Helium observation in the Martian ionoshpere by an X-ray ultraviolet scanner on Mars orbiter NOZOMI
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- Nakamura M.
- Earth and Planetary Science, University of Tokyo
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- Yamashita K.
- Graduate School of Science, Nagoya University
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- Yoshikawa I.
- Institute of Space and Astronautical Science
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- Shiomi K.
- Earth and Planetary Science, University of Tokyo
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- Yamazaki A.
- Earth and Planetary Science, University of Tokyo
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- Sasaki S.
- Geological Institute, University of Tokyo
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- Takizawa Y.
- Earth and Planetary Science, University of Tokyo
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- Hirahara M.
- College of Science, Rikkyo University
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- Miyake W.
- Communications Research Laboratory
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- Saito Y.
- Institute of Space and Astronautical Science
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- Chakrabarti S.
- Boston University
書誌事項
- タイトル別名
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- Helium observation in the Martian ionosphere by an X-ray ultraviolet scanner on Mars orbiter NOZOMI
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抄録
We have built an X-ray ultraviolet (XUV) scanner on board Mars orbiter NOZOMI (Planet-B). This scanner has the He I and II emissions from the Martian atmosphere and ionosphere as its main target. These EUV emissions provide important information for the study of both Martian geological history and the interaction between solar wind and the Martian ionosphere. The XUV scanner will be operated in the parking orbit around the earth and also in the transfer orbit to Mars, where the terrestrial plasmasphere and interplanetary emissions will be studied.
収録刊行物
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- Ｅａｒｔｈ， Ｐｌａｎｅｔｓ ａｎｄ Ｓｐａｃｅ
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Ｅａｒｔｈ， Ｐｌａｎｅｔｓ ａｎｄ Ｓｐａｃｅ 51 (1), 61-70, 1999
地球電磁気・地球惑星圏学会 、公益社団法人 日本地震学会、特定非営利活動法人 日本火山学会、日本測地学会、日本惑星科学会
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詳細情報 詳細情報について
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- CRID
- 1390001206510958336
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- NII論文ID
- 10003737139
- 130003955940
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- NII書誌ID
- AA11211921
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- COI
- 1:CAS:528:DyaK1MXivVCisbo%3D
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- ISSN
- 18805981
- 13438832
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- NDL書誌ID
- 4657968
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- 本文言語コード
- en
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- データソース種別
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- JaLC
- NDL
- Crossref
- CiNii Articles
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- 抄録ライセンスフラグ
- 使用不可