
%0 Journal Article
%A Sarma, SBSS 
%T Estimation of Magnetic Field Strength from Enhanced Solar Radio Emission
%J Australian Journal of Physics
%D 1994/12/01
%V 47
%N 6
%P 811-816
%K 
%R https://doi.org/10.1071/PH940811
%U https://www.publish.csiro.au/paper/PH940811 
%X The manifestation of solar activity on radio noise records at 28.6 MHz is discussed with special emphasis on Type-I noise storms and the associated coronal magnetic fields above the active regions in time. Magnetic fields are estimated, assuming that the Type-I radio emission at decametre wavelengths is due to shock waves, by making use of the observed shock velocity. The results are comparable with the existing estimates. 
