Cme Acceleration

CME Acceleration is a physical phenomenon in solar physics characterized by the rate of change in velocity of a coronal mass ejection as it propagates outward from the Sun, distinguishing it from other kinematic phases of CME evolution such as initiation or propagation.

53

Publications

4.1K

Citations

149

Authors

92

Institutions

Publications per year

2017–2026

5

Variants

Coronal Mass Ejection Acceleration

Authors

149

  1. BV
    B. Vršnak

    Croatian Geological Survey, Croatia

    7 publications · 880 citations

    7

    h-index

  2. AV
    Astrid Veronig

    University of Graz, Austria

    6 publications · 759 citations

    6

    h-index

  3. NG
    N. Gopalswamy

    Goddard Space Flight Center, United States

    5 publications · 209 citations

    5

    h-index

  4. MT
    Manuela Temmer

    University of Graz, Austria

    5 publications · 669 citations

    5

    h-index

  5. AL
    A. Lara

    Universidad Nacional Autónoma de México, Mexico

    4 publications · 666 citations

    4

    h-index

1–5 of 149

Venues

  1. The Astrophysical Journal

    ApJ · 30 publications · 2.5K citations

    25

    h-index

  2. Solar Physics

    4 publications · 176 citations

    4

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 3 publications · 253 citations

    3

    h-index

  4. Annales Geophysicae

    2 publications · 149 citations

    2

    h-index

  5. Geophysical Research Letters

    2 publications · 555 citations

    2

    h-index

1–5