Microwave Observations of Sub-second Pulses with Spatial Resolution

Details Microwave Observations of Sub-second Pulses with Spatial Resolution Microwave Observations of Sub-second Pulses with Spatial Resolution

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..279a&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

Scientific paper

A few tens of sub-second pulses (SSP) have been recorded since 1992 by the SSRT (5.7~GHz) and the Nobeyama Radioheliograph (17~GHz). At both frequencies, SSP occurred at any phase of flare bursts. Temporal and spatial characteristics of SSP observed at both frequencies were studied. For three 17~GHz events, BATSE/CGRO data of 64~ms resolution are available. There are several sub-second structures in HXR data which are highly correlated with microwave pulses. Emission mechanisms of SSP are discussed and plasma parameters in the sources are estimated.

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