We report multifrequency measurements of scatter-broadening times for nine
highly dispersed pulsars over a wide frequency range (0.6-4.9 GHz). We find
the scatter-broadening times to be larger than expected and to scale with
frequency with an average power-law index of 3.44 +/- 0.13, i.e., significa
ntly less than that expected from standard theories. Such possible discrepa
ncies have been predicted very recently by Cordes and Lazio.