Date of Award

2025

Document Type

Dissertation

Degree Name

Doctor of Philosophy (PhD)

Department

Space Science

Committee Chair

Peter Veres

Committee Member

Rob Preece

Committee Member

Jon Hakkila

Committee Member

Haihong Che

Committee Member

David Smith

Research Advisor

Michael Briggs

Subject(s)

Gamma ray detectors, Gamma ray bursts, Spectral theory (Mathematics)

Abstract

The Fermi Gamma-ray Burst Monitor (GBM) is a wide-field survey instrument in a low-Earth, low-inclination orbit. It contains twelve sodium iodide detectors and two bismuth germanate detectors which together span an energy range from ~8 keV to ~40 MeV and observe the entire unocculted sky (~70%). The highest resolution GBM data product is the time-tagged event data which has ~2 microseconds temporal resolution and 128 pseudo-logarithmically spaced spectral channels. All of these factors make Fermi the perfect instrument for detecting a wide variety of high-energy terrestrial and astrophysical phenomena. In this dissertation, I implement new data analysis techniques to explore the edge cases of GBM data: GRB 221009A in the extremely high count-rate regime and weak terrestrial gamma-ray flashes with lightning associations in the extremely low count-rate regime.

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