Abstract
A flare that began on 1993 June 3 was observed jointly by the Owens
Valley Radio Observatory
(OVRO) Solar Array and
the Nobeyama Radio Observatory (NRO)
Radioheliograph. We present
preliminary results from these observations, along with soft X-ray data
from the Yohkoh SXT and
GOES. The burst had a gradual time profile in the 17GHz NRO data, except
for a pair of unusual
spikes in the decay phase. However, the OVRO data show that the burst
was impulsize,
comprising several peaks at progressively higher frequencies. We suggest
that the gradual
17GHz emission is thermal, and discuss the relationship of the thermal
emission to the impulsive
emission.