Using the semiclassical perturbation approach, we have calculated electron-
, proton-, He II-, Mg II-, Si II- and Fe II-impact line widths and shifts f
or 189 Ca I multiplets as a function of temperature and perturber density.
Perturbers selected here are the main perturbers in solar atmospheres. Obta
ined results have been compared with the existing theoretical and experimen
tal data.