Flare Loop Structure

Flare Loop Structure is a physical construct in solar physics that denotes a magnetically confined, arch-shaped region of enhanced plasma emission in the solar corona, distinguishable by its role in guiding and confining energy release processes during a solar flare.

280

Publications

16.6K

Citations

501

Authors

229

Institutions

Publications per year

2017–2026

54

Authors

501

  1. BS
    B. Schmieder

    Observatoire de Paris, France

    9 publications · 391 citations

    11

    h-index

  2. ER
    E. R. Priest

    University of St Andrews, United Kingdom

    10 publications · 1.5K citations

    10

    h-index

  3. JQ
    Jiong Qiu

    Montana State University, United States

    9 publications · 334 citations

    9

    h-index

  4. HW
    Haimin Wang

    New Jersey Institute of Technology, United States

    8 publications · 349 citations

    9

    h-index

  5. VF
    V. F. Melnikov

    Radiophysical Research Institute, Russia

    8 publications · 388 citations

    9

    h-index

1–5 of 501

Venues

  1. The Astrophysical Journal

    ApJ · 114 publications · 8.1K citations

    48

    h-index

  2. Solar Physics

    48 publications · 2.5K citations

    32

    h-index

  3. The Astrophysical Journal Letters

    21 publications · 990 citations

    19

    h-index

  4. Astronomy and Astrophysics

    23 publications · 1.3K citations

    19

    h-index

  5. 8

    h-index

1–5