Solar Cycle Variations

Solar Cycle Variations is a scientific construct that denotes the systematic, long-term changes in solar irradiance arising from the approximately 11-year periodic fluctuations in the Sun's magnetic activity, distinguished from other radiative variability sources by their origin in cyclic solar dynamo processes.

1.7K

Publications

86.1K

Citations

3.2K

Authors

1K

Institutions

Publications per year

2017–2026

263

Authors

3.2K

  1. SK
    S. K. Solanki

    Max Planck Institute for Solar System Research, Germany

    26 publications · 3.1K citations

    21

    h-index

  2. NA
    N. A. Krivova

    Max Planck Institute for Solar System Research, Germany

    20 publications · 1.8K citations

    17

    h-index

  3. LL
    Libo Liu

    Chinese Academy of Sciences, China

    18 publications · 1.4K citations

    17

    h-index

  4. RP
    R. P. Kane

    Instituto Nacional de Pesquisas Espaciais, Brazil

    18 publications · 595 citations

    16

    h-index

  5. WW
    Weixing Wan

    Chinese Academy of Sciences, China

    15 publications · 1.2K citations

    15

    h-index

1–5 of 3.2K

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 235 publications · 15.7K citations

    69

    h-index

  2. The Astrophysical Journal

    ApJ · 157 publications · 9.6K citations

    59

    h-index

  3. Solar Physics

    162 publications · 9.8K citations

    44

    h-index

  4. Geophysical Research Letters

    89 publications · 6K citations

    41

    h-index

  5. Astronomy and Astrophysics

    78 publications · 3.6K citations

    33

    h-index

1–5