Slow Solar Wind

Slow Solar Wind is a type of solar wind characterized by lower velocities typically below 400 km/s, originating from the Sun's equatorial regions and distinguished from the fast solar wind by its higher density, lower speed, and association with closed magnetic field lines in the corona.

289

Publications

16.7K

Citations

648

Authors

273

Institutions

Publications per year

2017–2026

80

Parents

Authors

648

  1. RB
    R. Bruno

    National Institute for Astrophysics, Italy

    12 publications · 504 citations

    12

    h-index

  2. TH
    T. H. Zurbuchen

    University of Michigan, United States

    11 publications · 1.2K citations

    11

    h-index

  3. RV
    R. von Steiger

    International Space Science Institute, Switzerland

    11 publications · 1.2K citations

    11

    h-index

  4. JC
    J. C. Kasper

    University of Michigan, United States

    11 publications · 1.6K citations

    11

    h-index

  5. NA
    N. A. Schwadron

    University of New Hampshire, United States

    11 publications · 1.3K citations

    11

    h-index

1–5 of 648

Venues

  1. The Astrophysical Journal

    ApJ · 76 publications · 4.2K citations

    34

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 44 publications · 3.9K citations

    31

    h-index

  3. Journal of Geophysical Research Space Physics

    22 publications · 1K citations

    20

    h-index

  4. Geophysical Research Letters

    23 publications · 2.2K citations

    19

    h-index

  5. Astronomy and Astrophysics

    20 publications · 543 citations

    14

    h-index

1–5