Martian Dune Fields

Martian Dune Fields is a geomorphological construct denoting a large-scale assemblage of aeolian sedimentary features on the surface of Mars characterized by spatially contiguous dunes shaped by Martian atmospheric processes, distinguished from terrestrial dune fields by their formation under low-pressure, cold, and hyperarid planetary conditions.

112

Publications

7.4K

Citations

340

Authors

174

Institutions

Publications per year

2017–2026

33

Authors

340

  1. LK
    L. K. Fenton

    Search for Extraterrestrial Intelligence, United States

    18 publications · 1.3K citations

    17

    h-index

  2. NT
    N. T. Bridges

    Jet Propulsion Laboratory, United States

    12 publications · 1.1K citations

    12

    h-index

  3. MC
    M. C. Bourke

    Planetary Science Institute, United States

    9 publications · 659 citations

    9

    h-index

  4. MG
    M. G. A. Lapôtre

    Planetary Science Institute, United States

    9 publications · 733 citations

    9

    h-index

  5. SS
    S. Silvestro

    Search for Extraterrestrial Intelligence, United States

    9 publications · 443 citations

    9

    h-index

1–5 of 340

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 17 publications · 1.5K citations

    17

    h-index

  2. Icarus

    20 publications · 901 citations

    16

    h-index

  3. Journal of Geophysical Research Planets

    14 publications · 900 citations

    14

    h-index

  4. Geophysical Research Letters

    14 publications · 998 citations

    13

    h-index

  5. Geomorphology

    5 publications · 370 citations

    5

    h-index

1–5