Ring Optical Depth

Ring Optical Depth is a dimensionless radiative transfer metric that quantifies the attenuation of electromagnetic radiation through a planetary ring system due to absorption and scattering by constituent particles, distinguishing it from other ring properties by characterizing the probability of photon interaction per unit area along the line of sight.

111

Publications

5.5K

Citations

347

Authors

123

Institutions

Publications per year

2017–2026

9

Authors

347

  1. EA
    E. A. Marouf

    San Jose State University, United States

    9 publications · 702 citations

    9

    h-index

  2. GL
    G. L. Tyler

    Stanford University, United States

    8 publications · 680 citations

    8

    h-index

  3. JN
    Jeffrey N. Cuzzi

    Ames Research Center, United States

    8 publications · 926 citations

    8

    h-index

  4. PD
    P. D. Nicholson

    Cornell University, United States

    8 publications · 289 citations

    8

    h-index

  5. RG
    R. G. French

    Wellesley College, United States

    7 publications · 233 citations

    7

    h-index

1–5 of 347

Venues

  1. Icarus

    45 publications · 1.9K citations

    25

    h-index

  2. The Astronomical Journal

    AJ · 16 publications · 623 citations

    15

    h-index

  3. The Astrophysical Journal

    ApJ · 7 publications · 230 citations

    7

    h-index

  4. Geophysical Research Letters

    6 publications · 245 citations

    6

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 6 publications · 259 citations

    6

    h-index

1–5