The well known treatment of asymptotically flat vacuum fields is adapt
ed to pure radiation fields. In this approach we find a natural normal
ization of the radiation null vector. The energy balance at null infin
ity shows that the mass loss results from a linear superposition of th
e pure and the gravitational radiation parts. By transformation to Bon
di-Sachs coordinates the Kinnersley photon rocket is found to be the o
nly axisymmetric Robinson-Trautman pure radiation solution without gra
vitational radiation.