Global Ionospheric Response to Disturbances during Multistep Magnetic Storm on November 4–5, 2023

IF 0.4 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
L. F. Chernogor, M. Yu. Tkachenko
{"title":"Global Ionospheric Response to Disturbances during Multistep Magnetic Storm on November 4–5, 2023","authors":"L. F. Chernogor,&nbsp;M. Yu. Tkachenko","doi":"10.3103/S088459132604001X","DOIUrl":null,"url":null,"abstract":"<p>The ionosphere, as a medium for radio wave propagation, remains highly sensitive to disturbances in geospace and largely governs the accuracy and reliability of communication, navigation, and radar systems. The most powerful drivers of disturbances in the Earth–atmosphere–ionosphere–magnetosphere (EAIM) and Sun–interplanetary medium–magnetosphere–ionosphere–atmosphere–Earth (SIMMIAE) systems are coronal mass ejections. These events restructure the coupling strength and interaction dynamics across the coupled system, generating spatiotemporal ionospheric disturbances that degrade the performance of satellite- and ground-based technologies. This study addresses the need to better understand both global and local ionospheric responses to intense, nonstationary energy inputs. We investigate ionospheric disturbances during a unique multistage magnetic storm by analyzing maps of the rate of total electron content index (<i>ROTI</i>) and the temporal evolution of global electron content (<i>GEC</i>). We identify three consecutive <i>GEC</i> maxima: approximately 2.20 GECU on November 4 at 22:00 UTC, followed by 2.22–2.25 GECU during the second half of November 5, as well as a deep minimum of 1.63 GECU on November 6. The resulting ionospheric plasma “saturation–depletion” cycle had an amplitude of 0.62 GECU. We observe the highest <i>ROTI</i> values (3.8–4.3 TECU/min) in the polar region (60°–75° N) at 04:00 UTC on November 4, while the strongest equatorial enhancement (3.6 TECU/min) occurred at 00:00 UTC the same day over South America. Strong disturbances (<i>ROTI</i> ≥ 0.9 TECU/min) expanded to geomagnetic latitudes up to ±40° between 18:00 UTC on November 5 and 06:00 UTC on November 6, coinciding with a sharp decline in <i>GEC</i> and a peak in the Akasofu parameter (ε<sub>A</sub> ≈ 6.6 TJ/s). During the second day of the storm main phase, electrodynamic processes, including SAPS and substorms, dominated and produced a pronounced anticorrelation between reduced <i>GEC</i> values and enhanced <i>ROTI</i> activity. <i>ROTI</i> ≥ 1 TECU/min disturbances persisted for approximately 1 day after the <i>D</i><sub>st</sub> index recovered from –50 to –20 nT.</p>","PeriodicalId":681,"journal":{"name":"Kinematics and Physics of Celestial Bodies","volume":"42 4","pages":"141 - 154"},"PeriodicalIF":0.4000,"publicationDate":"2026-07-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Kinematics and Physics of Celestial Bodies","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.3103/S088459132604001X","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

The ionosphere, as a medium for radio wave propagation, remains highly sensitive to disturbances in geospace and largely governs the accuracy and reliability of communication, navigation, and radar systems. The most powerful drivers of disturbances in the Earth–atmosphere–ionosphere–magnetosphere (EAIM) and Sun–interplanetary medium–magnetosphere–ionosphere–atmosphere–Earth (SIMMIAE) systems are coronal mass ejections. These events restructure the coupling strength and interaction dynamics across the coupled system, generating spatiotemporal ionospheric disturbances that degrade the performance of satellite- and ground-based technologies. This study addresses the need to better understand both global and local ionospheric responses to intense, nonstationary energy inputs. We investigate ionospheric disturbances during a unique multistage magnetic storm by analyzing maps of the rate of total electron content index (ROTI) and the temporal evolution of global electron content (GEC). We identify three consecutive GEC maxima: approximately 2.20 GECU on November 4 at 22:00 UTC, followed by 2.22–2.25 GECU during the second half of November 5, as well as a deep minimum of 1.63 GECU on November 6. The resulting ionospheric plasma “saturation–depletion” cycle had an amplitude of 0.62 GECU. We observe the highest ROTI values (3.8–4.3 TECU/min) in the polar region (60°–75° N) at 04:00 UTC on November 4, while the strongest equatorial enhancement (3.6 TECU/min) occurred at 00:00 UTC the same day over South America. Strong disturbances (ROTI ≥ 0.9 TECU/min) expanded to geomagnetic latitudes up to ±40° between 18:00 UTC on November 5 and 06:00 UTC on November 6, coinciding with a sharp decline in GEC and a peak in the Akasofu parameter (εA ≈ 6.6 TJ/s). During the second day of the storm main phase, electrodynamic processes, including SAPS and substorms, dominated and produced a pronounced anticorrelation between reduced GEC values and enhanced ROTI activity. ROTI ≥ 1 TECU/min disturbances persisted for approximately 1 day after the Dst index recovered from –50 to –20 nT.

Abstract Image

2023年11月4-5日全球电离层对多步磁暴扰动的响应
电离层作为无线电波传播的媒介,对地球空间的干扰仍然高度敏感,在很大程度上决定着通信、导航和雷达系统的准确性和可靠性。在地球-大气-电离层-磁层(EAIM)和太阳-行星际介质-磁层-电离层-大气-地球(SIMMIAE)系统中,最强大的扰动驱动因素是日冕物质抛射。这些事件重构了耦合系统的耦合强度和相互作用动力学,产生时空电离层扰动,降低了卫星和地面技术的性能。这项研究解决了更好地理解全球和局部电离层对强烈的、非平稳的能量输入的响应的需要。通过分析总电子含量指数(ROTI)和全球电子含量(GEC)的时间演变图,研究了一次独特的多阶段磁暴期间的电离层扰动。我们确定了三个连续的GEC最大值:11月4日22:00 UTC约2.20 GECU,随后是11月5日下半月的2.22-2.25 GECU,以及11月6日的深度最小值1.63 GECU。电离层等离子体“饱和-耗竭”周期的振幅为0.62 GECU。在11月4日04:00,在极地地区(60°-75°N)观测到最高的ROTI值(3.8 ~ 4.3 TECU/min),而在同一天00:00,南美洲出现最强的赤道增强值(3.6 TECU/min)。11月5日18:00 ~ 11月6日06:00期间,强扰动(ROTI≥0.9 TECU/min)扩展至±40°地磁纬度,与GEC急剧下降和赤asofu参数(εA≈6.6 TJ/s)峰值一致。在风暴主阶段的第二天,电动力过程(包括SAPS和亚风暴)占主导地位,并在GEC值降低和ROTI活性增强之间产生明显的反相关关系。在Dst指数从-50 nT恢复到-20 nT后,ROTI≥1 TECU/min的扰动持续了约1天。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:604180095
Book学术官方微信
小红书