Prominence Heating

Prominence Heating is a physical process in solar physics that refers to the mechanism by which energy is transferred and dissipated within solar prominences, maintaining their observed thermal structure against radiative and conductive losses.

22

Publications

1.9K

Citations

46

Authors

41

Institutions

Publications per year

2017–2026

2

Authors

46

  1. SK
    S. K. Antiochos

    United States Naval Research Laboratory, United States

    3 publications · 317 citations

    3

    h-index

  2. PH
    P. Heinzel

    Czech Academy of Sciences, Astronomical Institute, Czechia

    3 publications · 501 citations

    3

    h-index

  3. JT
    J. T. Karpen

    Goddard Space Flight Center, United States

    2 publications · 100 citations

    2

    h-index

  4. BS
    B. Schmieder

    Observatoire de Paris, France

    2 publications · 441 citations

    2

    h-index

  5. PA
    Patrick Antolin

    Northumbria University, United Kingdom

    2 publications · 271 citations

    2

    h-index

1–5 of 46

Venues

  1. The Astrophysical Journal

    ApJ · 13 publications · 1.1K citations

    13

    h-index

  2. Solar Physics

    2 publications · 114 citations

    2

    h-index

  3. Astronomy and Astrophysics

    2 publications · 73 citations

    2

    h-index

  4. Space Science Reviews

    1 publications · 431 citations

    1

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 1 publications · 142 citations

    1

    h-index

1–5