On 25Mar26: 7 Events were detected

• 📁 **25Mar26**
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•     📁 **pi1-events-25Mar26**
•        📄 25-03-26T132745_557
•        📄 25-03-26T154559_998
•        📄 25-03-26T161132_408
•        📄 25-03-26T171119_956
•        📄 25-03-26T184342_567
•     📁 **pi10-events-25Mar26**
•        📄 25-03-26T171119_955
•        📄 25-03-26T194957_891
•     📁 **pi11-events-25Mar26**
•        📄 25-03-26T161132_453
•        📄 25-03-26T171119_847
•        📄 25-03-26T184342_625
•     📁 **pi3-events-25Mar26**
•        📄 25-03-26T132745_794
•        📄 25-03-26T154559_993
•        📄 25-03-26T155524_875
•        📄 25-03-26T161132_439
•        📄 25-03-26T184342_560
•        📄 25-03-26T194957_888
•     📁 **pi5-events-25Mar26**
•        📄 25-03-26T132745_770
•        📄 25-03-26T154559_978
•        📄 25-03-26T155524_877
•        📄 25-03-26T161132_440
•        📄 25-03-26T184342_575
•     📁 **pi6-events-25Mar26**
•        📄 25-03-26T154559_826
•        📄 25-03-26T155524_683
•        📄 25-03-26T161132_449
•        📄 25-03-26T171119_918
•        📄 25-03-26T194957_855

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 25Mar26  16.274+/-0.057  0.134 161627.324       60760.6781  1484.0+/-60.7 

#FIT 25Mar26  15.760+/-0.059  0.139 154536.353       60760.6567   695.0+/-18.0 

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