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  2. Theory of tides - Wikipedia

    en.wikipedia.org/wiki/Theory_of_tides

    High and low tide in the Bay of Fundy. The theory of tides is the application of continuum mechanics to interpret and predict the tidal deformations of planetary and satellite bodies and their atmospheres and oceans (especially Earth's oceans) under the gravitational loading of another astronomical body or bodies (especially the Moon and Sun).

  3. Tidal range - Wikipedia

    en.wikipedia.org/wiki/Tidal_range

    The largest annual tidal range can be expected around the time of the equinox if it coincides with a spring tide. Spring tides occur at the second and fourth (last) quarters of the lunar phases. By contrast, during neap tides, when the Moon and Sun's gravitational force vectors act in quadrature (making a right angle to the Earth's orbit), the ...

  4. Tide - Wikipedia

    en.wikipedia.org/wiki/Tide

    Mean high water springs (MHWS) – The average of the two high tides on the days of spring tides. Mean high water neaps (MHWN) – The average of the two high tides on the days of neap tides. Mean sea level (MSL) – This is the average sea level. The MSL is constant for any location over a long period.

  5. Earth tide - Wikipedia

    en.wikipedia.org/wiki/Earth_tide

    Terrestrial tides also need to be taken in account in the case of some particle physics experiments. [8] For instance, at the CERN or the SLAC National Accelerator Laboratory, the very large particle accelerators were designed while taking terrestrial tides into account for proper operation. Among the effects that need to be taken into account ...

  6. Tide table - Wikipedia

    en.wikipedia.org/wiki/Tide_table

    The dates of spring tides and neap tides, approximately seven days apart, can be determined by the heights of the tides on the classic tide tables: a small range indicates neaps and large indicates springs. This cycle of tides is linked to the phases of the moon, with the highest tides (spring tides) occurring near full moon and new moon.

  7. Tidal force - Wikipedia

    en.wikipedia.org/wiki/Tidal_force

    Figure 1: Tidal interaction between the spiral galaxy NGC 169 and a smaller companion [1]. The tidal force or tide-generating force is a gravitational effect that stretches a body along the line towards and away from the center of mass of another body due to spatial variations in strength in gravitational field from the other body.

  8. Love number - Wikipedia

    en.wikipedia.org/wiki/Love_number

    For Earth's tides one can calculate the tilt factor as + and the gravimetric factor as + (/), where subscript two is assumed. [ 5 ] Neutron stars are thought to have high rigidity in the crust, and thus a low Love number: 0.05 ≤ k 2 ≤ 0.17 {\displaystyle 0.05\leq k_{2}\leq 0.17} ; [ 6 ] [ 7 ] isolated, nonrotating black holes in vacuum have ...

  9. Primitive equations - Wikipedia

    en.wikipedia.org/wiki/Primitive_equations

    The primitive equations may be linearized to yield Laplace's tidal equations, an eigenvalue problem from which the analytical solution to the latitudinal structure of the flow may be determined. In general, nearly all forms of the primitive equations relate the five variables u, v, ω, T, W, and their evolution over space and time.