Variability of Ionospheric Total Electron Content Over Morocco During the Godzilla Sand and Dust Storm of June 2020

Uluma Edward, C. Uga, Athwart Odhiambo, B. Adhikari, S. Gautam, Ndinya Boniface, Omondi George, A. Giri, Dessalegn Teferi, Negasa Belay, A. Silwal
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Abstract

During sand and dust storm (SDS) events, atmospheric suspension and transport of sand and dust brings a reasonable amount of electrification in the atmosphere which plays a very important role in the atmosphere-ionosphere coupling. The Godzilla SDS began on 5th June 2020 in Algeria following a decrease in pressure and spread to other areas across the Sahara between 6th and 28th June 2020. Using SDS data from Copernicus Sentinel-5P satellite mission and Vertical Total Electron Content (VTEC) data from four GNSS receiver stations: IFR1 (Ifrane Seismic), MELI (Melilla), TETN (Tetouan) and OUCA (Ouca) over Morocco, we investigate the possible ionospheric TEC variability over the four GNSS receiver stations during the Godzilla SDS event which was tracked using the Sentinel-5P Satellite mission. Solar wind parameters: Horizontal component of Interplanetary Magnetic Field (IMF-Bz), interplanetary Electric Field (IEF-Ey) and solar wind speed (V) and geomagnetic indices: Disturbance Storm Time (Dst) and Planetary K (Kp) indices were examined and showed very minimal geomagnetic influence during the period. We observed major ionospheric disturbances over the four Global Navigation Satellite System (GNSS) receiver stations on 16th, 17th, 18th, 21st, 22nd, 23rd 25th and 26th June 2020: the period with the Sentinel-5P Aerosol Index (SAI) of more than 4 as recorded by the Sentinel-5P Satellite engine. The daily VTEC values over the four GNSS receiver stations recorded continuous electron density perturbations during these days. Apart from the ionospheric TEC perturbations, significant enhancements and decreases in daily maximum VTEC values over the four GNSS receiver stations were also noted. These were attributed to the changes in the atmospheric electric fields generated by the SDS event. The VTEC plots for each day exhibited similar trends, hence exhibited the same ionospheric dynamics. VTEC depletions of depths 3 to 6 TECU over all the four GNSS receiver stations were noted on 12th, 14th, 17th, 20th and 25th June 2020. Nighttime VTEC enhancements were also noted and majorly occurred between 20:00 and 21:00 UT on 9th, 13th, 15th, 17th, 19th, 20th and 21st June 2020. This was attributed to the development of the electron avalanche processes including dust and electron absorption or losses and the active conversion to electron dissociative attachment leading to electron excitation. In conclusion, the Godzilla SDS of June 2020 led to the electron density perturbations over Morocco.
2020 年 6 月哥斯拉沙尘暴期间摩洛哥上空电离层总电子含量的变异性
在沙尘暴(SDS)事件中,沙尘在大气中的悬浮和飘移会给大气带来一定量的电能,这在大气-电离层耦合中起着非常重要的作用。哥斯拉沙尘暴于 2020 年 6 月 5 日开始在阿尔及利亚出现,随后气压下降,并于 2020 年 6 月 6 日至 28 日扩散到撒哈拉沙漠的其他地区。利用哥白尼哨兵-5P 卫星任务提供的 SDS 数据和四个全球导航卫星系统接收站提供的垂直总电子含量(VTEC)数据:我们利用哥白尼哨兵-5P 卫星飞行任务跟踪的哥斯拉 SDS 事件期间摩洛哥上空的 IFR1(Ifrane 地震站)、MELI(梅利利亚站)、TETN(德图安站)和 OUCA(乌卡站),研究了这四个全球导航卫星系统接收站上空电离层 TEC 的可能变化。太阳风参数:行星际磁场水平分量(IMF-Bz)、行星际电场(IEF-Ey)和太阳风速度(V)以及地磁指数:对扰动风暴时间(Dst)和行星 K 指数(Kp)进行了研究,结果表明在此期间地磁影响非常小。2020 年 6 月 16 日、17 日、18 日、21 日、22 日、23 日、25 日和 26 日,即哨兵-5P 卫星引擎记录的哨兵-5P 气溶胶指数(SAI)超过 4 的时期,我们在四个全球导航卫星系统(GNSS)接收站上空观测到了严重的电离层扰动。在这几天里,四个全球导航卫星系统接收站的每日 VTEC 值记录了持续的电子密度扰动。除电离层 TEC 扰动外,还注意到四个全球导航卫星系统接收站的每日最大 VTEC 值显著增大和减小。这归因于 SDS 事件产生的大气电场变化。每天的 VTEC 图显示出相似的趋势,因此表现出相同的电离层动态。2020 年 6 月 12 日、14 日、17 日、20 日和 25 日,在所有四个全球导航卫星系 统接收站都发现了深度为 3 至 6 TECU 的甚低频衰减。还注意到夜间 VTEC 增强,主要发生在 2020 年 6 月 9 日、13 日、15 日、17 日、19 日、20 日和 21 日世界时 20:00 至 21:00 之间。这归因于电子雪崩过程的发展,包括尘埃和电子的吸收或损失,以及电子离解附着导致电子激发的主动转换。总之,2020 年 6 月的哥斯拉 SDS 导致了摩洛哥上空的电子密度扰动。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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