Stellar Activity Evolution

Stellar Activity Evolution is a theoretical construct that characterizes the temporal development of magnetic and radiative phenomena in stars over their lifetimes, distinguishing itself by its focus on the systematic changes in stellar activity levels—such as flaring, coronal mass ejections, and chromospheric emission—that influence planetary habitability conditions.

204

Publications

13.7K

Citations

838

Authors

331

Institutions

Publications per year

2017–2026

51

Authors

838

  1. FM
    F. Murgas

    Instituto de Astrofísica de Canarias, Spain

    12 publications · 538 citations

    12

    h-index

  2. LN
    L. Nortmann

    Instituto de Astrofísica de Canarias, Spain

    10 publications · 453 citations

    10

    h-index

  3. JH
    J. H. M. M. Schmitt

    Universität Hamburg, Germany

    9 publications · 251 citations

    9

    h-index

  4. IR
    I. Ribas

    Institute of Space Sciences, Spain

    8 publications · 692 citations

    8

    h-index

  5. HP
    H. Parviainen

    Instituto de Astrofísica de Canarias, Spain

    8 publications · 313 citations

    8

    h-index

1–5 of 838

Venues

  1. Astronomy and Astrophysics

    47 publications · 2.9K citations

    32

    h-index

  2. The Astrophysical Journal

    ApJ · 49 publications · 4.8K citations

    31

    h-index

  3. 19

    h-index

  4. The Astronomical Journal

    AJ · 14 publications · 883 citations

    14

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 10 publications · 653 citations

    10

    h-index

1–5