Solar Gravity Waves

Solar Gravity Waves is a type of internal solar oscillation mode characterized by buoyancy-driven restoring forces in stably stratified layers, where fluid elements oscillate under the influence of gravity and density stratification, predominantly occurring in the Sun's interior below the convection zone.

226

Publications

10.6K

Citations

641

Authors

270

Institutions

Publications per year

2017–2026

36

Variants

G-modes

Authors

641

  1. JP
    J. Provost

    Observatoire de la Côte d’Azur, France

    5 publications · 516 citations

    6

    h-index

  2. SL
    Sharon L. Vadas

    Northwest Research Associates, United States

    6 publications · 536 citations

    6

    h-index

  3. GB
    G. Berthomieu

    Observatoire de la Côte d’Azur, France

    4 publications · 233 citations

    5

    h-index

  4. RA
    R. A. García

    Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France

    4 publications · 482 citations

    4

    h-index

  5. GC
    Gang Chen

    Wuhan University, China

    4 publications · 157 citations

    4

    h-index

1–5 of 641

Venues

  1. The Astrophysical Journal

    ApJ · 33 publications · 1.9K citations

    23

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 32 publications · 2.2K citations

    23

    h-index

  3. Geophysical Research Letters

    21 publications · 1K citations

    17

    h-index

  4. Journal of Geophysical Research Space Physics

    18 publications · 649 citations

    16

    h-index

  5. 14

    h-index

1–5