Astrophysical Shocks

Astrophysical Shocks is a discontinuous flow structure in compressible fluid dynamics characterized by abrupt changes in fluid properties such as density, pressure, and temperature, arising from supersonic motions in astrophysical environments and governed by the conservation laws of mass, momentum, and energy.

1.2K

Publications

71.2K

Citations

2.4K

Authors

803

Institutions

Publications per year

2017–2026

176

Variants

Astrophysical Shock Waves

Authors

2.4K

  1. HK
    Hyesung Kang

    Pusan National University, South Korea

    26 publications · 1.8K citations

    21

    h-index

  2. JC
    J. C. Raymond

    Center for Astrophysics Harvard & Smithsonian, United States

    20 publications · 1.5K citations

    19

    h-index

  3. DR
    Dongsu Ryu

    Chungnam National University, South Korea

    22 publications · 1.9K citations

    19

    h-index

  4. GP
    G. P. Zank

    University of Alabama in Huntsville, United States

    23 publications · 984 citations

    17

    h-index

  5. RP
    R. P. Drake

    University of Michigan, United States

    17 publications · 1.2K citations

    15

    h-index

1–5 of 2.4K

Venues

  1. The Astrophysical Journal

    ApJ · 405 publications · 27.9K citations

    87

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    156 publications · 11.1K citations

    51

    h-index

  3. Journal of Geophysical Research Atmospheres

    JGR · 96 publications · 3.9K citations

    37

    h-index

  4. Astronomy and Astrophysics

    77 publications · 3K citations

    35

    h-index

  5. Geophysical Research Letters

    30 publications · 1.3K citations

    22

    h-index

1–5