Results of intraday variability observations with a sampling of approx
imately 20 minutes of the southern blazars PKS 0521-365 and PKS 0537-4
41 at 1.42 GHz are presented. PKS 0521-365 did not display flux densit
y variability whilst PKS 0537-441 showed strong fluctuations with a ma
jor out-burst towards J.D. 2449011 caracterized by a fluctuation index
of approximately 15%, variability amplitudes of approximately 45% and
time scales of approximately 10(4)s. After a discussion of possible s
cenarios for such kind of variability, this extremely violent behaviou
r is interpreted in terms of strong scattering by compact ionized stru
ctures in the interstellar medium. The physical properties of the refr
actors are estimated from the observed light curves, and a brief discu
ssion about the possible origin of these objects is presented.