INTRODUCTION
RAYLEIGH REFLECTION COEFFICIENTS
The amplitude of the reflected wave relative to the incident wave is given by the difference in the acoustic impedances divided by the sum of the acoustic impedances of the two media. This ratio is called the "Rayleigh reflection coefficient" after the work of Lord Rayleigh (John Strutt) in the nineteenth century.(For non-normal incidence we use the more complex Zoeppritz equations).
The relative amplitude of the transmitted wave continuing into the second medium is given by the ratio of twice the impedance in the incident layer divided by the sum of the two acoustic impedances. This ratio is called the "Rayleigh transmission coefficient".
The Rayleigh reflection coefficients hold for both compressional waves and shear waves. Just use the appropriate velocity in the acoustic impedance.
EXAMPLES OF RAYLEIGH REFLECTION COEFFICIENTS
In a second important case the impedances of the two media are almost the same. This is usual in a stack of sedimentary rock or sediment layers. In this case the reflected wave amplitude is almost zero. The sign depends on which impedance is larger. The transmitted wave, in contrast, retains most of its amplitude (close to one). In the limit as the impedances become equal the reflection amplitude is zero and the transmitted amplitude is one.
In the third important case the impedance of the incident layer is much greater than that of the other layer. Note that it doesn’t matter which layer is above and which is below. What matters is layer in which the incident wave is located. A common geological example deals with an incident wave in water reflecting from air at the sea surface. Here the water echo is strong with a reflection coefficient of almost minus one. The negative sign means that the phase of the echo is reversed 180 degrees with respect to the incident wave. The transmitted wave amplitude is almost two. It turns out that this wave transmitted into the air has very little energy despite it’s large amplitude (see below).
These amplitude relationships are similar to those for a wave propagated along a rope (the phase relations are a little different). Our first seismic case resembles what happens when we shake a light, flexible rope joined to a heavy, stiff one: the waves in the first rope are large whereas the heavy rope barely moves.
The second case corresponds to an almost uniform rope. Here the waves just travel along the rope with change or reflection. We have an almost perfect impedance match.
The third case shows behaviour similar to that of a heavy, stiff rope attached to a light, flexible one. Here the waves in the light rope are much larger than the incident waves. This case is somewhat analogous to a fly rod and fishing line.
ENERGY IN A WAVE
ENERGY FLUX
Using the equation for energy flux we can easily show that the Rayleigh reflection coefficients are consistent with conservation of energy. In other words the energy flux of the incident wave ("in") equals the sum of the energy fluxes of the reflected and transmitted waves ("out").
OTHER FACTORS INFLUENCING AMPLITUDES
As real waves travel some of their energy is converted to heat and so the waves get weaker even if they don’t spread at all. This attenuation or absorption is exponential with distance. The attenuation coefficient increases linearly with frequency so that high frequency waves decay more rapidly than low frequency ones. As we’ll see in the next class this differential decay leads to loss of resolution with depth.
Amplitudes also are affected by reflector shape. A dome or anticline tends to defocus reflected waves and thus to weaken echoes. A basin or syncline, on the other hand) tends to focus waves and leads to strong echoes. This phenomenon is similar to that of a mirror or satellite television antenna.
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