Statistical Study of Two Years of Solar Flare Radio Spectra Obtained with the Owens Valley Solar Array
We present results of analysis of 412 flares during 20012002 as detected by the Owens Valley Solar Array (OVSA). This is an in-depth study to investigate some results suggested by a previous study of solar bursts (Nita et al. 2002), which was limited to the peak time of the bursts at a few frequency bands. The new study includes the temporal dependence, at 4 s time resolution, of parameters measured at 40 frequencies in the range 118 GHz. We investigate
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