{"title":"Global Ionospheric Response to Disturbances during Multistep Magnetic Storm on November 4–5, 2023","authors":"L. F. Chernogor, 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.
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.