Bow Shock Physics

Bow Shock Physics is a theoretical framework that characterizes the nonlinear interaction and energy dissipation processes of supersonic magnetized plasmas at the boundary preceding a planetary magnetosphere, distinguished by its focus on collisionless shock formation, particle acceleration, and field compression mechanisms in space environments.

2.3K

Publications

120.7K

Citations

4.2K

Authors

950

Institutions

Publications per year

2017–2026

346

Authors

4.2K

  1. CT
    C. T. Russell

    University of California, Los Angeles, United States

    164 publications · 11.3K citations

    65

    h-index

  2. JT
    J. T. Gosling

    Los Alamos National Laboratory, United States

    54 publications · 5.9K citations

    40

    h-index

  3. SJ
    S. J. Bame

    Los Alamos National Laboratory, United States

    50 publications · 6.1K citations

    39

    h-index

  4. DG
    D. G. Sibeck

    Goddard Space Flight Center, United States

    66 publications · 3.6K citations

    34

    h-index

  5. JA
    J. A. Slavin

    Goddard Space Flight Center, United States

    41 publications · 3.3K citations

    33

    h-index

1–5 of 4.2K

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 647 publications · 42.2K citations

    104

    h-index

  2. The Astrophysical Journal

    ApJ · 252 publications · 15.8K citations

    65

    h-index

  3. Geophysical Research Letters

    245 publications · 11.7K citations

    58

    h-index

  4. Journal of Geophysical Research Space Physics

    180 publications · 6.9K citations

    47

    h-index

  5. Monthly Notices of the Royal Astronomical Society

    111 publications · 5.8K citations

    40

    h-index

1–5