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  2. Sunrise equation - Wikipedia

    en.wikipedia.org/wiki/Sunrise_equation

    Sunrise equation. A contour plot of the hours of daylight as a function of latitude and day of the year, using the most accurate models described in this article. It can be seen that the area of constant day and constant night reach up to the polar circles (here labeled "Anta. c." and "Arct. c."), which is a consequence of the earth's inclination.

  3. Haversine formula - Wikipedia

    en.wikipedia.org/wiki/Haversine_formula

    Δ λ = λ 2 − λ 1 {\displaystyle \Delta \lambda =\lambda _ {2}-\lambda _ {1}} . Finally, the haversine function hav (θ), applied above to both the central angle θ and the differences in latitude and longitude, is. The haversine function computes half a versine of the angle θ, or the squares of half chord of the angle on a unit circle ...

  4. Position of the Sun - Wikipedia

    en.wikipedia.org/wiki/Position_of_the_Sun

    The path of the Sun over the celestial sphere through the course of the day for an observer at 56°N latitude. The Sun's path changes with its declination during the year. The intersections of the curves with the horizontal axis show azimuths in degrees from North where the Sun rises and sets. The Sun appears to move northward during the ...

  5. Spherical coordinate system - Wikipedia

    en.wikipedia.org/wiki/Spherical_coordinate_system

    In mathematics, a spherical coordinate system is a coordinate system for three-dimensional space where the position of a given point in space is specified by three real numbers: the radial distance r along the radial line connecting the point to the fixed point of origin; the polar angle θ between the radial line and a polar axis; and the ...

  6. Rossby wave - Wikipedia

    en.wikipedia.org/wiki/Rossby_wave

    Rossby waves, also known as planetary waves, are a type of inertial wave naturally occurring in rotating fluids. [ 1] They were first identified by Sweden-born American meteorologist Carl-Gustaf Arvid Rossby in the Earth's atmosphere in 1939. They are observed in the atmospheres and oceans of Earth and other planets, owing to the rotation of ...

  7. Rossby radius of deformation - Wikipedia

    en.wikipedia.org/wiki/Rossby_radius_of_deformation

    In the ocean, the Rossby radius varies dramatically with latitude. Near the equator it is larger than 200 km, while in the high latitude regions it is less than 10 km. The size of ocean eddies varies similarly; in low latitude regions, near the equator, eddies are much larger than in high latitude regions.

  8. Kelvin wave - Wikipedia

    en.wikipedia.org/wiki/Kelvin_wave

    A Kelvin wave is a wave in the ocean, a large lake or the atmosphere that balances the Earth's Coriolis force against a topographic boundary such as a coastline, or a waveguide such as the equator. A feature of a Kelvin wave is that it is non-dispersive, i.e., the phase speed of the wave crests is equal to the group speed of the wave energy for ...

  9. Rossby number - Wikipedia

    en.wikipedia.org/wiki/Rossby_number

    The Rossby number ( Ro ), named for Carl-Gustav Arvid Rossby, is a dimensionless number used in describing fluid flow. The Rossby number is the ratio of inertial force to Coriolis force, terms and in the Navier–Stokes equations respectively. [1] [2] It is commonly used in geophysical phenomena in the oceans and atmosphere, where it ...