Gas-dynamical expansion and radiation transfer of Al vapour breakdown plasma induced by nanosecond laser action with an intensity of 109–2 × 1010 W cm−2 at the wavelengths of 1.06, 0.512, and 0.248 µm are modelled. Plasma evolution is described in the approximation of non-stationary radiative gas dynamics in the two-dimensional axially symmetrical formulation. Radiation transfer is found to exert a considerable effect on the evolution of the laser plasma. As the intensity increases, the radiative energy losses also increase, reaching 60% at 2 × 1010 W cm−2, and cause the plasma temperature to be reduced proportionally. The energy escapes mainly through the side and, to a smaller extent, the frontal boundaries, the amount of energy escaping in the direction of the target being negligible. The dependence of plasma processes on the laser wavelength is due to specific features of the absorption mechanisms and the photo-absorption contribution under the action of visible and ultraviolet ranges of radiation. The spectral composition of the escaping radiation differs considerably from that of the equilibrium spectrum and is typical of plasma with a variable optical density. It is possible to take into account the influence of radiation on the plasma characteristics by solving the equation of radiation transfer in the multi-group approximation with several tens of spectral intervals. If the maximum available number of groups is used for selected spectrum intervals, the computational results can be compared to the experimental data of plasma emission.