Time-averaged flux-density spectra of ten pulsars have been obtained on the basis of simultaneous observations at six frequencies between 250 and 8085 MHz. The effects of interstellar scintillation on the accuracy of the measurements are discussed. All of the pulsars exhibited a power-law spectrum at high frequencies with spectral indices between negative 1.6 and negative 3.0. Several of the pulsars show a more positive spectral index at the low-frequency end of the data.