Cme Internal Structure

CME Internal Structure is a scientific construct that characterizes the spatial and temporal organization of plasma, magnetic fields, and energetic particles within a coronal mass ejection, distinguishing it by its role in determining the eruption's dynamics, geomagnetic impact, and evolution through the heliosphere.

84

Publications

4.6K

Citations

328

Authors

173

Institutions

Publications per year

2017–2026

26

Authors

328

  1. AV
    A. Vourlidas

    United States Naval Research Laboratory, United States

    6 publications · 452 citations

    6

    h-index

  2. RA
    R. A. Howard

    United States Naval Research Laboratory, United States

    5 publications · 488 citations

    5

    h-index

  3. YW
    Yuming Wang

    University of Science and Technology of China, China

    5 publications · 211 citations

    5

    h-index

  4. CS
    Chenglong Shen

    University of Science and Technology of China, China

    4 publications · 174 citations

    4

    h-index

  5. HM
    Huw Morgan

    University of Waikato, New Zealand

    4 publications · 220 citations

    4

    h-index

1–5 of 328

Venues

  1. The Astrophysical Journal

    ApJ · 19 publications · 1.1K citations

    17

    h-index

  2. Solar Physics

    15 publications · 711 citations

    14

    h-index

  3. Astronomy and Astrophysics

    7 publications · 447 citations

    7

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 4 publications · 173 citations

    4

    h-index

  5. The Astrophysical Journal Letters

    3 publications · 52 citations

    3

    h-index

1–5