Bright ultraviolet knots as possible sources of coherent microwave radiation

N. Meshalkina, A. Altyntsev
{"title":"Bright ultraviolet knots as possible sources of coherent microwave radiation","authors":"N. Meshalkina, A. Altyntsev","doi":"10.12737/szf-94202302","DOIUrl":null,"url":null,"abstract":"A distinctive feature of the September 6, 2012 event was that sources of narrow-band (2–4 GHz) sub-second pulses (SSP) were observed in small areas of flare loops with so-called bright ultraviolet knots with high plasma density up to 10¹¹ cm⁻³. Time profiles of hard X-rays of the flare, although similar to microwave light curves, do not have structures corresponding to SSP. Analysis of microwave, X-ray, and ultraviolet data has shown that the observable pulses of microwave radiation with a narrow spectral band are coherent in nature and are generated by electrons with energies of several tens of kiloelectronvolt in bright knots at a double plasma frequency. The results of the observations suggest that the appearance of bright knots is associated with local processes of energy release due to interaction of flare loops.","PeriodicalId":351867,"journal":{"name":"Solnechno-Zemnaya Fizika","volume":"118 17","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2023-12-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Solnechno-Zemnaya Fizika","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.12737/szf-94202302","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

A distinctive feature of the September 6, 2012 event was that sources of narrow-band (2–4 GHz) sub-second pulses (SSP) were observed in small areas of flare loops with so-called bright ultraviolet knots with high plasma density up to 10¹¹ cm⁻³. Time profiles of hard X-rays of the flare, although similar to microwave light curves, do not have structures corresponding to SSP. Analysis of microwave, X-ray, and ultraviolet data has shown that the observable pulses of microwave radiation with a narrow spectral band are coherent in nature and are generated by electrons with energies of several tens of kiloelectronvolt in bright knots at a double plasma frequency. The results of the observations suggest that the appearance of bright knots is associated with local processes of energy release due to interaction of flare loops.
作为相干微波辐射可能来源的明亮紫外线结
2012年9月6日事件的一个显著特点是,在耀斑环路的小区域观测到了窄带(2-4 GHz)亚秒脉冲(SSP)源,这些脉冲具有所谓的明亮紫外线结,等离子体密度高达10¹¹ cm-³。耀斑的硬 X 射线时间曲线虽然与微波光曲线相似,但没有与 SSP 相对应的结构。对微波、X 射线和紫外线数据的分析表明,可观测到的窄频谱带微波辐射脉冲具有相干性,是由亮节中能量为几十千电子伏特的电子以双倍等离子频率产生的。观测结果表明,亮节的出现与耀斑环相互作用导致的局部能量释放过程有关。
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