Schultz Christopher J, Andrews Virginia P, Genareau Kimberly D, Naeger Aaron R
NASA's Short-Term Prediction and Research Transition Center, Marshall Space Flight Center, Huntsville, AL, 35812, USA.
Department of Geological Sciences, The University of Alabama, Box 870338, Tuscaloosa, AL, 35487, USA.
Sci Rep. 2020 Oct 22;10(1):18015. doi: 10.1038/s41598-020-74576-x.
Satellite and ground-based remote sensing are combined to characterize lightning occurrence during the 3 June 2018 Volcán de Fuego eruption in Guatemala. The combination of the space-based Geostationary Lightning Mapper (GLM) and ground-based Earth Networks Total Lightning Network observed two distinct periods of lightning during this eruption totaling 75 unique lightning flash occurrences over five hours (57 in cloud, 18 cloud-to-ground). The first period of lightning coincided with the rapid growth of the ash cloud, while the second maxima occurred near the time of a deadly pyroclastic density current (PDC) and thunderstorm. Ninety-one percent of the lightning during the event was observed by only one of the lightning sensors, thus showing the importance of combining lightning datasets across multiple frequencies to characterize electrical activity in volcanic eruptions. GLM flashes during the event had a median total optical energy and flash length of 16 fJ, and 12 km, respectively. These median GLM flash energies and lengths observed in the volcanic plume are on the lower end of the flash spectrum because flashes observed in surrounding thunderstorms on 3 June had larger median total optical energy values (130 fJ) and longer median flash lengths (20 km). All 18 cloud-to-ground flashes were negative polarity, supportive of net negative charge within the plume. Mechanisms for the generation of the secondary lightning maxima are discussed based on the presence and potential interaction between ash plume, thunderstorm, and PDC transport during this secondary period of observed lightning.
卫星遥感和地面遥感相结合,以描述2018年6月3日危地马拉富埃戈火山喷发期间的闪电发生情况。天基地球同步闪电成像仪(GLM)和地面地球网络总闪电网络相结合,在这次火山喷发期间观测到两个不同的闪电阶段,在五个小时内共有75次独特的闪电发生(云内闪电57次,云地闪电18次)。第一个闪电阶段与火山灰云的快速增长同时出现,而第二个闪电高峰出现在致命的火山碎屑流(PDC)和雷暴发生的时间附近。此次事件中91%的闪电仅由其中一个闪电传感器观测到,这表明结合多个频率的闪电数据集对于描述火山喷发中的电活动非常重要。此次事件期间GLM闪电的总光学能量中位数和闪击长度中位数分别为16飞焦和12千米。在火山羽流中观测到的这些GLM闪击能量和长度中位数处于闪击光谱的低端,因为6月3日在周围雷暴中观测到的闪击总光学能量中位数更大(130飞焦),闪击长度中位数更长(20千米)。所有18次云地闪电均为负极性,这支持了羽流内的净负电荷。基于观测到的第二次闪电期间火山灰羽流、雷暴和PDC输送之间的存在及潜在相互作用,讨论了二次闪电最大值产生的机制。