Solar Velocity Fields

Solar Velocity Fields is a physical construct in solar spectroscopy that represents the spatially resolved line-of-sight and horizontal motions of plasma on the Sun's surface, derived from Doppler shifts in spectral lines, to characterize dynamic atmospheric processes such as convection, oscillations, and flows.

126

Publications

6.5K

Citations

256

Authors

124

Institutions

Publications per year

2017–2026

5

Authors

256

  1. MR
    M. Rieutord

    Centre National de la Recherche Scientifique, France

    7 publications · 286 citations

    7

    h-index

  2. TR
    Th. Roudier

    Observatoire Midi-Pyrénées, France

    6 publications · 213 citations

    6

    h-index

  3. NR
    N. R. Sheeley

    United States Naval Research Laboratory, United States

    5 publications · 189 citations

    5

    h-index

  4. FD
    Franz‐Ludwig Deubner

    Fraunhofer Institute for Physical Measurement Techniques, Germany

    4 publications · 148 citations

    4

    h-index

  5. JM
    Jean-Marie Malherbe

    Observatoire de Paris, France

    4 publications · 145 citations

    4

    h-index

1–5 of 256

Venues

  1. The Astrophysical Journal

    ApJ · 33 publications · 2.7K citations

    24

    h-index

  2. Solar Physics

    28 publications · 1.5K citations

    19

    h-index

  3. Astronomy and Astrophysics

    19 publications · 774 citations

    17

    h-index

  4. 5

    h-index

  5. 3

    h-index

1–5