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 58Nov17 21.174+/-0.102 0.241 211025.559 0.8822 10348.1+/-200.9 #FIT 58Nov17 20.827+/-0.044 0.104 204936.715 0.8678 1952.0+/-72.2
Overview of Radio Detection of Cosmic Ray Flashes and access to observations.