Solar Ultraviolet Variability

Solar Ultraviolet Variability is a scientific construct that denotes the temporal fluctuations in solar ultraviolet radiation arising from changes in solar atmospheric processes, distinguishing it from steady-state or broadband solar emission models.

144

Publications

7.3K

Citations

436

Authors

158

Institutions

Publications per year

2017–2026

11

Authors

436

  1. JL
    J. Lean

    United States Naval Research Laboratory, United States

    16 publications · 1K citations

    15

    h-index

  2. TN
    T. N. Woods

    Laboratory for Atmospheric and Space Physics, United States

    14 publications · 1K citations

    13

    h-index

  3. GJ
    G. J. Rottman

    Laboratory for Atmospheric and Space Physics, United States

    8 publications · 430 citations

    8

    h-index

  4. SK
    S. K. Solanki

    Max Planck Institute for Solar System Research, Germany

    6 publications · 908 citations

    6

    h-index

  5. LL
    L. L. Hood

    University of Arizona, United States

    6 publications · 284 citations

    6

    h-index

1–5 of 436

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 31 publications · 2.4K citations

    25

    h-index

  2. Geophysical Research Letters

    16 publications · 772 citations

    15

    h-index

  3. Advances in Space Research

    11 publications · 396 citations

    11

    h-index

  4. Solar Physics

    10 publications · 300 citations

    10

    h-index

  5. Journal of Atmospheric and Solar-Terrestrial Physics

    JASTP · 6 publications · 243 citations

    6

    h-index

1–5