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ELF波動のみずほ-昭和基地同時観測
https://doi.org/10.15094/00008038
https://doi.org/10.15094/00008038aefcfc27-ad1a-4c5c-9424-b60ce6ea051b
名前 / ファイル | ライセンス | アクション |
---|---|---|
KJ00002477098 (6.7 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1979-02-01 | |||||
タイトル | ||||||
タイトル | ELF波動のみずほ-昭和基地同時観測 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | ELF Emissions Simultaneously Observad at Syowa and Mizuho Stations | |||||
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 | |||||
ID登録 | ||||||
ID登録 | 10.15094/00008038 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
論文名よみ | ||||||
その他のタイトル | ELF ハドウ ノ ミズホ ショウワ キチ ドウジ カンソク | |||||
著者名(日) |
佐藤, 夏雄
× 佐藤, 夏雄× 福西, 浩× 巻田, 和男 |
|||||
著者名(英) |
SATO, Natsuo
× SATO, Natsuo× FUKUNISHI, Hiroshi× MAKITA, Kazuo |
|||||
著者所属(日) | ||||||
国立極地研究所 | ||||||
著者所属(日) | ||||||
国立極地研究所 | ||||||
著者所属(日) | ||||||
東京大学理学部地球物理研究施設 | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Polar Research | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Polar Research | ||||||
著者所属(英) | ||||||
en | ||||||
Geophysics Research Laboratory, University of Tokyo | ||||||
抄録(日) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 地磁気子午面に沿って約270km離れた昭和基地とみすほ基地において,地磁気,地磁気脈動,オーロラ,ELF・VLF波動,オーロラ等の同時観測を行った.この論文ては,ELF波動の強度比およびスペクトル構造の相互についての解析結果を報告する.その結果は,1)周波数-時間スペクトルは非常に似ている.2)発生周波数の強度比はみすほ基地ては低周波数帯域が強く,昭和基地では高周波数帯域が強い.3)QPエミッションの周期は全く同してある. | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Simultaneous observations of ELF・VLF emissions, magnetic variations, cosmic noise absorption and auroras have been carried out at Syowa and Mizuho Stations since June 1976. Mizuho Station is located at a distance of ~270 km poleward on the same magnetic meridian as that of Syowa. From the ELF emission data observed at both the stations, the following results were obtamed 1) Frequency-time spectra of ELF chorus emissions were quite similar at both the stations. However, it ls found that the intensity in the lower frequency range (<15 kHz) is greater at Mizuho than at Syowa, and veisa in the higher frequency range 2) The period of QP emissions was same at both the stations | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AN00181831 | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 00857289 | |||||
書誌情報 |
南極資料 巻 64, p. 134-145, 発行日 1979-02 |
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国際十進分類法 | ||||||
主題Scheme | UDC | |||||
主題 | 551.510.535/.537 | |||||
出版者 | ||||||
出版者 | 国立極地研究所 |