Coronal Activity

Coronal Activity is a stellar phenomenon characterized by the emission of high-energy radiation and plasma ejections from the outer atmosphere of a star, distinguished by its origin in the magnetically driven processes within the stellar corona.

603

Publications

36K

Citations

1.4K

Authors

466

Institutions

Publications per year

2017–2026

60

Authors

1.4K

  1. JH
    J. H. M. M. Schmitt

    Universität Hamburg, Germany

    20 publications · 797 citations

    18

    h-index

  2. NR
    N. R. Sheeley

    United States Naval Research Laboratory, United States

    13 publications · 679 citations

    13

    h-index

  3. RA
    R. A. Howard

    United States Naval Research Laboratory, United States

    15 publications · 1.6K citations

    13

    h-index

  4. RM
    R. M. MacQueen

    NSF NCAR High Altitude Observatory, United States

    11 publications · 1.3K citations

    11

    h-index

  5. MR
    M. R. Kundu

    University of Maryland, College Park, United States

    10 publications · 273 citations

    10

    h-index

1–5 of 1.4K

Venues

  1. The Astrophysical Journal

    ApJ · 173 publications · 11.9K citations

    63

    h-index

  2. Astronomy and Astrophysics

    83 publications · 4.6K citations

    41

    h-index

  3. Solar Physics

    99 publications · 5K citations

    36

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 27 publications · 3.9K citations

    24

    h-index

  5. Monthly Notices of the Royal Astronomical Society

    24 publications · 1.1K citations

    19

    h-index

1–5