[1] 吴伟仁,王琼,唐玉华,等. “嫦娥4号”月球背面软着陆任务设计[J]. 深空探测学报,2017,4(02):111-117
WU W R,WANG Q,TANG Y H,et al. Design of Chang’e-4 lunar farside soft-landing mission [J]. Journal of Deep Space Exploration,2017,4(02):111-117
[2] SPUDIS P D,RIESSE R A,GILLIS J G. Ancient multiring basins on the moon revealed by clementine laser altimetry [J]. Science,1994,266:1848-1851
[3] OHTAKE M,UEMOTO K,YOKOTA Y,et al. Geologic structure generated by large-impact basin formation observed at the South Pole-Aitken basin on the Moon[J]. Geophysical Research Letters,2014,41(8):2738-2745
[4] ZUBER M T,SMITH D E,LEMOINE F G,et al. The shape and internal structure of the moon from the Clementine mission [J]. Science,1994,266:1839-1843
[5] 张健,缪秉魁,廖庆园,等. 月球南极艾特肯盆地的地质特征:探索月球深部的窗口[J]. 矿物岩石地球化学通报,2011,30(02):234-240+244
ZHANG J,MIAO B K,LIAO Q Y,et al. The geological characteristics of the South Pole-Aitken basin on the Moon:the window to explore the deep composition of the Moon [J]. The Window to Explore the Deep Composition of the Moon,2011,30(02):234-240
[6] LUCEY P G,BLEWETT D T,JOLLIFF B L. Lunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet-visible images[J]. Journal of Geophysical Research Planets,2000,105(E8):20297-20305
[7] YAN B K,WANG R S,GAN F P,et al. Minerals mapping of the lunar surface with clementine UV-VIS-NIR data based on spectra unmixing method and hapke model[C]// Lunar and Planetary Science Conference.USA:[s.n.],2010.
[8] OHTAKE M,MATSUNAGA T,HARUYAMA J,et al. The global distribution of pure anorthosite on the Moon[J]. Nature,2009,461(7261):236
[9] MENG ZHIGUO,ZHAO RUI,CAI ZHANCHUAN,et al. Microwave thermal emission at tycho area and its geological significance[C]//IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing. [S.l.]:IEEE,2017.
[10] MENG Z G,ZHANG J D,CAI Z C,et al. Microwave thermal emission features of Mare orientale revealed by CELMS Data[C]//IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing. [S.l.]:IEEE ,2017. DOI(identifier)10.1109/JSTARS.2017.2700397.
[11] 雷利卿,姜景山,张晓辉,等. 月球若干地区微波辐射特征研究[J]. 遥感技术与应用,2009,(04):423-434
LEI L Q,JIANG J S,ZHANG X H,et al. Microwave radiation analysis for some regions on the Moon [J]. Remote Sensing Technology and Application,2009,(04):423-434
[12] 张卫国,姜景山,刘和光,等.月球南极的微波辐射分布与异常[J]. 中国科学(D辑:地球科学),2009,39(08):1059-1068
ZHANG W G,JIANG J S,LIU H G,et al. Distribution and anomaly of microwave emission at lunar south pole [J].Sci China Ser D-Earth Sci,2009,39(08):1059-1068
[13] ZHENG Y C,TSANG K T,CHAN K L. First microwave map of the Moon with Chang’E-1 data:the role of local time in global imaging[J]. Icarus,2012,219:194-210
[14] CHAN K L,KANG T T,KONG B,et al. Lunar regolith thermal behavior revealed by Chang’E-1 microwave brightness temperature data[J]. Earth & Planetary Science Letters,2010,295(s 1-2):287-291
[15] 胡国平,陈柯,李青侠,等. 月球表面微波亮温的时变趋势[J]. 华中科技大学学报:自然科学版,2013,41(5):64-67
HU G P,CHEN K,LI Q X,et al. Diurnal variation trend of microwave brightness temperature on the moon[J]. Journal of Huazhong University of Science and Technology(Natural Science Edition),2013,41(5):64-67
[16] 宫晓蕙,金亚秋. “嫦娥一号”对月球新生环行山表面热辐射“热点”与“冷点”昼夜变化的观测[J].中国科学:信息科学,2012,42(8):923-935
GONG X H,JIN Y Q. Diurnal change of thermal emission with “hot spots” and “cold spots” of fresh lunar craters observed by Chinese Chang’E-1[J].Scientic Sinica Informationis,2012,42(8):923-935
[17] 朱永超,郑永春,邹永廖. 月球表面“冷点”和“热区”研究:嫦娥二号微波亮温数据分析[J].矿物学报,2016(2):231-240
ZHU Y C,ZHENG Y C,ZOU Y L. Cold spots and warm regions on the lunar surface:analysis of brightness temperatures data from Chang’E-2 microwave cbservation[J].Acta Mineralogica Sinica,2016(2):231-240
[18] 孟治国,平劲松,徐懿,等. 厚度对月壤微波辐射亮温的影响[J]. 地理研究,2014,33(6):1015-1022
MENG Z G,PING J S,XU Y,et al. Influence of layer thickness on microwave emission of lunar regolith[J]. Geographical Research,2014,33(6):1015-1022
[19] MENG Z G,YANG G D,PING J S,et al. Influence of(FeO+TiO2)abundance on the microwave thermal emissions of lunar regolith[J]. Science China Earth Sciences,2016,59:1498-1507,doi:10.1007/s11430-016-5280-1
[20] ZHENG Y C,TSANG Z S,CHAN K L,et al. First microwave map of the Moon with Chang’E-1 data:the role of local time in global imaging [J]. Icarus,2012,219(1):194-210
[21] 陈思,孟治国,张吉栋,等. Tycho撞击坑地区微波热辐射特性研究[J]. 中国科学:物理学 力学 天文学,2016,46(2):029608
CHEN S,MENG Z G,ZHANG J D,et al. Research on microwave radiation characteristics at Tycho crater area [J]. Scientia Sinica:Physica,Mechanica & Astronomica,2016,46(2):029608
[22] FANG T,FA W. High frequency thermal emission from the lunar surface and near surface temperature of the Moon from Chang’E-2 microwave radiometer [J]. Icarus,2014,232:34-53
[23] MENG Z G,XU Y,CAI Z C,et al. Influence of lunar topography on simulated surface temperature[J]. Advances in Space Research,2014,54(10):2131-2139
[24] ROSENBURG M A,AHARONSON O,HEAD J W,et al. Global surface slopes and roughness of the Moon from the Lunar Orbiter Laser Altimeter[J]. Journal of Geophysical Research Planets,2011,116(E2):1161-1172
[25] 严艳梓,汤国安,熊礼阳,等. 基于DEM的月球雨海地区粗糙度研究[J]. 地理研究,2014,33(8):1442-1456
YAN Y Z,TANG G A,XIONG L Y,et al. Lunar surface roughness of Mare Imbrium based on DEMs[J]. Geographical Research,2014,33(8):1442-1456