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ISIS-1, 2で観測されたVLFソーサーの特性
https://doi.org/10.15094/00008041
https://doi.org/10.15094/00008041bdfdde7b-1879-458b-acd7-10fb349db0b3
名前 / ファイル | ライセンス | アクション |
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KJ00002477101 (5.1 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 | ISIS-1, 2で観測されたVLFソーサーの特性 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Characteristics of VLF Saucers Observed by ISIS-1, 2 Satellites | |||||
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 | 10.15094/00008041 | |||||
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 | ISIS-1 2 デ カンソク サレタ VLF ソーサー ノ トクセイ d. ジキケン ナイ ノ ULF・VLF ハドウ ダイ1カイ キョクチ ニオケル デンリケン ジキ ソウゴウ カンソク シンポジウム PART 2 | |||||
著者名(日) |
尾崎, 孝之
× 尾崎, 孝之× 岩瀬, 政之× 吉野, 赳夫× 松尾, 敏郎× 福西, 浩 |
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著者名(英) |
OZAKI, Takayuki
× OZAKI, Takayuki× IWASE, Masayuki× YOSHINO, Takeo× MATSUO, Toshiro× FUKUNISHI, Hiroshi |
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著者所属(日) | ||||||
電気通信大学 | ||||||
著者所属(日) | ||||||
電気通信大学 | ||||||
著者所属(日) | ||||||
電気通信大学 | ||||||
著者所属(日) | ||||||
京都大学工学部 | ||||||
著者所属(日) | ||||||
国立極地研究所 | ||||||
著者所属(英) | ||||||
en | ||||||
University of Electro-Communications | ||||||
著者所属(英) | ||||||
en | ||||||
University of Electro-Communications | ||||||
著者所属(英) | ||||||
en | ||||||
University of Electro-Communications | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Electrical Engineering II, Faculty of Engineering, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Polar Research | ||||||
抄録(日) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 第17次観測隊(1976-1977)の手によって,昭和基地においてISISのVLF広帯域テータがテレメトリー受信された.その磁気テープ記録を周波数分析することにより作成されたタイナミックスペクトラムからVLFソーサーについて以下の点が明らかとなった.1)ソーサーは冬の真夜中付近て発生頻度か高い.2)緯度的には夜間は地磁気緯度60°-75°,昼間ては70°-80°でよく観測される.3)f-tスペクトルの形状から大きく分けて,双曲線状のものとV字形のものがある.4)ソーサーの発生領域はプラスマポースの外側て,VLFヒスの領域の低緯度側,またその発生源は1000-1500km以上の高度に存在していると考えられる. | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Characteristics of the saucer emissions are studied by using ISIS VLF data which were received at Syowa Station by the wintering party of the 17th Japanese Antarctic Research Expedition in 1976-1977. Saucers were observed most frequently in the nighttime in winter and were scarcely observed in summer, The magnetic latitude ranges in which saucers were observed are ~60゜-75° in the nighttime and ~70°-80゜ in the daytime. These occurrence regions are located at the higher latitude side of the plasmapause and at the lower latitude side of the hiss occurrence regions. The shapes of saucers on frequency-time spectra showed generally two different types,i e, symmetrical hyperbolic shapes and symmetrical V-shapes | |||||
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. 167-178, 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 |