Apollo16登月区Hapke模型参数反演及模型敏感性分析

doi:10.13278/j.cnki.jjuese.20170214

吉林大学学报(地球科学版) ›› 2018, Vol. 48 ›› Issue (3): 934-940.doi: 10.13278/j.cnki.jjuese.20170214

• 地球探测与信息技术 • 上一篇

Apollo16登月区Hapke模型参数反演及模型敏感性分析

辛欣, 陈圣波, 覃文汉, 李东辉, 陆天启, 田粉粉

吉林大学地球探测科学与技术学院, 长春 130026

收稿日期:2017-09-25 出版日期:2018-05-26 发布日期:2018-05-26
通讯作者: 陈圣波(1967-),男,教授,博士生导师,主要从事遥感技术研究,E-mail:chensb@jlu.edu.cn E-mail:chensb@jlu.edu.cn
作者简介:辛欣(1993-),女,硕士研究生,主要从事定量遥感反演与应用研究,E-mail:xinxin_1123@foxmail.com
基金资助:
国家自然科学基金项目（41490630，41372337）；国家科技重大专项（04-Y20A35-9001-15/17）

Hapke Model Parameter Inversion of Apollo 16 Landing Area and Model Sensitivity Analysis

Xin Xin, Chen Shengbo, Qin Wenhan, Li Donghui, Lu Tianqi, Tian Fenfen

College of GeoExploration Science and Technology, Jilin University, Changchun 130026, China

Received:2017-09-25 Online:2018-05-26 Published:2018-05-26
Supported by:
Supported by National Natural Science Foundation of China (41490630, 41372337) and National Science and Technology Major Project of the Ministry of Science and Technology of China (04-Y20A35-9001-15/17)

摘要/Abstract

摘要： 月表光度行为描述了月表物质反射的太阳光随入射、出射和太阳相角的变化，其反射率的不同取决于月壤颗粒大小、粒子形状、透明度、孔隙度、表面粗糙度等因素。为了分析月表光度行为，了解区域反射率差异原因，本文以Apollo16登月区为例，使用M³（moon mineralogy mapper）数据反演Hapke模型物理参数，并分析了Hapke模型光度参数对二向性反射率的影响程度。反演结果显示，本文研究区域光度参数b、h_S变化很小，光度参数w有一定的变化；表明本文研究区域反射率不同主要是w的差异造成的。研究区域月壤中各类矿物颗粒的前向散射占主导地位，月壤结构和粒径总体相近，但在孔隙度、风化层填充物状态及表面粗糙度等因素中至少有一种因素存在差异。

关键词: 反射率, 光度行为, M³数据, Hapke模型

Abstract: The photometric behavior of the moon's surface describes how the reflected solar radiation varies with incidence, emission, and solar phase angles, depending on the physical and chemical properties of the lunar soils, such as the particle size, the shape, the porosity, and the mineralogical composition. In order to analyze the lunar photometric behavior and understand the reason of regional differences, we retrieved the photometric parameters of Hapke model using the moon mineralogy mapper data in the Apollo 16 landing area. The influence of the Hapke model photometric parameters on the bidirectional reflectance was analyzed. The inversion results showed that the parameter b and h_S of the model varied slightly, while the parameter w of the model changed to certain extent. The difference of reflectance is mainly caused by the w in the study area. The mineral particles in the study area in lunar soil forward scattering dominates. The soil structure and particle size are overall similar, but at least one factor of the porosity, the weathering layer filling state, the surface roughness and other factors is different.

Key words: reflectance, photometric behavior, M³ data, Hapke model

中图分类号:

P691

辛欣, 陈圣波, 覃文汉, 李东辉, 陆天启, 田粉粉. Apollo16登月区Hapke模型参数反演及模型敏感性分析[J]. 吉林大学学报(地球科学版), 2018, 48(3): 934-940.

Xin Xin, Chen Shengbo, Qin Wenhan, Li Donghui, Lu Tianqi, Tian Fenfen. Hapke Model Parameter Inversion of Apollo 16 Landing Area and Model Sensitivity Analysis[J]. Journal of Jilin University(Earth Science Edition), 2018, 48(3): 934-940.

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Apollo16登月区Hapke模型参数反演及模型敏感性分析

Hapke Model Parameter Inversion of Apollo 16 Landing Area and Model Sensitivity Analysis

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