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ハレー彗星最接近時の太陽風パラメータと水イオンの検出
https://jaxa.repo.nii.ac.jp/records/32983
https://jaxa.repo.nii.ac.jp/records/32983c102698a-078b-41d1-b575-9ec49719d5fa
名前 / ファイル | ライセンス | アクション |
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SA0166812.pdf (587.4 kB)
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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 | ハレー彗星最接近時の太陽風パラメータと水イオンの検出 | |||||
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 | Detection of water group ions at the distance of 7 million Kilometers from comet Halley | |||||
著者 |
小山, 孝一郎
× 小山, 孝一郎× 阿部, 琢美× 平尾, 邦雄× 斎藤, 尚生× 湯元, 清文× OYAMA, Koh-ichiro× ABE, Takumi× HIRAO, Kunio× SAITO, Takao× YUMOTO, Kiyofumi |
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著者所属 | ||||||
電気通信大学 | ||||||
著者所属 | ||||||
東海大学工学部 | ||||||
著者所属 | ||||||
東北大学理学部 | ||||||
著者所属 | ||||||
東北大学理学部 | ||||||
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: ハレー彗星探査計画報告 巻 19, p. 103-110, 発行日 1987-03 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | ハレー彗星最接近時の太陽風パラメータを議論した。最接近時には"さきがけ"は磁気中性面付近にあり, この時惑星間空間はやや擾乱状態にあった。ハレー彗星によって太陽風が減速された確証は現在までの解析では得られていないが, 太陽風パラメータの周波数解析の結果はハレー彗星の水グループのイオンの存在を示している。 | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Solar wind parameters measured by SAKIGAKE around the time of encounter with Halley comet are discussed Sakigake was in or near the neutral sheet of Heliomagnetosphere and therefore the solar wind velocily was comparatively slow. Interplanetary space was in a small disturbance period. Although a firm evidence does not exist that solar wind velocity was decelerated by Halley's comet, frequency spectrum analysis of the solar wind parameters shows the exisistence of water group ions. | |||||
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: SA0166812000 |