Pressure changes associated with substorm depolarization in the near-Earth plasma sheet

We have studied plasma (ion) pressure changes that occurred in association with the dipolarization in the near‐Earth plasma sheet around substorm onsets. Using Geotail data, we have performed a superposed epoch analysis in addition to detailed examinations of two individual cases with special emphas...

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Published inJournal of Geophysical Research: Space Physics Vol. 115; no. A12
Main Authors Miyashita, Y., Machida, S., Ieda, A., Nagata, D., Kamide, Y., Nosé, M., Liou, K., Mukai, T., Christon, S. P., Russell, C. T., Shinohara, I., Saito, Y.
Format Journal Article
LanguageEnglish
Published Blackwell Publishing Ltd 01.12.2010
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ISSN0148-0227
2156-2202
DOI10.1029/2010JA015608

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Abstract We have studied plasma (ion) pressure changes that occurred in association with the dipolarization in the near‐Earth plasma sheet around substorm onsets. Using Geotail data, we have performed a superposed epoch analysis in addition to detailed examinations of two individual cases with special emphasis on the contribution of high‐energy particles to the plasma pressure. It is found that, unlike previously reported results, the plasma pressure does increase in association with the initial dipolarization at X > ∼−12 RE and −2 < Y < 6 RE, with the increase largely due to high‐energy particles. Outside the initial dipolarization region, particularly tailward and duskward of this region, the plasma pressure begins to decrease owing to the magnetic reconnection before onset or before the dipolarization region reaches there. At later times, the plasma pressure tends to increase there, related to the expanding dipolarization region, but the contribution of high‐energy particles is not very large. These observations suggest the following. The rarefaction wave scenario proposed in the current disruption model is questionable. The radial and azimuthal pressure gradients may strengthen between the initial dipolarization and outside regions, possibly resulting in stronger braking of fast earthward flows and changes in field‐aligned currents. The characteristics of the dipolarization may differ between the initial dipolarization and tailward regions, which would be possibly reflected in the auroral features. Furthermore, we have examined the specific entropy and the ion β. The specific entropy increases in the plasma sheet in the dipolarization region as well as in the midtail region in conjunction with substorm onsets, suggesting from the ideal MHD point of view that the substorm processes are nonadiabatic. The ion β is found to peak at the magnetic equator in the initial dipolarization region around dipolarization onsets.
AbstractList We have studied plasma (ion) pressure changes that occurred in association with the dipolarization in the near‐Earth plasma sheet around substorm onsets. Using Geotail data, we have performed a superposed epoch analysis in addition to detailed examinations of two individual cases with special emphasis on the contribution of high‐energy particles to the plasma pressure. It is found that, unlike previously reported results, the plasma pressure does increase in association with the initial dipolarization at X > ∼−12 RE and −2 < Y < 6 RE, with the increase largely due to high‐energy particles. Outside the initial dipolarization region, particularly tailward and duskward of this region, the plasma pressure begins to decrease owing to the magnetic reconnection before onset or before the dipolarization region reaches there. At later times, the plasma pressure tends to increase there, related to the expanding dipolarization region, but the contribution of high‐energy particles is not very large. These observations suggest the following. The rarefaction wave scenario proposed in the current disruption model is questionable. The radial and azimuthal pressure gradients may strengthen between the initial dipolarization and outside regions, possibly resulting in stronger braking of fast earthward flows and changes in field‐aligned currents. The characteristics of the dipolarization may differ between the initial dipolarization and tailward regions, which would be possibly reflected in the auroral features. Furthermore, we have examined the specific entropy and the ion β. The specific entropy increases in the plasma sheet in the dipolarization region as well as in the midtail region in conjunction with substorm onsets, suggesting from the ideal MHD point of view that the substorm processes are nonadiabatic. The ion β is found to peak at the magnetic equator in the initial dipolarization region around dipolarization onsets.
We have studied plasma (ion) pressure changes that occurred in association with the dipolarization in the near‐Earth plasma sheet around substorm onsets. Using Geotail data, we have performed a superposed epoch analysis in addition to detailed examinations of two individual cases with special emphasis on the contribution of high‐energy particles to the plasma pressure. It is found that, unlike previously reported results, the plasma pressure does increase in association with the initial dipolarization at X > ∼−12 R E and −2 < Y < 6 R E , with the increase largely due to high‐energy particles. Outside the initial dipolarization region, particularly tailward and duskward of this region, the plasma pressure begins to decrease owing to the magnetic reconnection before onset or before the dipolarization region reaches there. At later times, the plasma pressure tends to increase there, related to the expanding dipolarization region, but the contribution of high‐energy particles is not very large. These observations suggest the following. The rarefaction wave scenario proposed in the current disruption model is questionable. The radial and azimuthal pressure gradients may strengthen between the initial dipolarization and outside regions, possibly resulting in stronger braking of fast earthward flows and changes in field‐aligned currents. The characteristics of the dipolarization may differ between the initial dipolarization and tailward regions, which would be possibly reflected in the auroral features. Furthermore, we have examined the specific entropy and the ion β . The specific entropy increases in the plasma sheet in the dipolarization region as well as in the midtail region in conjunction with substorm onsets, suggesting from the ideal MHD point of view that the substorm processes are nonadiabatic. The ion β is found to peak at the magnetic equator in the initial dipolarization region around dipolarization onsets.
Author Miyashita, Y.
Machida, S.
Ieda, A.
Mukai, T.
Christon, S. P.
Kamide, Y.
Nosé, M.
Nagata, D.
Russell, C. T.
Liou, K.
Saito, Y.
Shinohara, I.
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  surname: Machida
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  organization: Department of Geophysics, Kyoto University, Kyoto, Japan
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1995; 71
1977; 25
1991; 96
2007; 100
1997; 24
1993; 64
1984; 89
1999; 26
2009
2007
1994; 46
2008; 35
2000; 91
1970
2008; 321
1992; 97
2004; 109
1999; 104
1996; 101
1988; 93
2009; 27
2009; 114
2001; 63
1998; 25
2001; 106
1997; 102
2009; 36
1989; 94
2004; 31
2003; 108
2005; 19
2002; 29
2000; 105
2010; 115
2002; 107
2005; 32
1998; 103
1995; 100
2008; 113
1989; 37
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Snippet We have studied plasma (ion) pressure changes that occurred in association with the dipolarization in the near‐Earth plasma sheet around substorm onsets. Using...
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wiley
istex
SourceType Enrichment Source
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Publisher
SubjectTerms dipolarization
plasma pressure
substorm expansion onset
Title Pressure changes associated with substorm depolarization in the near-Earth plasma sheet
URI https://api.istex.fr/ark:/67375/WNG-0QRGZBML-7/fulltext.pdf
https://onlinelibrary.wiley.com/doi/abs/10.1029/2010JA015608
Volume 115
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