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Phenomenology of plume-surface interactions and preliminary results from the Tianwen-1 landing crater on Mars

Tao Xu Bo Zheng ZhaoBin Zhang Juan Li ShouDing Li XinShuo Chen XiuKuo Sun YanFang Wu YiMing Diao

地球与行星物理(英文)2023,Vol.7Issue(3):311-330,20.
地球与行星物理(英文)2023,Vol.7Issue(3):311-330,20.DOI:10.26464/epp2023044

Phenomenology of plume-surface interactions and preliminary results from the Tianwen-1 landing crater on Mars

Phenomenology of plume-surface interactions and preliminary results from the Tianwen-1 landing crater on Mars

Tao Xu 1Bo Zheng 1ZhaoBin Zhang 1Juan Li 2ShouDing Li 1XinShuo Chen 1XiuKuo Sun 1YanFang Wu 1YiMing Diao1

作者信息

  • 1. Key Laboratory of Shale Gas and Geoengineering,Institute of Geology and Geophysics,Chinese Academy of Sciences,Beijing 100029,China||College of Earth and Planetary Sciences,University of Chinese Academy of Sciences,Beijing 100049,China||Innovation Academy for Earth Sciences,Chinese Academy of Sciences,Beijing 100029,China
  • 2. Key Laboratory of Earth and Planetary Physics,Institute of Geology and Geophysics,Chinese Academy of Sciences,Beijing 100029,China||College of Earth and Planetary Sciences,University of Chinese Academy of Sciences,Beijing 100049,China||Innovation Academy for Earth Sciences,Chinese Academy of Sciences,Beijing 100029,China
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摘要

关键词

plume-surface interaction/phenomenology analysis/terrestrial test/Tianwen-1/landing crater

Key words

plume-surface interaction/phenomenology analysis/terrestrial test/Tianwen-1/landing crater

引用本文复制引用

Tao Xu,Bo Zheng,ZhaoBin Zhang,Juan Li,ShouDing Li,XinShuo Chen,XiuKuo Sun,YanFang Wu,YiMing Diao..Phenomenology of plume-surface interactions and preliminary results from the Tianwen-1 landing crater on Mars[J].地球与行星物理(英文),2023,7(3):311-330,20.

基金项目

We thank all the scientists and engineers who were involved in the Tianwen-1 mission,including the CNSA,the National Astro-nomical Observatories of the Chinese Academy of Sciences(NAOC),China Academy of Space Technology(CAST),Beijing Aerospace Control Center(BACC),and other critical institutes.The scientific data were provided by CNSA and the State Administration of Science Technology and Industry for National Defense.We also appreciate the instruction and discussions on photogrammetry,engineering and engine data,and Martian composition from Geng Yan,Dong Jie,Lin Yangting,Qin Xiaoguang,Zhang Jinhai,Du Aimin,Di Kaichang,Wan Wenhui,Liu Shaochuang,Zhang Zhigang,Yue Zongyu,Liu Yike,Ren Xin,Gou Sheng,Zhang Shuo,Xu Changyi,Chai Lihui,Guo Guangjun,Zhang Lei,Ye Qing,Xiao Zhuowei,Maryelin Josefina Briceno,Guo Jingyun,and other experts supporting our work.In addition,we appreciate the support from Wu Fuyuan and Pan Yongxin,leaders of the Mars Mission at the Institute of Geology and Geophysics,Chinese Academy of Sciences(CAS).This work was supported by the National Natural Science Foundation of China(Grant 42230111),the Key Research Program of the Institute of Geology and Geophysics,CAS(Mars Mission (NAOC)

Grant IGGCAS-202102),the Key Research Program of the Institute of Geology and Geophysics,CAS(Grant IGGCAS-201904),and the CAS Key Technology Talent Program. (Grant IGGCAS-201904)

地球与行星物理(英文)

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