The Illumination of Thunderclouds by Lightning: Part 2: The Effect of
GLM Instrument Threshold on Detection and Clustering
Abstract
Lightning is measured from space using optical instruments that detect
transient changes in the illumination of the cloud top. How much of the
flash (if any) is recorded by the instrument depends on the instrument
detection threshold. NOAA’s Geostationary Lightning Mapper (GLM) employs
a dynamic threshold that varies across the imaging array and changes
over time. This causes flashes in certain regions and at night to be
recorded in greater detail than other flashes, and threshold
inconsistencies will impose biases on all levels of GLM data products.
In this study, we quantify the impact of the varying GLM threshold on
event / group detection, flash clustering, and gridded product
generation by imposing artificial thresholds on the event data taken
from a thunderstorm with a low instrument threshold
(~0.7 fJ). We find that even modest increases in
threshold severely impact event (60% loss by 2 fJ, 90% loss by 10 fJ)
and group (25% loss by 2 fJ, 81% loss by 10 fJ) detection by
suppressing faint illumination of the cloud-top from weak sources and
scattering. Flash detection is impacted less by threshold increases (4%
loss by 2 fJ), but reductions are still significant at higher thresholds
(35% loss by 10 fJ, or 44% if single-group flashes are removed).
Undetected pulses cause individual flashes to be split and severely
impact the construction of gridded products. All these factors
complicate the interpretation of GLM data, particularly when trended
over time under a changing threshold.