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Laboratory Experiment on the Solar Wind Interaction with Planetary Bodies
https://jaxa.repo.nii.ac.jp/records/34437
https://jaxa.repo.nii.ac.jp/records/3443756f7fa68-1232-4d54-8cf2-20b77c6fcaa9
名前 / ファイル | ライセンス | アクション |
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SA2400787.pdf (559.1 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 | ||||||
言語 | en | |||||
タイトル | Laboratory Experiment on the Solar Wind Interaction with Planetary Bodies | |||||
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 | |||||
著者 |
KUBO, Haruya
× KUBO, Haruya× ITOH, Tomizo× YAMORI, Akira |
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出版者 | ||||||
出版者 | 東京大学宇宙航空研究所 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Aeronautical Science,University of Tokyo | |||||
書誌情報 |
en : ISAS report/Institute of Space and Aeronautical Science,University of Tokyo 巻 35, 号 16, p. 513-522, 発行日 1970-12 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The electric field generated by the interaction of solar wind with planetary bodies is discussed by the laboratory simulation. It is inferred from this experiment that an upper limit of the electric field behind Moon would be in the order of 10^<-2>V/m, and almost zero behind Venus. The mechanisms generating the electric and the magnetic field by the solar wind interaction are also discussed, and they would respectively be due to charge separation and pressure gradient drift. | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 0372-1418 | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA00675986 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: SA2400787000 |