| タイトル | On the three-dimensional magnetic structure of the plasmoid created in the magnetotail at substorm onset |
| 著者（英） | Birn, J.; Bame, S. J.; Russell, C. T.; Hones, E. W., Jr.; Paschmann, G. |
| 著者所属（英） | Max-Planck-Inst. fuer Physik und Astrophysik|Los Alamos Scientific Lab.|Ruhr Univ.|California Univ. |
| 発行日 | 1982-03-01 |
| 言語 | eng |
| 内容記述 | The magnetic field in the plasmoid which is created by the reconnection of magnetic field lines at a neutral line formed in the near-earth region of the plasma sheet at substorm onset, and which flows out of the magnetotail into the magnetosphere's wake, displays a strong positive or negative Y(SM) component that has been difficult to reconcile with the standard, two-dimensional reconnection geometry. It is shown that this deviation of the magnetic field is a manifestation of the newly-reconnected field line loop's draping toward the tail's central or midnight meridian, and that the draping is a consequence of the three-dimensional plasma flow associated with the reconnection process. |
| NASA分類 | GEOPHYSICS |
| レポートNO | 82A27015 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/411360 |
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