On February 8, 1992, the Ulysses spacecraft passed through Jupiter's Io plasma torus, where rich spectra of narrow-band resonances were stimulated by the relaxation sounder of the Ulysses unified radio and plasma wave (URAP) instrument. Since the gyrofrequency ƒg is comparable to the plasma frequency ƒp in the Io torus, it was predicted that the general classification of stimulated ionospheric Dn resonances, developed for 1 ≤ ƒp/ ƒg ≤ 8 in the Earth's topside ionosphere, should apply in the Io torus as well as the Earth's magnetosphere (Osherovich, 1989). The URAP plasmagrams (sounder spectra) in the portions of the Io torus satisfying these plasma conditions are dominated by the Dn resonances for frequencies below ƒp. On most of these plasmagrams the ƒp resonance is also present, but it is seldom the dominant resonance. Neither upper hybrid nor nƒg resonances have been found on these plasmagrams. The identification of Dn resonances has allowed both the electron density and the magnetic field amplitude to be calculated. The derived densities on the outbound pass agree well with a Voyager model of Bagenal (1992). The derived magnetic field values are close to the Goddard Space Flight Center O6 magnetic field model.