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The electron density profiles in auroras were measured by the rockets which penetrated into intensely bright (\u0026acd;30kR for OI 5577 Å), bright (\u0026acd;10kR) and weak (\u0026acd;5kR) auroras. The E-region electron density amounts to \u0026acd;1.2×(10)^6 el/(cm)^3,\u0026acd;5.0×(10)^5 el/(cm)^3 and \u0026acd;6.0×(10)^4el/(cm)^3 for intensely bright, bright and weak auroras respectively, while it is \u0026acd;6.0×(10)^3el/(cm)^3 for no aurora during the night. The electron density in the D-region beneath the lower boundary of an intensely bright arc (75-98 m in altitude) is also considerably enhanced, up to 0.7-1.0×(10)^6 el/(cm)^3. In bright auroral arcs, the electric field becomes small and points in the equatorward direction, whereas it becomes large with the predominant westward direction in the near space outside of a bright auroral arc. The electric field fluctuations (up to 240Hz in frequency) are greatly enhanced in auroras over a wide frequency range, at altitudes of 100-120km. Various kinds of VLF and HF emissions are observed in the auroral ionosphere. 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SUBSTORMS DURING THE IMS PERIOD OBSERVED BY SOUNDING ROCKETS
https://nipr.repo.nii.ac.jp/records/1069
https://nipr.repo.nii.ac.jp/records/10699b4641f4-29b6-4bf2-812c-e7f30f48c4f2
名前 / ファイル | ライセンス | アクション |
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KJ00000768393.pdf (2.2 MB)
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Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
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公開日 | 1980-09-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | SUBSTORMS DURING THE IMS PERIOD OBSERVED BY SOUNDING ROCKETS | |||||
言語 | ||||||
言語 | eng | |||||
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 | |||||
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 | SUBSTORMS DURING THE IMS PERIOD OBSERVED BY SOUNDING ROCKETS | |||||
著者名よみ |
ナガタ, タケシ
× ナガタ, タケシ× ヒラサワ, タケオ× フクニシ, ヒロシ× ヤマギシ, ヒサオ× キムラ, イワネ× オガワ, トシオ |
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著者名(英) |
NAGATA, Takesi
× NAGATA, Takesi× HIRASAWA, Takeo× FUKUNISHI, Hiroshi× YAMAGISHI, Hisao× KIMURA, Iwane× OGAWA, Toshio |
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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 | ||||||
National Institute of Polar Research | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Polar Research | ||||||
著者所属(英) | ||||||
en | ||||||
Faculty of Engineering, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Faculty of Science, Kyoto University | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Experimental results obtained by the sounding rockets at Syowa Station, Antarctica, are briefly summarized. The electron density profiles in auroras were measured by the rockets which penetrated into intensely bright (∿30kR for OI 5577 Å), bright (∿10kR) and weak (∿5kR) auroras. The E-region electron density amounts to ∿1.2×(10)^6 el/(cm)^3,∿5.0×(10)^5 el/(cm)^3 and ∿6.0×(10)^4el/(cm)^3 for intensely bright, bright and weak auroras respectively, while it is ∿6.0×(10)^3el/(cm)^3 for no aurora during the night. The electron density in the D-region beneath the lower boundary of an intensely bright arc (75-98 m in altitude) is also considerably enhanced, up to 0.7-1.0×(10)^6 el/(cm)^3. In bright auroral arcs, the electric field becomes small and points in the equatorward direction, whereas it becomes large with the predominant westward direction in the near space outside of a bright auroral arc. The electric field fluctuations (up to 240Hz in frequency) are greatly enhanced in auroras over a wide frequency range, at altitudes of 100-120km. Various kinds of VLF and HF emissions are observed in the auroral ionosphere. Characteristics of these emissions and their relations to the precipitating electron flux are discussed. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA00733561 | |||||
書誌情報 |
Memoirs of National Institute of Polar Research. Special issue 巻 16, p. 1-16, 発行日 1980-09 |