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Marine Science

Tides

Tides are regular rises and falls in sea level, accompanied by horizontal flows of water, that are caused by gravitational interactions between the Moon, Sun, and Earth. They occur all over the world’s oceans but are most noticeable near coasts. The basic daily pattern of high and low tides is caused by the Moon’s influence on Earth. Variations in the range between high and low tides over a monthly cycle are caused by the combined influence of the Sun and Moon.

High and Low Tides

Although the Moon is usually thought of as orbiting Earth, in fact both bodies orbit around a common center of mass—a point located inside Earth. As Earth and the Moon move around this point, two forces are created at Earth’s surface: a gravitational pull toward the Moon, and an inertial or centrifugal force directed away from the Moon. These forces combine to produce two tidal bulges in Earth’s oceans: one toward the Moon, and the other away from it. As Earth spins on its axis, these bulges sweep over the planet’s surface, producing high and low tides. The cycle repeats every 24 hours 50 minutes (one lunar day) rather than every 24 hours (one solar day), because during each cycle, the Moon moves around a little in its orbit.

Tidal Patterns

If no continents existed and the Moon orbited in Earth’s equatorial plane, the sweeping of the tidal bulges over the oceans would produce two equal daily rises and falls in sea level (a semidiurnal tide) everywhere on Earth. In practice, landmasses interfere with the movement of the tidal bulges, and the Moon’s orbit tilts to the equatorial plane.

Consequently, many parts of the world experience tides that differ from the semi-diurnal pattern. A few have just one high and one low tide per day (called diurnal tides), and many experience high and low tides of unequal size (known as mixed semidiurnal tides). In addition, the tidal range, or difference in sea level between high and low water, varies considerably across the globe.

Monthly Tidal Cycle

In addition to the daily cycle of high and low tides, there is a second, monthly, cycle. In this case, the Sun and Moon combine to drive the cycle. As with the Moon, the interaction between Earth and the Sun causes tidal bulges in Earth’s oceans, though these are smaller than those caused by the Moon. Twice a month, at the times of new and full moon, the Sun, Moon, and Earth are aligned, and the two sets of tidal bulges reinforce each other. The result is spring tides—high tides that are exceptionally high and low tides that are exceptionally low. By contrast, at the times of first- and last-quarter moon, the effects of the Sun and Moon partly cancel out, bringing tides with a smaller range, called neaps.

Tidal Currents

The vertical variation in sea level that occurs locally with tides can happen only through horizontal flows of water, called tidal currents. Over each daily tidal cycle, the currents generally run fastest about halfway between high and low tide at that location—at intermediate times, they slow (“slack water”) and then reverse direction.

The shape of a coast can have a crucial influence on current strength. Bottlenecks to water flow, such as narrow channels and promontories, are often associated with very powerful currents, called tidal races, that develop twice or four times a day. Where the flowing water meets under-water obstructions, phenomena such as whirlpools or vortices (spiraling, funnel-shaped disturbances), eddies (larger, flatter, circular currents), and standing waves may develop. Other tide-related phenomena include tide rips—turbulence caused by converging currents—and overfalls, defined as a tidal current flowing against the wind.

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Low tide at Bamburgh Beach Due to tides, large swaths of coast around the world are alternately covered and uncovered by the sea. This intertidal sandflat in Northumberland, England, has a tidal range averaging about 13 ft (4 m).