Interplanetary Coronal Mass Ejections

Interplanetary Coronal Mass Ejections is a large-scale transient phenomenon in the heliosphere characterized by the propagation of magnetized plasma clouds originating from the Sun, distinguishable from other solar wind disturbances by its enhanced magnetic field strength, low proton temperature, and coherent magnetic flux rope structure.

932

Publications

58.5K

Citations

2K

Authors

605

Institutions

Publications per year

2017–2026

265

Variants

Icmes

Authors

2K

  1. JG
    J. G. Luhmann

    University of California, Berkeley, United States

    44 publications · 3.6K citations

    33

    h-index

  2. IG
    I. G. Richardson

    Goddard Space Flight Center, United States

    43 publications · 6.1K citations

    32

    h-index

  3. CT
    C. T. Russell

    University of California, Los Angeles, United States

    33 publications · 2.6K citations

    27

    h-index

  4. RA
    R. A. Howard

    United States Naval Research Laboratory, United States

    31 publications · 4.1K citations

    24

    h-index

  5. EK
    Emilia Kilpua

    University of Helsinki, Finland

    31 publications · 2.3K citations

    24

    h-index

1–5 of 2K

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 183 publications · 19K citations

    72

    h-index

  2. The Astrophysical Journal

    ApJ · 169 publications · 8.8K citations

    52

    h-index

  3. Geophysical Research Letters

    74 publications · 5.1K citations

    39

    h-index

  4. Solar Physics

    81 publications · 5.3K citations

    38

    h-index

  5. Journal of Geophysical Research Space Physics

    81 publications · 3.5K citations

    36

    h-index

1–5