The Semi-diurnal Lunar Tidal Motion of the Red Sea.

Grace, S. F.

doi:10.1111/j.1365-246x.1930.tb05413.x

Cited by 9 publications

(2 citation statements)

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“…For example, a tidal motion of 0.01-cm:/s kinematic molecular viscosity, 100-km characteristic wave length (about 1 ø mesh size (section 4a)), and moderate characteristic velocity of 0.1 cm/s possesses a characteristic Reynolds number of 108, which [e.g., $chlichting, 1968] is well in the turbulent flow regime. Accordingly, any comprehensive study of ocean tidal currents must augment the LTE's (18) by two additional vector terms modeling eddy dissipation and bottom friction.In his study of tides in the Red Sea,Grace [1930a] introduced the effects of the solid earth tide into ocean tidal research (see alsoMunk et al [1970],Hendershott and Munk [1970], andCartwright [1971]). Recent gravity measurements [e.g.,Kuo et al, 1970a, b] revealed a significant interaction between the oceanic and terrestrial tides.…”

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confidence: 99%

On charting global ocean tides

Schwiderski¹

1980

Reviews of Geophysics

522

260

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This review article highlights the three‐century development of our scientific understanding of ocean tides, culminating through myths, paradoxes, and controversies in a global tide model that now permits the prediction of the instantaneous total tide anywhere in the open oceans with an accuracy of better than 10 cm. All major aspects of tidal research, including empirical, mathematical, and empirical‐mathematical methods, are considered. Particular attention is drawn to the most recently developed computerized techniques comprehending hydrodynamical dissipation and secondary tide‐generating forces, finite‐differencing schemes, geometric boundary and bathymetry modeling, and hydrodynamical interpolation of properly selected empirical tide data. Numerous computer experiments are mentioned that were carried out by various researchers in order to evaluate the magnitudes of the featured effects. Further possible improvements are mentioned, especially in nearshore areas, in the Arctic Sea, and near Antarctica, where empirical tide and bathymetry data are either rough or marginal.

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confidence: 99%

On charting global ocean tides

Schwiderski¹

1980

Reviews of Geophysics

522

260

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“…Let £ be the sea level relative to the Earth s , as measured by a tide gauge. Then, neglecting the small phase lag between the Earth-tide and the gravita tional potential, Laplace's tidal equations may be applied directly with £ as height variable, provided the forcing function is multiplied by the Love-number factor (1+ k -h) -0.70 (Proudman 1928;Grace 1930;M.S.W., pp. 182-183).…”

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confidence: 99%

Tides and waves in the vicinity of Saint Helena

1971

Phil. Trans. R. Soc. Lond. A

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Sea-bed pressures taken close to the shore-line at St Helena over 39 days are analysed for information on tides, swell, and medium frequency waves. The tidal records are analysed in conjunction with short records taken by others from Ascension, Trindade and Tristan da Cunha Islands. A nine-year series from Simons Bay, South Africa, is also investigated as a possible reference base. It is found to be partially unsuitable on account of a node in the diurnal tides, previously unsuspected, but this itself is relevant to the diurnal cotidal map. A phenomenal monthly tide at Simons Bay, with sidereal rather than anomalistic monthly periodicity, is also noted. Taking a year’s record from Ascension Island as tidal reference, new constants are evaluated for all four islands, and these are used to deduce cotidal maps fo the open South Atlantic. Two types of maps are considered, one a linear interpolation of the constants, the other derived from a locally forced tide (modified by the Earth tide) and a pair of Poincare waves calculated for a ‘(β-plane ’ approximation, assuming constant depth. Although not entirely realistic, the latter scheme fits the semi-diurnal tide data very closely, but not the diurnal data. Both types of map confirm positive semi-diurnal amphidromes, according with the computations of Pekeris and Accad and of Bogdanov and Magarik, and negative diurnal amphidromes according with Dietrich’s maps. Tidal records made at St Helena in 1761 by Maskelyne and Mason provide a unique opportunity to search for possible instabilities in the ocean tides. By careful comparison of the two sets of data, it is concluded that the semi-diurnal tides are virtually unchanged, but there is a significant change in phase of about 10° at all diurnal frequencies which may point to an instability in the diurnal modes in the Atlantic, as suggested by Garrett & Munk from other considerations. A frequency-time plot of the swell wave spectra shows dispersive ridges as found in the Pacific and elsewhere. These point to storm origins principally in the South Pacific and the North Atlantic Oceans. Large-scale ' rollers ’ were not encountered, but there was some evidence that they have similar origins. Medium frequency waves (1 to 30 mHz) were recorded simultaneously at two points round the St Helena coast. Their spectra and coherence were studied with a view to identifying trapped modes. A theory is evaluated for waves trapped by a circular island with paraboloidal shelf (as approximately at St Helena) in contrast to the vertical wall models studied by Longuet-Higgins and others. Its main feature is that resonance peaks are much flatter than in the vertical wall cases, and do not increase with frequency. Analysis of the data shows features in common with the theory up to about 3 mHz and at some other energy peaks, but at higher frequencies there is evidence for energy leakage due to topographical roughness.

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The Historical Development of Tidal Science, and the Liverpool Tidal Institute

Cartwright¹

1980

Oceanography: The Past

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The Semi-diurnal Lunar Tidal Motion of the Red Sea.

Cited by 9 publications

References 2 publications

On charting global ocean tides

On charting global ocean tides

Tides and waves in the vicinity of Saint Helena

The Historical Development of Tidal Science, and the Liverpool Tidal Institute

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