
%0 Journal Article
%A Gopala Rao, UV 
%T The Polarization Structure of Type III Solar Radio Bursts
%J Australian Journal of Physics
%D 1965/06/01
%V 18
%N 3
%P 283-286
%K 
%R https://doi.org/10.1071/PH650283
%U https://www.publish.csiro.au/paper/PH650283 
%X The polarization of type III bursts was measured, using a swept.phase technique, at 40 and 60 Mc/s. The great majority of type III bursts show slight to moderate polarization. The results indicate a double structure for the type III burst-a sharp, intense, drifting feature with relatively strong polarization, and a diffuse background of longer duration with relatively weak or zero polarization. 
