
TY  - JOUR
A1  - Ellis, GRA 
A1  - McCulloch, PM 
T1  - Frequency Splitting of Solar Radio Bursts
JF  - Australian Journal of Physics
JO  - Aust. J.  Phys.
Y1  - 1967
VL  - 20
IS  - 5
SP  - 583
EP  - 594
KW  - 
UR  - https://doi.org/10.1071/PH670583 
N2  - Solar radio bursts showing frequency splitting have been observed regularly below 60 MHz. The bursts have a duration of 1-2 sec and a frequency interval between their elements of 0·1-1·0 MHz. Their wave frequency generally decreases with time at about O· 1 MHz/sec. The bursts may occur either in isolation, in chains associated with type III bursts, or in large numbers during noise storms. Triple splitting is observed in about 10% of the bursts. The properties of the bursts are not inconsistent with those expected from magnetic splitting of the radiation. 
ER  -

