
TY  - JOUR
A1  - Sarma, SBSS 
T1  - Estimation of Magnetic Field Strength from Enhanced Solar Radio Emission
JF  - Australian Journal of Physics
JO  - Aust. J.  Phys.
Y1  - 1994
VL  - 47
IS  - 6
SP  - 811
EP  - 816
KW  - 
UR  - https://doi.org/10.1071/PH940811 
N2  - 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. 
ER  -

