On 25Aug03: 4 Events were detected

• 📁 **25Aug03**
•    📄
•    📄
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•     📁 **pi1-events-25Aug03**
•        📄 25-08-03T180752_780
•        📄 25-08-03T181025_549
•        📄 25-08-03T182335_421
•        📄 25-08-03T183000_048
•     📁 **pi11-events-25Aug03**
•        📄 25-08-03T180752_853
•        📄 25-08-03T181025_306
•        📄 25-08-03T182335_406
•        📄 25-08-03T183000_076
•     📁 **pi3-events-25Aug03**
•        📄 25-08-03T181025_619
•        📄 25-08-03T182335_430
•        📄 25-08-03T183000_045
•     📁 **pi5-events-25Aug03**
•        📄 25-08-03T180752_771
•        📄 25-08-03T181025_599
•        📄 25-08-03T182335_436
•        📄 25-08-03T183000_034
•     📁 **pi6-events-25Aug03**
•        📄 25-08-03T180752_781
•        📄 25-08-03T181025_372
•        📄 25-08-03T182335_423
•        📄 25-08-03T183000_011
•     📁 **pi9-events-25Aug03**
•        📄 25-08-03T180752_781
•        📄 25-08-03T181025_600
•        📄 25-08-03T182335_400
•        📄 25-08-03T183000_010

Successfully fit 1 Event Group.
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 25Aug03  18.322+/-0.172  0.406 181920.335       60890.7634 10656.8+/-288.1 

Overview of Radio Detection of Cosmic Ray Flashes and access to observations.