基于月船一号Mini-SAR数据的月球陨石坑研究与表征

P. Mishra, U. Rajashekhar, Dharmendra Singh
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引用次数: 3

摘要

用各种方法分析月球表面仍然是一项非常具有挑战性的任务。因此,本文尝试采用多种方法对月球表面进行批判性分析,从而预测水冰存在的可能性。极化法有助于确定目标的物理和电学性质。利用m-δ分解和m-χ分解两种极化方法获得了散射机制的信息。为了确定月球表面的电学性质,用坎贝尔的方法测量了月球表面的介电常数。然后,根据表面粗糙度和水冰沉积的可能性,应用镜面漫反射模型识别各种陨石坑。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Study and characterization of lunar craters using Mini-SAR data of Chandrayaan-1
Analyzing lunar surface with various approaches is still a very challenging task. Therefore, in this paper, an attempt has been made to critically analyze the lunar surface by using various approaches so that the possibility of water ice can be predicted. The polarimetric approach helps in determining physical and electrical properties of target. The polarimetric approaches, `m-δ' decomposition and `m-χ' decomposition, have been used for obtaining the information of scattering mechanisms. In order to determine electrical properties of lunar surface, dielectric constant has been measured using Campbell's approach. Then, specular diffuse model has been applied for identifying various craters with reference to surface roughness and possibility of water-ice deposits.
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