Photometric Correction

Photometric Correction is a radiometric processing technique that adjusts observed planetary surface brightness measurements to account for variations in illumination and viewing geometry, thereby enabling accurate comparison and interpretation of reflectance properties across different observational conditions.

334

Publications

21.5K

Citations

1.8K

Authors

553

Institutions

Publications per year

2017–2026

63

Variants

Photometric Normalization

Authors

1.8K

  1. JL
    Jian‐Yang Li

    Planetary Science Institute, United States

    8 publications · 517 citations

    8

    h-index

  2. DL
    D. L. Domingue

    Johns Hopkins University Applied Physics Laboratory, United States

    6 publications · 207 citations

    6

    h-index

  3. BJ
    B. J. Buratti

    Jet Propulsion Laboratory, United States

    5 publications · 252 citations

    5

    h-index

  4. CM
    C. M. Pieters

    Brown University, United States

    5 publications · 310 citations

    5

    h-index

  5. YY
    Y. Yokota

    Japan Aerospace Exploration Agency, Japan

    5 publications · 284 citations

    5

    h-index

1–5 of 1.8K

Venues

  1. Icarus

    44 publications · 2.4K citations

    27

    h-index

  2. Astronomy and Astrophysics

    23 publications · 2.7K citations

    20

    h-index

  3. The Astronomical Journal

    AJ · 21 publications · 1.6K citations

    18

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    20 publications · 1.9K citations

    17

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 18 publications · 2.4K citations

    15

    h-index

1–5