Tides result from the gravitational pull of the moon and, to a lesser degree, the sun.
They are very long-period waves originating in the ocean, appearing as the regular rise and fall of the sea surface along coastlines.
Equilibrium Theory (Isaac Newton):
Assumes a perfectly uniform Earth, very deep water, and no landmasses.
Too simplistic.
Dynamic Theory (Pierre-Simon Laplace):
Modified Newton’s model to account for tidal variations.
Shows multiple tidal bulges, not just two.
The moon's gravitational pull is the primary driver of tides.
The sun also exerts a gravitational influence, though to a lesser extent.
High tide occurs when the crest of the tidal wave reaches the coast.
Low tide occurs when the trough of the tidal wave reaches the coast.
The tidal range is the difference in height between high and low tide.
A tidal current is the horizontal movement of water accompanying the rising and falling tide.
Flood Current: The incoming tide along the coast and into bays/estuaries.
Ebb (or Slack) Current: The outgoing tidal current.
Daily tides create currents that flow into and out of bays, rivers, harbors, and other restricted areas.
Inflow: Flood current
Outflow: Slack current
Midpoint: Slack tide
The moon's gravitational field pulls the Earth’s oceans on opposite sides, creating tidal bulges.
The Earth rotates in and out of these tidal bulges.
Most coastlines experience two high tides and two low tides each day.
High tides can be unequal in height due to the axial angle of the Earth’s rotation.
Gravity and inertia are opposing forces creating tidal bulges on opposite sides of the planet.
Spring Tides:
Occur during new moon (no moon visible) and full moon (sun and moon aligned on opposite sides of the Earth).
Result in the highest and lowest tides.
Neap Tides:
Occur when the moon is in a quarter phase, forming a right angle with the sun relative to the Earth.
The sun's gravity pulls to the side of the moon’s tidal bulge, raising low tide and lowering high tide.
Weaker tides.
The Moon’s declination (angle of the Moon’s orbit with respect to the Earth’s equator) varies over an 18.6-year cycle from ~28^\circ to ~18^\circ.
The Earth’s tidal bulges track the position of the Moon and influence the height of tides.
The Earth’s orbit around the Sun is slightly eccentric.
Perihelion: Earth’s closest approach to the Sun at 147.1 \times 10^6 km.
Aphelion: Earth’s farthest distance from the Sun at 152.1 \times 10^6 km.
The difference between perihelion and aphelion is ~5 \times 10^6 km.
This small change results in a small change in the solar tidal component (height of tide) because the tidal influence of the Sun is a function of distance.
The orbit of the Moon around the Earth is slightly eccentric.
Perigee: Moon’s closest approach to the Earth is 363,396 km.
Apogee: Moon’s farthest distance from the Earth is 405,504 km.
The difference between perigee and apogee is ~42,000 km.
The tide-generating influence of the Moon increases during perigee.
When the Moon is at perigee, it appears ~14% larger and is known as a super moon.
The effect of eccentric orbits of the Earth and Moon have a very small influence on tides.
This effect may be only a few inches but can be additive with other factors.
“King tide” describes extra-large high tides, occurring when the Earth, Moon, and Sun are aligned at perigee and perihelion.
Tidal range varies considerably along different coastlines.
Underwater bathymetry (shape of seafloor) and coastline shape dramatically affect the local tidal range.
As the Earth rotates within the tidal bulges, continents disrupt the migration of the bulge in the oceans.
Most coastal areas experience two high tides and two low tides in a lunar day of 24 hours and 50 minutes.
A lunar day is the time it takes for a specific point on Earth to rotate from an exact point under the Moon to the same point under the Moon.
Diurnal Tide: Having a single low and high tide daily (e.g., Gulf of Mexico).
Semidiurnal Tide: Having two roughly equal high and low tides daily (e.g., East coast of the US).
Mixed Tide: Having two unequal high and low tides daily (e.g., West coast of the US).
If the Earth had no continents and was uniformly covered by ocean, the entire planet would experience two equally proportioned high and low tides every lunar day.
Continents block the migration of tidal bulges, resulting in complex tidal patterns depending on coastline shape and seafloor bathymetry.
A tidal bore forms when the incoming tide produces a wave that flows into a river or other narrow area.
This is a true tidal wave and can be several meters/feet high in places (e.g., Amazon River).
Besides lunar and solar gravity, the imperfect sphere of the Earth, the season, the shape of the ocean basin, and the Coriolis effect influence tides.
Tides rotate around amphidromic points, where water doesn’t rise and fall with the tides.
Predicting tides is important for shipping, marine industries, and commercial fishing.
Navigating ships through shallow water ports requires knowledge of the time and height of the tides, as well as the speed and direction of tidal currents.
A tide gauge measures the change in sea level relative to a baseline.
Sensors continuously record the height of the water level.
Tide gauges are automated with electronic sensors, and real-time tide data are available online.
Data are available from more than 1,750 tide gauges worldwide.
Tide gauges have been an important source of data for documenting the increase in mean sea level due to climate change.
Global sea level has risen by ~2.0 mm/year.