In this paper we present a semi-analytical model which enables the aco
ustic pressure field created by two spheres radiating close together t
o be predicted at any point outside the spheres. By representing the p
ressure field from each sphere as a finite sum of spherical harmonics
and satisfying the boundary conditions at a finite number of points on
the surface of each sphere, the problem reduces to the solution of a
system of simultaneous linear equations whose unknown variables are th
e relative amplitudes of each spherical harmonic. The results from thi
s model have been compared with those obtained using a boundary elemen
t method approach. It is shown that for values of ka < 10 both methods
give results with a relative error less than 1% for separated spheres
. The case for contacting spheres is discussed and results presented.
Numerical examples demonstrate the accuracy and convergence rates of t
he two methods. A detailed analysis of the radiation problem when the
spheres are in contact is given in an Appendix.