Solar Declination

Solar Declination is the angular position of the Sun relative to the Earth's equatorial plane, specifically defined as the latitude on Earth where the Sun is directly overhead at solar noon on a given day, distinguishing it from other solar angles by its annual variation due to the tilt of the Earth's axis.

82

Publications

3.4K

Citations

224

Authors

148

Institutions

Publications per year

2017–2026

17

Variants

Solar Declination Angle

Authors

224

  1. MG
    M. Grossi

    Arcetri Astrophysical Observatory, Italy

    3 publications · 199 citations

    3

    h-index

  2. MP
    Martha P. Haynes

    Cornell University, United States

    3 publications · 199 citations

    3

    h-index

  3. CG
    C. Giovanardi

    Arcetri Astrophysical Observatory, Italy

    3 publications · 199 citations

    3

    h-index

  4. SP
    Silvia Pellegrini

    University of Bologna, Italy

    3 publications · 199 citations

    3

    h-index

  5. SD
    S. di Serego Alighieri

    Arcetri Astrophysical Observatory, Italy

    3 publications · 199 citations

    3

    h-index

1–5 of 224

Venues

  1. Journal of Geophysical Research Atmospheres

    JGR · 8 publications · 453 citations

    8

    h-index

  2. The Astronomical Journal

    AJ · 4 publications · 112 citations

    4

    h-index

  3. Astronomy and Astrophysics

    3 publications · 253 citations

    3

    h-index

  4. Geophysical Research Letters

    3 publications · 50 citations

    3

    h-index

  5. Australian Journal of Physics

    2 publications · 62 citations

    2

    h-index

1–5