Dynamic processes in the ionosphere during magnetic storms from the Kharkov incoherent scatter radar observations

L. Chernogor, Y. Grigorenko, V. Lysenko, V. Taran
{"title":"Dynamic processes in the ionosphere during magnetic storms from the Kharkov incoherent scatter radar observations","authors":"L. Chernogor, Y. Grigorenko, V. Lysenko, V. Taran","doi":"10.1029/2005GI000125","DOIUrl":null,"url":null,"abstract":"[1] Results of studying the ionosphere behavior during several magnetic storms of various intensities are presented. The features of pronounced negative ionospheric disturbances accompanying the severe magnetic storms on 25 September 1998 and 29‐30 May 2003 (Kp 8) are considered. Among them there are a decrease in the electron density by a factor of 3‐4, uplifting of the ionospheric F2 layer by 100‐160 km, increase in the temperature of the charged and neutral atmospheric components, and infringement of plasma transfer processes and thermal balance in the ionosphere‐plasmasphere system. In the morning of 25 September 1998, an unusual increase in the upward plasma drift velocity was registered. On 29‐30 May 2003 during the storm main phase, a depletion of the relative density of hydrogen ions by more than an order of magnitude was observed that could manifest an emptying of the magnetic flux tube over Kharkov. These eects are explained in terms of thermospheric disturbances, Joule heating, particle precipitation, penetration of magnetospheric electric fields to midlatitudes, the shift of the main ionospheric trough and related structures toward the radar latitude, etc. The ionospheric storm on 20‐21 March 2003 had two phases. Its strong negative phase proceeded against a background of a minor geomagnetic disturbance (Kp 5). The destabilizing impact of the electric field pulse and traveling atmospheric disturbance generated by magnetospheric substorms could be the cause of the change in the storm phase that occurred in the sunset period. INDEX TERMS: 2431 Ionosphere: Ionosphere/magnetosphere interactions; 2788 Magnetospheric Physics: Magnetic storms and substorms; 6969 Radio Science: Remote sensing; KEYWORDS: ionosphere; magnetic storms; incoherent scatter radar observations.","PeriodicalId":135868,"journal":{"name":"International Journal of Geomagnetism and Aeronomy","volume":"40 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2007-10-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"12","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"International Journal of Geomagnetism and Aeronomy","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1029/2005GI000125","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 12

Abstract

[1] Results of studying the ionosphere behavior during several magnetic storms of various intensities are presented. The features of pronounced negative ionospheric disturbances accompanying the severe magnetic storms on 25 September 1998 and 29‐30 May 2003 (Kp 8) are considered. Among them there are a decrease in the electron density by a factor of 3‐4, uplifting of the ionospheric F2 layer by 100‐160 km, increase in the temperature of the charged and neutral atmospheric components, and infringement of plasma transfer processes and thermal balance in the ionosphere‐plasmasphere system. In the morning of 25 September 1998, an unusual increase in the upward plasma drift velocity was registered. On 29‐30 May 2003 during the storm main phase, a depletion of the relative density of hydrogen ions by more than an order of magnitude was observed that could manifest an emptying of the magnetic flux tube over Kharkov. These eects are explained in terms of thermospheric disturbances, Joule heating, particle precipitation, penetration of magnetospheric electric fields to midlatitudes, the shift of the main ionospheric trough and related structures toward the radar latitude, etc. The ionospheric storm on 20‐21 March 2003 had two phases. Its strong negative phase proceeded against a background of a minor geomagnetic disturbance (Kp 5). The destabilizing impact of the electric field pulse and traveling atmospheric disturbance generated by magnetospheric substorms could be the cause of the change in the storm phase that occurred in the sunset period. INDEX TERMS: 2431 Ionosphere: Ionosphere/magnetosphere interactions; 2788 Magnetospheric Physics: Magnetic storms and substorms; 6969 Radio Science: Remote sensing; KEYWORDS: ionosphere; magnetic storms; incoherent scatter radar observations.
哈尔科夫非相干散射雷达观测磁暴期间电离层的动态过程
[1]本文介绍了几次不同强度磁暴期间电离层行为的研究结果。考虑了1998年9月25日和2003年5月29 ~ 30日的强磁暴(Kp 8)所伴随的电离层显著负扰动特征。其中,电子密度下降了3 - 4倍,电离层F2层上升了100 - 160 km,带电和中性大气成分温度升高,电离层-等离子体层系统的等离子体传递过程和热平衡受到破坏。1998年9月25日上午,观测到等离子体向上漂移速度异常增加。2003年5月29日至30日,在风暴主阶段,观测到氢离子的相对密度下降了一个数量级以上,这可能表明哈尔科夫上空的磁通量管被清空。这些效应可以从热层扰动、焦耳加热、粒子降水、磁层电场向中纬度的渗透、电离层主槽和相关结构向雷达纬度的移动等方面加以解释。2003年3月20 ~ 21日的电离层风暴有两个阶段。它的强负相位是在一个较小的地磁扰动(Kp 5)的背景下进行的。磁场脉冲的不稳定影响和磁层亚暴产生的行进大气扰动可能是日落期间发生的风暴相位变化的原因。索引项:2431电离层:电离层/磁层相互作用;2788磁层物理:磁暴和亚暴;无线电科学:遥感;关键词:电离层;磁性风暴;非相干散射雷达观测。
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
自引率
0.00%
发文量
0
×
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