Fast Solar Wind

Fast Solar Wind is a type of solar wind characterized by high velocity streams, typically exceeding 500 km/s, that originate from coronal holes and exhibit lower density and temperature compared to the slow solar wind.

270

Publications

15.4K

Citations

658

Authors

276

Institutions

Publications per year

2017–2026

49

Parents

Authors

658

  1. EM
    E. Marsch

    Max Planck Institute for Solar System Research, Germany

    16 publications · 1.7K citations

    16

    h-index

  2. TS
    T. S. Horbury

    Imperial College London, United Kingdom

    14 publications · 1.3K citations

    14

    h-index

  3. DJ
    D. J. McComas

    Southwest Research Institute, United States

    13 publications · 1.2K citations

    13

    h-index

  4. NA
    N. A. Schwadron

    University of New Hampshire, United States

    13 publications · 973 citations

    12

    h-index

  5. SR
    S. R. Habbal

    Center for Astrophysics Harvard & Smithsonian, United States

    11 publications · 449 citations

    11

    h-index

1–5 of 658

Venues

  1. The Astrophysical Journal

    ApJ · 74 publications · 4.4K citations

    37

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 56 publications · 3.7K citations

    35

    h-index

  3. Geophysical Research Letters

    20 publications · 1.5K citations

    18

    h-index

  4. The Astrophysical Journal Letters

    15 publications · 771 citations

    14

    h-index

  5. Astronomy and Astrophysics

    17 publications · 519 citations

    13

    h-index

1–5