Abstract:
The frequency drift and time splitting of solar radio bursts are observed
with a multi-channel radiometer and a polarimeter at frequencies around 25
MHz. It is found that a majority of noise storm bursts have drift rates
between + 1.0 and -1.0 MHz/sec. Two types of unusual bursts with frequency
drift are described. The two components of a double burst are found to be
polarized to the same degree and in the same sense.