  kappa Psc (HD 220825) is a typical Chromium Ap star that happens to have
optimal parameters for Doppler imaging (DI). Its short rotational period of
less then 2 days, rotational velocity of ~40 km/s, and a moderate inclination
of the rotational axis put modest requirements on spectroscopic observations.
Anomalies of iron peak elements are clearly present, but small enough to cause
significant deviations from model atmospheres with scaled solar abundances. We
applied DI to kappa Psc once before, determining the distribution of Cr
(Ryabchikova et al. 1996, hereafter Paper I). However, due to strong blending
of Fe, the image was based on two short (~2 Angstroems) spectral intervals,
dominated by Cr lines. Since the first paper we obtained additional spectra and
developed a new code that allows to perform multi-element DI and thus to use
larger spectral interval(s). We demonstrate the abilities of the new code and
present new maps of Cr and Fe. A much larger time base allowed us to improve
the rotational period of kappa Psc as well.
