Solar Microflares

Solar microflares are a class of solar flare phenomena characterized by their relatively low energy release and compact spatial structure, distinguished from larger flares by their weaker X-ray emission and limited impact on the solar atmosphere, typically observed in the soft X-ray spectrum.

160

Publications

7.9K

Citations

436

Authors

218

Institutions

Publications per year

2017–2026

28

Authors

436

  1. HS
    H. S. Hudson

    University of California, Berkeley, United States

    13 publications · 1.9K citations

    13

    h-index

  2. SK
    Säm Krucker

    University of California, Berkeley, United States

    12 publications · 960 citations

    12

    h-index

  3. IG
    I. G. Hannah

    University of Glasgow, United Kingdom

    8 publications · 581 citations

    8

    h-index

  4. SM
    S. M. White

    University of Maryland, College Park, United States

    7 publications · 262 citations

    7

    h-index

  5. RP
    R. P. Lin

    University of California, Berkeley, United States

    6 publications · 1.2K citations

    6

    h-index

1–5 of 436

Venues

  1. The Astrophysical Journal

    ApJ · 46 publications · 3.3K citations

    30

    h-index

  2. Solar Physics

    42 publications · 2.2K citations

    23

    h-index

  3. Astronomy and Astrophysics

    8 publications · 172 citations

    8

    h-index

  4. The Astrophysical Journal Letters

    8 publications · 320 citations

    8

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 6 publications · 154 citations

    6

    h-index

1–5