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tides
Diederik Willemsen www.sailingissues.com
Tidal movements
The
tide is the vertical rise and fall of the sea level surface caused
primarily by the change in gravitational attraction of the moon, and to a
lesser extent the sun.
As the earth spins on its axis the centrifugal force results in slightly
deeper water near the equator as opposed to shallower water at the poles.
In fact it causes a flow from the poles to the equator.
The earth is also in orbit around the sun (one revolution in one year)
creating not only another centrifugal force but also a gravitational
interaction. These two yield a bulge on the night site (centrifugal) and a
bulge on the day site (gravitational) both of them moving as the world
turns. Therefore, a certain place on this world will experience two high
and two low tides each day.
With these forces alone, we would not have spring
tides
and neap tides. Spring tides have higher high
tides and lower low tides whereas neap tides have lower high tides and
higher low tides. Hence, the
range (difference in water level between high
and low tide) is much larger in a spring tide than in a low tide.
These differences in range
can be explained if we include the moon into our earth-sun system. The
moon and the earth orbit each other around a point (called the barycenter
or baricenter) 2000 odd kilometres inside the earth, creating a
centrifugal and a gravitational bulge. Moreover, despite the sun's
immensely larger mass, the moon exerts a 2.25 times larger gravitational
attraction, since the moon is much closer to our earth.
It is the combined effect of the sun and moon that creates spring and neap
tides. In the animation the gravitational forces of both the sun and the
moon are taken into account. When aligned with the earth they combine
their attraction and otherwise they counteract their attraction. The sun
is located in the corner right below, far outside this picture (note the
eclipse) while the moon is revolving round the earth. One full circle
corresponds to one lunar cycle (about 28 days).
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This
animation shows how the tide changes during the lunar cycle. When
the sun, moon and earth are aligned : spring tide.
When at right angles the forces are not aligned:
neap tide.
The time between spring and neap is approximately 7 days. |
The figure below shows the ideal sinusoids of both spring and neap tides.
Vertically the water height is shown versus horizontally the time.
Ideally, the time between a low and a successive high is somewhat more
than 6 hours.
The time difference
between spring tide and neap tide is normally 7 days and is in accordance
with the
phases of the moon. Yet, water has mass and therefore momentum.
Moreover, it is a viscous fluid that generates friction if moved.
Therefore, the actual spring tide lags a day or so behind a full moon or
new moon occurrence.
So, tidal movements are
intrinsically periodical, resulting in a
Tidal day of 24 hours and 50 minutes
containing one tidal cycle, namely two highs
and two lows. This basic pattern may be distorted by the effects of
landmasses, constrained waterways, friction, the Coriolis effect, or other
factors. Hence, predictions are possible and we expect the the next day's
high tide to come about 50 minutes later.
However, a closer look at the orbit of the moon reveals that the moon is
not always in the equatorial plane, resulting in three types of tides:
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Semi-diurnal tide: Featuring two
highs and two lows each day, with minimal variation in the height of
successive high or low waters. This type is more likely to occur when
the moon is over the equator.
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Diurnal tide: Only a single high
and a single low during each tidal day; successive high and low waters
do not vary by a great deal. This tends to occur in certain areas when
the moon is at its furthest from the equator.
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Mixed tide: Characterized by
wide variations in heights of successive high and low waters, and by
longer tidal cycles than those of the semi-diurnal cycle. These tides
also tend to occur as the moon moves furthest north or south of the
equator.
Chart Datums
The depths and heights in
the chart need a plane of reference: the Chart Datum (see interactive
figure below). Depths are usually described with respect to low water
reference planes (yielding lower charted depths, which are safer) and
heights are shown with respect to high water reference planes (again,
yielding lower vertical clearances on the chart, which are safer). As
such, the chance that the
observed depth or vertical clearance beneath a bridge is smaller than
the charted depth or
height is rather small.
Chart Datums
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MHWS
: Mean High Water Spring
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HW
: High Water
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MHWN
: Mean High Water Neap
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ML
: Mean Level
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MLWN
: Mean Low Water Neap
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MLWS
: Mean Low Water Spring
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LAT
: Low Astronomical Tide
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Overview
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Tide: The vertical rise and fall of the
surface of a body of water caused primarily by the differences in
gravitational attraction of the moon, and to a lesser extent the sun,
upon different parts of the earth when the positions of the moon and sun
change with respect to the earth.
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Spring Tide: The tidal effect of the sun
and the moon acting in concert twice a month, when the sun, earth and
moon are all in a straight line (full moon or new moon). The range of
tide is larger than average.
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Neap Tide: This opposite effect occurs
when the moon is at right angles to the earth-sun line (first or last
quarter). The range of tide is smaller than average.
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Range: The vertical difference between
the high and low tide water levels during one tidal cycle.
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Tidal Day: 24 hours and 50 minutes. The
moon orbits the earth every month, and the earth rotates (in the same
direction as the moon's orbit) on its axis once every 24 hours.
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Tidal Cycle: One high tide plus a
successive low tide.
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Semi-diurnal Tide: The most common tidal
pattern, featuring two highs and two lows each day, with minimal
variation in the height of successive high or low waters.
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Diurnal Tide: Only a single high and a
single low during each tidal day; successive high and low waters do not
vary by a great deal. Such tides occur, for example, in the Gulf of
Mexico, Java Sea and in the Tonkin Gulf.
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Mixed Tide: Characterized by wide
variation in heights of successive high and low waters, and by longer
tide cycles than those of the semidiurnal cycle. Such tides occur, for
example, in the U.S. Pacific coast and many Pacific islands.
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Chart Datum or
Tidal reference planes: These fictitious planes are used as the
sounding datum for the tidal heights.
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Drying Height: Clearance in meters (or
feet in old charts) above the chart datum.
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Charted Depth: Clearance in meters (or
feet in old charts) below the chart datum.
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Observed Depth: Height of tide + charted
depth: the actual depth in meters.
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Height of light: The height of light
above the bottom of its structure.
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Elevation: The height of the light above
the chart datum.
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Rule of Twelve: Assuming a tidal curve
to be a perfect sinusoid with a period of 12 hours. The height changes
over the full range in the six hours between HW and LW with the
following fractions during each respective hour: 1/12 2/12 3/12 3/12
2/12 1/12.
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Rule of Seven: The change from spring
range to neap range can be assumed linear, each day the range changes
with 1/7th of difference between the spring and neap ranges. Hence, the
daily change in range = (spring range - neap range)/7.
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