Prominence Morphology

Prominence Morphology is a scientific construct in solar physics that characterizes the structural form and spatial configuration of solar prominences, distinguishing it from other prominence properties by focusing specifically on their observable shape, fine-scale organization, and topological arrangement within the solar corona.

260

Publications

12.9K

Citations

552

Authors

254

Institutions

Publications per year

2017–2026

24

Authors

552

  1. BS
    B. Schmieder

    Observatoire de Paris, France

    13 publications · 539 citations

    11

    h-index

  2. PH
    P. Heinzel

    Czech Academy of Sciences, Astronomical Institute, Czechia

    11 publications · 358 citations

    11

    h-index

  3. ER
    E. R. Priest

    University of St Andrews, United Kingdom

    9 publications · 259 citations

    9

    h-index

  4. UA
    U. Anzer

    Max Planck Institute for Astrophysics, Germany

    9 publications · 331 citations

    9

    h-index

  5. SG
    S. Gunár

    Czech Academy of Sciences, Astronomical Institute, Czechia

    9 publications · 280 citations

    9

    h-index

1–5 of 552

Venues

  1. Solar Physics

    77 publications · 3.3K citations

    32

    h-index

  2. The Astrophysical Journal

    ApJ · 31 publications · 2K citations

    22

    h-index

  3. Astronomy and Astrophysics

    16 publications · 661 citations

    15

    h-index

  4. 8

    h-index

  5. Okajimas Folia Anatomica Japonica

    7 publications · 223 citations

    7

    h-index

1–5