Flare related geomagnetic storms with coronal mass ejections, radio bursts and jumps in solar wind plasma density

Shiva Soni, Preetam Singh Gour
{"title":"Flare related geomagnetic storms with coronal mass ejections, radio bursts and jumps in solar wind plasma density","authors":"Shiva Soni, Preetam Singh Gour","doi":"10.26671/ijirg.2020.2.10.101","DOIUrl":null,"url":null,"abstract":"In this work we have studied flare related geomagnetic storms of magnitude ≤-90nT during the period of 1997-2012 and analyzed with coronal mass ejections, X-ray solar flares and disturbances in solar wind plasma parameter. We have found total number of flare related geomagnetic storms are 87. Out of 87 geomagnetic storms 67(77.00%) geomagnetic storms are found to be associated with coronal mass ejections (CMEs). Further we observed that 68.66% and 31.34% geomagnetic storms are associated with halo and partial halo CMEs. Statistically there is positive correlation between magnitude of flare related geomagnetic storms and speed of associated CMEs with correlation coefficient 0.28. All the geomagnetic storms have been identified as being associated with X-ray solar flares and 42(48.27 %) flare related geomagnetic storms have been found to be associated with radio bursts of different categories type-II and type-IV. Further we have analyzed those jumps in solar wind plasma density (JSWD) which are associated with flare related geomagnetic storms and see the statistical behavior with CMEs. Positive co-relation has been found between speed of CMEs and peak value of associated JSWD events with coefficient 0.23. Again there is a Positive co-relation with correlation coefficient 0.28 has been found between magnitudes of JSWD events and speed of associated CMEs.","PeriodicalId":118199,"journal":{"name":"International Journal of Innovative Research and Growth","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2021-01-29","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"International Journal of Innovative Research and Growth","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.26671/ijirg.2020.2.10.101","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

Abstract

In this work we have studied flare related geomagnetic storms of magnitude ≤-90nT during the period of 1997-2012 and analyzed with coronal mass ejections, X-ray solar flares and disturbances in solar wind plasma parameter. We have found total number of flare related geomagnetic storms are 87. Out of 87 geomagnetic storms 67(77.00%) geomagnetic storms are found to be associated with coronal mass ejections (CMEs). Further we observed that 68.66% and 31.34% geomagnetic storms are associated with halo and partial halo CMEs. Statistically there is positive correlation between magnitude of flare related geomagnetic storms and speed of associated CMEs with correlation coefficient 0.28. All the geomagnetic storms have been identified as being associated with X-ray solar flares and 42(48.27 %) flare related geomagnetic storms have been found to be associated with radio bursts of different categories type-II and type-IV. Further we have analyzed those jumps in solar wind plasma density (JSWD) which are associated with flare related geomagnetic storms and see the statistical behavior with CMEs. Positive co-relation has been found between speed of CMEs and peak value of associated JSWD events with coefficient 0.23. Again there is a Positive co-relation with correlation coefficient 0.28 has been found between magnitudes of JSWD events and speed of associated CMEs.
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
耀斑相关的地磁风暴与日冕物质抛射,无线电爆发和跳跃在太阳风等离子体密度
本文研究了1997-2012年期间小于-90nT量级的耀斑相关地磁风暴,并对日冕物质抛射、x射线太阳耀斑和太阳风等离子体扰动参数进行了分析。我们发现与耀斑相关的地磁风暴总数为87次。在87个地磁风暴中,有67个(77.00%)地磁风暴被发现与日冕物质抛射(cme)有关。此外,我们还观察到68.66%和31.34%的地磁风暴与日晕和部分日晕cme有关。在统计上,耀斑相关磁暴强度与cme速度呈正相关,相关系数为0.28。所有的地磁风暴都被确定与x射线太阳耀斑有关,42个(48.27%)与耀斑有关的地磁风暴被发现与不同类型的射电暴有关- ii型和iv型。我们进一步分析了与耀斑相关的地磁风暴有关的太阳风等离子体密度(JSWD)的跳跃,并观察了cme的统计行为。日冕物质抛射速度与相关JSWD事件峰值呈显著正相关,相关系数为0.23。JSWD事件的震级与相关日冕物质抛射的速度之间存在正相关关系,相关系数为0.28。
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 去求助
来源期刊
自引率
0.00%
发文量
0
期刊最新文献
Assessment of Micronutrient Deficiencies and their Impact on Maternal Health in Secunderabad Analyzing Global Terrorism Database for Identification of Terrorist Group Geomagnetic Storms in Relation to Magnetic Clouds, Hard X-Ray Solar Flares, and Disturbances in Interplanetary Magnetic Fields During 1996-2008 The generalized K-function and its recurrence relations Fractional calculus and generalized K-function
×
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
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 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 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1