Theoretical line ratios for the Al VIII ion have been investigated usi
ng an atomic model including the first fifteen energy levels, and taki
ng account of various physical processes. The line emissivities as a f
unction of electron density have been computed. Density-dependent theo
retical line ratios are presented and their diagnostic applications in
the solar atmosphere are discussed with the help of theoretical line
intensities computed using an atmospheric model for the quiet Sun.