@InProceedings{BelzAKKLPRRSSS:2022:NeObIn,
author = "Belz, John and Abbasi, Rasha and Kieu, Ny and Krehbiel, Paul R.
and LeVon, Ryan and Petrizze, Alex and Remington, Jackson and
Rison, William and Saba, Marcelo Magalh{\~a}es Fares and Smout,
Kieran and Stanley, Mark A.",
affiliation = "{University of Utah} and {University of Utah} and {Loyola
University Chicago} and {New Mexico Tech} and {University of Utah}
and {University of Utah} and {University of Utah} and {New Mexico
Tech} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{University of Utah} and {New Mexico Institute of Mining and
Technology}",
title = "New Observations of Intermediate-Duration Downward Terrestrial
Gamma-ray Flashes",
year = "2022",
organization = "AGU Fall Meeting",
publisher = "AGU",
abstract = "We present the most recent observations of the lightning research
program at the Telescope Array cosmic ray observatory in Utah,
U.S.A. This program focuses on understanding the initial breakdown
stage of lightning through observations of downward Terrestrial
Gamma-ray Flashes (TGFs). The Telescope Array Surface Detector
(TASD) is a 700 square kilometer array of plastic scintillator
detectors located in Utah's western desert. It consists of 507
three-square-meter detectors on a 1.2 km grid. The TASD was
designed to detect particle showers generated by the interaction
of ultra-high energy cosmic rays with the Earth's atmosphere.
Recent observations have demonstrated that Terrestrial Gamma-ray
Flashes (TGFs) detected by satellites are associated with
high-current energetic in-cloud pulses during ascending negative
leaders. Meanwhile, a relatively small number of observations have
been made of TGFs on the ground, owing to the greater atmospheric
attenuation of gamma rays and the relatively rare occurrence of
TGFs sufficiently close to detectors. Previously (Abbasi et al
2018, Belz et al 2020) we reported joint observations by TASD,
Lightning Mapping Array (LMA), sferic sensor and broadband
interferometer of particle showers coincident with lightning.
These consisted of energetic showers of approximately 5
microsecond duration with footprints on the ground of order 10
square kilometers, originating in the first one to two
milliseconds of downward lightning leaders and coincident with
high-current processes within the leaders. Scintillator waveform
and simulation studies confirmed that these showers must consist
primarily of gamma radiation, thus the observations were
identified TGFs near their initiation threshold. The TASD-observed
downward TGFs were in general of shorter duration and lower
fluence than their satellite-detected upward counterparts. Here,
we report the new observation and study via the Monte Carlo
technique of several events of significantly longer duration and
higher fluence than previously observed. These events bridge the
gap between the prior TASD and satellite based detections, and
thus further demonstrate the similarity between the upward and
downward varieties of TGF.",
conference-location = "Chicago, IL",
conference-year = "12-16 Dec. 2022",
urlaccessdate = "06 jun. 2024"
}