Plasma sheet changes caused by sudden enhancements of the solar wind pressure
Using Geotail data, we have studied the response of the plasma sheet in the magnetotail to sudden enhancements of the solar wind pressure. We have selected three events in which there were no indications of substorm expansions around the corresponding sudden impulses (SIs) on the ground. It is shown...
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| Published in | Journal of Geophysical Research: Space Physics Vol. 115; no. A5 |
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| Main Authors | , , , , , , , , , |
| Format | Journal Article |
| Language | English |
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Washington, DC
Blackwell Publishing Ltd
01.05.2010
American Geophysical Union |
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| Abstract | Using Geotail data, we have studied the response of the plasma sheet in the magnetotail to sudden enhancements of the solar wind pressure. We have selected three events in which there were no indications of substorm expansions around the corresponding sudden impulses (SIs) on the ground. It is shown that the ion number density and temperature, as well as the ion pressure, increase significantly due to the plasma sheet compression. The specific entropy does not significantly change, suggesting that the plasma sheet compression is nearly adiabatic. This plasma behavior is in contrast to the nonadiabatic substorm‐associated processes. Hence examining the correlation between the number density and the temperature, and especially the specific entropy is critical for distinguishing between substorm‐associated and SI‐associated changes of the plasma sheet. The northward magnetic field in the plasma sheet also increases, or at least does not decrease, associated with the compression, implying that the lateral magnetotail compression suppresses the triggering of magnetic reconnection and therefore substorm expansion onsets. |
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| AbstractList | Using Geotail data, we have studied the response of the plasma sheet in the magnetotail to sudden enhancements of the solar wind pressure. We have selected three events in which there were no indications of substorm expansions around the corresponding sudden impulses (SIs) on the ground. It is shown that the ion number density and temperature, as well as the ion pressure, increase significantly due to the plasma sheet compression. The specific entropy does not significantly change, suggesting that the plasma sheet compression is nearly adiabatic. This plasma behavior is in contrast to the nonadiabatic substorm‐associated processes. Hence examining the correlation between the number density and the temperature, and especially the specific entropy is critical for distinguishing between substorm‐associated and SI‐associated changes of the plasma sheet. The northward magnetic field in the plasma sheet also increases, or at least does not decrease, associated with the compression, implying that the lateral magnetotail compression suppresses the triggering of magnetic reconnection and therefore substorm expansion onsets. |
| Author | Miyashita, Y. Machida, S. Mukai, T. Kamide, Y. Liou, K. Matsumoto, Y. Saito, Y. Shinohara, I. Keika, K. Miyoshi, Y. |
| 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, Japan – sequence: 2 givenname: K. surname: Keika fullname: Keika, K. organization: Center for Solar-Terrestrial Research, New Jersey Institute of Technology, New Jersey, Newark, USA – sequence: 3 givenname: K. surname: Liou fullname: Liou, K. organization: Johns Hopkins University Applied Physics Laboratory, Maryland, Laurel, USA – sequence: 4 givenname: S. surname: Machida fullname: Machida, S. organization: Department of Geophysics, Kyoto University, Kyoto, Japan – sequence: 5 givenname: Y. surname: Kamide fullname: Kamide, Y. organization: Research Institute for Sustainable Humanosphere, Kyoto University, Uji, Japan – sequence: 6 givenname: Y. surname: Miyoshi fullname: Miyoshi, Y. organization: Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Japan – sequence: 7 givenname: Y. surname: Matsumoto fullname: Matsumoto, Y. organization: Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Japan – sequence: 8 givenname: I. surname: Shinohara fullname: Shinohara, I. organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan – sequence: 9 givenname: Y. surname: Saito fullname: Saito, Y. organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan – sequence: 10 givenname: T. surname: Mukai fullname: Mukai, T. organization: Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan |
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| Cites_doi | 10.1029/2001JA009148 10.1029/2008JA013445 10.1029/95JA03753 10.1029/95JA02834 10.1029/96JA00460 10.1029/2005JA011091 10.1029/2007GL029909 10.1029/2008JA013147 10.1007/BF00751335 10.1029/92JA01250 10.1029/91JA02517 10.5636/jgg.46.39 10.1029/JA088iA12p10025 10.1029/JA082i001p00074 10.1029/91JA00775 10.1029/2003JA010076 10.1029/2007JA012763 10.1029/2007JA012443 10.5636/jgg.46.669 10.1029/JA094iA07p09139 10.1029/2003JA009984 10.1029/97JA02870 10.1007/BF00751330 10.1029/2000JA000233 10.1029/97JA02986 10.1029/2002JA009544 10.1029/96JA00079 10.1029/1999GL003737 10.1007/BF00751326 10.1007/BF00819660 10.1029/2000JA003028 10.1029/2008JA013127 10.1029/2003JA010317 10.5194/angeo-23-609-2005 10.5636/jgg.46.7 10.1029/93JA02288 10.1029/98GL02633 10.1029/JA088iA09p06969 10.1029/2002JA009442 10.1029/2008JA013225 10.1029/2005JA011089 |
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| Keywords | Plasma Magnetic reconnection magnetic field density pressure expansion solar wind entropy correlation temperature Magnetospheric tail ions Plasma layer compression Triggering |
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| Snippet | Using Geotail data, we have studied the response of the plasma sheet in the magnetotail to sudden enhancements of the solar wind pressure. We have selected... |
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| SubjectTerms | Atmospheric sciences Earth sciences Earth, ocean, space Entropy Exact sciences and technology Magnetic fields Magnetism magnetotail compression substorm trigger sudden impulse Wind pressure |
| Title | Plasma sheet changes caused by sudden enhancements of the solar wind pressure |
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