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Comparison of CO2 absorption databases with application to Venus near-infrared "Window" spectra
https://jaxa.repo.nii.ac.jp/records/20412
https://jaxa.repo.nii.ac.jp/records/2041254cb1127-5bc4-43e0-b556-58f8e1c41139
Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Comparison of CO2 absorption databases with application to Venus near-infrared "Window" spectra | |||||
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_5794 | |||||
資源タイプ | conference paper | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
佐藤, 毅彦
× 佐藤, 毅彦× 今村, 剛× 空華, 智子× Satoh, Takehiko× Imamura, Takeshi× Sorahana, Satoko |
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著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属 | ||||||
東京大学大学院理学系研究科 | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | ||||||
著者所属(英) | ||||||
en | ||||||
Graduate School for Science, University of Tokyo | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構宇宙科学研究本部 | |||||
出版者(英) | ||||||
出版者 | Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
en : Proceedings of the ISAS lunar and planetary symposium 巻 41, p. 143-146, 発行日 2009 |
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会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The 41st ISAS Lunar and Planetary Symposium (August 6-8, 2008. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)) | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We have performed radiative transfer computations to reproduce emissions observed in the near-infrared "windows" of CO2 atmosphere of Venus. Different databases of molecular absorption parameters (HITEMP, CDSD 296 K and 1000 K) are tested to evaluate appropriateness of given line list and absorption parameters. It is found that none of these can reproduce the observations with sufficient accuracy. Merging of a few databases for simulation of Venus atmosphere is probably needed. | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA12268968 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064291033 |