On 25Sep08: 4 Events were detected

• 📁 **25Sep08**
•    📄
•    📄
•    📄
•    📄
•     📁 **pi1-events-25Sep08**
•        📄 25-09-08T181443_755
•     📁 **pi11-events-25Sep08**
•        📄 25-09-08T174953_729
•        📄 25-09-08T210438_090
•     📁 **pi3-events-25Sep08**
•        📄 25-09-08T174953_727
•        📄 25-09-08T181443_742
•        📄 25-09-08T210438_184
•        📄 25-09-08T235624_492
•     📁 **pi5-events-25Sep08**
•        📄 25-09-08T174953_724
•        📄 25-09-08T181443_752
•        📄 25-09-08T210438_170
•     📁 **pi6-events-25Sep08**
•        📄 25-09-08T174953_725
•        📄 25-09-08T181443_669
•        📄 25-09-08T210438_180
•        📄 25-09-08T235624_491
•     📁 **pi9-events-25Sep08**
•        📄 25-09-08T181443_709
•        📄 25-09-08T210438_161
•        📄 25-09-08T235624_594

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 25Sep08  18.228+/-0.043  0.102 181340.164       60926.7595   225.0+/- 4.8 

#FIT 25Sep08  21.084+/-0.034  0.079 210501.812       60926.8785    55.0+/- 1.3 

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