tide

tide¹

—tideful, adj. —tideless, adj. —tidelessness, n. —tidelike, adj.

/tuyd/, n., v., tided, tiding.

n.

1. the periodic rise and fall of the waters of the ocean and its inlets, produced by the attraction of the moon and sun, and occurring about every 12 hours.

2. the inflow, outflow, or current of water at any given place resulting from the waves of tides.

3. See flood tide.

4. a stream or current.

5. anything that alternately rises and falls, increases and decreases, etc.: the tide of the seasons.

6. current, tendency, or drift, as of events or ideas: the tide of international events.

7. any extreme or critical period or condition: The tide of her illness is at its height.

8. a season or period in the course of the year, day, etc. (now used chiefly in combination): wintertide; eventide.

9. Eccles. a period of time that includes and follows an anniversary, festival, etc.

10. Archaic. a suitable time or occasion.

11. Obs. an extent of time.

12. turn the tide, to reverse the course of events, esp. from one extreme to another: The Battle of Saratoga turned the tide of the American Revolution.

v.i.

13. to flow as the tide; flow to and fro.

14. to float or drift with the tide.

v.t.

15. to carry, as the tide does.

16. tide over,

a. to assist in getting over a period of difficulty or distress.

b. to surmount (a difficulty, obstacle, etc.); survive.

[bef. 900; ME (n.); OE tid time, hour; c. D tijd, G Zeit, ON tith; akin to TIME]

tide²

/tuyd/, v.i., tided, tiding. Archaic.

to happen or befall.

[bef. 1000; ME tiden, OE tidan. See BETIDE]

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Regular, periodic rise and fall of the surface of the sea, occurring in most places twice a day.

Tides result from differences in the gravitational forces exerted at different points on the Earth's surface by another body (such as the Moon). Although any celestial body (e.g., Jupiter) produces minute tidal effects, the majority of the tidal forces on the Earth are raised by the Sun (because of its enormous mass) and the Moon (because of its proximity to Earth). In fact, the tidal forces from the Moon are about twice as strong as those from the Sun. The largest tides (spring tides, exhibiting very large change in sea level between high and low tides) occur at the new and full moon, when the Earth, the Moon, and the Sun are aligned and the Sun's tidal forces are added to those of the Moon. The smallest tides (neap tides) occur when the Sun and Moon are at right angles (from Earth), when the tidal forces from the Sun partially cancel those from the Moon. The geometry of the coastline and of the water's basin also affects the range of the tides.

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▪ physics

 any of the cyclic deformations of one astronomical body caused by the gravitational forces exerted by others. The most familiar are the periodic variations in sea level on the Earth that correspond to changes in the relative positions of the Moon and the Sun.

      A brief treatment of tides follows. For full treatment of oceanic tides, see ocean: Ocean tides (ocean).

      At the surface of the Earth the gravitational force of the Moon is about 2.2 times greater than that of the Sun. The tide-producing action of the Moon arises from the variations in its gravitational field over the surface of the Earth as compared with its strength at the Earth's centre. The effect is that the water tends to accumulate on the parts of the Earth's surface directly toward and directly opposite the Moon and to be depleted elsewhere. The regions of accumulation move over the surface as the position of the Moon varies relative to the Earth, mainly because of the Earth's rotation but also because of the Moon's orbital motion around the Earth. There are approximately two high and two low tides per day at any given place, but they occur at times that change from day to day; the average interval between consecutive high tides is 12 hours 25 minutes. The effect of the Sun is similar and additive to that of the Moon. Consequently, the tides of largest range or amplitude (spring tides (spring tide)) occur at New Moon, when the Moon and the Sun are in the same direction, and at Full Moon, when they are in opposite directions; the tides of smallest range (neap tides (neap tide)) occur at intermediate phases of the Moon.

      Although the observed tides possess the aforementioned broad features, this pattern does not correspond to a pair of bulges that move around the Earth. The inertia of the water, the existence of continents, and effects associated with the water depth result in much more complicated behaviour. For the main oceans, a combination of theory and observation indicates the existence of amphidromic points, at which the tidal rise and fall is zero: patterns of high and low tides rotate around these points (either clockwise or counterclockwise). Amplitudes are typically less than a metre.

      Tides are most easily observed—and of greatest practical importance—along seacoasts, where the amplitudes are exaggerated. When tidal motions run into the shallow waters of the continental shelf, their rate of advance is reduced, energy accumulates in a smaller volume, and the rise and fall is amplified. The details of tidal motions in coastal waters, particularly in channels, gulfs, and estuaries, depend on the details of coastal geometry and water-depth variation. Tidal amplitudes, the contrast between spring and neap tides, and the variation of times of high and low tide all vary widely from place to place.

      For these reasons, purely theoretical calculation of the times and heights of tides at a particular station is quite impossible. Nevertheless, tides are quite successfully predicted on the basis of accumulated observations of the tides at the place concerned. The analysis of the observations relies on the fact that any tidal pattern (in time) is a superposition of variations associated with periodicities in the motions of the Moon and the Sun relative to the Earth. The periods involved are the same everywhere, ranging from about 12 hours to a year or more, but the relative sizes of their contributions are highly variable. Observations over a sufficient time make it possible to calculate which contributions are significant at a particular location and, thus, to forecast tidal times and heights. It is common that 40 components may be significant for practical calculations at one location.

      In addition to tides in the oceans (and in large lakes, where similar processes occur with smaller amplitudes), there are analogous gravitational effects on the atmosphere and on the interior of the Earth. Atmospheric tides are detectable meteorological phenomena but are a comparatively minor component in atmospheric motions. An Earth tide differs from oceanic and atmospheric ones in that the response to it is an elastic deformation rather than a flow. Observations of Earth tides contribute to knowledge of the internal structure of the Earth.

      Tidal processes can, of course, also occur on other members of the solar system. As just one example, it has been suggested that the volcanic activity of Jupiter's satellite Io is the consequence of internal heating by frictional resistance to tidal deformation.

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