Cme Shocks

CME Shock is a transient magnetohydrodynamic shock wave in the solar wind that is driven by a coronal mass ejection and characterized by a sudden increase in plasma density, temperature, and magnetic field strength at the interface between the ejecta and the ambient solar wind.

330

Publications

18.4K

Citations

824

Authors

337

Institutions

Publications per year

2017–2026

79

Variants

Cme Shock

Authors

824

  1. RA
    R. A. Howard

    United States Naval Research Laboratory, United States

    20 publications · 2.5K citations

    18

    h-index

  2. RV
    Rami Vainio

    University of Turku, Finland

    18 publications · 530 citations

    17

    h-index

  3. NG
    N. Gopalswamy

    Goddard Space Flight Center, United States

    23 publications · 985 citations

    17

    h-index

  4. SY
    S. Yashiro

    Goddard Space Flight Center, United States

    20 publications · 1.7K citations

    16

    h-index

  5. AV
    A. Vourlidas

    United States Naval Research Laboratory, United States

    16 publications · 1.1K citations

    15

    h-index

1–5 of 824

Venues

  1. The Astrophysical Journal

    ApJ · 86 publications · 4.5K citations

    37

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 44 publications · 4.2K citations

    29

    h-index

  3. Astronomy and Astrophysics

    32 publications · 1.3K citations

    24

    h-index

  4. Geophysical Research Letters

    24 publications · 1.6K citations

    20

    h-index

  5. Solar Physics

    25 publications · 1.2K citations

    18

    h-index

1–5