A solution to the cylindrical wave equation
(2.23) is
where
p˜+
is the amplitude of the sound pressure in the outgoing wave at unit distance from the axis of symmetry and
p˜−
is the same for the reflected wave.
H
0
(1) (
x) and
H
0
(2) (
x) are Hankel functions defined by
where
J
0(
x) and
Y
0(
x) are Bessel functions of the first and second kind respectively, as plotted in
Fig. 2.10. The “2” in parentheses denotes an outgoing cylindrical wave and the “1” denotes an incoming one. In the far field
We can see from
Fig. 2.10 that cylindrical waves, which are essentially two-dimensional because of the lack of axial dependency, differ from plane ones in two respects: firstly the radial wavelength is longer nearer the axis of symmetry than in the far field; secondly they decay in amplitude as they spread out, adopting an inverse square-root law in the far field. The latter makes sense when we consider that the area of the wave front is proportional to the radial distance
w. The radiated power is the intensity multiplied by the area, where the intensity is given by
Eq. (1.12). The intensity, in turn, is proportional to the square of the pressure and therefore inversely proportional to the radial distance. Hence the power remains constant. The same kind of wave deformation can be seen if you drop a pebble in a pond. Note the singularity in the
Y(
x) function when
x
=
0. If there are no reflecting surfaces in the medium, only the first term of
Eq. (2.125) is needed, i.e.,