Prominence Formation

Prominence Formation is a theoretical framework in solar physics that explains the process by which cool, dense plasma becomes suspended in the Sun's corona through the interplay of magnetic field structures and thermodynamic instabilities, distinguishing it from general coronal activity models by focusing specifically on the initiation and structuring of prominence plasma within filament channels.

196

Publications

15.9K

Citations

464

Authors

235

Institutions

Publications per year

2017–2026

27

Variants

Filament Formation

Authors

464

  1. SK
    S. K. Antiochos

    United States Naval Research Laboratory, United States

    14 publications · 1.2K citations

    13

    h-index

  2. RK
    Rony Keppens

    KU Leuven, Belgium

    8 publications · 516 citations

    8

    h-index

  3. ER
    E. R. Priest

    University of St Andrews, United Kingdom

    7 publications · 197 citations

    7

    h-index

  4. CR
    C. R. DeVore

    United States Naval Research Laboratory, United States

    6 publications · 474 citations

    6

    h-index

  5. JA
    J. A. Klimchuk

    Goddard Space Flight Center, United States

    6 publications · 656 citations

    6

    h-index

1–5 of 464

Venues

  1. The Astrophysical Journal

    ApJ · 54 publications · 5.1K citations

    39

    h-index

  2. Solar Physics

    32 publications · 1.5K citations

    23

    h-index

  3. Astronomy and Astrophysics

    15 publications · 714 citations

    15

    h-index

  4. 7

    h-index

  5. Geophysical Research Letters

    4 publications · 355 citations

    4

    h-index

1–5