K lines in the sulphur isonuclear sequence

Accurate and complete sets of atomic data are being computed for the radiative and Auger processes giving rise to K lines in ions of sulphur. autostructure, hfr and bprm codes are used, taking into account configuration interaction, core relaxation and relativistic effects so as to generate data following an approach used in our previous studies on iron and oxygen. Level energies, wavelengths, A-values and Auger rates are compared with available measurements and previous calculations.