1 Events were detected

Successfully fit 2 Event Groups. When many flashes are detected we fit the average time of events FWHM is the time interval of gaussain fit, in hours # Date Fit Hour FWYM HHmmSS.sss MJD Event Counts #FIT 25Nov07 1.083+/-0.031 0.074 010500.041 60986.0451 597.0+/- 1.5 #FIT 25Nov07 21.444+/-0.031 0.073 212637.759 60986.8935 17.0+/- 0.5
Overview of Radio Detection of Cosmic Ray Flashes and access to observations.