Martian Lava Flows
Martian Lava Flows is a geological phenomenon consisting of solidified basaltic lava formations on the surface of Mars, distinguished from terrestrial lava flows by their extensive scale, lower gravity-induced morphologies, and preservation in an arid, low-atmospheric environment.
409
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22K
Citations
1.2K
Authors
435
Institutions
Publications per year
2017–2026
72
Parents
409
A young multilayered terrane of the northern Mare Imbrium revealed by Chang’E-3 mission
Long Xiao, Peimin Zhu, Guangyou Fang et al. · Science · 2015 · 245 citations
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United States Geological Survey
Reston, United States
25 h-index
102 publications
7.7K citations
Planetary Science Institute
Tucson, United States
24 h-index
58 publications
3.4K citations
University of Arizona
Tucson, United States
21 h-index
64 publications
5.5K citations
Arizona State University
Tempe, United States
21 h-index
43 publications
3.1K citations
Jet Propulsion Laboratory
Pasadena, United States
21 h-index
59 publications
4K citations
Astrogeology Science Center
Flagstaff, United States
20 h-index
50 publications
4.4K citations

Centre National de la Recherche Scientifique
Paris, France
19 h-index
82 publications
4.6K citations
Brown University
Providence, United States
18 h-index
33 publications
2.6K citations
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JGR · 99 publications · 7.6K citations
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30 publications · 1.9K citations
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24 publications · 775 citations
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23 publications · 1.1K citations
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25 publications · 1.6K citations
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