Comparing the solution with reality



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Comparing the solution with reality

The horizontal velocity can be found by substituting , made up of its sines and cosines, back into equation (3.1), differentiating with respect to then integrating with respect to . Now, differentiating and integrating sines and cosines still gives sines and cosines: the horizontal velocity of the ocean also oscillates sinusoidally with time and distance. If, when we first wrote down the acceleration in the Newton's Second Law equation (1.5), we had considered the acceleration in the vertical (-direction) as well as in the horizontal, we would have found that the vertical velocity, too, oscillates sinusoidally. This is what we experience when floating well out from shore; fluid particles in the ocean (and the swimmers and surfboards and fish buoyed up by them) trace out elliptical paths in vertical planes - the result of a combined sinusoidal velocity in the horizontal and vertical.

  
Figure 4: Waves propagate but particles in the ocean bob up and down.

Using the standard identities for sums and products of sines and cosines, (3.14) and (3.15) can be re-arranged to give a better way of looking at the wave solution,

 

where and are constants. Look only at the first term (the cosine) and draw a graph of it at time , as in figure 4(a). (Things turn out similarly for the sine term.) In figure 4(b) the graph has been redrawn for a time of second. The wave pattern has moved metres to the right, and as more time goes by it will move further to the right. But the actual particles in the ocean (like the boat and the fish) do not move in the same way as the wave pattern; they just bob around on their elliptical paths. This is consistent with what we know happens in reality, for the ocean far from shore. Since the wave pattern moves metres in a second, its wave speed is given by

 

(The sine term in equation (4.1) represents a wave pattern going the other way, with a wave speed in reality, a disturbance in the ocean makes waves that travel both ways, away from the disturbance.)

A practical application of this wave solution can already be made. Say there is a cyclone making a giant disturbance out in the Capricorn Channel 500 km north of Brisbane - a physical situation for which our equations are relevant. The ocean in the Capricorn Channel has a depth of about 40 m (and by the way, this isn't far off the scaling assumption we made in assuming that the ocean was `something like' 50 m deep). The acceleration due to gravity, , is about . Then from (4.2),

 

The big waves generated by the cyclone travel at , and make it to the coast near Brisbane in 25000 seconds - about 7 hours, enough time for everyone to be warned. (In practice, more sophisticated equations would be used, but the principles of the analysis are similar.)

However the linear wave solution (4.1) - the one obtained by scaling out the nonlinear terms - does not always describe reality. Physically, as the wave pattern travels into shallower water - towards a reef or beach, say, its speed slows down, because the depth of the ocean is getting less. The fluid particles, however, have an enormous momentum behind them as they oscillate to and fro, and they do not slow down as much as the wave pattern. As the water gets shallower and shallower, the fluid particles start to `catch up' with the crests of the wave pattern; the front of the wave pattern gets steeper. Eventually the wave is slowed down so much that the fluid particles actually overshoot the crest, plunging out from the tip of the crest in a curling breaker.

Mathematically, the scaling assumptions, in particular the assumption , begin to get unrealistic when the wave gets into shallower water. This is what we should expect; we chose the scalings to represent the conditions far from shore. As the water gets shallower, gets smaller (and often gets smaller too, for reefs and beaches often have horizontal scales less than 100 m). Because and are the denominators of the nonlinear terms, the nonlinear terms get larger until they can no longer be neglected. Eventually, the nonlinear terms dominate the acceleration in the Newton's Second Law equation, causing wild variations from the linear wave solution which has completely broken down.

In summary, the mathematical equations of fluid dynamics are `nonlinear differential equations'. The nonlinear terms in the equations come from the acceleration in Newton's Second Law, and represent a fluid particle's special ability to change its velocity by changing its position within the flowing mass. Most of the time, as with the ocean far from shore, the nonlinear terms are unimportant - the behaviour is described by the solutions to the scaled or `linearized' equations. However, the ocean waves that are a fundamental feature of the linear solution eventually break as the conditions change and the nonlinear terms take control. Surf is the final, chaotic solution to the nonlinear equations. Solving nonlinear equations, analytically or by computer, is one of the most interesting areas of applied mathematics and is a skill increasingly demanded of scientists and engineers - especially those working with fluids!



next up previous R. Manasseh Papers R. Manasseh Home
Next: Further reading Up: Fluid dynamicswaves & Previous: Solving




Wed Mar 15 15:33:52 EST 1995
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