Cme Propagation

CME Propagation is a physical process in heliophysics that describes the transit of coronal mass ejections through the heliosphere, distinguished by the evolution of their kinematic, thermal, and magnetic properties as they interact with the ambient solar wind and interplanetary magnetic field.

125

Publications

6.1K

Citations

428

Authors

177

Institutions

Publications per year

2017–2026

35

Authors

428

  1. AV
    A. Vourlidas

    United States Naval Research Laboratory, United States

    10 publications · 629 citations

    10

    h-index

  2. MT
    Manuela Temmer

    University of Graz, Austria

    9 publications · 792 citations

    9

    h-index

  3. YW
    Yuming Wang

    University of Science and Technology of China, China

    8 publications · 327 citations

    8

    h-index

  4. DO
    D. Odstrčil

    Goddard Space Flight Center, United States

    7 publications · 372 citations

    7

    h-index

  5. SP
    Stefaan Poedts

    KU Leuven, Belgium

    7 publications · 331 citations

    7

    h-index

1–5 of 428

Venues

  1. The Astrophysical Journal

    ApJ · 28 publications · 1.7K citations

    24

    h-index

  2. Solar Physics

    30 publications · 1.6K citations

    21

    h-index

  3. Astronomy and Astrophysics

    7 publications · 229 citations

    7

    h-index

  4. Advances in Space Research

    7 publications · 223 citations

    7

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 6 publications · 331 citations

    6

    h-index

1–5