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Tidal Energy Chapter | 3 59


             where H n is the amplitude, g n is the phase lag (e.g. relative to Greenwich), and
             ω n is the angular speed of the constituent.
                If we are interested in predicting how the surface elevation η varies over
             time, then
                                   η n = H n cos (ω n t − g n )        (3.18)
                Through observations and/or numerical simulations, we can obtain values
             for H and g, and we know the angular speeds of the various constituents (M2,
             S2, K1, O1, etc.), and so we have the basis for making a tidal prediction.
                At the port of Holyhead (Fig. 3.6), information on the four principal tidal
             constituents can be obtained from Admiralty tide tables (Table 3.1). Taking a
             timestep of 15 min, we can easily predict the elevation time series at Holyhead
             for an arbitrary start time (Fig. 3.12). This time series shows a spring-neap
             cycle (due to combination of the M2 and S2 semidiurnal constituents), and



                TABLE 3.1 Tidal Data for Holyhead

                                                              Speed (degrees
                Constituent  Name          H (m)  g (degrees)  per solar hour)
                M2          Principal lunar  1.81  292        28.984
                            semidiurnal
                S2          Principal solar  0.59  329        30.000
                            semidiurnal
                K1          Lunisolar diurnal  0.11  177      15.041
                O1          Lunar diurnal  0.10   029         13.943























             FIG. 3.12  Predicted elevation time series at the port of Holyhead, based on a limited number of
             tidal constituents (Table 3.1).
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