日本地球惑星科学連合2014年大会

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セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS23_2AM1] 月の科学と探査

2014年5月2日(金) 09:00 〜 10:45 413 (4F)

コンビーナ:*諸田 智克(名古屋大学大学院環境学研究科)、本田 親寿(会津大学)、西野 真木(名古屋大学太陽地球環境研究所)、長岡 央(早稲田大学先進理工学部)、座長:本田 親寿(会津大学)、嵩 由芙子(京都大学理学研究科)

10:30 〜 10:45

[PPS23-07] ボロノイダイアグラムを用いた月面クレーターから二次クレーターの抽出について

木下 達生1、*本田 親寿1平田 成1諸田 智克2 (1.会津大学、2.名古屋大学大学院環境学研究科)

キーワード:二次クレーター, ボロノイダイアグラム

We developed an automatic method for detecting crater clusters with crater spatial distribution based on the Area Voronoi tessellation technique. In the method based on the hierarchical cluster analysis, the evaluation of crater strongly depends on the closest one crater (or one cluster). In the method based on Voronoi tessellation on the other hand, it depends on the adjacent all craters. Since, this approach does not misjudge the pair craters evaluated cluster by the method based on the hierarchical cluster analysis. When a small crater is close adjacent a large crater, a boundary line of Voronoi tessellation is in the rim of the crater. This is different from the line a person pulls by intuition. So, we select Area Voronoi tessellation. For estimate an area of Voronoi, we adopted the wave front method (Watanabe and Murashima, 2006). We applied the Area Voronoi tessellation to observed crater spatial distribution. If the area of Voronoi cell is small, the crater becomes the candidate of the crater cluster. As a result, for the evaluation of crater spatial distribution, we propose that the Area Voronoi diagram is suitable to identify candidates of secondary crater.