Martian Interior Structure

Martian Interior Structure is a geophysical construct that specifies the compositional and mechanical layering of Mars's subsurface, distinguished from other planetary interior models by its reliance on Martian seismic, thermal, and magnetic field data to characterize core, mantle, and crustal properties unique to the planet's evolutionary history.

100

Publications

6.6K

Citations

332

Authors

155

Institutions

Publications per year

2017–2026

35

Authors

332

  1. PL
    Philippe Lognonné

    Institut de physique du globe de Paris, France

    17 publications · 1.4K citations

    16

    h-index

  2. WB
    W. B. Banerdt

    Jet Propulsion Laboratory, United States

    11 publications · 1.1K citations

    11

    h-index

  3. VD
    V. Dehant

    Royal Observatory of Belgium, Belgium

    11 publications · 821 citations

    11

    h-index

  4. DG
    Domenico Giardini

    ETH Zurich, Switzerland

    11 publications · 1.1K citations

    11

    h-index

  5. MP
    M. P. Panning

    Jet Propulsion Laboratory, United States

    9 publications · 978 citations

    9

    h-index

1–5 of 332

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 11 publications · 1.2K citations

    11

    h-index

  2. Icarus

    9 publications · 771 citations

    9

    h-index

  3. Geophysical Research Letters

    8 publications · 407 citations

    8

    h-index

  4. Physics of The Earth and Planetary Interiors

    7 publications · 297 citations

    7

    h-index

  5. Planetary and Space Science

    6 publications · 207 citations

    6

    h-index

1–5