{"title":"2024年5月10-13日电离层F区一次独特地球空间风暴的全球表现","authors":"L. F. Chernogor, V. O. Bessarabova","doi":"10.3103/S0884591325050022","DOIUrl":null,"url":null,"abstract":"<p>Powerful transient processes on the Sun lead to solar storms and to geospace storms on Earth. Ionospheric storms are an integral part of geospace storms; they are extreme manifestations of ionospheric weather. Its variations have a significant impact on the functioning of civilization. It has been established that the manifestations of storms significantly depend not only on the characteristics of solar and geospace storms but also on the season, time of day, magnetic and geographical coordinates, etc. All this determines the relevance of studying each new ionospheric storm, especially when it comes to unique events. The purpose of this work is to study the features of the global manifestation of a unique geospace storm on May 10–13, 2024, in the F region of the ionosphere. The main features of the global manifestation of a unique geospace storm on May 10–13, 2024, in the F region of the ionosphere have been studied. The largest negative disturbances were observed on May 11, 2024, during the recovery phase of the geomagnetic storm. At most stations, the storm was strong or severe during the daytime. At night, manifestations of strong, severe, and extreme storms were mainly observed. The storm of May 13, 2024, was less intense compared to the storm of May 11, 2024. During the daytime, it was minor and moderate, while it was mainly strong and even severe at night. Negative and positive ionospheric storms sometimes replaced each other. Positive ionospheric storms were weaker. The duration of the blackout tended to decrease with decreasing geographical latitude of the station.</p>","PeriodicalId":681,"journal":{"name":"Kinematics and Physics of Celestial Bodies","volume":"41 5","pages":"209 - 220"},"PeriodicalIF":0.7000,"publicationDate":"2025-09-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Global Manifestations of a Unique Geospace Storm on May 10–13, 2024, in the F Region of the Ionosphere\",\"authors\":\"L. F. Chernogor, V. O. Bessarabova\",\"doi\":\"10.3103/S0884591325050022\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Powerful transient processes on the Sun lead to solar storms and to geospace storms on Earth. Ionospheric storms are an integral part of geospace storms; they are extreme manifestations of ionospheric weather. Its variations have a significant impact on the functioning of civilization. It has been established that the manifestations of storms significantly depend not only on the characteristics of solar and geospace storms but also on the season, time of day, magnetic and geographical coordinates, etc. All this determines the relevance of studying each new ionospheric storm, especially when it comes to unique events. The purpose of this work is to study the features of the global manifestation of a unique geospace storm on May 10–13, 2024, in the F region of the ionosphere. The main features of the global manifestation of a unique geospace storm on May 10–13, 2024, in the F region of the ionosphere have been studied. The largest negative disturbances were observed on May 11, 2024, during the recovery phase of the geomagnetic storm. At most stations, the storm was strong or severe during the daytime. At night, manifestations of strong, severe, and extreme storms were mainly observed. The storm of May 13, 2024, was less intense compared to the storm of May 11, 2024. During the daytime, it was minor and moderate, while it was mainly strong and even severe at night. Negative and positive ionospheric storms sometimes replaced each other. Positive ionospheric storms were weaker. The duration of the blackout tended to decrease with decreasing geographical latitude of the station.</p>\",\"PeriodicalId\":681,\"journal\":{\"name\":\"Kinematics and Physics of Celestial Bodies\",\"volume\":\"41 5\",\"pages\":\"209 - 220\"},\"PeriodicalIF\":0.7000,\"publicationDate\":\"2025-09-08\",\"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/S0884591325050022\",\"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}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Kinematics and Physics of Celestial Bodies","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.3103/S0884591325050022","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}
Global Manifestations of a Unique Geospace Storm on May 10–13, 2024, in the F Region of the Ionosphere
Powerful transient processes on the Sun lead to solar storms and to geospace storms on Earth. Ionospheric storms are an integral part of geospace storms; they are extreme manifestations of ionospheric weather. Its variations have a significant impact on the functioning of civilization. It has been established that the manifestations of storms significantly depend not only on the characteristics of solar and geospace storms but also on the season, time of day, magnetic and geographical coordinates, etc. All this determines the relevance of studying each new ionospheric storm, especially when it comes to unique events. The purpose of this work is to study the features of the global manifestation of a unique geospace storm on May 10–13, 2024, in the F region of the ionosphere. The main features of the global manifestation of a unique geospace storm on May 10–13, 2024, in the F region of the ionosphere have been studied. The largest negative disturbances were observed on May 11, 2024, during the recovery phase of the geomagnetic storm. At most stations, the storm was strong or severe during the daytime. At night, manifestations of strong, severe, and extreme storms were mainly observed. The storm of May 13, 2024, was less intense compared to the storm of May 11, 2024. During the daytime, it was minor and moderate, while it was mainly strong and even severe at night. Negative and positive ionospheric storms sometimes replaced each other. Positive ionospheric storms were weaker. The duration of the blackout tended to decrease with decreasing geographical latitude of the station.
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.