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A rocky hill on the continuous ejecta of Ziwei crater revealed by the Chang’e-3 mission 被引量:2
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作者 ChunYu Ding YuZhen Cai +1 位作者 ZhiYong Xiao Yan Su 《Earth and Planetary Physics》 CSCD 2020年第2期105-110,共6页
The Chinese Chang’e-3 mission landed close to the eastern rim of the ~450 m diameter Ziwei crater. Regional stratigraphy of the landing site and impact excavation model suggest that the bulk continuous ejecta deposit... The Chinese Chang’e-3 mission landed close to the eastern rim of the ~450 m diameter Ziwei crater. Regional stratigraphy of the landing site and impact excavation model suggest that the bulk continuous ejecta deposits of the Ziwei crater are composed by Erathothenian-aged mare basalts. Along the traverse of the Yutu rover, the western segment features a gentle topographic uplift(~0.5 m high over ~4 m), which is spatially connected with the structurally-uplifted crater rim. Assuming that this broad topographic uplift has physical properties discontinuous with materials below, we use data returned by the high-frequency lunar penetrating radar onboard the Yutu rover to estimate the possible range of relative permittivity for this topographic uplift. Only when the relative permittivity is ~9 is the observed radar reflection consistent with the observed topography, suggesting that the topographic uplift is composed of basaltic blocks that were excavated by the Ziwei crater. This result is consistent both with the impact excavation model that predicts deeper basaltic materials being deposited closer to the crater rim, and with observation of numerous half-buried boulders on the surface of this hill. We note that this study is the first to use topography and radargram data to estimate the relative permittivity of lunar surface uplifts, an approach that has had many successful applications on Mars. Similar approaches can apply other ground penetrating radar data for the Moon, such as will be available from the ongoing Chang’e-4 mission. 展开更多
关键词 lunar penetrating radar impact crater ejecta deposits Chang'e-3 PERMITTIVITY MOON
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基于YOLO V3算法改进的月表砾石检测优化方法
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作者 张金铭 刘秀清 《电子设计工程》 2023年第12期38-42,47,共6页
月球表面溅射物中的砾石检测可用于实现自主着陆、航天器和月球车自动避障等任务。针对与月表背景差异不明显的砾石检测问题,提出一种检测方法,该方法基于改进后的YOLO V3模型对美国月球侦察轨道器(Lunar Reconnaissance Orbiter,LRO)... 月球表面溅射物中的砾石检测可用于实现自主着陆、航天器和月球车自动避障等任务。针对与月表背景差异不明显的砾石检测问题,提出一种检测方法,该方法基于改进后的YOLO V3模型对美国月球侦察轨道器(Lunar Reconnaissance Orbiter,LRO)窄角相机(Narrow Angle Camera,NAC)高分辨率月球遥感影像进行训练和测试。实验对比了原始YOLO V3和改进后的YOLO V3方法的检测效果。结果表明,改进后的YOLO V3模型较原始模型的准确率提高了10.5%,召回率提升22.8%,检测速度提升1.69倍,在数据集中的漏检和误检现象也轻于原始YOLO V3网络。 展开更多
关键词 目标检测 月球溅射物 深度学习 月球侦察轨道器 YOLO V3
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月球撞击坑溅射堆积与辐射纹蒙特卡洛模拟 被引量:1
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作者 张新琴 夏秀文 王永江 《地球物理学进展》 CSCD 北大核心 2014年第6期2604-2608,共5页
撞击坑是月球上最常见的地质构造之一,通常只有较大规模的撞击坑才能形成超长辐射纹.然而最近我们的研究发现,在一些大规模撞击坑的边缘,溅射堆积发育有良好的孔隙结构;在这些多孔的撞击坑边缘区域,即使是小规模撞击事件,也易于形成具... 撞击坑是月球上最常见的地质构造之一,通常只有较大规模的撞击坑才能形成超长辐射纹.然而最近我们的研究发现,在一些大规模撞击坑的边缘,溅射堆积发育有良好的孔隙结构;在这些多孔的撞击坑边缘区域,即使是小规模撞击事件,也易于形成具有辐射纹的撞击坑.本文建立了包含孔隙结构的撞击抛射模型,并利用蒙特卡洛方法模拟了垂直撞击溅射堆积构造和超长辐射纹,不仅揭示了在多孔结构岩石区域易于形成超长辐射纹的原因,同时为撞击辐射纹的形成提供了一种可行的解释方案. 展开更多
关键词 月球撞击坑 溅射堆积 辐射纹 蒙特卡洛方法
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