We have searched for discrete refractive scattering events (including effec
ts due to possible non-multiple diffractive scattering) at meter wavelength
s in the direction of two close by pulsars B0950+08 and B1929+10, where we
looked for spectral signatures associated with the multiple imaging of puls
ars due to scattering in the interstellar medium. We do not find any signat
ures of such events in the direction of either source over a spectral perio
dicity range of 50 KHz to 5 MHz. Our analysis puts strong upper limits on t
he column density contrast associated with a range of spatial scales of the
interstellar electron density irregularities along these lines of sight.