Ring Mass Distribution

Ring Mass Distribution is a physical model that characterizes the spatial variation of mass density across a planetary ring system, distinguishing it from other ring properties by quantifying how mass is radially and azimuthally distributed relative to the central planet.

59

Publications

3.1K

Citations

431

Authors

222

Institutions

Publications per year

2017–2026

5

Authors

431

  1. LW
    L. W. Esposito

    Laboratory for Atmospheric and Space Physics, United States

    5 publications · 274 citations

    5

    h-index

  2. JN
    Jeffrey N. Cuzzi

    Ames Research Center, United States

    4 publications · 301 citations

    4

    h-index

  3. MS
    M. Sremčević

    Laboratory for Atmospheric and Space Physics, United States

    3 publications · 131 citations

    3

    h-index

  4. FS
    F. Spahn

    University of Potsdam, Germany

    3 publications · 82 citations

    3

    h-index

  5. MC
    Mark C. Lewis

    Trinity University, United States

    3 publications · 155 citations

    3

    h-index

1–5 of 431

Venues

  1. Icarus

    18 publications · 1.1K citations

    17

    h-index

  2. 5

    h-index

  3. Geophysical Research Letters

    3 publications · 91 citations

    3

    h-index

  4. Nature

    3 publications · 239 citations

    3

    h-index

  5. Astronomy and Astrophysics

    3 publications · 140 citations

    3

    h-index

1–5