Coronal Plasma Dynamics

Coronal Plasma Dynamics is a theoretical framework within solar physics that characterizes the motion, acceleration, and energy transfer processes of ionized gases in the Sun's corona, distinguished by its focus on magnetohydrodynamic behaviors and thermal structuring under the influence of magnetic fields.

2.4K

Publications

143.4K

Citations

3.3K

Authors

820

Institutions

Publications per year

2017–2026

408

Authors

3.3K

  1. VM
    V. M. Nakariakov

    University of Warwick, United Kingdom

    55 publications · 4.7K citations

    35

    h-index

  2. JA
    J. A. Linker

    Predictive Science (United States), United States

    37 publications · 3.5K citations

    29

    h-index

  3. ZM
    Z. Mikić

    Science Applications International Corporation (United States), United States

    40 publications · 3.9K citations

    29

    h-index

  4. LO
    L. Ofman

    Goddard Space Flight Center, United States

    41 publications · 3.4K citations

    29

    h-index

  5. SK
    S. K. Antiochos

    United States Naval Research Laboratory, United States

    40 publications · 2.1K citations

    29

    h-index

1–5 of 3.3K

Venues

  1. The Astrophysical Journal

    ApJ · 911 publications · 62.7K citations

    119

    h-index

  2. Astronomy and Astrophysics

    275 publications · 12.8K citations

    60

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 133 publications · 9.8K citations

    57

    h-index

  4. Solar Physics

    257 publications · 13K citations

    56

    h-index

  5. The Astrophysical Journal Letters

    88 publications · 4.2K citations

    38

    h-index

1–5