The theory of tides is the application of continuum mechanics to interpret and predict the tide deformations of planetary and satellite bodies and their atmospheres and (especially Earth's oceans) under the gravitational loading of another astronomical body or bodies (especially the Moon and Sun).
Ultimately the link between the Moon (and Sun) and the tides became known to the Ancient Greece, although the exact date of discovery is unclear; references to it are made in sources such as Pytheas of Massilia in 325 BC and Pliny the Elder's Natural History in 77 AD. Although the schedule of the tides and the link to lunar and solar movements was known, the exact mechanism that connected them was unclear. Classicists Thomas Little Heath claimed that both Pytheas and Posidonius connected the tides with the moon, "the former directly, the latter through the setting up of winds". Seneca mentions in De Providentia the periodic motion of the tides controlled by the lunar sphere.Seneca, De Providentia, section IV Eratosthenes (3rd century BC) and Posidonius (1st century BC) both produced detailed descriptions of the tides and their relationship to the Lunar phase, Posidonius in particular making lengthy observations of the sea on the Spanish coast, although little of their work survived. The influence of the Moon on tides was mentioned in Ptolemy's Tetrabiblos as evidence of the reality of astrology. Seleucus of Seleucia is thought to have theorized around 150 BC that tides were caused by the Moon as part of his Heliocentrism model.Lucio Russo, Flussi e riflussi, Feltrinelli, Milano, 2003, .
Aristotle, judging from discussions of his beliefs in other sources, is thought to have believed the tides were caused by winds driven by the Sun's heat, and he rejected the theory that the Moon caused the tides. An apocryphal legend claims that he committed suicide in frustration with his failure to fully understand the tides. Heraclides also held "the sun sets up winds, and that these winds, when they blow, cause the high tide and, when they cease, the low tide". Dicaearchus also "put the tides down to the direct action of the sun according to its position". Philostratus discusses tides in Book Five of Life of Apollonius of Tyana (circa 217-238 AD); he was vaguely aware of a correlation of the tides with the phases of the Moon but attributed them to spirits moving water in and out of caverns, which he connected with the legend that spirits of the dead cannot move on at certain phases of the Moon.
Medieval rule-of-thumb methods for predicting tides were said to allow one "to know what Moon makes high water" from the Moon's movements. Dante Alighieri references the Moon's influence on the tides in his Divine Comedy.
Medieval European understanding of the tides was often based on works of Muslim astronomers that became available through Latin translation starting from the 12th century. Abu Ma'shar al-Balkhi, in his Introductorium in astronomiam, taught that ebb and flood tides were caused by the Moon. Abu Ma'shar discussed the effects of wind and Moon's phases relative to the Sun on the tides. In the 12th century, al-Bitruji contributed the notion that the tides were caused by the general circulation of the heavens. Medieval Arabic astrologers frequently referenced the Moon's influence on the tides as evidence for the reality of astrology; some of their treatises on the topic influenced western Europe. Some theorized that the influence was caused by lunar rays heating the ocean's floor.
In 1616, Galileo Galilei wrote Discourse on the Tides.Rice University: Galileo's Theory of the Tides, by Rossella Gigli, retrieved 10 March 2010 He strongly and mockingly rejects the lunar theory of the tides, and tries to explain the tides as the result of the Earth's rotation and heliocentrism, believing that the oceans moved like water in a large basin: as the basin moves, so does the water. But his contemporaries noticed that this made predictions that did not fit observations.
René Descartes theorized that the tides (alongside the movement of planets, etc.) were caused by aetheric vortices, without reference to Kepler's theories of gravitation by mutual attraction; this was extremely influential, with numerous followers of Descartes expounding on this theory throughout the 17th century, particularly in France. However, Descartes and his followers acknowledged the influence of the Moon, speculating that pressure waves from the Moon via the aether were responsible for the correlation.
Isaac Newton, in the Principia, provides a correct explanation for the tidal force, which can be used to explain tides on a planet covered by a uniform ocean but which takes no account of the distribution of the continents or ocean bathymetry.
The equilibrium theory—based on the gravitational gradient from the Sun and Moon but ignoring the Earth's rotation, the effects of continents, and other important effects—could not explain the real ocean tides.Bryden, I.G. (2003). "Tidal Power Systems", in Meyers, R.A. (ed.) Encyclopedia of Physical Science and Technology. Aberdeen: Academic Press, p. 753. doi: 10.1016/b0-12-227410-5/00778-x Since measurements have confirmed the dynamic theory, many things have possible explanations now, like how the tides interact with deep sea ridges, and chains of seamounts give rise to deep eddies that transport nutrients from the deep to the surface. The equilibrium tide theory calculates the height of the tide wave of less than half a meter, while the dynamic theory explains why tides are up to 15 meters.
Satellite observations confirm the accuracy of the dynamic theory, and the tides worldwide are now measured to within a few centimeters. Measurements from the CHAMP satellite closely match the models based on the TOPEX data.http://www.geomag.us/info/Ocean/m2_CHAMP+longwave_SSH.swf Accurate models of tides worldwide are essential for research since the variations due to tides must be removed from measurements when calculating gravity and changes in sea levels.
For a fluid sheet of average thickness D, the vertical tidal elevation ζ, as well as the horizontal velocity components u and v (in the latitude φ and longitude λ directions, respectively) satisfy Laplace's tidal equations:
\begin{align} \frac{\partial \zeta}{\partial t} &+ \frac{1}{a \cos( \varphi )} \left[ \frac{\partial}{\partial \lambda} (uD) + \frac{\partial}{\partial \varphi} \left(vD \cos( \varphi )\right) \right] = 0, \\[2ex] \frac{\partial u}{\partial t} &- v \, 2 \Omega \sin( \varphi ) + \frac{1}{a \cos( \varphi )} \frac{\partial}{\partial \lambda} \left( g \zeta + U \right) = 0, \quad \text{and} \\[2ex] \frac{\partial v}{\partial t} &+ u \, 2 \Omega \sin( \varphi ) + \frac{1}{a} \frac{\partial}{\partial \varphi} \left( g \zeta + U \right) = 0, \end{align}where Ω is the angular frequency of the planet's rotation, g is the planet's gravitational acceleration at the mean ocean surface, a is the planetary radius, and U is the external gravitational tidal-forcing potential.
William Thomson (Lord Kelvin) rewrote Laplace's momentum terms using the curl to find an equation for vorticity. Under certain conditions this can be further rewritten as a conservation of vorticity.
Darwin's harmonic developments of the tide-generating forces were later improved when A.T. Doodson, applying the lunar theory of E.W. Brown, developed the tide-generating potential (TGP) in harmonic form, distinguishing 388 tidal frequencies.S Casotto, F Biscani, "A fully analytical approach to the harmonic development of the tide-generating potential accounting for precession, nutation, and perturbations due to figure and planetary terms", AAS Division on Dynamical Astronomy, April 2004, vol.36(2), 67. Doodson's work was carried out and published in 1921.A T Doodson (1921), "The Harmonic Development of the Tide-Generating Potential", Proceedings of the Royal Society of London. Series A, Vol. 100, No. 704 (1 December 1921), pp. 305–329. Doodson devised a practical system for specifying the different harmonic components of the tide-generating potential, the Doodson numbers, a system still in use.
Since the mid-twentieth century further analysis has generated many more terms than Doodson's 388. About 62 constituents are of sufficient size to be considered for possible use in marine tide prediction, but sometimes many fewer can predict tides to useful accuracy. The calculations of tide predictions using the harmonic constituents are laborious, and from the 1870s to about the 1960s they were carried out using a mechanical tide-predicting machine, a special-purpose form of analog computer. More recently digital computers, using the method of matrix inversion, are used to determine the tidal harmonic constituents directly from tide gauge records.
Principal lunar semidiurnal | M2 | 12.4206012 | 28.9841042 | 2 | 255.555 | 268.7 | 3.9 | 15.9 | 97.3 | 58.0 | 23.0 | 1 | |||
Principal solar semidiurnal | S2 | 12 | 30 | 2 | 2 | −2 | 273.555 | 42.0 | 3.3 | 2.1 | 32.5 | 13.7 | 9.2 | 2 | |
Larger lunar elliptic semidiurnal | N2 | 12.65834751 | 28.4397295 | 2 | −1 | 1 | 245.655 | 54.3 | 1.1 | 3.7 | 20.1 | 12.3 | 4.4 | 3 | |
Larger lunar evectional | ν2 | 12.62600509 | 28.5125831 | 2 | −1 | 2 | −1 | 247.455 | 12.6 | 0.2 | 0.8 | 3.9 | 2.6 | 0.9 | 11 |
Variational | μ2 | 12.8717576 | 27.9682084 | 2 | −2 | 2 | 237.555 | 2.0 | 0.1 | 0.5 | 2.2 | 0.7 | 0.8 | 13 | |
Lunar elliptical semidiurnal second-order | 2 N2 | 12.90537297 | 27.8953548 | 2 | −2 | 2 | 235.755 | 6.5 | 0.1 | 0.5 | 2.4 | 1.4 | 0.6 | 14 | |
Smaller lunar evectional | λ2 | 12.22177348 | 29.4556253 | 2 | 1 | −2 | 1 | 263.655 | 5.3 | 0.1 | 0.7 | 0.6 | 0.2 | 16 | |
Larger solar elliptic | T2 | 12.01644934 | 29.9589333 | 2 | 2 | −3 | 272.555 | 3.7 | 0.2 | 0.1 | 1.9 | 0.9 | 0.6 | 27 | |
Smaller solar elliptic | R2 | 11.98359564 | 30.0410667 | 2 | 2 | −1 | 274.555 | 0.9 | 0.2 | 0.1 | 0.1 | 28 | |||
Shallow water semidiurnal | 2 SM2 | 11.60695157 | 31.0158958 | 2 | 4 | −4 | 291.555 | 0.5 | 31 | ||||||
Smaller lunar elliptic semidiurnal | L2 | 12.19162085 | 29.5284789 | 2 | 1 | −1 | 265.455 | 13.5 | 0.1 | 0.5 | 2.4 | 1.6 | 0.5 | 33 | |
Lunisolar semidiurnal | K2 | 11.96723606 | 30.0821373 | 2 | 2 | 275.555 | 11.6 | 0.9 | 0.6 | 9.0 | 4.0 | 2.8 | 35 |
Lunisolar diurnal | K1 | 23.93447213 | 15.0410686 | 1 | 1 | 165.555 | 15.6 | 16.2 | 9.0 | 39.8 | 36.8 | 16.7 | 4 | ||
Lunar diurnal | O1 | 25.81933871 | 13.9430356 | 1 | −1 | 145.555 | 11.9 | 16.9 | 7.7 | 25.9 | 23.0 | 9.2 | 6 | ||
Lunar diurnal | OO1 | 22.30608083 | 16.1391017 | 1 | 3 | 185.555 | 0.5 | 0.7 | 0.4 | 1.2 | 1.1 | 0.7 | 15 | ||
Solar diurnal | S1 | 24 | 15 | 1 | 1 | −1 | 164.555 | 1.0 | 0.5 | 1.2 | 0.7 | 0.3 | 17 | ||
Smaller lunar elliptic diurnal | M1 | 24.84120241 | 14.4920521 | 1 | 155.555 | 0.6 | 1.2 | 0.5 | 1.4 | 1.1 | 0.5 | 18 | |||
Smaller lunar elliptic diurnal | J1 | 23.09848146 | 15.5854433 | 1 | 2 | −1 | 175.455 | 0.9 | 1.3 | 0.6 | 2.3 | 1.9 | 1.1 | 19 | |
Larger lunar evectional diurnal | ρ | 26.72305326 | 13.4715145 | 1 | −2 | 2 | −1 | 137.455 | 0.3 | 0.6 | 0.3 | 0.9 | 0.9 | 0.3 | 25 |
Larger lunar elliptic diurnal | Q1 | 26.868350 | 13.3986609 | 1 | −2 | 1 | 135.655 | 2.0 | 3.3 | 1.4 | 4.7 | 4.0 | 1.6 | 26 | |
Larger elliptic diurnal | 2 Q1 | 28.00621204 | 12.8542862 | 1 | −3 | 2 | 125.755 | 0.3 | 0.4 | 0.2 | 0.7 | 0.4 | 0.2 | 29 | |
Solar diurnal | P1 | 24.06588766 | 14.9589314 | 1 | 1 | −2 | 163.555 | 5.2 | 5.4 | 2.9 | 12.6 | 11.6 | 5.1 | 30 |
Lunar monthly | Mm | 661.3111655 27.554631896 | 0.5443747 | 0 | 1 | −1 | 65.455 | 0.7 | 1.9 | 20 | |||||
Solar semiannual | Ssa | 4383.076325 182.628180208 | 0.0821373 | 0 | 2 | 57.555 | 1.6 | 2.1 | 1.5 | 3.9 | 21 | ||||
Solar annual | Sa | 8766.15265 365.256360417 | 0.0410686 | 0 | 1 | 56.555 | 5.5 | 7.8 | 3.8 | 4.3 | 22 | ||||
Lunisolar synodic fortnightly | MSf | 354.3670666 14.765294442 | 1.0158958 | 0 | 2 | −2 | 73.555 | 1.5 | 23 | ||||||
Lunisolar fortnightly | Mf | 327.8599387 13.660830779 | 1.0980331 | 0 | 2 | 75.555 | 1.4 | 2.0 | 0.7 | 24 |
Shallow water overtides of principal lunar | M4 | 6.210300601 | 57.9682084 | 4 | 455.555 | 6.0 | 0.6 | 0.9 | 2.3 | 5 | |||||
Shallow water overtides of principal lunar | M6 | 4.140200401 | 86.9523127 | 6 | 655.555 | 5.1 | 0.1 | 1.0 | 7 | ||||||
Shallow water terdiurnal | MK3 | 8.177140247 | 44.0251729 | 3 | 1 | 365.555 | 0.5 | 1.9 | 8 | ||||||
Shallow water overtides of principal solar | S4 | 6 | 60 | 4 | 4 | −4 | 491.555 | 0.1 | 9 | ||||||
Shallow water quarter diurnal | MN4 | 6.269173724 | 57.4238337 | 4 | −1 | 1 | 445.655 | 2.3 | 0.3 | 0.9 | 10 | ||||
Shallow water overtides of principal solar | S6 | 4 | 90 | 6 | 6 | −6 | * | 0.1 | 12 | ||||||
Lunar terdiurnal | M3 | 8.280400802 | 43.4761563 | 3 | 355.555 | 0.5 | 32 | ||||||||
Shallow water terdiurnal | 2 MK3 | 8.38630265 | 42.9271398 | 3 | −1 | 345.555 | 0.5 | 0.5 | 1.4 | 34 | |||||
Shallow water eighth diurnal | M8 | 3.105150301 | 115.9364166 | 8 | 855.555 | 0.5 | 0.1 | 36 | |||||||
Shallow water quarter diurnal | MS4 | 6.103339275 | 58.9841042 | 4 | 2 | −2 | 473.555 | 1.8 | 0.6 | 1.0 | 37 |
The Doodson arguments are specified in the following way, in order of decreasing frequency: and T D Moyer (2003) already cited.
In these expressions, the symbols , , and refer to an alternative set of fundamental angular arguments (usually preferred for use in modern lunar theory), in which:-
It is possible to define several auxiliary variables on the basis of combinations of these.
In terms of this system, each tidal constituent frequency can be identified by its Doodson numbers. The strongest tidal constituent "M2" has a frequency of 2 cycles per lunar day, its Doodson numbers are usually written 255.555, meaning that its frequency is composed of twice the first Doodson argument, and zero times all of the others. The second strongest tidal constituent "S2" is influenced by the sun, and its Doodson numbers are 273.555, meaning that its frequency is composed of twice the first Doodson argument, +2 times the second, -2 times the third, and zero times each of the other three.See for example Melchior (1971), already cited, at p.191. This aggregates to the angular equivalent of mean solar time +12 hours. These two strongest component frequencies have simple arguments for which the Doodson system might appear needlessly complex, but each of the hundreds of other component frequencies can be briefly specified in a similar way, showing in the aggregate the usefulness of the encoding.
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