Solar Surface Flows

Solar Surface Flows is a physical phenomenon within solar physics that denotes the large-scale horizontal motions of plasma across the Sun's photosphere, distinguished by their role in advecting magnetic fields and contributing to the evolution of surface magnetic topology.

400

Publications

21.1K

Citations

779

Authors

354

Institutions

Publications per year

2017–2026

80

Authors

779

  1. LG
    L. Gizon

    Max Planck Institute for Solar System Research, Germany

    12 publications · 357 citations

    12

    h-index

  2. FH
    F. Hill

    National Solar Observatory, United States

    12 publications · 1.1K citations

    12

    h-index

  3. MS
    M. Sobotka

    Czech Academy of Sciences, Astronomical Institute, Czechia

    8 publications · 392 citations

    9

    h-index

  4. MR
    M. Rieutord

    Centre National de la Recherche Scientifique, France

    9 publications · 386 citations

    9

    h-index

  5. TL
    T. L. Duvall

    Goddard Space Flight Center, United States

    8 publications · 740 citations

    9

    h-index

1–5 of 779

Venues

  1. The Astrophysical Journal

    ApJ · 102 publications · 7.5K citations

    43

    h-index

  2. Astronomy and Astrophysics

    61 publications · 2.3K citations

    28

    h-index

  3. Solar Physics

    33 publications · 1.4K citations

    21

    h-index

  4. Solar Energy

    12 publications · 466 citations

    12

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 12 publications · 889 citations

    11

    h-index

1–5