| Item type |
紀要論文 / Departmental Bulletin Paper(1) |
| 公開日 |
2015-03-26 |
| タイトル |
|
|
タイトル |
科学衛星 KYOKKO によるプラズマ波動の観測 |
| 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 |
Observation of plasma waves by the scientific satellite KYOKKO |
| 著者 |
中村, 良治
野村, 雄二
伊藤, 富造
向井, 利典
平尾, 邦雄
NAKAMURA, Yoshiharu
NOMURA, Yuzi
ITOH, Tomizo
MUKAI, Toshifumi
HIRAO, Kunio
|
| 出版者 |
|
|
出版者 |
宇宙科学研究所 |
| 出版者（英） |
|
|
出版者 |
Institute of Space and Astronautical Science |
| 書誌情報 |
宇宙科学研究所報告. 特集: 宇宙観測研究報告
巻 2,
p. 87-98,
発行日 1982-03
|
| 抄録（英） |
|
|
内容記述タイプ |
Other |
|
内容記述 |
Observation of plasma waves performed by the plasma wave receiver on board KYOKKO satellite in the frequency range from 45 kHz to 3 MHz is described. Plasma emissions have been detected mainly in two regions. In the auroral region, the auroral hiss is associated with the electron precipitation. The hiss occurrs in two frequency regions. One exists below the minimum of f_p^- or f_g^- where f_p^- and f_g^- are the plasma and cyclotron frequenceis of electrons, respectively and the other extends to above it. The hiss which extends to above the minimum of f_p^- or f_g^- is correlated with the inverted V electron precipitation with a peak energy of a few keV to 10 keV. In the equatorial region, a hiss has been also observed. Two different modes coexist in the hiss. One is a usual whistler mode observed in geographically limited regions. The other is a UHR wave which sometimes continues to be observed in the polar regions. |
| ISSN |
|
|
収録物識別子タイプ |
ISSN |
|
収録物識別子 |
0285-9920 |
| 書誌レコードID |
|
|
収録物識別子タイプ |
NCID |
|
収録物識別子 |
AN00354485 |
| 資料番号 |
|
|
内容記述タイプ |
Other |
|
内容記述 |
資料番号: SA0166527000 |
SA0166527.pdf (811.2 kB)
