The evolution of magnetic activity on V711 Tauri and evidence for a significant facular contribution

The nature of the long-term evolution of magnetic activity in the RS CVn binary V711 Tauri is investigated using the complete set of available archival IUE SWP low-dispersion spectra of V711 Tau for the period covering August 1978 - December 1984. An analysis of the spectra confirmed the pattern of a long-term smooth variation of chromospheric and transition region emission found previosly by Dorren et al. (1986). An explanation of the relationship between the different facets of the magnetic activity on V711 Tau is presented.