Effects of dead time losses on terrestrial gamma ray flash measurements with the Burst and Transient Source Experiment

Details Effects of dead time losses on terrestrial gamma ray flash measurements with the Burst and Transient Source Experiment Effects of dead time losses on terrestrial gamma ray flash measurements with the Burst and Transient Source Experiment

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jgra..11500e21g&link_type=abstract

Journal of Geophysical Research, Volume 115, Issue 3, CiteID A00E21

Physics

Geophysics

11

Atmospheric Processes: Atmospheric Electricity, Mathematical Geophysics: Instruments And Techniques, Mathematical Geophysics: Spectral Analysis (3205, 3280), Atmospheric Composition And Structure: Instruments And Techniques

Scientific paper

Measurements from the Burst and Transient Source Experiment (BATSE) instrument on the Compton Gamma Ray Observatory (CGRO) are the only ones where characteristics of single terrestrial gamma ray flashes (TGFs) have been obtained thus far. However, it has been reported that the measurements suffer from significant dead time losses which complicates the analysis and raises question about earlier BATSE studies. These losses are due to the high-intensity flux combined with limitations of the time resolution of the instrument. Since these losses will affect both the spectrum and the temporal distribution of the individual TGFs, results based on BATSE data need to be revisited, including our own. We have therefore developed a Monte Carlo method to study the effects of these dead time losses. We show that the energy spectrum of TGFs becomes softer as the dead time losses increase. We also show that the time delay between the light curves of hard (E > 300 keV) and soft (E < 300 keV) photons increases significantly as the dead time losses increase. The Monte Carlo approach also enables us to identify the BATSE TGFs where the dead time effects can be corrected. These are the short-duration single-peaked TGFs. Without correcting for dead time losses we find that these short single-peak TGFs have a softer energy spectrum and larger time delay than the multipeaked TGFs. After correcting for dead time losses we perform a new analysis of production altitudes and find that the production altitude is reduced compared to analysis without dead time losses. The new production altitudes combined with dead time losses are also consistent with the apparent large time delays. Our method gives consistent results regarding production altitude and time delays and indicates that the corrected TGF intensities measured by BATSE are 3 to 4 times brighter than the uncorrected measurements would indicate. We also show that the production mechanism of these TGFs has a typical duration of 250 μs.

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