摘要
Remote-sensing images of Mars contain rich information about its surface morphology,topography,and geological structure.These data are fundamental for scientific research and exploration.Prior to China’s first Mars exploration mission,data from six advanced optical imaging systems of different missions in the Martian orbit had been used to generate Mars global/near-global image datasets with spatial resolutions of better than 1 km:the visual imaging system of Mariner 9,visual imaging subsystem cameras of Viking 1 and 2,Mars Orbiter Camera-Wide Angle(MOC-WA)of the Mars Global Surveyor(MGS),Context Camera(CTX)of the Mars Reconnaissance Orbiter(MRO),High Resolution Stereo Camera(HRSC)of Mars Express(MEX),and Thermal Emission Imaging System(THEMIS)of the Mars Odyssey Orbiter[1,2].
作者
刘建军
任鑫
严韦
陈王丽
曾兴国
张晓霞
谭旭
高兴烨
付强
刘定心
郭林
张庆
张菁菁
余国彬
何志平
耿言
张荣桥
李春来
Jianjun Liu;Xin Ren;Wei Yan;Wangli Chen;Xingguo Zeng;Xiaoxia Zhang;Xu Tan;Xingye Gao;Qiang Fu;Dingxin Liu;Lin Guo;Qing Zhang;Jingjing Zhang;Guobin Yu;Zhiping He;Yan Geng;Rongqiao Zhang;Chunlai Li(Key Laboratory of Lunar and Deep Space Exploration,National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China;University of Chinese Academy of Sciences,Beijing 100049,China;Institute of Optics and Electronics,Chinese Academy of Sciences,Chengdu 610209,China;Shanghai Institute of Technical Physics,Chinese Academy of Sciences,Shanghai 200083,China;Lunar Exploration and Space Engineering Center,Beijing 100190,China)
基金
supported by the China National Space Administration(CNSA)
the National Key R&D Program of China(2022YFF0503204)
the Key Research Program of the Chinese Academy of Sciences(ZDBS-SSW-TLC001)
the National Natural Science Foundation of China(12203073,42371384)。
