On 25Mar29: 7 Events were detected

• 📁 **25Mar29**
•    📄
•    📄
•    📄
•    📄
•    📄
•    📄
•    📄
•     📁 **pi1-events-25Mar29**
•        📄 25-03-29T222036_849
•        📄 25-03-29T225055_809
•     📁 **pi10-events-25Mar29**
•        📄 25-03-29T000157_218
•        📄 25-03-29T155413_145
•        📄 25-03-29T170637_078
•        📄 25-03-29T175101_711
•        📄 25-03-29T225055_857
•     📁 **pi11-events-25Mar29**
•        📄 25-03-29T000156_999
•        📄 25-03-29T222036_869
•     📁 **pi3-events-25Mar29**
•        📄 25-03-29T000157_224
•        📄 25-03-29T145414_482
•        📄 25-03-29T155413_369
•        📄 25-03-29T170636_941
•        📄 25-03-29T175101_710
•        📄 25-03-29T225055_637
•     📁 **pi5-events-25Mar29**
•        📄 25-03-29T145414_490
•        📄 25-03-29T155413_310
•        📄 25-03-29T170636_844
•        📄 25-03-29T175101_622
•        📄 25-03-29T222036_886
•     📁 **pi6-events-25Mar29**
•        📄 25-03-29T145414_486
•        📄 25-03-29T155413_373
•        📄 25-03-29T175101_712

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 25Mar29  14.925+/-0.069  0.163 145529.571       60763.6219   312.0+/-14.3 

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