Solar Tides

Solar Tides is a tidal phenomenon within the equilibrium tide theory characterized by the periodic deformation of Earth's oceans due to the gravitational attraction of the Sun, distinguished from lunar tides by its dependence on the Sun–Earth orbital configuration and its semiannual and semi-diurnal harmonic components.

215

Publications

12.1K

Citations

500

Authors

225

Institutions

Publications per year

2017–2026

38

Authors

500

  1. JM
    J. M. Forbes

    University of Colorado Boulder, United States

    29 publications · 2.9K citations

    25

    h-index

  2. RS
    Richard S. Lindzen

    Massachusetts Institute of Technology, United States

    6 publications · 602 citations

    6

    h-index

  3. ME
    M. E. Hagan

    NSF National Center for Atmospheric Research, United States

    6 publications · 1K citations

    6

    h-index

  4. NM
    N. M. Pedatella

    NSF National Center for Atmospheric Research, United States

    6 publications · 416 citations

    6

    h-index

  5. AM
    Astrid Maute

    NSF NCAR High Altitude Observatory, United States

    6 publications · 382 citations

    6

    h-index

1–5 of 500

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 43 publications · 3.6K citations

    27

    h-index

  2. Journal of Geophysical Research Space Physics

    18 publications · 818 citations

    16

    h-index

  3. Geophysical Research Letters

    17 publications · 1.1K citations

    15

    h-index

  4. Journal of the Atmospheric Sciences

    11 publications · 777 citations

    11

    h-index

  5. Journal of Atmospheric and Terrestrial Physics

    11 publications · 644 citations

    11

    h-index

1–5