Stellar Activity Cycles

Stellar Activity Cycles is a periodic variation in a star's chromospheric and magnetic activity, analogous to the solar cycle, that manifests through changes in ultraviolet emission, starspots, and other activity indicators over time.

225

Publications

13.2K

Citations

657

Authors

298

Institutions

Publications per year

2017–2026

62

Variants

Stellar Magnetic Activity Cycles

Authors

657

  1. SV
    S. V. Jeffers

    University of Göttingen, Germany

    13 publications · 1.1K citations

    13

    h-index

  2. JH
    J. H. M. M. Schmitt

    Universität Hamburg, Germany

    11 publications · 381 citations

    11

    h-index

  3. PP
    P. Petit

    Centre National de la Recherche Scientifique, France

    11 publications · 1K citations

    11

    h-index

  4. SC
    S. C. Marsden

    University of Southern Queensland, Australia

    10 publications · 971 citations

    10

    h-index

  5. NC
    N. C. Santos

    Universidade do Porto, Portugal

    9 publications · 693 citations

    9

    h-index

1–5 of 657

Venues

  1. Astronomy and Astrophysics

    59 publications · 3.4K citations

    34

    h-index

  2. The Astrophysical Journal

    ApJ · 47 publications · 3.7K citations

    32

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    27 publications · 1.5K citations

    19

    h-index

  4. The Astronomical Journal

    AJ · 8 publications · 406 citations

    8

    h-index

  5. arXiv (Cornell University)

    Repository · 8 publications · 291 citations

    8

    h-index

1–5