D. Batchelor, ANOTHER CLUE ABOUT PARTICLE-ACCELERATION IN IMPULSIVE HARD X-RAY MICROWAVE BURSTS/, The Astrophysical journal. Supplement series, 90(2), 1994, pp. 697-700
In a sample of impulsive bursts with rise times less than 30 s, a corr
elation between burst rise times and the frequency of maximum microwav
e emission has been found. The implications for source structure and d
ynamics are discussed in this paper. Previously evidence was found tha
t such bursts are caused by some propagating disturbance such as a sho
ck wave or thermal conduction front. Combining that evidence with the
microwave and hard X-ray spectral information suggests that the most r
apid bursts are emitted from the most compact and intensely magnetized
sources. The most rapid bursts also exhibited the hardest X-ray spect
ra, as published previously. These facts are important clues to unders
tanding the physical process responsible for impulsive bursts. A model
for the bursts is suggested, based on the observations and inferences
described.