Data processing and preliminary results of the Chang'e-3 VIS/NIR Imaging Spectrometer in-situ analysis

	Data processing and preliminary results of the Chang'e-3 VIS/NIR Imaging Spectrometer in-situ analysis
	Liu, Bin 1; Li, Chun-Lai1 ; Zhang, Guang-Liang1 ; Xu, Rui 2; Liu, Jian-Jun1 ; Ren, Xin1 ; Tan, Xu1 ; Zhang, Xiao-Xia1 ; Zuo, Wei1 ; Wen, Wei-Bin1
刊名	RESEARCH IN ASTRONOMY AND ASTROPHYSICS
	2014-12-01
卷号	14 期号:12 页码:1578-1594
关键词	Chang'e-3 VNIS in-situ analysis data processing
英文摘要	The Chang'e-3 Visible and Near-infrared Imaging Spectrometer (VNIS) is one of the four payloads on the Yutu rover. After traversing the landing site during the first two lunar days, four different areas are detected, and Level 2A and 2B radiance data have been released to the scientific community. The released data have been processed by dark current subtraction, correction for the effect of temperature, radiometric calibration and geometric calibration. We emphasize approaches for reflectance analysis and mineral identification for in-situ analysis with VNIS. Then the preliminary spectral and mineralogical results from the landing site are derived. After comparing spectral data from VNIS with data collected by the M-3 instrument and samples of mare that were returned from the Apollo program, all the reflectance data have been found to have similar absorption features near 1000 nm except lunar sample 71061. In addition, there is also a weak absorption feature between 1750 similar to 2400nm on VNIS, but the slopes of VNIS and M-3 reflectance at longer wavelengths are lower than data taken from samples of lunar mare. Spectral parameters such as Band Centers and Integrated Band Depth Ratios are used to analyze mineralogical features. The results show that detection points E and N205 are mixtures of high-Ca pyroxene and olivine, and the composition of olivineat point N205 is higher than that at point E, but the compositions of detection points S3 and N203 are mainly olivine-rich. Since there are no obvious absorption features near 1250 nm, plagioclase is not directly identified at the landing site.
收录类别	SCI
语种	英语
WOS记录号	WOS:000346124700007
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/6577]
专题	国家天文台_月球与深空探测研究部
作者单位	1.Chinese Acad Sci, Natl Astron Observ, Key Lab Lunar & Deep Space Explorat, Beijing 100012, Peoples R China 2.Chinese Acad Sci, Shanghai Inst Tech Phys, Key Lab Space Act Optoelect Technol, Shanghai 200083, Peoples R China
推荐引用方式 GB/T 7714	Liu, Bin,Li, Chun-Lai,Zhang, Guang-Liang,et al. Data processing and preliminary results of the Chang'e-3 VIS/NIR Imaging Spectrometer in-situ analysis[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2014,14(12):1578-1594.
APA	Liu, Bin.,Li, Chun-Lai.,Zhang, Guang-Liang.,Xu, Rui.,Liu, Jian-Jun.,...&Wen, Wei-Bin.(2014).Data processing and preliminary results of the Chang'e-3 VIS/NIR Imaging Spectrometer in-situ analysis.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,14(12),1578-1594.
MLA	Liu, Bin,et al."Data processing and preliminary results of the Chang'e-3 VIS/NIR Imaging Spectrometer in-situ analysis".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 14.12(2014):1578-1594.