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- 2017
全月球撞击坑的空间分布模式
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Abstract:
以基于嫦娥探月工程公开数据识别的全月球直径大于500 m的106 016个撞击坑为研究对象，划分月海、月陆、经向、纬向研究区域，采用核密度估计与Ripley's K函数的规格化函数-L函数相结合的GIS点模式分析方法，研究全月球撞击坑的空间模式。研究结果表明，全月球撞击坑分布形成了三个聚集中心，南北两极核密度低，东半球核密度高，西半球核密度低，北半球核密度高，南半球核密度低；月陆地区的核密度大于月海地区的核密度，在撞击坑直径范围1~500 km范围内，月陆地区的撞击坑数量是月海地区平均水平的5倍；全月球撞击坑的L（d）曲线随距离变化的过程中在总体上呈现先增后减的态势，经向、纬向研究区位在不同空间尺度上的聚集程度存在差异
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