
TY  - JOUR
A1  - Gopala Rao, UV 
T1  - The Polarization Structure of Type III Solar Radio Bursts
JF  - Australian Journal of Physics
JO  - Aust. J.  Phys.
Y1  - 1965
VL  - 18
IS  - 3
SP  - 283
EP  - 286
KW  - 
UR  - https://doi.org/10.1071/PH650283 
N2  - 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. 
ER  -

