High Peak‐Current Lightning Discharges Associated With Downward Terrestrial Gamma‐Ray Flashes

Author(s):  
Y. Wada ◽  
T. Enoto ◽  
Y. Nakamura ◽  
T. Morimoto ◽  
M. Sato ◽  
...  
2021 ◽  
Author(s):  
Andrey Mezentsev ◽  
Nikolai Østgaard ◽  
Torsten Neubert ◽  
Victor Reglero

<p>The Atmosphere-Space Interactions Monitor (ASIM) has been installed on board of the International Space Station in April 2018, successfully providing science data for 2.5 years. The Modular X- and Gamma-ray Sensor (MXGS) of ASIM is designed to detect Terrestrial Gamma-ray Flashes (TGFs) (short intense bursts of gamma-ray photons), produced during the initial breakdown phase of the +IC lightning discharges.</p><p> </p><p>In this contribution we report and summarize the results on the ASIM TFGs associated with high peak current lightning detections (detected by GLD and WWLLN networks). High peak current detections tend to be associated with short duration TGFs and do not exhibit a tendency to correlate with the fluence of the TGF.</p>


2006 ◽  
Vol 24 (12) ◽  
pp. 3197-3214 ◽  
Author(s):  
C. J. Rodger ◽  
S. Werner ◽  
J. B. Brundell ◽  
E. H. Lay ◽  
N. R. Thomson ◽  
...  

Abstract. An experimental Very Low Frequency (VLF) World-Wide Lightning Location Network (WWLLN) has been developed through collaborations with research institutions across the world, providing global real-time locations of lightning discharges. As of April 2006, the network included 25 stations providing coverage for much of the Earth. In this paper we examine the detection efficiency of the WWLLN by comparing the locations from this network with lightning location data purchased from a commercial lightning location network operating in New Zealand. Our analysis confirms that WWLLN favours high peak current return stroke lightning discharges, and that discharges with larger currents are observed by more stations across the global network. We then construct a first principles detection efficiency model to describe the WWLLN, combining calibration information for each station with theoretical modelling to describe the expected amplitudes of the VLF sferics observed by the network. This detection efficiency model allows the prediction of the global variation in WWLLN lightning detection, and an estimate of the minimum CG return stroke peak current required to trigger the network. There are strong spatial variations across the globe, primarily due to station density and sensitivity. The WWLLN is currently best suited to study the occurrence and impacts of high peak-current lightning. For example, in 2005 about 12% of the global elve-producing lightning will have been located by the network. Since the lightning-EMP which produce elves has a high mean rate (210 per minute) it has the potential to significantly influence the ionosphere on regional scales.


2016 ◽  
Vol 37 (2) ◽  
pp. 205-208 ◽  
Author(s):  
Wanjun Chen ◽  
Chao Liu ◽  
Xuefeng Tang ◽  
Lunfei Lou ◽  
Wu Cheng ◽  
...  
Keyword(s):  
Turn On ◽  

2006 ◽  
Vol 33 (18) ◽  
pp. n/a-n/a ◽  
Author(s):  
U. S. Inan ◽  
M. B. Cohen ◽  
R. K. Said ◽  
D. M. Smith ◽  
L. I. Lopez

1991 ◽  
Vol 38 (4) ◽  
pp. 758-766 ◽  
Author(s):  
K.W. Harris ◽  
G. McDuff ◽  
T.R. Burkes

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