A Rock Model for the Cold and Hot Spots in the Chang'E Microwave Brightness Temperature Map
文献类型：期刊论文
| 作者 | Hu, Guo-Ping1,2; Chan, Kwing Lam1,2; Zheng, Yong-Chun1,2,3; Xu, Ao-Ao1,2 |
| 刊名 | IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING
 |
| 出版日期 | 2018-09-01 |
| 卷号 | 56期号:9页码:5471-5480 |
| 关键词 | Chang'E (CE) microwave brightness temperature (TB) radiation transfer model |
| ISSN号 | 0196-2892 |
| DOI | 10.1109/TGRS.2018.2817654 |
| 英文摘要 | Thermal anomaly spots (both hot and cold) have been found in the global 37-GHz brightness temperature (TB) map of the moon based on the Chang'E (CE) microwave radiometer measurements. To explain their origin, a rock model is proposed to simulate the TB variation against latitude along the profile of a fresh crater in a single track way, which is selected to highlight the topographic effect and avoid any modification to the data. A mixed upper layer made up of rock and soil (regolith and dust) was employed into our previous multilayer model. The thermal properties (thermal conductivity and heat capacity) of the mixture layer are presumed to be linear with the fraction of rocks. Given that high-frequency (37 GHz) measurements are chosen, only the meter size and larger rocks of the upper mixed layer are considered to avoid scattering effects. Several fresh craters poor/rich in ilmenite are selected as testing sites. Despite uncertainties in parameters such as rock abundance (RA), and iron and titanium abundances, three conclusions can be reached from these cases: 1) RA has a significant effect on both the TB value and TB variation trend against latitude; its contribution over some craters may be as high as 15 K; 2) the simulations based on our rock model fit the CE observations better than those when rocks are not included; and 3) the rock and ilmenite contributions could be the main cause for the cold and hot spots found in the CE microwave map. |
| WOS关键词 | SURFACE TEMPERATURES ; TITANIUM ABUNDANCE ; MOON ; IRON ; PROGRAM ; ICE |
| 资助项目 | Science and Technology Development Fund in Macao SAR[119/2017/A3] ; NSFC Program[41490633] ; Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China[2013DP173157] |
| WOS研究方向 | Geochemistry & Geophysics ; Engineering ; Remote Sensing ; Imaging Science & Photographic Technology |
| 语种 | 英语 |
| WOS记录号 | WOS:000443147600040 |
| 出版者 | IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC |
| 资助机构 | Science and Technology Development Fund in Macao SAR ; Science and Technology Development Fund in Macao SAR ; NSFC Program ; NSFC Program ; Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China ; Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China ; Science and Technology Development Fund in Macao SAR ; Science and Technology Development Fund in Macao SAR ; NSFC Program ; NSFC Program ; Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China ; Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China ; Science and Technology Development Fund in Macao SAR ; Science and Technology Development Fund in Macao SAR ; NSFC Program ; NSFC Program ; Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China ; Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China ; Science and Technology Development Fund in Macao SAR ; Science and Technology Development Fund in Macao SAR ; NSFC Program ; NSFC Program ; Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China ; Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/22569]  |
| 专题 | 中国科学院国家天文台 |
| 通讯作者 | Zheng, Yong-Chun |
| 作者单位 | 1.Macau Univ Sci & Technol, Space Sci Inst, Macau, Peoples R China 2.Macau Univ Sci & Technol, Chinese Acad Sci, Lunar & Planetary Sci Lab, Partner Lab,Key Lab Lunar & Deep Space Explorat, Macau, Peoples R China 3.Chinese Acad Sci, Natl Astron Observ, Key Lab Lunar & Deep Space Explorat, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Hu, Guo-Ping,Chan, Kwing Lam,Zheng, Yong-Chun,et al. A Rock Model for the Cold and Hot Spots in the Chang'E Microwave Brightness Temperature Map[J]. IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING,2018,56(9):5471-5480. |
| APA | Hu, Guo-Ping,Chan, Kwing Lam,Zheng, Yong-Chun,&Xu, Ao-Ao.(2018).A Rock Model for the Cold and Hot Spots in the Chang'E Microwave Brightness Temperature Map.IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING,56(9),5471-5480. |
| MLA | Hu, Guo-Ping,et al."A Rock Model for the Cold and Hot Spots in the Chang'E Microwave Brightness Temperature Map".IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING 56.9(2018):5471-5480. |
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来源：国家天文台
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