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 in | Journal of Geophysical Research: Space Physics Vol. 115; no. A12 |
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Main Authors | , , , , , , , , , , , |
Format | Journal Article |
Language | English |
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Blackwell Publishing Ltd
01.12.2010
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ISSN | 0148-0227 2156-2202 |
DOI | 10.1029/2010JA015608 |
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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. |
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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. |
Author_xml | – sequence: 1 givenname: Y. surname: Miyashita fullname: Miyashita, Y. email: miyasita@stelab.nagoya-u.ac.jp organization: Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi, Japan – sequence: 2 givenname: S. surname: Machida fullname: Machida, S. organization: Department of Geophysics, Kyoto University, Kyoto, Japan – sequence: 3 givenname: A. surname: Ieda fullname: Ieda, A. organization: Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi, Japan – sequence: 4 givenname: D. surname: Nagata fullname: Nagata, D. organization: Air Liquide Engineering Japan, Harima-cho, Kako-gun, Hyogo, Japan – sequence: 5 givenname: Y. surname: Kamide fullname: Kamide, Y. organization: Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi, Japan – sequence: 6 givenname: M. surname: Nosé fullname: Nosé, M. organization: Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University, Kyoto, Japan – sequence: 7 givenname: K. surname: Liou fullname: Liou, K. organization: Johns Hopkins University Applied Physics Laboratory, Maryland, Laurel, USA – sequence: 8 givenname: T. surname: Mukai fullname: Mukai, T. organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan – sequence: 9 givenname: S. P. surname: Christon fullname: Christon, S. P. organization: Focused Analysis and Research, Maryland, Columbia, USA – sequence: 10 givenname: C. T. surname: Russell fullname: Russell, C. T. organization: Institute of Geophysics and Planetary Physics, University of California, California, Los Angeles, USA – sequence: 11 givenname: I. surname: Shinohara fullname: Shinohara, I. organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan – sequence: 12 givenname: Y. surname: Saito fullname: Saito, Y. organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan |
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(e_1_2_7_49_1) 2005; 19 e_1_2_7_4_1 e_1_2_7_8_1 e_1_2_7_18_1 e_1_2_7_16_1 e_1_2_7_40_1 e_1_2_7_61_1 e_1_2_7_2_1 e_1_2_7_14_1 e_1_2_7_42_1 e_1_2_7_44_1 e_1_2_7_10_1 e_1_2_7_46_1 e_1_2_7_48_1 Frey H. U. (e_1_2_7_12_1) 2007 e_1_2_7_27_1 e_1_2_7_29_1 e_1_2_7_51_1 e_1_2_7_30_1 e_1_2_7_53_1 e_1_2_7_24_1 e_1_2_7_32_1 e_1_2_7_55_1 e_1_2_7_22_1 e_1_2_7_34_1 e_1_2_7_57_1 e_1_2_7_20_1 e_1_2_7_36_1 e_1_2_7_59_1 e_1_2_7_38_1 |
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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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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 |
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