Characterization of downward Terrestrial Gamma-ray Flashes detected at the Pierre Auger Observatory
Roberta Colalillo (for the Pierre Auger Collaboration), Joseph Dwyer, John Ortberg, David M Smith

TL;DR
This paper reports on the characterization of downward Terrestrial Gamma-ray Flashes detected at the Pierre Auger Observatory, revealing complex source structures and discussing future research directions involving lightning and gamma emission analysis.
Contribution
It presents the first observations of asymmetric azimuthal structures in downward TGFs, indicating complex source geometries and suggesting new research avenues.
Findings
First detection of asymmetric azimuthal TGF structures
Evidence for complex source geometries in TGFs
Potential for combined lightning and gamma emission studies
Abstract
Downward Terrestrial Gamma-ray Flashes (TGFs) are sub-millisecond bursts of MeV gamma rays produced in thunderclouds. According to the Relativistic Runaway Electron Avalanche model, gamma rays are produced, via bremsstrahlung, from electron cascades activated by a relativistic "seed" electron. It is not clear what mechanism is responsible for the acceleration of electrons to relativistic energies in electric discharges. To better understand the acceleration sites and the TGF production mechanisms, it is critically important to identify the TGF source position and geometry in the atmosphere and to study the gamma emission characteristics. The Surface Detector of the Pierre Auger Observatory, with its 1600 water-Cherenkov detectors very sensitive to high-energy photons and with a very fine time-sampling, is a valuable instrument to study downward TGFs. The possibility to analyze the…
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