通过磁偶中质子的漂移-反弹共振激发二次谐波极坐标超低频波

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2024-11-21 DOI:10.1029/2024JA032804
Yan Zhuang, Chao Yue, Li Li, Xu-Zhi Zhou, Qiu-Gang Zong, Shan Wang, Ying Liu, Xing-Yu Li, Ze-Fan Yin, Yong-Fu Wang, Zhi-Yang Liu, Haobo Fu
{"title":"通过磁偶中质子的漂移-反弹共振激发二次谐波极坐标超低频波","authors":"Yan Zhuang,&nbsp;Chao Yue,&nbsp;Li Li,&nbsp;Xu-Zhi Zhou,&nbsp;Qiu-Gang Zong,&nbsp;Shan Wang,&nbsp;Ying Liu,&nbsp;Xing-Yu Li,&nbsp;Ze-Fan Yin,&nbsp;Yong-Fu Wang,&nbsp;Zhi-Yang Liu,&nbsp;Haobo Fu","doi":"10.1029/2024JA032804","DOIUrl":null,"url":null,"abstract":"<p>The drift-bounce resonance between ultralow-frequency (ULF) waves and charged particles is an efficient way to transfer energy. In this study, we report the excitation of ULF waves through drift-bounce resonance with protons in the magnetic dip for the first time. On 4 September 2015, Van Allen probe B observed ULF signals with a frequency of ∼10 mHz inside the magnetic dip during substorms at the dusk side. The ULF waves are further diagnosed as second harmonic poloidal waves. The 54–67 keV protons in the magnetic dip exhibit oscillations with the same period as ULF waves, providing evidence for drift-bounce resonance. Through finite Larmor radius effects, we determined that the ULF waves propagate eastward with an azimuthal wave number in the range of 237–277. The ULF waves are excited with free energy related to the enhanced proton phase space density in the magnetic dip.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"129 11","pages":""},"PeriodicalIF":2.6000,"publicationDate":"2024-11-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"The Excitation of Second Harmonic Poloidal ULF Waves Through Drift-Bounce Resonance With Protons in the Magnetic Dip\",\"authors\":\"Yan Zhuang,&nbsp;Chao Yue,&nbsp;Li Li,&nbsp;Xu-Zhi Zhou,&nbsp;Qiu-Gang Zong,&nbsp;Shan Wang,&nbsp;Ying Liu,&nbsp;Xing-Yu Li,&nbsp;Ze-Fan Yin,&nbsp;Yong-Fu Wang,&nbsp;Zhi-Yang Liu,&nbsp;Haobo Fu\",\"doi\":\"10.1029/2024JA032804\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>The drift-bounce resonance between ultralow-frequency (ULF) waves and charged particles is an efficient way to transfer energy. In this study, we report the excitation of ULF waves through drift-bounce resonance with protons in the magnetic dip for the first time. On 4 September 2015, Van Allen probe B observed ULF signals with a frequency of ∼10 mHz inside the magnetic dip during substorms at the dusk side. The ULF waves are further diagnosed as second harmonic poloidal waves. The 54–67 keV protons in the magnetic dip exhibit oscillations with the same period as ULF waves, providing evidence for drift-bounce resonance. Through finite Larmor radius effects, we determined that the ULF waves propagate eastward with an azimuthal wave number in the range of 237–277. The ULF waves are excited with free energy related to the enhanced proton phase space density in the magnetic dip.</p>\",\"PeriodicalId\":15894,\"journal\":{\"name\":\"Journal of Geophysical Research: Space Physics\",\"volume\":\"129 11\",\"pages\":\"\"},\"PeriodicalIF\":2.6000,\"publicationDate\":\"2024-11-21\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Geophysical Research: Space Physics\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://onlinelibrary.wiley.com/doi/10.1029/2024JA032804\",\"RegionNum\":2,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JA032804","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

摘要

超低频(ULF)波与带电粒子之间的漂移-反弹共振是一种有效的能量传递方式。在这项研究中,我们首次报告了超低频波通过与磁偶中的质子发生漂跳共振而被激发的情况。2015年9月4日,范艾伦探测器B在黄昏侧的亚暴期间,在磁偶内部观测到频率为10 mHz的超低频信号。超低频波被进一步诊断为二次谐波极性波。磁偶中 54-67 千伏的质子表现出与超低频波相同周期的振荡,为漂移-反弹共振提供了证据。通过有限拉莫尔半径效应,我们确定超低频波以方位角波数 237-277 的范围向东传播。超低频波被激发的自由能与磁倾角中增强的质子相空间密度有关。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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
The Excitation of Second Harmonic Poloidal ULF Waves Through Drift-Bounce Resonance With Protons in the Magnetic Dip

The drift-bounce resonance between ultralow-frequency (ULF) waves and charged particles is an efficient way to transfer energy. In this study, we report the excitation of ULF waves through drift-bounce resonance with protons in the magnetic dip for the first time. On 4 September 2015, Van Allen probe B observed ULF signals with a frequency of ∼10 mHz inside the magnetic dip during substorms at the dusk side. The ULF waves are further diagnosed as second harmonic poloidal waves. The 54–67 keV protons in the magnetic dip exhibit oscillations with the same period as ULF waves, providing evidence for drift-bounce resonance. Through finite Larmor radius effects, we determined that the ULF waves propagate eastward with an azimuthal wave number in the range of 237–277. The ULF waves are excited with free energy related to the enhanced proton phase space density in the magnetic dip.

求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
期刊最新文献
The Excitation of Second Harmonic Poloidal ULF Waves Through Drift-Bounce Resonance With Protons in the Magnetic Dip GOES-R Series X-Ray Sensor (XRS): 1. Design and Pre-Flight Calibration First Meteor Radar Observations of Gravity Waves in the Mesosphere and Lower Thermosphere Over Yinchuan (38.8°N, 106.8°E), China Influence of Lower Atmospheric Variability: An Investigation of Delayed Ionospheric Response to Solar Activity Direction Finding Studies of Simultaneous Auroral 2fce and 3fce Roar Cyclotron Harmonic Radio Emissions
×
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