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地球型惑星探査の研究課題
https://jaxa.repo.nii.ac.jp/records/33110
https://jaxa.repo.nii.ac.jp/records/331107da2a126-c87e-48df-85ac-f156f5ce7efe
名前 / ファイル | ライセンス | アクション |
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SA0166984.pdf (558.1 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 | ||||||
タイトル | 地球型惑星探査の研究課題 | |||||
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 | Science objectives of planetary missions to Mars and Venus | |||||
著者 |
前沢, 洌
× 前沢, 洌× MAEZAWA, K. |
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著者所属 | ||||||
名古屋大学理学部 | ||||||
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: 宇宙観測研究報告 巻 28, p. 103-110, 発行日 1991-03 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Mars and Venus are very different from other planets of the solar system in that their intrinsic magnetic field is minimal and cannot fully withstand the solar wind pressure. Therefore, the planetary ionospheres may directly interact with the solar wind plasma. This fact, established for Venus and to be confirmed for Mars, has made these planets interesting targets for future planetary missions. In this article, a brief review is presented on what we have learned from previous missions on these unique planetary environments. Scientific returns from the future missions are discussed with emphasis on the value of comparisons of diverse magnetospheres. This approach is the key to the ultimate understanding of the interaction between the solar wind and planetary magnetospheres. | |||||
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: SA0166984000 |