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         LESSON              Tides and How
           5.1               To Allow for Them
   I
       n this module we will be looking at the factors which cause the tides and how to calculate their effects. At first
       this subject might seem a little daunting, but our easy explanation and methods will make things very clear and
       simple.
   Let’s make a start by looking at the amazing systems of tides and what causes them.
   WHAT CAUSES THE TIDES
    The major influences on the water surrounding the earth’s surface are the Sun and the Moon. The gravitational
   pull of these bodies causes the water to have a tidal effect and this effect is maximised or minimised according to
   the the relative positions of the Earth, Sun and Moon. The overall effect is also governed by the distance that Sun,
   Moon and Earth are apart. As these bodies are in elliptical orbits you will begin to see that the systems can
   become quite complicated. Add to this the fact that the earth consists of Continents, and very irregular land
   masses, and you will see that the Tidal System can be, and is, very intrinsic.
   However, from the user’s point of view tidal data is less complicated. It is derived from the history of water levels
   at various places and therefore can be predicted to an extreme degree of accuracy.
   As mentioned above the Sun and Moons gravitational effects cause the tides. The Moon being the nearer body
   has the main influence. We will assume that the earth consists of all sea and no land. Looking at Fig 5-1 you will
   see that the effect of sun and moon will cause the water to “hump” up on one side. In fact if you look at Fig 5-1
   on the left hand side the moon is causing the ‘humping’ of water on the side nearest to it. Because of the laws of
   equilibrium (we will not get into physics here) the water will also “hump” up on the side opposite to that of the
   Moon.
    MOON ORBITS EARTH        EARTH SPINS ROUND
                                                                                                             SUN
         ONCE PER              ONCE PER DAY
     28 DAYS (APPROX)
                                                              FIRST QUARTER                NEW MOON
                                         LW
                                                                                   SPRINGS
                                                                     NEAPS
     MOON
                HW                    NORTH                  HW
                                       POLE                                        NP
                                                                                           NEAPS
                                                                            SPRINGS
                                         LW
                                                                FULL MOON                LAST QUARTER
     Fig 5-1
   Fig 5.1.1
   The Moon takes approximately 28 days to orbit the earth and of course the earth is spinning on it’s own axis
   once in 24 hours. Again looking at Fig 5-1, you will see that the Sun and Moon are in line with one another on
   two occasions each month, New Moon and Full Moon.During this time the tidal influence is at its greatest and
   will produce very high high tides,and very low low tides.
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                       NEAP RANGE                                                                                                              SPRING RANGE
                                                                                                                       Charted heights of land objects
      Heights of lights and cables                                                                                  are given above MHWS (Mean High
  are measured above HAT (Highest                                                                                   Water Springs), which is the
                                                        Height of light                                                                                                   Height of object
  Astronomical Tide).                                                                                               average of all high waters.
                            HAT (Highest Astronomical Tide)                                                                            HAT (Highest Astronomical Tide)
                            MHWS (Mean High Water Springs)                                                                            MHWS (Mean High Water Springs)
                                     Mean High Water Neaps
                                                                                                                       SPRING RANGE
                                                                          NEAP RANGE
         Height of Tide                  Tidal Rise
                                                       Depth
                                                                                                                                      Tidal Rise   Height of Tide
                  Mean Low Water Neaps                                                                                                                 MLWS (Mean Low Water Springs)
   CHART DATUM            LAT (Lowest Astronomical Tide)                                                                                     LAT (Lowest Astronomical Tide)            CHART DATUM
         The height of the tide is         All Charted depths are                          The range of each tide           All Charted depths are
   how far above Chart Datum the        measured below Chart                           is the difference between         measured below Chart
   tide stands at a given time.         Datum (LAT).                                   High and Low Water.               Datum (LAT).
   Chart Datum is at the level of
   LAT.
  Fig 5.1.2 Tidal Heights and Ranges
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    Fig 5.1.2A Charted Depths and Drying Heights
    MLWN
    MLWS
                                                          DRYING HEIGHT
    CHART DATUM LAT (LOWEST ASTRONOMICAL TIDE)
                     CHARTED DEPTH
   For example:
                                              3
                                                  7
                                                                                      ( 16 )
                                     Rock or Sandbank                        Rock or isolated point
       Rock or Sandbank           Showing drying height                   Showing drying height
    awash at Chart Datum          above Chart Datum                       above Chart Datum
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        Fig 5.1.2A
        HEIGHTS UNDER A BRIDGE
                                   Mast clearance
       Charted height of bridge
                            Mast height                               Total clearance
                              Above
                             waterline
                          HAT
                                                                 Drop
                         MLWN
       Air Draught (or clearance) under Bridges and Cables
       As you can see from the diagram all clearances under Bridges and Cables are measured above
       HAT (Highest Astronomical tide. The correct term for this is the Air Draught
       On a recent trip to Norway on a cruise liner the ship had an air draught of 72 metres and the
       height of a cable spanning the Fjord was 74 metres. From the deck it looked as though we
       would hit the cable but the Captain and Norwegian Pilot had done their homework and the ship
       cleared the cable with 2m to spare!
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   Also twice per month the Sun and Moon are at right angles to one another, known as the first quarter and the last
   quarter. This causes what we define as Neap tides where we have lower high waters and higher low waters.
   This sounds complicated so have a look at Fig 5.1.2 which shows you the effect of Spring and Neap tides. You
   will see here examples of what we call the Spring and Neap range of tides.
   As a matter of interest, a Spring tide will not necessarily occur exactly at new or full Moon but about 2 days after
   it. This is because the water does not respond to the gravitational pull of the Sun and Moon instantly, but in fact
   lags for approximately two days.
   Semi-Diurnal Tides
   Around the UK we experience usually two high tides and two low tides each day. These are called Semi-Diurnal
   Tides with successive High and Low waters being spaced just over six hours apart.
   Now let’s have a more detailed look at Fig 5.1.2. You will see first the Spring and Neap Ranges of the tide.
   Highest Astronomical Tide (HAT)
   This is the the point above which all vertical clearances on a chart are shown. For example if the clearance height
   of a bridge is 4 metres then it is 4m above HAT
   All other heights on a chart are above MHWS. Underlined figures are drying heights above Chart Datum (see
   below).
   Mean High Water Springs (MHWS) & Mean High Water Neaps (MHWN)
   These are the average or predicted heights of the Spring or Neap tides at High Water (HW) over a period of
   18.6 years.
   Mean Low Water Springs (MLWS) & Mean Low Water Neaps (MLWN)
   These again are the average heights of Spring Low Water and Neap Low Water over the 18.6 year period.
   Chart Datum and Lowest Astronomical Tide (LAT)
   All Depths on a chart and Drying Heights are measured from the level of Chart Datum. This used to be from
   MLWS but it was decided about 15 years ago to make this even safer. Therefore a new datum called Lowest
   Astronomical Tide (LAT) was introduced. This is the lowest level to which the tide is ever predicted to fall (for
   Astronomical reasons). It does not take into account any meteorological conditions which can effect the tide.
                   Chart Datum (LAT) therefore, can be defined as the level from which all heights of tide
                   are calculated and the level from which all depths on a chart are measured. Also any
                   areas that dry out (Sandbanks, Rocks etc.) are measured from this datum.
   Range of the tide
   This is the difference between the heights of High and Low Water. It can be either the Spring Range which is the
   difference between MHWS & MLWS or the Neap Range which is the difference between MHWN & MLWN.
   Now please take time to review the simulations on the next page:
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             Now view the simulations shown below on your resource CD:
              Tides                    SEARCH
              Chart Datum              SEARCH
              Using Rule of Twelfths   SEARCH
              Calculating Height of Tide SEARCH