On 25Mar05: 14 Events were detected

• 📁 **25Mar05**
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•     📁 **pi1-events-25Mar05**
•        📄 25-03-05T192827_889
•        📄 25-03-05T194252_967
•        📄 25-03-05T195845_537
•        📄 25-03-05T200008_582
•        📄 25-03-05T201347_526
•        📄 25-03-05T210215_242
•        📄 25-03-05T211031_099
•        📄 25-03-05T212558_737
•        📄 25-03-05T213143_415
•        📄 25-03-05T214540_676
•        📄 25-03-05T215235_739
•        📄 25-03-05T221334_625
•     📁 **pi11-events-25Mar05**
•        📄 25-03-05T192827_878
•        📄 25-03-05T195845_580
•        📄 25-03-05T200008_554
•        📄 25-03-05T201347_498
•        📄 25-03-05T205446_116
•        📄 25-03-05T210215_245
•        📄 25-03-05T211031_083
•        📄 25-03-05T212558_733
•        📄 25-03-05T214540_645
•     📁 **pi3-events-25Mar05**
•        📄 25-03-05T185755_088
•        📄 25-03-05T192827_889
•        📄 25-03-05T194252_955
•        📄 25-03-05T195845_537
•        📄 25-03-05T200008_589
•        📄 25-03-05T201347_524
•        📄 25-03-05T205446_091
•        📄 25-03-05T210215_240
•        📄 25-03-05T211031_103
•        📄 25-03-05T212558_759
•        📄 25-03-05T213143_421
•        📄 25-03-05T214540_682
•        📄 25-03-05T215235_753
•        📄 25-03-05T221334_639
•     📁 **pi5-events-25Mar05**
•        📄 25-03-05T185755_068
•        📄 25-03-05T192827_873
•        📄 25-03-05T195845_549
•        📄 25-03-05T200008_563
•        📄 25-03-05T201347_544
•        📄 25-03-05T210215_235
•        📄 25-03-05T211031_093
•        📄 25-03-05T212558_712
•        📄 25-03-05T213143_390
•        📄 25-03-05T214540_654
•     📁 **pi6-events-25Mar05**
•        📄 25-03-05T185755_066
•        📄 25-03-05T192827_819
•        📄 25-03-05T194252_920
•        📄 25-03-05T195845_546
•        📄 25-03-05T200008_560
•        📄 25-03-05T201347_518
•        📄 25-03-05T205446_073
•        📄 25-03-05T210215_229
•        📄 25-03-05T211031_088
•        📄 25-03-05T212558_704
•        📄 25-03-05T213143_377
•        📄 25-03-05T214540_637
•        📄 25-03-05T215235_755
•        📄 25-03-05T221334_594

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 25Mar05  21.095+/-0.078  0.183 210543.771       60739.8790   718.9+/-31.5 

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