  The present status of the calculation of radiative corrections to chargino
and neutralino pair production processes in the MSSM is summarized. The main
focus will be on the use of the on-shell renormalization scheme for charginos
and neutralinos in conjunction with DR-bar parameters, such as those of the SPA
conventions. Associated soft and hard bremsstrahlung and an appropriate
separation of QED-like parts in the full one-loop contributions will be
addressed.
