Prominence Flares

Prominence Flares is a phenomenon in solar physics denoting a sudden, localized eruption of magnetic energy within a solar prominence, characterized by rapid brightening and intensified radiation emission due to plasma heating and particle acceleration.

267

Publications

12.8K

Citations

630

Authors

283

Institutions

Publications per year

2017–2026

18

Variants

Filament Flares

Authors

630

  1. ET
    E. Tandberg‐Hanssen

    Marshall Space Flight Center, United States

    8 publications · 180 citations

    8

    h-index

  2. PH
    P. Heinzel

    Czech Academy of Sciences, Astronomical Institute, Czechia

    7 publications · 584 citations

    7

    h-index

  3. KS
    Kazunari Shibata

    Kyoto University, Japan

    7 publications · 472 citations

    7

    h-index

  4. BS
    B. Schmieder

    Observatoire de Paris, France

    6 publications · 612 citations

    6

    h-index

  5. RA
    R. A. Harrison

    Rutherford Appleton Laboratory, United Kingdom

    6 publications · 353 citations

    6

    h-index

1–5 of 630

Venues

  1. Solar Physics

    101 publications · 5K citations

    35

    h-index

  2. The Astrophysical Journal

    ApJ · 51 publications · 2.6K citations

    28

    h-index

  3. Astronomy and Astrophysics

    15 publications · 635 citations

    13

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 10 publications · 706 citations

    10

    h-index

  5. Advances in Space Research

    7 publications · 243 citations

    7

    h-index

1–5