Solar Flare Loop Modeling

Solar Flare Loop Modeling is a computational and theoretical framework within solar astrophysics that simulates the dynamic evolution, thermal structure, and radiative emission of magnetically confined plasma loops during solar flares to elucidate energy transport and dissipation mechanisms in the solar corona.

117

Publications

5.9K

Citations

251

Authors

151

Institutions

Publications per year

2017–2026

28

Authors

251

  1. KS
    Kazunari Shibata

    Kyoto University, Japan

    5 publications · 299 citations

    5

    h-index

  2. MJ
    Markus J. Aschwanden

    Lockheed Martin (United States), United States

    5 publications · 241 citations

    5

    h-index

  3. GP
    G. Pérès

    Osservatorio Astronomico di Palermo, Italy

    5 publications · 78 citations

    5

    h-index

  4. SS
    S. Serio

    Osservatorio Astronomico di Palermo, Italy

    5 publications · 78 citations

    5

    h-index

  5. FR
    F. Reale

    Osservatorio Astronomico di Palermo, Italy

    5 publications · 77 citations

    5

    h-index

1–5 of 251

Venues

  1. The Astrophysical Journal

    ApJ · 70 publications · 3.6K citations

    36

    h-index

  2. Astronomy and Astrophysics

    9 publications · 324 citations

    9

    h-index

  3. Solar Physics

    7 publications · 845 citations

    7

    h-index

  4. The Astrophysical Journal Supplement Series

    5 publications · 244 citations

    5

    h-index

  5. The Astrophysical Journal Letters

    4 publications · 199 citations

    4

    h-index

1–5