On 25Mar28: 6 Events were detected

• 📁 **25Mar28**
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•     📁 **pi1-events-25Mar28**
•        📄 25-03-28T190035_389
•     📁 **pi10-events-25Mar28**
•        📄 25-03-28T010352_863
•        📄 25-03-28T142849_854
•        📄 25-03-28T201539_356
•        📄 25-03-28T213620_762
•     📁 **pi11-events-25Mar28**
•        📄 25-03-28T190035_405
•        📄 25-03-28T201539_355
•     📁 **pi3-events-25Mar28**
•        📄 25-03-28T010353_109
•        📄 25-03-28T142849_974
•        📄 25-03-28T171449_458
•        📄 25-03-28T201539_429
•        📄 25-03-28T213620_965
•     📁 **pi5-events-25Mar28**
•        📄 25-03-28T142849_951
•        📄 25-03-28T171449_489
•        📄 25-03-28T213620_966
•     📁 **pi6-events-25Mar28**
•        📄 25-03-28T010353_168
•        📄 25-03-28T142849_943
•        📄 25-03-28T171449_641
•        📄 25-03-28T190035_409
•        📄 25-03-28T201539_422
•        📄 25-03-28T213620_897

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 25Mar28  19.108+/-0.060  0.141 190628.629       60762.7962   623.0+/- 9.1 

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