| タイトル | Numerical simulation of the interaction of the plasma sheet with the lobes of the Earth's magnetotail |
| 本文（外部サイト） | http://hdl.handle.net/2060/19820008760 |
| 著者（英） | Swift, D. W. |
| 著者所属（英） | Alaska Univ. |
| 発行日 | 1982-01-01 |
| 言語 | eng |
| 内容記述 | Codes involving one and two spatial dimensions and three velocity dimensions were used to model the Earth's magnetotail. It was shown that the magnetotail can become inflated as a consequence of low energy plasma convection toward the neutral plane. The computer study exhibits a conversion of both magnetic field energy and of energy supplied by the convection electric field into particle energy. The numerical simulations suggest that much of the magnetotail substorm morphology may be a simple consequence of an increase, followed by a decrease, in the convection electric field, without the requirement of any magnetospheric size scale plasma instability or other disruptive processes. It is also concluded that the presence of the convection electric field and a continuing replenishment of low energy particles in the magnetotail are both necessary for maintenance of the magnetotail. |
| NASA分類 | GEOPHYSICS |
| レポートNO | 82N16634
NASA-CR-168508 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/167109 |
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