AE31A-3390:
Bayesian Block Analysis of Terrestrial Gamma-ray Flashes Detected by the Gamma-ray Burst Monitor
Wednesday, 17 December 2014
Oliver Roberts1, Gerard Fitzpatrick1, Sheila McBreen1 and Michael S Briggs2, (1)University College Dublin, Dublin, Ireland, (2)University of Alabama in Huntsville, Huntsville, AL, United States
Abstract:
The Gamma-ray Burst Monitor (GBM) is one of two instruments aboard the Fermi Gamma-ray Space Telescope. Since the launch of the spacecraft in 2008, a sequence of flight software enhancements and new observing modes have resulted in the detection of over 2500 Terrestrial Gamma-ray Flashes (TGFs) by GBM. As a result, a catalogue of TGFs will be published and released online to provide the community with information on the most important characteristics of these TGFs. We will present a Bayesian Block analysis of the TGFs of this catalogue, obtaining for this large sample size the durations, peak times, hardness ratios, and delays between soft and hard counts.
