Cme Deflection

CME Deflection is a physical phenomenon in heliophysics whereby a coronal mass ejection deviates from its initially radial trajectory in the solar corona and inner heliosphere due to interactions with ambient solar wind structures, magnetic fields, or other coronal mass ejections.

29

Publications

1.9K

Citations

82

Authors

56

Institutions

Publications per year

2017–2026

8

Variants

Coronal Mass Ejection Deflection

Authors

82

  1. CK
    Christina Kay

    Goddard Space Flight Center, United States

    5 publications · 271 citations

    5

    h-index

  2. YW
    Yuming Wang

    University of Science and Technology of China, China

    5 publications · 342 citations

    5

    h-index

  3. CS
    Chenglong Shen

    University of Science and Technology of China, China

    5 publications · 342 citations

    5

    h-index

  4. MO
    M. Opher

    Boston University, United States

    4 publications · 226 citations

    4

    h-index

  5. PY
    Pinzhong Ye

    University of Science and Technology of China, China

    3 publications · 286 citations

    3

    h-index

1–5 of 82

Venues

  1. The Astrophysical Journal

    ApJ · 13 publications · 930 citations

    12

    h-index

  2. Solar Physics

    6 publications · 410 citations

    6

    h-index

  3. Journal of Geophysical Research Space Physics

    3 publications · 191 citations

    3

    h-index

  4. The Astrophysical Journal Letters

    2 publications · 76 citations

    2

    h-index

  5. Astronomy and Astrophysics

    1 publications · 18 citations

    1

    h-index

1–5