On 25Apr04: 4 Events were detected

• 📁 **25Apr04**
•    📄
•    📄
•    📄
•    📄
•     📁 **pi1-events-25Apr04**
•        📄 25-04-04T073925_780
•        📄 25-04-04T074109_231
•        📄 25-04-04T140023_287
•     📁 **pi10-events-25Apr04**
•        📄 25-04-04T180753_761
•     📁 **pi11-events-25Apr04**
•        📄 25-04-04T074109_187
•     📁 **pi3-events-25Apr04**
•        📄 25-04-04T073925_779
•        📄 25-04-04T074109_227
•        📄 25-04-04T140023_282
•        📄 25-04-04T180753_556
•     📁 **pi5-events-25Apr04**
•        📄 25-04-04T073925_784
•        📄 25-04-04T074109_234
•        📄 25-04-04T140023_159
•     📁 **pi6-events-25Apr04**
•        📄 25-04-04T073925_767
•        📄 25-04-04T074109_224
•        📄 25-04-04T140023_288
•        📄 25-04-04T180753_558

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 25Apr04   7.699+/-0.070  0.164 074157.107       60769.3208   661.0+/- 8.8 

#FIT 25Apr04  14.083+/-0.033  0.078 140500.175       60769.5868   103.0+/- 2.0 

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