Initiation of ballooning instability in the near-Earth plasma sheet prior to the 23 March 2007 THEMIS substorm expansion onset

In this work, we analyze the ballooning stability of the near-Earth plasma sheet prior to the initial expansion onset of the 23 March 2007 THEMIS substorm event. Using solar wind data from WIND satellite observation for the substorm event as an input at dayside, we reconstructed a sequence of gl...

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Main Authors: P. Zhu, J. Raeder, K. Germaschewski, C. C. Hegna
Format: Article
Language:English
Published: Copernicus Publications 2009-03-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/27/1129/2009/angeo-27-1129-2009.pdf
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author P. Zhu
J. Raeder
K. Germaschewski
C. C. Hegna
author_facet P. Zhu
J. Raeder
K. Germaschewski
C. C. Hegna
author_sort P. Zhu
collection DOAJ
description In this work, we analyze the ballooning stability of the near-Earth plasma sheet prior to the initial expansion onset of the 23 March 2007 THEMIS substorm event. Using solar wind data from WIND satellite observation for the substorm event as an input at dayside, we reconstructed a sequence of global magnetospheric configurations around the expansion onset by means of OpenGGCM simulation. These simulations have reproduced most of the salient features, including the onset timing, observed in the THEMIS substorm event (Raeder et al., 2008). The ballooning instability criterion is evaluated using eigenvalue analyses for the near-Earth plasma sheet region when the configuration attains a quasi-static equilibrium condition prior to the onset. Our analysis of the evolution of the near-Earth magnetotail region during the substorm growth phase (10:10 UT to 10:43 UT) reveals a correlation between the breaching of the ballooning stability condition and the initial expansion onset in the temporal domain. The analysis indicates that the ballooning instability is at first initiated by the stretching of closed field lines near the region with a local nonzero minimum in normal component of magnetic field (<I>B<sub>z</sub></I>&gt;0) associated with the formation of a bipolar-flow pattern in the near-Earth plasma sheet around 10 <I>R<sub>E</sub></I>. The subsequent initiation of ballooning instability with enhanced growth rate occurs (about 28 min later) on those most stretched closed field lines Earthward of the neutral line following the formation and the tailward recession of a plasmoid.
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spelling doaj.art-1b8f267d5e98450bab02a98901803aac2022-12-21T17:33:34ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762009-03-01271129113810.5194/angeo-27-1129-2009Initiation of ballooning instability in the near-Earth plasma sheet prior to the 23 March 2007 THEMIS substorm expansion onsetP. Zhu0J. Raeder1K. Germaschewski2C. C. Hegna3Department of Engineering Physics, University of Wisconsin-Madison, Madison, WI 53706, USADepartment of Physics, University of New Hampshire, Durham, NH 03824, USADepartment of Physics, University of New Hampshire, Durham, NH 03824, USADepartment of Engineering Physics, University of Wisconsin-Madison, Madison, WI 53706, USAIn this work, we analyze the ballooning stability of the near-Earth plasma sheet prior to the initial expansion onset of the 23 March 2007 THEMIS substorm event. Using solar wind data from WIND satellite observation for the substorm event as an input at dayside, we reconstructed a sequence of global magnetospheric configurations around the expansion onset by means of OpenGGCM simulation. These simulations have reproduced most of the salient features, including the onset timing, observed in the THEMIS substorm event (Raeder et al., 2008). The ballooning instability criterion is evaluated using eigenvalue analyses for the near-Earth plasma sheet region when the configuration attains a quasi-static equilibrium condition prior to the onset. Our analysis of the evolution of the near-Earth magnetotail region during the substorm growth phase (10:10 UT to 10:43 UT) reveals a correlation between the breaching of the ballooning stability condition and the initial expansion onset in the temporal domain. The analysis indicates that the ballooning instability is at first initiated by the stretching of closed field lines near the region with a local nonzero minimum in normal component of magnetic field (<I>B<sub>z</sub></I>&gt;0) associated with the formation of a bipolar-flow pattern in the near-Earth plasma sheet around 10 <I>R<sub>E</sub></I>. The subsequent initiation of ballooning instability with enhanced growth rate occurs (about 28 min later) on those most stretched closed field lines Earthward of the neutral line following the formation and the tailward recession of a plasmoid.https://www.ann-geophys.net/27/1129/2009/angeo-27-1129-2009.pdf
spellingShingle P. Zhu
J. Raeder
K. Germaschewski
C. C. Hegna
Initiation of ballooning instability in the near-Earth plasma sheet prior to the 23 March 2007 THEMIS substorm expansion onset
Annales Geophysicae
title Initiation of ballooning instability in the near-Earth plasma sheet prior to the 23 March 2007 THEMIS substorm expansion onset
title_full Initiation of ballooning instability in the near-Earth plasma sheet prior to the 23 March 2007 THEMIS substorm expansion onset
title_fullStr Initiation of ballooning instability in the near-Earth plasma sheet prior to the 23 March 2007 THEMIS substorm expansion onset
title_full_unstemmed Initiation of ballooning instability in the near-Earth plasma sheet prior to the 23 March 2007 THEMIS substorm expansion onset
title_short Initiation of ballooning instability in the near-Earth plasma sheet prior to the 23 March 2007 THEMIS substorm expansion onset
title_sort initiation of ballooning instability in the near earth plasma sheet prior to the 23 march 2007 themis substorm expansion onset
url https://www.ann-geophys.net/27/1129/2009/angeo-27-1129-2009.pdf
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AT kgermaschewski initiationofballooninginstabilityinthenearearthplasmasheetpriortothe23march2007themissubstormexpansiononset
AT cchegna initiationofballooninginstabilityinthenearearthplasmasheetpriortothe23march2007themissubstormexpansiononset