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Interpretation of the effect of sun-elevation on crater size-frequency distribution
https://jaxa.repo.nii.ac.jp/records/20478
https://jaxa.repo.nii.ac.jp/records/204785f7c9fce-d3ef-4d24-89d3-cc183a56da41
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Interpretation of the effect of sun-elevation on crater size-frequency distribution | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 月探査 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 月面 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 月クレータ | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | クレータ形成 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | クレータサイズ頻度分布 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 空間分解能 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 高解像度 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | レゴリス | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | サイズ分布 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | マッピング | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 入射角 | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | 影 | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | lunar exploration | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | lunar surface | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | lunar crater | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | cratering | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | crater size-frequency distribution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | spatial resolution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | high resolution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | regolith | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | size distribution | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | mapping | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | incident angle | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | shadow | |||||
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 |
本田, 親寿
× 本田, 親寿× 諸田, 智克× 春山, 純一× Honda, Chikatoshi× Morota, Tomokatsu× Haruyama, Junichi |
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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 | ||||||
宇宙航空研究開発機構 宇宙科学研究本部 | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Aerospace Exploration Agency Institute of Space and Astronautical Science | ||||||
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/ISAS) | |||||
書誌情報 |
第39回月・惑星シンポジウム en : Proceedings of the 39th ISAS Lunar and Planetary Symposium p. 61-64, 発行日 2006-08-07 |
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抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The Crater Size-Frequency Distribution (CSFD) has been used to evaluate the age of planetary and satellite's surfaces that have been resurfaced by the geological activity and/or the ejecta blanket from large impact cratering. However, there are some difficulties to determine the surface age using the CSFD on an area less than 4 km in diameter, because the detection limit of degraded craters appears in this size range. We examined the effect of illumination condition to the CSFD. In the southeastern part of Mare Serenitatis, the degraded craters less than 1 km in diameter account for 30 percent of the craters using two images with different sun-elevation. | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0063505016 |