalles Bibliográficos
Autores principales: Burch, J. L, Angelopoulos, V
Lenguaje:eng
Publicado: Springer 2009
Materias:
Acceso en línea:https://dx.doi.org/10.1007/978-0-387-89820-9
http://cds.cern.ch/record/1338951
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author Burch, J. L
Angelopoulos, V
author_facet Burch, J. L
Angelopoulos, V
author_sort Burch, J. L
collection CERN
description The THEMIS mission aims to determine the trigger and large-scale evolution of substorms by employing five identical micro-satellites which line up along the Earth's magnetotail to track the motion of particles, plasma, and waves from one point to another and for the first time, resolve space-time ambiguities in key regions of the magnetosphere on a global scale. The primary goal of THEMIS is to elucidate which magnetotail process is responsible for substorm onset at the region where substorm auroras map: (i) local disruption of the plasma sheet current (current disruption) or (ii) the interaction of the current sheet with the rapid influx of plasma emanating from reconnection. The probes also traverse the radiation belts and the dayside magnetosphere, allowing THEMIS to address additional baseline objectives. This volume describes the mission, the instrumentation, and the data derived from them.
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spelling cern-13389512021-04-22T01:02:41Zdoi:10.1007/978-0-387-89820-9http://cds.cern.ch/record/1338951engBurch, J. LAngelopoulos, VThe THEMIS MissionAstrophysics and AstronomyThe THEMIS mission aims to determine the trigger and large-scale evolution of substorms by employing five identical micro-satellites which line up along the Earth's magnetotail to track the motion of particles, plasma, and waves from one point to another and for the first time, resolve space-time ambiguities in key regions of the magnetosphere on a global scale. The primary goal of THEMIS is to elucidate which magnetotail process is responsible for substorm onset at the region where substorm auroras map: (i) local disruption of the plasma sheet current (current disruption) or (ii) the interaction of the current sheet with the rapid influx of plasma emanating from reconnection. The probes also traverse the radiation belts and the dayside magnetosphere, allowing THEMIS to address additional baseline objectives. This volume describes the mission, the instrumentation, and the data derived from them.Springeroai:cds.cern.ch:13389512009
spellingShingle Astrophysics and Astronomy
Burch, J. L
Angelopoulos, V
The THEMIS Mission
title The THEMIS Mission
title_full The THEMIS Mission
title_fullStr The THEMIS Mission
title_full_unstemmed The THEMIS Mission
title_short The THEMIS Mission
title_sort themis mission
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1007/978-0-387-89820-9
http://cds.cern.ch/record/1338951
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