Flare Classification

Flare Classification is a systematic framework used in solar physics to categorize solar flares according to their peak X-ray flux measured in the 0.1–0.8 nm wavelength range, distinguishing it from other observational methods by its reliance on standardized magnitude-based classes (A, B, C, M, X) to represent increasing levels of energy output.

271

Publications

14K

Citations

986

Authors

496

Institutions

Publications per year

2017–2026

83

Variants

Solar Flare Classification

Authors

986

  1. DS
    D. Shaun Bloomfield

    Trinity College Dublin, Ireland

    4 publications · 289 citations

    4

    h-index

  2. YM
    Yong‐Jae Moon

    Kyung Hee University, South Korea

    4 publications · 141 citations

    4

    h-index

  3. HW
    Haimin Wang

    New Jersey Institute of Technology, United States

    3 publications · 65 citations

    4

    h-index

  4. RQ
    Rami Qahwaji

    University of Bradford, United Kingdom

    4 publications · 488 citations

    4

    h-index

  5. JT
    Joan T. Merrill

    Oklahoma Medical Research Foundation, United States

    4 publications · 555 citations

    4

    h-index

1–5 of 986

Venues

  1. The Astrophysical Journal

    ApJ · 59 publications · 4.3K citations

    35

    h-index

  2. Solar Physics

    40 publications · 1.5K citations

    23

    h-index

  3. Astronomy and Astrophysics

    16 publications · 971 citations

    16

    h-index

  4. 10

    h-index

  5. Space Weather

    7 publications · 443 citations

    7

    h-index

1–5