Solar Coronal Heating

Solar Coronal Heating is a physical process in solar astrophysics referring to the mechanism by which the Sun's corona attains and maintains temperatures significantly higher than those of the photosphere, despite being farther from the energy-generating core.

613

Publications

39.9K

Citations

1.1K

Authors

355

Institutions

Publications per year

2017–2026

113

Authors

1.1K

  1. ER
    E. R. Priest

    University of St Andrews, United Kingdom

    19 publications · 1.5K citations

    17

    h-index

  2. AR
    Amy R. Winebarger

    Marshall Space Flight Center, United States

    16 publications · 985 citations

    16

    h-index

  3. VH
    V. H. Hansteen

    University of Oslo, Norway

    19 publications · 1.5K citations

    16

    h-index

  4. HP
    Hardi Peter

    Max Planck Institute for Solar System Research, Germany

    16 publications · 1.1K citations

    14

    h-index

  5. LG
    L. Golub

    Center for Astrophysics Harvard & Smithsonian, United States

    14 publications · 1.5K citations

    14

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 292 publications · 21.7K citations

    81

    h-index

  2. Astronomy and Astrophysics

    64 publications · 3.2K citations

    31

    h-index

  3. The Astrophysical Journal Letters

    28 publications · 1.4K citations

    22

    h-index

  4. Solar Physics

    29 publications · 1.6K citations

    16

    h-index

  5. 13

    h-index

1–5