TY - JOUR
T1 - Characteristics of Negative Leader Propagation Area of Lightning Flashes Initiated in the Stratiform Regions of Mesoscale Convective Systems
AU - Wang, Fei
AU - Zhang, Yijun
AU - Dong, Wansheng
AU - Liu, Hengyi
AU - Li, Feng
AU - Yao, Wen
N1 - Publisher Copyright:
© 2020. American Geophysical Union. All Rights Reserved.
PY - 2021/2/16
Y1 - 2021/2/16
N2 - To investigate the characteristics of extension areas (mainly the propagation areas of negative leaders in this study), the lightning location data of 254 lightning flashes initiated in the stratiform regions (stratiform lightning flashes) of 14 mesoscale convective systems (MCSs) are analyzed. The results show that most of the flashes have a relatively small lightning area (LA) (≤100 km2), although they are initiated in the stratiform regions. In small or developing MCSs, most negative leaders of stratiform lightning flashes concentrate within the 9–12-km altitude range. In other MCSs with a large-sized and developed stratiform region, besides being in this high-altitude range, the negative leaders are also found to propagate more frequently in a low-altitude range of 5–7 km. Further analysis indicates that most of the stratiform lightning flashes with a large LA (>100 km2) propagate their negative leaders within the high-altitude range, no matter where they are initiated. Moreover, the stratiform lightning flashes with or near the largest LA tend to be initiated 4–6 km below their negative leaders, while most of the stratiform lightning flashes usually propagate their negative leaders horizontally within ±1 km of the first detected very-high-frequency (VHF) radiation source. It is inferred that some in-situ electrifications occurring before and during the formation of the high reflectivity layers in the low-altitude range contribute to these flashes, although the influence of the advection charges from the convective regions still cannot be totally ruled out.
AB - To investigate the characteristics of extension areas (mainly the propagation areas of negative leaders in this study), the lightning location data of 254 lightning flashes initiated in the stratiform regions (stratiform lightning flashes) of 14 mesoscale convective systems (MCSs) are analyzed. The results show that most of the flashes have a relatively small lightning area (LA) (≤100 km2), although they are initiated in the stratiform regions. In small or developing MCSs, most negative leaders of stratiform lightning flashes concentrate within the 9–12-km altitude range. In other MCSs with a large-sized and developed stratiform region, besides being in this high-altitude range, the negative leaders are also found to propagate more frequently in a low-altitude range of 5–7 km. Further analysis indicates that most of the stratiform lightning flashes with a large LA (>100 km2) propagate their negative leaders within the high-altitude range, no matter where they are initiated. Moreover, the stratiform lightning flashes with or near the largest LA tend to be initiated 4–6 km below their negative leaders, while most of the stratiform lightning flashes usually propagate their negative leaders horizontally within ±1 km of the first detected very-high-frequency (VHF) radiation source. It is inferred that some in-situ electrifications occurring before and during the formation of the high reflectivity layers in the low-altitude range contribute to these flashes, although the influence of the advection charges from the convective regions still cannot be totally ruled out.
KW - first detected VHF radiation source
KW - lightning flashes
KW - mesoscale convective systems
KW - propagation area of negative leaders
KW - stratiform regions
UR - http://www.scopus.com/inward/record.url?scp=85101039860&partnerID=8YFLogxK
U2 - 10.1029/2020JD033336
DO - 10.1029/2020JD033336
M3 - Article
AN - SCOPUS:85101039860
SN - 2169-897X
VL - 126
JO - Journal of Geophysical Research: Atmospheres
JF - Journal of Geophysical Research: Atmospheres
IS - 3
M1 - e2020JD033336
ER -