Cme Source Regions

CME Source Regions is a solar atmospheric construct denoting specific localized areas on the Sun, typically associated with active regions or magnetic complexity, from which coronal mass ejections originate due to the destabilization of magnetic field configurations.

93

Publications

5.8K

Citations

357

Authors

184

Institutions

Publications per year

2017–2026

21

Authors

357

  1. LV
    L. van Driel‐Gesztelyi

    Observatoire de Paris, France

    8 publications · 670 citations

    8

    h-index

  2. PD
    P. Démoulin

    Observatoire de Paris, France

    7 publications · 659 citations

    7

    h-index

  3. CH
    C. H. Mandrini

    Institute of Astronomy and Space Physics, Argentina

    7 publications · 431 citations

    7

    h-index

  4. GD
    G. D. R. Attrill

    University College London, United Kingdom

    6 publications · 523 citations

    6

    h-index

  5. LK
    L. K. Harra

    University College London, United Kingdom

    5 publications · 334 citations

    5

    h-index

1–5 of 357

Venues

  1. The Astrophysical Journal

    ApJ · 34 publications · 2.7K citations

    23

    h-index

  2. Solar Physics

    17 publications · 969 citations

    17

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 9 publications · 514 citations

    9

    h-index

  4. Astronomy and Astrophysics

    8 publications · 659 citations

    8

    h-index

  5. Journal of Atmospheric and Solar-Terrestrial Physics

    JASTP · 3 publications · 101 citations

    3

    h-index

1–5