White-light Flares

White-Light Flares is a phenomenon in solar physics characterized by a transient enhancement of continuum radiation across the visible spectrum during a solar flare, distinguished from typical flares by the prominence of broadband white-light emission originating from the photosphere or chromosphere.

263

Publications

12.7K

Citations

796

Authors

314

Institutions

Publications per year

2017–2026

80

Variants

White-light Solar Flares

Authors

796

  1. MD
    M. D. Ding

    Nanjing University, China

    13 publications · 436 citations

    12

    h-index

  2. CF
    Cheng Fang

    Nanjing University, China

    13 publications · 388 citations

    11

    h-index

  3. HW
    Haimin Wang

    New Jersey Institute of Technology, United States

    10 publications · 606 citations

    10

    h-index

  4. RA
    R. A. Howard

    United States Naval Research Laboratory, United States

    9 publications · 592 citations

    9

    h-index

  5. AV
    A. Vourlidas

    United States Naval Research Laboratory, United States

    8 publications · 485 citations

    8

    h-index

1–5 of 796

Venues

  1. The Astrophysical Journal

    ApJ · 92 publications · 5.6K citations

    42

    h-index

  2. Solar Physics

    52 publications · 2.1K citations

    26

    h-index

  3. Astronomy and Astrophysics

    17 publications · 894 citations

    15

    h-index

  4. The Astrophysical Journal Letters

    14 publications · 626 citations

    13

    h-index

  5. 8

    h-index

1–5