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Diurnal Variation of Martian Exospheric Temperature
https://jaxa.repo.nii.ac.jp/records/34435
https://jaxa.repo.nii.ac.jp/records/3443515487d6c-26cc-4610-80dd-189f81564893
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
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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 | Diurnal Variation of Martian Exospheric Temperature | |||||||
| 言語 | en | |||||||
| 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 |
SHIMIZU, Mikio
× SHIMIZU, Mikio
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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 14, p. 459-467, 発行日 1970-09 |
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| 抄録(英) | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | Diurnal variations of Martian exospheric temperatures at the times of Mariner 4,6,and 7 observations are computed by solving the time dependent heat balance equations. It is found that steep temperature gradients exist between the day and night sides of this plante, mainly due to very low temperatures at the dark side where the infrared emissions from CO_2 cool the atmosphere efficiently. They can produce a strong wind system in the Martian thermosphere. The adiabatic cooling of the atmosphere associated with the vertical wind may play a role in explainning the observed low exospheric temperatures at the sunlit side. This wind system may also work to dilute the photochemical products such as CO and O at the dayside of the ionosphere. | |||||||
| ISSN | ||||||||
| 収録物識別子タイプ | ISSN | |||||||
| 収録物識別子 | 0372-1418 | |||||||
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| 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: SA2400779000 | |||||||