Zhurnal Preprint is available here . 3 Institute of Astronomy, Russian Academy of Sciences, Pyatnitskaya ul. Magnetic field has been approximated by a magnetic dipole arbitrary shifted relative to the star center. Ti,Cr and Fe abundance anomalies were obtained as the result of the inverse problem solution, and coordinates of local magnetic vectors on the star surface were computed.
Fe abundance shows a secondary enhancement also near the magnetic equator.
The factors which may restrict the accuracy of Doppler-Zeeman mapping of real stars are also considered.