2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/15314We report preliminary results of our study of linear polarization in the pulsar emission at 35 & 327 MHz. We have exploited for this purpose the spectral modulation resulting from the differential Faraday rotation across the observed band. We discuss the results on a few bright pulsars by comparing them with the existing measurements at higher radio frequencies.2 pages, 4 figures, To appear in the Proceedings of IAU Colloquium 177 : "Pulsar Astronomy - 2000 & Beyond", Ed. Kramer, Wex, & Wielebinski, ASP conf.Series. Gzipped PS file also available from http://www.rri.res.in/~ashish/html_files/reprints.htmlAstrophysicsLinear Polarisation Properties of Pulsars at 35 & 327 MHztext