For with the observation distance much larger than the scatterer, expand . The far-field pattern in the Born approximation for scalar wave scattering is consequently
This convention includes the factor in ; moving that factor into the outgoing-wave definition would change the pattern's normalization.
The absolute energy flux depends on what physical amplitude represents. For acoustic pressure in a homogeneous fluid of mass density and wave speed , the momentum equation gives the particle-velocity amplitude . The time average of harmonic power and acoustic intensity then give
The radial derivative of the outgoing factor is . Its imaginary current is therefore to leading order. The incident unit-amplitude plane wave has imaginary current . Hence, with ,
The scattered energy flux points along at leading order, and the incident energy flux along . If is a velocity-potential amplitude instead, both leading expressions use the common prefactor in place of . A normalized scalar current uses as the common prefactor. The paper does not specify this amplitude normalization; the ratio in part (c) is independent of that choice.
For real harmonic quantities
define the period average by
This is the time average of harmonic power.
At , put . The velocity and pressure amplitudes are
Hence the mean outward work rate per unit area is
Multiplication by the area yields
This is the mean acoustic power of a pulsating sphere.