On the performance of CARISMA – Akademik Vernadsky station Schumann resonance monitoring

Q4 Agricultural and Biological Sciences
O. Koloskov, P. T. Jayachandran, Yu. Yampolski
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引用次数: 0

Abstract

The main objective of this study is to evaluate the effectiveness of the CARISMA (Canadian Array for Realtime Investigations of Magnetic Activity) – Akademik Vernadsky station (65.25°S 64.25°W, Vernadsky) Extremely Low Frequency (ELF) induction magnetometer network as a planetary monitoring system for thunderstorm activity, with observation sites located in the Arctic and Antarctic regions, respectively. To achieve this, daily ELF records from Vernadsky and Fort Churchill (FCHU, 58.76°N 94.08°W) collected in January 2022 were processed and analyzed. For CARISMA, data from the FCHU site were used due to the better signal-to-noise ratio. The horizontal magnetic components of Schumann signals obtained at Vernadsky and FCHU underwent spectral and polarization processing. ELF transients were identified, and subsequent geolocation was performed as well. Both regular (quiet) thunderstorm activity periods and an unprecedented local amplification of lightning activity near the Hunga Tonga-Hunga Ha'apai volcano during its eruption on January 15, 2022, were studied. Throughout the quiet periods, ELF signal processing yielded similar characteristics of integral lightning activity derived from CARISMA and Vernadsky records, consistent with findings in the literature and previous investigations at the Vernadsky site. On the other hand, the analysis of Schumann spectra and ELF transients during the Tonga volcano eruption confirmed that most thunderstorms were concentrated within a relatively small area around the epicenter, validating the point source model for the global lightning center. This paper demonstrates that the CARISMA and Vernadsky magnetometer network is well-suited for establishing a global lightning activity monitoring andintense lightning geolocation system. Such a system can be employed to assess and study global temperature trends, monitor the growth of lightning activity in high latitudes, and detect terrestrial, atmospheric, and geospace disaster phenomena.
关于CARISMA - Akademik Vernadsky站舒曼共振监测的性能
本研究的主要目的是评估CARISMA(加拿大磁活动实时调查阵列)- Akademik Vernadsky站(65.25°S 64.25°W, Vernadsky)极低频(ELF)感应磁力计网络作为雷暴活动行星监测系统的有效性,观测站点分别位于北极和南极地区。为了实现这一目标,对2022年1月收集的Vernadsky和Fort Churchill (FCHU, 58.76°N 94.08°W)的每日ELF记录进行了处理和分析。由于信噪比更好,CARISMA使用了FCHU站点的数据。在Vernadsky和FCHU获得的Schumann信号的水平磁分量进行了光谱和极化处理。识别ELF瞬变,并进行后续的地理定位。研究了2022年1月15日Hunga Tonga-Hunga Ha'apai火山喷发期间的常规(安静)雷暴活动期和前所未有的局部闪电活动放大。在整个平静期,极低频信号处理产生了CARISMA和Vernadsky记录的整体闪电活动的相似特征,与文献中的发现和Vernadsky站点先前的调查结果一致。另一方面,对汤加火山喷发期间的Schumann光谱和极低频瞬变分析证实,大多数雷暴集中在震中周围相对较小的区域内,验证了全球闪电中心的点源模型。本文论证了CARISMA和Vernadsky磁力计网络非常适合建立全球闪电活动监测和强闪电地理定位系统。这样一个系统可以用来评估和研究全球温度趋势,监测高纬度地区闪电活动的增长,探测地面、大气和地球空间灾害现象。
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来源期刊
Ukrayins''kii antarktichnii zhurnal
Ukrayins''kii antarktichnii zhurnal Biochemistry, Genetics and Molecular Biology-Biochemistry, Genetics and Molecular Biology (miscellaneous)
CiteScore
1.10
自引率
0.00%
发文量
11
审稿时长
10 weeks
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