Abstract
We present 221 Terrestrial Gamma-ray flashes (TGFs) and associated
optical pulses observed by the Atmosphere-Space Interactions Monitor on
board the International Space Station. The events were detected between
the end of March 2019 and November 2020 and consist of X- and Gamma-ray
energy detections, as well as photometer data (180-230 nm, 337 nm and
777 nm) and optical camera data (337 nm and 777 nm). Using the available
ASIM data and applying a consistency check based on TGF characteristics
and lightning detections from lightning radio atmospherics close in
time, we determine the most likely position of the TGFs in relation to
the photometer field of view (FoV), and the association to the observed
optical pulses. Out of the 221 events we find 72 events where the TGF
and optical data are determined to be associated and inside the
photometer FoV. Using the measured TGF durations and the time between
the onsets of the TGFs and optical pulses we find 1) That the TGF onsets
are always before or at the same time as the optical pulse onsets
(taking into account cloud scattering). 2) A tendency for longer
duration TGFs to have longer delays between onsets. 3) Two groups of
events: a) where there is a possible overlap between the TGFs and the
optical emissions, as the TGFs last longer than the delay between onsets
and b) where the TGFs and optical emissions do not overlap, as there
are long delays between the onsets, which cannot be explained by cloud
scattering.
| Original language | English |
|---|---|
| Article number | e2022JD037128 |
| Journal | Journal of Geophysical Research |
| Volume | 127 |
| Issue number | 17 |
| ISSN | 0148-0227 |
| DOIs | |
| Publication status | Published - 2022 |
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