For an aluminium plasma produced by laser irradiation of 1.06 mu m, 0.15 ns and 3*1014 W cm-2, hydrogen-, helium- and lithium-like emission-line intensities have been measured. Population equations of the helium-like ion have been solved for as many as 60 excited levels, where the escape factor has been incorporated to take account of the effect of radiation trapping for optically thick lines. The dominant broadening has been assumed to be due to the expanding streaming motion of the plasma. Fitting the calculation to the experimental data leads to this conclusion: the plasma is predominantly recombining while the lines are emitted, Te approximately=1.3*106K, ne approximately=3*1021 cm-3, N(Al11+)R/v0 approximately=2*1010 cm-3 s (R is the radius of the plasma and v0 is the typical expansion velocity), and the ion abundance ratio is N(Al13+):N(Al12+):N(Al11+)=1:102:3*105.