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Rays and fronts

It is natural to begin studies of waves with equations that describe plane waves in a medium of constant velocity.

Figure 3.7 depicts a ray moving down into the earth at an angle $ \theta $ from the vertical.

front
Figure 7.
Downgoing ray and wavefront.
front
[pdf] [png] [xfig]

Perpendicular to the ray is a wavefront. By elementary geometry the angle between the wavefront and the earth's surface is also $ \theta $. The ray increases its length at a speed $v$. The speed that is observable on the earth's surface is the intercept of the wavefront with the earth's surface. This speed, namely $ v / \sin \theta $, is faster than $v$. Likewise, the speed of the intercept of the wavefront and the vertical axis is $ v / \cos \theta $. A mathematical expression for a straight line like that shown to be the wavefront in Figure 3.7 is
\begin{displaymath}
z   =  z_0  - x  \tan   \theta
\end{displaymath} (4)

In this expression $ z_0 $ is the intercept between the wavefront and the vertical axis. To make the intercept move downward, replace it by the appropriate velocity times time:

\begin{displaymath}
z   =  {v   t \over \cos   \theta }  - x  \tan   \theta
\end{displaymath} (5)

Solving for time gives
\begin{displaymath}
t(x,z)   =  {z\over v } \cos \theta  + {x \over v } \sin   \theta
\end{displaymath} (6)

Equation (3.6) tells the time that the wavefront will pass any particular location $(x,z)$. The expression for a shifted waveform of arbitrary shape is $ f(t - t_0 ) $. Using (3.6) to define the time shift $ t_0 $ gives an expression for a wavefield that is some waveform moving on a ray.
\begin{displaymath}
\hbox{moving wavefield}   = \
f\left(  t - {x \over v} \sin \theta  - {z\over v} \cos \theta\right)
\end{displaymath} (7)


next up previous [pdf]

Next: Snell waves Up: DIPPING WAVES Previous: DIPPING WAVES

2009-03-16