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  2. Theory of tides - Wikipedia

    en.wikipedia.org/wiki/Theory_of_tides

    The second strongest tidal constituent "S 2" is influenced by the sun, and its Doodson numbers are 273.555, meaning that its frequency is composed of twice the first Doodson argument, +2 times the second, -2 times the third, and zero times each of the other three. [50] This aggregates to the angular equivalent of mean solar time +12 hours.

  3. Iribarren number - Wikipedia

    en.wikipedia.org/wiki/Iribarren_number

    The parameter used to describe breaking wave types on beaches; or wave run-up on – and reflection by – beaches, breakwaters and dikes. [4] [5] [6] Iribarren Number (ξ 0) as a function of wave height with constant beach steepness of 7.5 degrees. Iribarren's work was further developed by Jurjen Battjes in 1974, who named the parameter after ...

  4. Internal tide - Wikipedia

    en.wikipedia.org/wiki/Internal_tide

    Internal tides are generated as the surface tides move stratified water up and down sloping topography, which produces a wave in the ocean interior. So internal tides are internal waves at a tidal frequency. The other major source of internal waves is the wind which produces internal waves near the inertial frequency.

  5. Tide table - Wikipedia

    en.wikipedia.org/wiki/Tide_table

    Tide tables, sometimes called tide charts, are used for tidal prediction and show the daily times and levels of high and low tides, usually for a particular location. [1] Tide heights at intermediate times (between high and low water) can be approximated by using the rule of twelfths or more accurately calculated by using a published tidal ...

  6. Tidal acceleration - Wikipedia

    en.wikipedia.org/wiki/Tidal_acceleration

    Tidal acceleration is an effect of the tidal forces between an orbiting natural satellite (e.g. the Moon) and the primary planet that it orbits (e.g. Earth). The acceleration causes a gradual recession of a satellite in a prograde orbit (satellite moving to a higher orbit, away from the primary body, with a lower orbital velocity and hence a ...

  7. Significant wave height - Wikipedia

    en.wikipedia.org/wiki/Significant_wave_height

    Significant wave height H 1/3, or H s or H sig, as determined in the time domain, directly from the time series of the surface elevation, is defined as the average height of that one-third of the N measured waves having the greatest heights: [5] / = = where H m represents the individual wave heights, sorted into descending order of height as m increases from 1 to N.

  8. Amphidromic point - Wikipedia

    en.wikipedia.org/wiki/Amphidromic_point

    When neglecting friction, the position of the amphidromic points would be in the middle of the basin, as the initial amplitude and the amplitude decay of the incident wave and the reflected wave are equal, this can be seen in Animations 1 and 2 [8] However, tidal waves in the ocean are subject to friction from the seabed and from interaction ...

  9. Atmospheric tide - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_tide

    It depends on local time and travels westward with the Sun. It is an external mode of class 2 and has the eigenvalue of ε 1 −2 = −12.56. Its maximum pressure amplitude on the ground is about 60 Pa. [5] The largest solar semidiurnal wave is mode (2, 2) with maximum pressure amplitudes at the ground of 120 Pa. It is an internal class 1 wave.