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Inversion of the Main Mineral Compositions and Subdivision of Tectonic Units on Lunar LQ-4 based on Chang'e Data

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Acta Geologica Sinica(English Edition) 2015年第6期89卷 1882-1894页

作者： WANG Xiang CHEN Jianping XU Yanbo zheng yongchun YAN Bokun WU Yunzhao China University of Geosciences The Institute of High and New Techniques applied to Land Resources China University of Geosciences Shandong Gold Geology and Mineral Exploration Co. Ltd. National Astronomical Observatories Chinese Academy of Sciences China Aero Geophysical Survey and Remote Sensing Center for Land and Resources School of Geographic and Oceanographic Sciences of Nanjing University

Spectra are sensitive in detecting main minerals on the lunar surface from visible light to infrared light. Since spectral characteristics of minerals are closely related to their compositions and the maturity level of soil on the Moon, studying the compositions and distribution of elements and minerals on the lunar surface can help to understand the evolution of the Moon through remote sensing technology. The correlation between the spectral characteristics of Chang＇e-1 interference imaging spectrometry（IIM） reflectance images and the mineral contents of LSCC（Lunar Soil Characterization Consortium） lunar surface mineral samples was discussed and the spatial distributions of Fe O and Al_2O_3 contained in both pyroxene and plagioclase on LQ-4 were studied using the improved angle parameter method, MNF, and band ratio statistics. A comparison of the mapping results of the optical models by Lucey, Shkuractov and other researchers on Clementine and the gamma ray spectrometry data shows that the content error is within 0.6% for lunar mare areas and close to 1% for the highland areas. The tectonic framework on the lunar surface was also investigated. And based on integrated analysis of previous findings on topography of the lunar surface, Chang＇e LAM, CCD and LOLA images and the gravity anomalies data（Clementine GLGM-2）, the tectonic unit subdivision was established for LQ-4, the idea of subdividing the lunar tectonic units was proposed, and this will provide a good foundation for studying the lunar tectonic evolution.

关键词： Lunar Chang'e-1 mineral composition MNF tectonic units tectonic elements

Review on physical models of lunar brightness temperature

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Chinese Journal Of Geochemistry 2010年第2期29卷 204-211页

作者： FENG Jianqing ZOU Yongliao BIAN Wei zheng yongchun LI Chunlai National Astronomical Observatories Chinese Academy of Sciences Beo＇ing 100012 China Graduate University of the Chinese Academy of Sciences Beijing 100049 China

Brightness temperature is a main index to reflect the energy of microwave radiation of an object. Using lunar brightness temperature data, physical properties of lunar regolith, such as thickness, heat flow and dielectric permittivity, could be interpreted. There are two methods to study brightness temperature distribution of the moon: the first is used to measure lunar brightness temperature by radio observation or spaceborne microwave radiometers, and the second is used to simulate calculation by the physical model. On the basis of the measurements of lunar brightness temperature in the history, this study analyzed the main physical model of lunar brightness temperature, also including its theory and influence factors. The authors concluded that surface and subsurface temperatures of the moon, dielectric properties and layered structure of lunar regolith were the main factors affecting the global brightness temperature of the moon. These factors should be quantified in detail in the future research.

关键词：亮度温度物理模型月球星载微波辐射计综述测量计算辐射能量温度数据

Mineral surface modification induced by low energy ion irradiation: Implications for solar-wind exposure effects in lunar soil

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Chinese Journal Of Geochemistry 2014年第4期33卷 351-356页

作者： ZHU Yongchao FU Xiaohui XU Lin ZHANG Feng zheng yongchun ZOU Yongliao Key Laboratory of Lunar and Deep Space Exploration National Astronomical Observatories Chinese Academy of Sciences University of Chinese Academy of Sciences Space Science Institute Macao University of Science and Technology

We performed ion irradiation on olivine and ilmenite to simulate solar-wind exposure effects in lunar soil. The surface morphology and microstructure after ion irradiation were characterized by field emission scanning electron microscopy. Sputtering erosion significantly modified the surface of irradiated Luobusha olivine grains. All irradiated grains show smooth surface and round shape. The cleavage fractures on the unirradiated olivine surface were widened and deeply etched after He+ irradiation. Both of these are the consequence of ion sputtering erosion. There are no bubbles or voids foundin the irradiated olivine grains, because He+ dose in this study is lower than saturated fluence. Irradiated Panzhihua ilmenite grains are all covered with smooth flakes with the thickness of about 400 nm. The formation of the flakes should be related with helium bubbles and their growth during He+ implantation. Some columnar-shaped particles are found at the surface of irradiated Panzhihua ilmenite. We speculate that these particles should be sulfide because of significantly high sulfur contents.

关键词：低能离子辐照表面改性月球土壤光效果太阳风场发射扫描电子显微镜诱导矿物

新时代应用型高校“双创”教育实践基地建设模式研究

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黑龙江农业科学 2024年第8期 86-90页

作者：郑永春宋宇鹏李海涛吉林农业科技学院中药学院吉林吉林132109

在新时代背景下,应用型高校的“双创”教育实践基地建设具有深远意义。实践基地不仅促进了实践教学体系的完善,还通过打造“产教融合”实践基地样板,加强了高水平实践教师团队的建设,并提升了实践基地的硬件设施。此外,提升实践基地的... 详细信息

在新时代背景下,应用型高校的“双创”教育实践基地建设具有深远意义。实践基地不仅促进了实践教学体系的完善,还通过打造“产教融合”实践基地样板,加强了高水平实践教师团队的建设,并提升了实践基地的硬件设施。此外,提升实践基地的知名度、科研创新能力,以及优化实践基地的管理机制也是促进其发展的重要方面。这些措施共同构建了新时代中药“双创”教育实践基地的发展路径,对于培养具有“卓越创新”高素质应用技术型专业人才,以及一流专业的建设都起到重要的推动作用。

关键词：应用型高校实践基地建设 “双创”教育

Two Lunar Mare Soil Simulants

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Acta Geologica Sinica(English Edition) 2011年第5期85卷 1016-1021页

作者： Yongquan LI Jianzhong LIU Yongliao ZOU Ziyuan OUYANG yongchun zheng Zongyu YUE China University of Geosciences Beijing 100083 China National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 China Institute of Geochemistry Chinese Academy of Sciences Guiyang 550002 China Institute of Remote Sensing Applications Chinese Academy of Sciences Beijing 100012 China

Two new lunar mare soil simulants,NAO-2 and NAO-3,have been created in National Astronomical Observatories(NAO),Chinese Academy of *** two simulants were produced from low-titanium basalt and high-titanium basalt *** chemical composition,mineralogy, particle size distribution,density,angle of internal friction,and cohesion of both simulants have been analyzed,indicating that some characteristics of NAO-2 and NAO-3 are similar to those of Apollo 14 and Apollo 11 landing site ***-2 and NAO-3 will be of great benefit to the scientific and engineering research on lunar soil.

关键词： lunar mare soil simulants

Research on the inversion of elemental abundances from Chang'E-2 X-ray spectrometry data

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Chinese Journal Of Geochemistry 2014年第3期33卷 289-299页

作者： BAN Chao zheng yongchun ZHU Yongchao ZHANG Feng XU Lin ZOU Yongliao National Astronomical Observatories Chinese Academy of Sciences University of Chinese Academy of Sciences Space Science Institute Macao University of Science and Technology

The elemental abundances of lunar surface are the important clues to study the formation and evolution history of the Moon. In 2010, China's Chang'E-2(CE-2) lunar orbiter carried a set of X-ray spectrometer(XRS) to investigate the elemental abundances of the lunar surface. During CE-2's life span around the Moon, the XRS experienced several events of solar flare. The X-ray solar monitor onboard recorded the spectra of solar X-rays at the same time. In this paper, we introduced the XRS instrument and data product. We analyzed the characteristics of the XRS data. Using the data obtained during an M solar flare event which had occurred on Feb. 16, 2011, we derived the elemental abundances of Mg, Al, Si, Ca and Fe of the lunar surface in the Oceanus Procellarum. Finally, we discussed the factors that influence the accuracy of the inversion.

关键词： X射线光谱元素丰度数据反演月球表面太阳耀斑月球探测器演化历史数据产品

A misleading way to transform the natural desert into farmland

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The Innovation 2022年第3期3卷 11-12页

作者： Benli Liu Bo Wu Ziqiang Lei Jinnian Tang yongchun zheng Department of Desert and Desertification Northwest Institute of Eco-environment and ResourcesChinese Academy of SciencesLanzhou 730000China Institute of Desertification Studies/Institute of Ecological Conservation and Restoration Chinese Academy of ForestryBeijing 100091China College of Chemistry and Chemical Engineering Northwest Normal UniversityLanzhou 730070China Gansu Desert Control Research Institute Lanzhou 730071China National Astronomical Observatories Chinese Academy of SciencesBeijing 100101China

Yi et *** a concept of“desert soilization”and an idea of“omni-directional integrative(ODI)constraint”in the paper of The Innovation.1 In their practice,a“constraining material”was used to bind the sands in the Ulan Buh *** is claimed that theirmethod can transform the desert into *** havemany doubts about this method and disagree with their *** would like to discuss these questions and clarify our stand *** et *** make it clear that their test is only valid in areas with shallow groundwater levels.

关键词： shallow groundwater Desert

Geotectonic evolution of lunar LQ-4 region based on multisource data

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Geoscience Frontiers 2014年第2期5卷 227-235页

作者： Jianping Chen Yanbo Xu Xiang Wang Shujun He Danping Yan Shaofeng Liu Yongliao Zou yongchun zheng School of Earth Sciences and Resources China University of Geosciences (Beijing) The Institute of High and New Techniques Applied to Land Resources China University of Geosciences (Beijing) Shandong Gold Geology and Mineral Exploration Co. Ltd. Development Research Center China Geological Survey CAS National Astronomical Observatories

The Sinus Iridum region, the first choice for China＇s＂Lunar Exploration Project＂is located at the center of the lunar LQ-4 area and is the site of Chang＇e-3 （CE-3）＇s soft landing. To make the scientific exploration of Chang＇e-3 more targeted and scientific, and to obtain a better macro-level understanding of the geotectonic environment of the Sinus Iridum region, the tectonic elements in LQ-4 region have been studied and the typical structures were analyzed statistically using data from CE-1, Clementine, LRO and Lunar Prospector missions. Also, the mineral components and periods of mare basalt activities in the study area have been ascertained. The present study divides the tectonic units and establishes the major tectonic events and sequence of evolution in the study area based on morphology, mineral constituents, and tectonic element distribution.

关键词： Lunar Tectonic elements Tectonic units Evolution LQ-4 region

Global absorption center map of the mafic minerals on the Moon as viewed by CE-1 IIM data

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Science China(Physics,Mechanics & Astronomy) 2010年第12期53卷 2160-2171页

作者： WU YunZhao ZHANG Xia YAN BoKun GAN FuPing TANG ZeSheng XU AoAo zheng yongchun ZOU YongLiao School of Geographic and Oceanographic Sciences Nanjing UniversityNanjing 210093China Institute of Remote Sensing Applications Chinese Academy of SciencesBeijing 100101China Institute for Remote Sensing Method China Aero Geophysical Survey and Remote Sensing Center for Land and ResourcesBeijing 100083China Collaborative Research Laboratory on Lunar and Planetary Exploration Macao University of Science and TechnologyTaipaMacaoChina National Astronomical Observatories Chinese Academy of SciencesBeijing 100012China

Determining the global distribution of minerals on the Moon has been an important goal of lunar science. Hyperspectral remote sensing is an important approach to acquiring minerals on the Moon on the global scale. The wavelength of the absorption band center is the key parameter for identifying minerals with reflectance spectra as well as remote sensing data. The global absorption center map of the mafic minerals of the Moon was produced for the first time with the Chang’E-1 IIM data. This map shows the global distribution of mafic minerals such as orthopyroxenes, clinopyroxenes, and olivine and even plagioclase feldspar of the Moon. The validation for some representative areas indicates that the global map is reliable and even more detailed than the results derived from Clementine-data. Moreover, our method is insensitive to the topography and viewing and illumination geometries. The global absorption band center map not only contributes to the lunar science research, but also has other implications to be further studied. Moreover, the preprocessing methods such as calibration and correction introduced in this study can be useful in other research with IIM data.

关键词： Chang’E-1 IIM absorption band center calibration Moon