Venusian Tectonics

Venusian Tectonics is a geological framework that characterizes the deformational processes and structural evolution of Venus's lithosphere, distinguished from terrestrial tectonics by the absence of global plate recycling and the prominence of crustal thickening, radial fracturing, and mantle-driven resurfacing mechanisms.

103

Publications

5.6K

Citations

190

Authors

106

Institutions

Publications per year

2017–2026

15

Authors

190

  1. JW
    J. W. Head

    Brown University, United States

    12 publications · 548 citations

    11

    h-index

  2. VL
    Vicki L. Hansen

    Southern Methodist University, United States

    7 publications · 446 citations

    7

    h-index

  3. GS
    G. Schubert

    University of California, Los Angeles, United States

    6 publications · 644 citations

    6

    h-index

  4. ER
    E. R. Stofan

    Jet Propulsion Laboratory, United States

    6 publications · 705 citations

    6

    h-index

  5. SE
    S. E. Smrekar

    Jet Propulsion Laboratory, United States

    6 publications · 289 citations

    6

    h-index

1–5 of 190

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 22 publications · 1.6K citations

    18

    h-index

  2. Icarus

    18 publications · 921 citations

    16

    h-index

  3. Geophysical Research Letters

    8 publications · 275 citations

    8

    h-index

  4. Planetary and Space Science

    6 publications · 136 citations

    6

    h-index

  5. Journal of Geophysical Research Planets

    5 publications · 283 citations

    5

    h-index

1–5