Fourier Analysis of Ocean Tides I
5. The lunar tide
The lunar tide is more complicated to study because the motion of the Moon around the Earth is considerably more complicated than that of the Earth around the Sun.




The moon travels in an orbit
ot significant eccentricity.
Speed: s = 0.55^{o}/hour 
The axis of that ellipse precesses
in the plane of the moon's orbit.
Speed: p = 0.0046^{o}/hour 
That plane precesses with respect
to the plane of the Earth's orbit.
Speed: N = 0.0022^{o}/hour 
For example, the change in the moon's longitude per hour is T+hs = 14.49 degrees/hour.
Nevertheless, when the vertical component of the lunar tideproducing force is computed as a function of time, geometric and trigonometric analysis like that performed on the solar tideproducing force leads to the analogous result:
The vertical component of the lunar tideproducing force at a point P is, as a function of time, a finite linear combination of cosines and sines, whose speeds are certain integral linear combinations of T, h, s, p and N. 
The tidal record at any port is not periodic, even when transient weatherrelated effects are subtracted. It never repeats itself exactly. But knowing that the tideproducing force can be expressed as a linear combination of functions which are themselves periodic, with known frequencies, we can expect that the tidal record at any port will also be such a linear combination, with the same frequencies. The coefficients will depend on the port, and can be determined by Fourier analysis of the tidal record. Once the coefficients are known, the tides can be predicted. This is the method of ``harmonic analysis of tides."
For example, here are the speeds of some important "constituents" of the ocean tide. These are the ten frequencies that occur with the highest coefficients in the analysis of the tide at Bridgeport, Connecticut.
symbol 
speed 
symbol 
speed 
M_{2} 
2T2s+2h 
N_{2} 
2T3s+2h+p 
S_{2} 
2T 
K_{1} 
T+h 
L_{2} 
2Ts+2hp 
O_{1} 
T2s+h 
Sa 
h 
nu_{2} 
2T3s+4hp 
K_{2} 
2T2h 
Mm 
sp 