Solar Wind

Solar Wind is a continuous stream of charged particles, primarily electrons and protons, emitted from the Sun's corona that propagates through interplanetary space as a plasma flow distinct from discrete solar eruptions.

13.6K

Publications

790.9K

Citations

14.6K

Authors

2.6K

Institutions

Publications per year

2017–2026

2.4K

Authors

14.6K

  1. JT
    J. T. Gosling

    Los Alamos National Laboratory, United States

    190 publications · 19.3K citations

    80

    h-index

  2. SJ
    S. J. Bame

    Los Alamos National Laboratory, United States

    163 publications · 18K citations

    79

    h-index

  3. CT
    C. T. Russell

    University of California, Los Angeles, United States

    291 publications · 20.4K citations

    77

    h-index

  4. DJ
    D. J. McComas

    Southwest Research Institute, United States

    208 publications · 19.1K citations

    71

    h-index

  5. WH
    W. H. Matthaeus

    University of Delaware, United States

    152 publications · 16.6K citations

    69

    h-index

1–5 of 14.6K

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 3K publications · 227.7K citations

    196

    h-index

  2. The Astrophysical Journal

    ApJ · 1.8K publications · 115.1K citations

    152

    h-index

  3. Geophysical Research Letters

    1.1K publications · 67.8K citations

    117

    h-index

  4. Solar Physics

    894 publications · 44K citations

    93

    h-index

  5. Space Science Reviews

    231 publications · 28.5K citations

    82

    h-index

1–5