Pitted Terrain

Pitted Terrain is a planetary landform characterized by a surface densely marked with small, bowl-shaped depressions formed primarily by impact cratering, volcanic activity, or sublimation processes, distinguishing it from other terrains by its distinctive clustered depressions at various scales.

12

Publications

672

Citations

100

Authors

52

Institutions

Publications per year

2017–2026

1

Authors

100

  1. CA
    C. A. Raymond

    Jet Propulsion Laboratory, United States

    3 publications · 220 citations

    3

    h-index

  2. FT
    F. Tosi

    Institute for Space Astrophysics and Planetology, Italy

    3 publications · 220 citations

    3

    h-index

  3. MC
    M. C. De Sanctis

    Institute for Space Astrophysics and Planetology, Italy

    3 publications · 220 citations

    3

    h-index

  4. CT
    C. T. Russell

    University of California, Los Angeles, United States

    3 publications · 220 citations

    3

    h-index

  5. JW
    J. W. Head

    Brown University, United States

    2 publications · 63 citations

    2

    h-index

1–5 of 100

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 4 publications · 282 citations

    4

    h-index

  2. Geophysical Research Letters

    3 publications · 148 citations

    3

    h-index

  3. Geographical Review

    1 publications · 11 citations

    1

    h-index

  4. Icarus

    1 publications · 57 citations

    1

    h-index

  5. 1

    h-index

1–5