| Item type |
紀要論文 / Departmental Bulletin Paper(1) |
| 公開日 |
2015-03-26 |
| タイトル |
|
|
タイトル |
磁気圏尾部に注入したプラズマのふるまいについてのシュミレーション実験 |
| 言語 |
|
|
言語 |
jpn |
| 資源タイプ |
|
|
資源タイプ識別子 |
http://purl.org/coar/resource_type/c_6501 |
|
資源タイプ |
departmental bulletin paper |
| その他のタイトル（英） |
|
|
その他のタイトル |
Twined Plasma Produced by Powered Double Probe in the Tail Region : Simulation Experiment of the Magnetsphere |
| 著者 |
南, 繁行
広瀬, 義晃
竹屋, 芳夫
MINAMI, Shigeyuki
HIROSE, Yoshiaki
TAKEYA, Yoshio
|
| 著者所属 |
|
|
|
大阪市大工学部 |
| 著者所属 |
|
|
|
川崎重工K・K |
| 著者所属 |
|
|
|
大阪市大工学部 |
| 出版者 |
|
|
出版者 |
東京大学宇宙航空研究所 |
| 書誌情報 |
東京大学宇宙航空研究所報告
巻 13,
号 3_C,
p. 1019-1028,
発行日 1977-10
|
| 抄録（英） |
|
|
内容記述タイプ |
Other |
|
内容記述 |
Simulation experiments have been operated by some workers in order to make clear the behavior of plasma in the magnetosphere. The large-scales survays of the upper atmosphere with the use of satellite were not done in those days, so this simulated magnetospheric experiments in the laboratory was watched. These early experiments were done in order to konw the structure of the shock front and its time variation at the front of the earth which was generated by the interaction of the high speed plasma flow and magnetic dipole, and also to konw the magnetic field distribution in the solar cusp near the shock front. At this paper, the results obtanied by optical method for the behavior and the stractures in the region at tail of the magnetosphere are dealed. In order to know the tail region, active power source of named powered double probe is used. |
| ISSN |
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|
収録物識別子タイプ |
ISSN |
|
収録物識別子 |
0563-8100 |
| 書誌レコードID |
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|
収録物識別子タイプ |
NCID |
|
収録物識別子 |
AN00161914 |
| 資料番号 |
|
|
内容記述タイプ |
Other |
|
内容記述 |
資料番号: SA0124804000 |
SA0124804.pdf (1.1 MB)
