Moderate Magnetic Storms on April 28–May 2, 2023

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Kinematics and Physics of Celestial Bodies Pub Date : 2024-12-04 DOI:10.3103/S0884591324060023
L. F. Chernogor, M. Yu. Holub
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Abstract

Magnetic storm, ionospheric storm, atmospheric storm, and electrical storm are the components of a geospace storm resulting from a solar storm. In the literature, the main attention is paid to the analysis of severe and extreme geospace storms. It is these storms that have the greatest impact on the Earth–atmosphere–ionosphere–magnetosphere system. They are most dangerous for space-based and ground-based technological systems. Such storms have a significant impact on human well-being and health. Minor and moderate storms are much less studied than severe and extreme ones. There are good reasons to believe that such storms can have some impact on the systems and people. It is important that the frequency of occurrence of moderate storms is much greater than the frequency of occurrence of severe storms. All this determined the relevance of this work, which consists in the study of magnetic disturbances that arise during moderate geospace storms, which receive undeservedly little attention. The purpose of this paper is to analyze on a global scale the temporal variations of geomagnetic field components during moderate magnetic storms on April 28–29 and May 1–2, 2023. The latitudinal dependence of the geomagnetic field components temporal variations during two moderate magnetic storms in April–May 2023 and on reference days was analyzed on a global scale using the data of the global network of Intermagnet stations. The limits of fluctuations in the level of the geomagnetic field under quiet conditions and during moderate storms were estimated. The range of variations in the geomagnetic field level under quiet conditions decreased from 200–260 to 30–50 nT with decreasing geographic latitude. During the storms, these limits increased 1.3–2.1 times. The variations in the level of components at stations equidistant from the equator were close. This is true for both the Western and Eastern Hemispheres. The fluctuations of the geomagnetic field level at the stations operating approximately at the same latitude but in different hemispheres were also close.

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2023年4月28日至5月2日的中度磁暴
磁暴、电离层风暴、大气风暴和电风暴是由太阳风暴引起的地球空间风暴的组成部分。在文献中,主要关注的是对严重和极端地球空间风暴的分析。正是这些风暴对地球-大气-电离层-磁层系统的影响最大。它们对天基和地面技术系统最为危险。这类风暴对人类福祉和健康产生重大影响。对轻微和中度风暴的研究远远少于对严重和极端风暴的研究。有充分的理由相信,这样的风暴会对系统和人产生一些影响。重要的是,中等风暴的发生频率远远大于强风暴的发生频率。所有这些都决定了这项工作的相关性,这项工作包括对中等地球空间风暴期间产生的磁干扰的研究,这受到了不应有的关注。本文的目的是分析2023年4月28-29日和5月1-2日中磁暴期间地磁场分量在全球尺度上的变化。利用全球磁体台网资料,在全球尺度上分析了2023年4 - 5月两次中磁暴和参考日期间地磁场分量时间变化的纬向依赖性。估计了安静条件下和中等风暴期间地磁场水平波动的极限。安静条件下地磁场水平的变化幅度随着地理纬度的减小而减小,从200-260 ~ 30-50 nT。在风暴期间,这些极限增加了1.3-2.1倍。与赤道等距的各站点的分量水平变化接近。西半球和东半球都是如此。在大致相同纬度但不同半球的台站,地磁场水平的波动也很接近。
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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.
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