基于CELMS数据的月球东海微波辐射特性研究

孟治国; 平劲松; AlexanderGUSEV; 蔡占川; 陈思

doi:10.15982/j.issn.2095-7777.2014.03.009

中文核心期刊

中国科技核心期刊

中国科学引文数据库（CSCD）来源期刊

中国高校百佳科技期刊

中国宇航学会深空探测技术专业委员会会刊

高级检索

留言板

尊敬的读者、作者、审稿人, 关于本刊的投稿、审稿、编辑和出版的任何问题, 您可以本页添加留言。我们将尽快给您答复。谢谢您的支持!

姓名
邮箱
手机号码
标题
留言内容
验证码

x 关闭永久关闭

天文导航技术专题征稿函

基于CELMS数据的月球东海微波辐射特性研究

孟治国, 平劲松, AlexanderGUSEV, 蔡占川, 陈思

文章导航 > 深空探测学报(中英文） > 2014 > 1(3): 214-219

孟治国, 平劲松, AlexanderGUSEV, 蔡占川, 陈思. 基于CELMS数据的月球东海微波辐射特性研究[J]. 深空探测学报(中英文）, 2014, 1(3): 214-219. doi: 10.15982/j.issn.2095-7777.2014.03.009

引用本文:

Meng Zhiguo, Ping Jinsong, Alexander Gusev, CAI Zhanchuan, Chen Si. Research on Microwave Emission Features of Mare Orientale Using CELMS Data[J]. Journal of Deep Space Exploration, 2014, 1(3): 214-219. doi: 10.15982/j.issn.2095-7777.2014.03.009

Citation:

Meng Zhiguo, Ping Jinsong, Alexander Gusev, CAI Zhanchuan, Chen Si. Research on Microwave Emission Features of Mare Orientale Using CELMS Data[J]. Journal of Deep Space Exploration, 2014, 1(3): 214-219. doi: 10.15982/j.issn.2095-7777.2014.03.009

基于CELMS数据的月球东海微波辐射特性研究

doi: 10.15982/j.issn.2095-7777.2014.03.009

1.
吉林大学地球探测科学与技术学院
2.
中国科学院国家天文台月球与深空探测重点实验室
3.
俄罗斯喀山联邦大学,天文系
4.
澳门科技大学太空研究所

基金项目: 国家自然科学基金(41371332、40901159);国家重点基础研究发展计划(973计划)项目(2015CB857101);澳门科技发展基金(084/2012/A3);浙江大学CAD&CG国家重点实验室开放课题(A1513)

Research on Microwave Emission Features of Mare Orientale Using CELMS Data

1.
College of Geoexploration Science and Technology, Jilin University
2.
Key Laboratory of Lunar and Planetary Exploration Research, National Astronomical Observatories, CAS
3.
Geology institute, Kazan federal university
4.
Institute of Space, Macau University of Science and Technology

摘要: 根据月壤(FeO+TiO2)含量数据和“嫦娥2号”卫星CELMS数据,对月球东海地区微波辐射特性进行了研究。结果表明,在东海内部(FeO+TiO2)含量较高的地区,其正午和午夜时刻的亮温值都比较高,亮温差值也比较大,但亮温及亮温差值的分布随频率变化呈现不均匀性;Maunder撞击坑的(FeO+TiO2)含量较低,但其低频和高频亮温及亮温差值的表现正好相反;区域F(约10°S/106°W)、G(约5°S/104°W)和以(13°S/103°W)为中心的区域的微波辐射存在明显异常。这些区域的微波辐射特性对研究东海地区的形成演化过程具有重要意义。
- 东海 /
- 微波辐射 /
- CELMS数据
Abstract: As Mare Orientale is the youngest and best preserved multiring impact basin on the Moon, it is of essential importance to study its composition and structure for clues to the processes and histories of older, more degraded features. In this paper, the (FeO+TiO2) abundance derived from Clementine UV-VIS data and the CELMS data from Chang’e-2 satellite are employed to study the Microwave Emission features of the Mare Orientale. The results indicate that the regions with high CELMS data and high brightness temperature difference agree well with high (FeO+TiO2) abundance both on noon and on midnight. However, the change of the area with high CELMS data and high brightness temperature difference with the frequency indicates that the composition of the lunar regolith is varied with depth. The (FeO+TiO2) abundance in Maunder Crater is low, whereas the CELMS data and the brightness temperature differences in the low frequencies and the high frequencies show distinctly different features, which indicates that the composition of the lunar regolith here in the upper layer and the lower layer may be different. The abnormal microwave emission apparently exists in the regions (10°S /106°W), (5°S /104°W) and (13°S /103°W) in highland with low (FeO+TiO2) abundance, which is likely related to the temperature gradient of the deep regolith.. The microwave emission features in these areas are of special significance to study the evolution of the Mare Orientale.
- Mare Orientale /
- microwave emission /
- CELMS data

[1]	牛东文, 段建锋, 欧阳琦, 张宇, 陈略, 王美. “嫦娥四号”中继星再生伪码测距数据定轨精度分析 . 深空探测学报(中英文）, 2022, 9(1): 21-28. doi: 10.15982/j.issn.2096-9287.2022.20191213002
[2]	黄靖, 郭华东, 刘广, 邓玉. 基于月基观测几何的地球辐射能量模拟研究 . 深空探测学报(中英文）, 2022, 9(3): 278-284. doi: 10.15982/j.issn.2096-9287.2022.20210078
[3]	叶罕霖, 邓玉, 刘广, 郭华东. 月基观测地球大气层顶辐射特性研究 . 深空探测学报(中英文）, 2022, 9(3): 285-291. doi: 10.15982/j.issn.2096-9287.2022.20210074
[4]	王赤, 李磊, 张爱兵, 张珅毅, 侯东辉, 徐子贡, 谢良海, 王慧姿, 罗朋威, 郭静楠, 史全岐, 张小平. 月表太阳风和粒子辐射环境—“嫦娥四号”观测新结果 . 深空探测学报(中英文）, 2022, 9(3): 239-249. doi: 10.15982/j.issn.2096-9287.2022.20220020
[5]	陈少伍, 刘敏, 王静温, 强立, 卢欧欣. 基于帧同步的深空极低码速率数据回溯方法 . 深空探测学报(中英文）, 2021, 8(6): 608-613. doi: 10.15982/j.issn.2096-9287.2021.20210122
[6]	刘奇祺, 陈楠, 林偲蔚. 月表可照时间谱和太阳辐射谱空间分布特征研究 . 深空探测学报(中英文）, 2021, 8(6): 614-624. doi: 10.15982/j.issn.2096-9287.2021.20210100
[7]	刘攀, 王志国, 刘建峰, 闵康磊, 游红俊. “嫦娥五号”载荷数据存储管理方法 . 深空探测学报(中英文）, 2021, 8(3): 299-305. doi: 10.15982/j.issn.2096-9287.2021.20210001
[8]	柳青峰, 李博, 康冬鹏, 杨清波, 马晶, 谭立英, 于思源, 赵生, 王淇. 深空辐射条件下EDFA波分复用性能研究 . 深空探测学报(中英文）, 2019, 6(6): 545-552. doi: 10.15982/j.issn.2095-7777.2019.06.005
[9]	蔡明辉, 杨涛, 韩建伟. 载人深空探测磁场主动辐射防护技术研究 . 深空探测学报(中英文）, 2019, 6(2): 165-172. doi: 10.15982/j.issn.2095-7777.2019.02.008
[10]	侯东辉, 张珅毅, RobertFWimmer-Schweingruber, 于佳, SoenkeBurmeister, 沈国红, 袁斌, 王春琴, 张斌全. 月球粒子辐射环境探测现状 . 深空探测学报(中英文）, 2019, 6(2): 127-133. doi: 10.15982/j.issn.2095-7777.2019.02.003
[11]	杨轩, 鄢建国, 叶茂, 金炜桐, 曲春凯, 刘素艳. 对一种月球与火星探测多程微波测量链路定轨定位的数值模拟初步分析 . 深空探测学报(中英文）, 2018, 5(2): 154-161. doi: 10.15982/j.issn.2095-7777.2018.02.007
[12]	王慧慧, 孟治国, 李翠, 朱蕴哲, 蔡占川, 李向月. 基于LOLA数据的冯·卡门地区地形特征分析 . 深空探测学报(中英文）, 2018, 5(1): 57-65. doi: 10.15982/j.issn.2095-7777.2018.01.008
[13]	郑晨, 姚鸿泰. 基于影像数据的冯·卡门撞击坑形貌分析 . 深空探测学报(中英文）, 2018, 5(1): 50-56. doi: 10.15982/j.issn.2095-7777.2018.01.007
[14]	杨成伟, 郑建华. 脉冲星X射线数据处理与分析 . 深空探测学报(中英文）, 2018, 5(3): 219-225. doi: 10.15982/j.issn.2095-7777.2018.3.003
[15]	徐茂格, 施为华. 深空微波测距测速现状及发展建议 . 深空探测学报(中英文）, 2018, 5(2): 140-146. doi: 10.15982/j.issn.2095-7777.2018.02.005
[16]	张吉栋, 孟治国, 朱蕴哲, 曾昭发, 平劲松. 基于LOLA数据的冯·卡门撞击坑太阳辐射研究 . 深空探测学报(中英文）, 2018, 5(1): 12-19. doi: 10.15982/j.issn.2095-7777.2018.01.002
[17]	胡硕, 孟治国, 朱蕴哲, 连懿, 李翠, GUSEVAlexander. 基于“嫦娥2号”CELMS数据的冯·卡门撞击坑微波辐射特性 . 深空探测学报(中英文）, 2018, 5(1): 20-26. doi: 10.15982/j.issn.2095-7777.2018.01.003
[18]	张吉栋, 孟治国, 平劲松, 李文潇, 王明远, 赵瑞. 基于LOLA数据的Aristarchus高原光照特性初步研究 . 深空探测学报(中英文）, 2017, 4(2): 171-177. doi: 10.15982/j.issn.2095-7777.2017.02.011
[19]	杨懿, 金双根, 薛岩松. 利用CRISM数据探测火星表面含水矿物及其演化 . 深空探测学报(中英文）, 2016, 3(2): 187-194. doi: 10.15982/j.issn.2095-7777.2016.02.015
[20]	张羽飞, 刘景昊, 黄勇, 谢懿. 利用"火星快车"三程多普勒跟踪数据限定局部洛伦兹不变性 . 深空探测学报(中英文）, 2015, 2(2): 144-148. doi: 10.15982/j.issn.2095-7777.2015.02.007

点击查看大图

计量

文章访问数: 2594
HTML全文浏览量: 32
PDF下载量: 2063
被引次数: 0

基于CELMS数据的月球东海微波辐射特性研究

doi: 10.15982/j.issn.2095-7777.2014.03.009

1. 吉林大学地球探测科学与技术学院

2. 中国科学院国家天文台月球与深空探测重点实验室

3. 俄罗斯喀山联邦大学,天文系

4. 澳门科技大学太空研究所

收稿日期: 2014-07-28
修回日期: 2014-08-18

关键词:

东海 /

微波辐射 /

CELMS数据

摘要: 根据月壤(FeO+TiO2)含量数据和“嫦娥2号”卫星CELMS数据,对月球东海地区微波辐射特性进行了研究。结果表明,在东海内部(FeO+TiO2)含量较高的地区,其正午和午夜时刻的亮温值都比较高,亮温差值也比较大,但亮温及亮温差值的分布随频率变化呈现不均匀性;Maunder撞击坑的(FeO+TiO2)含量较低,但其低频和高频亮温及亮温差值的表现正好相反;区域F(约10°S/106°W)、G(约5°S/104°W)和以(13°S/103°W)为中心的区域的微波辐射存在明显异常。这些区域的微波辐射特性对研究东海地区的形成演化过程具有重要意义。

English Abstract

Research on Microwave Emission Features of Mare Orientale Using CELMS Data

1. College of Geoexploration Science and Technology, Jilin University

2. Key Laboratory of Lunar and Planetary Exploration Research, National Astronomical Observatories, CAS

3. Geology institute, Kazan federal university

4. Institute of Space, Macau University of Science and Technology

Received Date: 2014-07-28
Rev Recd Date: 2014-08-18

Keywords:

Abstract: As Mare Orientale is the youngest and best preserved multiring impact basin on the Moon, it is of essential importance to study its composition and structure for clues to the processes and histories of older, more degraded features. In this paper, the (FeO+TiO2) abundance derived from Clementine UV-VIS data and the CELMS data from Chang’e-2 satellite are employed to study the Microwave Emission features of the Mare Orientale. The results indicate that the regions with high CELMS data and high brightness temperature difference agree well with high (FeO+TiO2) abundance both on noon and on midnight. However, the change of the area with high CELMS data and high brightness temperature difference with the frequency indicates that the composition of the lunar regolith is varied with depth. The (FeO+TiO2) abundance in Maunder Crater is low, whereas the CELMS data and the brightness temperature differences in the low frequencies and the high frequencies show distinctly different features, which indicates that the composition of the lunar regolith here in the upper layer and the lower layer may be different. The abnormal microwave emission apparently exists in the regions (10°S /106°W), (5°S /104°W) and (13°S /103°W) in highland with low (FeO+TiO2) abundance, which is likely related to the temperature gradient of the deep regolith.. The microwave emission features in these areas are of special significance to study the evolution of the Mare Orientale.

引用本文: