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

Publications

22K

Citations

1.2K

Authors

435

Institutions

Publications per year

2017–2026

72

Authors

1.2K

  1. JW
    J. W. Head

    Brown University, United States

    16 publications · 1.6K citations

    16

    h-index

  2. GN
    G. Neukum

    Freie Universität Berlin, Germany

    15 publications · 911 citations

    14

    h-index

  3. LK
    L. Keszthelyi

    United States Geological Survey, United States

    13 publications · 1.6K citations

    13

    h-index

  4. PJ
    P. J. Mouginis‐Mark

    University of Hawaii System, United States

    11 publications · 583 citations

    11

    h-index

  5. AS
    A. S. McEwen

    University of Arizona, United States

    11 publications · 1.5K citations

    11

    h-index

1–5 of 1.2K

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 99 publications · 7.6K citations

    51

    h-index

  2. Geophysical Research Letters

    30 publications · 1.9K citations

    24

    h-index

  3. Journal of Geophysical Research Planets

    24 publications · 775 citations

    19

    h-index

  4. Journal of Volcanology and Geothermal Research

    23 publications · 1.1K citations

    19

    h-index

  5. Icarus

    25 publications · 1.6K citations

    19

    h-index

1–5