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<論文>「たんせい4号」による太陽フレアX線輝線スペクトルの観測
https://jaxa.repo.nii.ac.jp/records/32602
https://jaxa.repo.nii.ac.jp/records/326026978cbd5-476f-46e4-9961-d88e8ab97118
名前 / ファイル | ライセンス | アクション |
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SA0125933.pdf (1.0 MB)
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
タイトル | <論文>「たんせい4号」による太陽フレアX線輝線スペクトルの観測 | |||||
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 | Observations of Soft X-ray Line Emissions, from Solar Flares by Tansei 4 Satellite | |||||
著者 |
田中, 捷雄
× 田中, 捷雄× 渡辺, 鉄哉× 西, 恵三× 守山, 史生× 宮崎, 英昭× TANAKA, Katsuo× WATANBE, Tetsuya× NISHI, Keizo× MORIYAMA, Fumio× MIYAZAKI, Hideaki |
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著者所属 | ||||||
東京大学東京天文台 | ||||||
著者所属 | ||||||
東京大学東京天文台 | ||||||
著者所属 | ||||||
東京大学東京天文台 | ||||||
著者所属 | ||||||
東京大学東京天文台 | ||||||
著者所属 | ||||||
東京大学東京天文台 | ||||||
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 16, 号 4_B, p. 1445-1468, 発行日 1980-12 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Observations of soft X-ray line emissions of highly ionized iron and calcium have been made by Bragg spectrometer (LiF) aboard Tansei 4 satellite. Two wave length regions: 1.8-2.0A and 3.1-3.25A are measured simultaneously with spectral resolution of 0.005 A. A combination of high sensitivity and high time resolution measurements enabled to detect initial heating phase of flares. Rapid shift of the peak intensity in the iron line spectrun from 1,885A region to 1.865A region together with K_α emmission has been observed at the very initial phase of impulsive flares in coincidence with hard X-ray and microwave bursts. This indicates that individual heating occurs in less than 10 seconds simultaneously with the production of high energy electrons. Rapid increase of turbulence during the heating phase has been found from line broademing of FeXXV resonance line. It is also found that temperature and emission measure of soft X-ray emitting plasma increase and decrease simultaneously for small flares contrary to previous results by soft X-ray continuum emission. Plasma compression has been suggested for the heating mechanism of flares. | |||||
ISSN | ||||||
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 | ||||||
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: SA0125933000 |