On 26May30: 2 Events were detected

• 📁 **26May30**
•    📄
•    📄
•     📁 **pi7-events-26May30**
•        📄 26-05-30T162410_198
•        📄 26-05-30T203810_628
•     📁 **pi11-events-26May30**
•        📄 26-05-30T203810_632
•        📄 26-05-30T162410_040
•     📁 **pi9-events-26May30**
•        📄 26-05-30T203810_563
•        📄 26-05-30T162409_961
•     📁 **pi5-events-26May30**
•        📄 26-05-30T162410_010
•     📁 **pi3-events-26May30**
•        📄 26-05-30T203810_569
•        📄 26-05-30T162410_186
•     📁 **pi1-events-26May30**
•        📄 26-05-30T203810_529
•        📄 26-05-30T162410_194

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 26May30  20.583+/-0.034  0.080 203500.251       61190.8576   214.0+/- 4.7 

#FIT 26May30  16.417+/-0.035  0.082 162459.985       61190.6840    53.0+/- 1.5 

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