Prominence Oscillations

Prominence Oscillations is a dynamic phenomenon in solar physics characterized by periodic displacements of plasma within solar prominences, distinguished by its manifestation as magnetohydrodynamic waves propagating along magnetic field lines in the Sun's corona.

165

Publications

7.7K

Citations

253

Authors

151

Institutions

Publications per year

2017–2026

22

Authors

253

  1. JL
    J. L. Ballester

    Universitat de les Illes Balears, Spain

    35 publications · 1.6K citations

    25

    h-index

  2. RO
    R. Oliver

    Universitat de les Illes Balears, Spain

    26 publications · 1.4K citations

    21

    h-index

  3. RS
    R. Soler

    Universitat de les Illes Balears, Spain

    15 publications · 486 citations

    13

    h-index

  4. AJ
    A. J. Díaz

    Universitat de les Illes Balears, Spain

    7 publications · 401 citations

    7

    h-index

  5. JT
    J. Terradas

    Universitat de les Illes Balears, Spain

    6 publications · 264 citations

    6

    h-index

1–5 of 253

Venues

  1. The Astrophysical Journal

    ApJ · 37 publications · 2K citations

    27

    h-index

  2. Astronomy and Astrophysics

    35 publications · 1.5K citations

    24

    h-index

  3. Solar Physics

    37 publications · 1.2K citations

    22

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 7 publications · 152 citations

    7

    h-index

  5. The Astrophysical Journal Letters

    7 publications · 448 citations

    6

    h-index

1–5