ECH与Whistler波相互作用的参数化研究:细胞内粒子模拟

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
Tong Shao, Xinliang Gao, Yangguang Ke, Jiuqi Ma, Wentian Lei, Quanming Lu
{"title":"ECH与Whistler波相互作用的参数化研究:细胞内粒子模拟","authors":"Tong Shao,&nbsp;Xinliang Gao,&nbsp;Yangguang Ke,&nbsp;Jiuqi Ma,&nbsp;Wentian Lei,&nbsp;Quanming Lu","doi":"10.1029/2025JA033980","DOIUrl":null,"url":null,"abstract":"<p>Electron Cyclotron Harmonic (ECH) waves and whistler waves are common plasma waves in the Earth's magnetosphere, and they play an important role in regulating electron dynamics. Recent observations reveal that whistler waves can suppress ECH waves by reshaping the electron distribution, but a comprehensive study on the effects of various plasma parameters on their interplay is still lacking. Using a two-dimensional (2-D) particle-in-cell (PIC) simulation model, we have thoroughly studied the evolution of ECH waves under various initial plasma conditions by relaxing anisotropic hot electrons with a loss-cone distribution. Overall, ECH waves are significantly suppressed once whistler waves appear, and their damping rate is strongly dependent on the amplitude of whistler waves, which is positively correlated with the hot electron proportion and the temperature anisotropy. Moreover, the final amplitude ratio <i>R</i> between ECH and whistler waves tends to increase with a higher hot electron proportion <span></span><math>\n <semantics>\n <mrow>\n <msub>\n <mi>n</mi>\n <mi>h</mi>\n </msub>\n <mo>/</mo>\n <msub>\n <mi>n</mi>\n <mi>e</mi>\n </msub>\n </mrow>\n <annotation> ${n}_{h}/{n}_{e}$</annotation>\n </semantics></math>, lower temperature anisotropy <span></span><math>\n <semantics>\n <mrow>\n <mi>A</mi>\n </mrow>\n <annotation> $A$</annotation>\n </semantics></math>, and higher ratio of plasma frequency to electron cyclotron frequency <span></span><math>\n <semantics>\n <mrow>\n <msub>\n <mi>f</mi>\n <mtext>pe</mtext>\n </msub>\n <mo>/</mo>\n <msub>\n <mi>f</mi>\n <mtext>ce</mtext>\n </msub>\n </mrow>\n <annotation> ${f}_{\\text{pe}}/{f}_{\\text{ce}}$</annotation>\n </semantics></math>. However, it shows little dependence on the size of loss-cone width <span></span><math>\n <semantics>\n <mrow>\n <mi>β</mi>\n </mrow>\n <annotation> $\\beta $</annotation>\n </semantics></math> and parallel temperature <span></span><math>\n <semantics>\n <mrow>\n <msub>\n <mi>T</mi>\n <mo>∥</mo>\n </msub>\n </mrow>\n <annotation> ${T}_{\\mathit{{\\Vert} }}$</annotation>\n </semantics></math>. This study not only supports that the suppression of ECH waves by whistler waves is a common phenomenon but also provides some new insights into understanding the global distribution of ECH waves in the Earth's magnetosphere.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":"130 7","pages":""},"PeriodicalIF":2.9000,"publicationDate":"2025-07-25","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Parametric Study on the Interplay Between ECH and Whistler Waves: Particle-In-Cell Simulations\",\"authors\":\"Tong Shao,&nbsp;Xinliang Gao,&nbsp;Yangguang Ke,&nbsp;Jiuqi Ma,&nbsp;Wentian Lei,&nbsp;Quanming Lu\",\"doi\":\"10.1029/2025JA033980\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>Electron Cyclotron Harmonic (ECH) waves and whistler waves are common plasma waves in the Earth's magnetosphere, and they play an important role in regulating electron dynamics. Recent observations reveal that whistler waves can suppress ECH waves by reshaping the electron distribution, but a comprehensive study on the effects of various plasma parameters on their interplay is still lacking. Using a two-dimensional (2-D) particle-in-cell (PIC) simulation model, we have thoroughly studied the evolution of ECH waves under various initial plasma conditions by relaxing anisotropic hot electrons with a loss-cone distribution. Overall, ECH waves are significantly suppressed once whistler waves appear, and their damping rate is strongly dependent on the amplitude of whistler waves, which is positively correlated with the hot electron proportion and the temperature anisotropy. Moreover, the final amplitude ratio <i>R</i> between ECH and whistler waves tends to increase with a higher hot electron proportion <span></span><math>\\n <semantics>\\n <mrow>\\n <msub>\\n <mi>n</mi>\\n <mi>h</mi>\\n </msub>\\n <mo>/</mo>\\n <msub>\\n <mi>n</mi>\\n <mi>e</mi>\\n </msub>\\n </mrow>\\n <annotation> ${n}_{h}/{n}_{e}$</annotation>\\n </semantics></math>, lower temperature anisotropy <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>A</mi>\\n </mrow>\\n <annotation> $A$</annotation>\\n </semantics></math>, and higher ratio of plasma frequency to electron cyclotron frequency <span></span><math>\\n <semantics>\\n <mrow>\\n <msub>\\n <mi>f</mi>\\n <mtext>pe</mtext>\\n </msub>\\n <mo>/</mo>\\n <msub>\\n <mi>f</mi>\\n <mtext>ce</mtext>\\n </msub>\\n </mrow>\\n <annotation> ${f}_{\\\\text{pe}}/{f}_{\\\\text{ce}}$</annotation>\\n </semantics></math>. However, it shows little dependence on the size of loss-cone width <span></span><math>\\n <semantics>\\n <mrow>\\n <mi>β</mi>\\n </mrow>\\n <annotation> $\\\\beta $</annotation>\\n </semantics></math> and parallel temperature <span></span><math>\\n <semantics>\\n <mrow>\\n <msub>\\n <mi>T</mi>\\n <mo>∥</mo>\\n </msub>\\n </mrow>\\n <annotation> ${T}_{\\\\mathit{{\\\\Vert} }}$</annotation>\\n </semantics></math>. This study not only supports that the suppression of ECH waves by whistler waves is a common phenomenon but also provides some new insights into understanding the global distribution of ECH waves in the Earth's magnetosphere.</p>\",\"PeriodicalId\":15894,\"journal\":{\"name\":\"Journal of Geophysical Research: Space Physics\",\"volume\":\"130 7\",\"pages\":\"\"},\"PeriodicalIF\":2.9000,\"publicationDate\":\"2025-07-25\",\"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/10.1029/2025JA033980\",\"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/10.1029/2025JA033980","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

电子回旋谐波(ECH)波和哨声波是地球磁层中常见的等离子体波,它们在电子动力学中起着重要的调节作用。近年来的观测表明,哨声波可以通过重塑电子分布来抑制ECH波,但对各种等离子体参数对其相互作用的影响还缺乏全面的研究。利用二维(2-D)粒子池(PIC)模拟模型,我们深入研究了各向异性热电子在不同初始等离子体条件下具有损失锥分布的ECH波的演化。总体而言,当哨声波出现时,ECH波被显著抑制,其衰减率与哨声波的振幅密切相关,且与热电子比例和温度各向异性呈正相关。随着热电子比n h / n e ${n}_{h}}/{n}_{e}$的增大,终振幅比R随热电子比n h / n e}$的增大而增大。较低的温度各向异性A$ A$,较高的等离子体频率/电子回旋频率f pe / f ce ${f}_{\text{pe}}/{f}_{\text{ce}}$。然而,它对损失锥宽度的大小β $\beta $和平行温度T∥${T}_{\mathit{{\Vert}}}$的依赖不大。该研究不仅支持了哨声波对高强电磁波的抑制是一种普遍现象,而且为理解地球磁层中高强电磁波的全球分布提供了一些新的见解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Parametric Study on the Interplay Between ECH and Whistler Waves: Particle-In-Cell Simulations

Electron Cyclotron Harmonic (ECH) waves and whistler waves are common plasma waves in the Earth's magnetosphere, and they play an important role in regulating electron dynamics. Recent observations reveal that whistler waves can suppress ECH waves by reshaping the electron distribution, but a comprehensive study on the effects of various plasma parameters on their interplay is still lacking. Using a two-dimensional (2-D) particle-in-cell (PIC) simulation model, we have thoroughly studied the evolution of ECH waves under various initial plasma conditions by relaxing anisotropic hot electrons with a loss-cone distribution. Overall, ECH waves are significantly suppressed once whistler waves appear, and their damping rate is strongly dependent on the amplitude of whistler waves, which is positively correlated with the hot electron proportion and the temperature anisotropy. Moreover, the final amplitude ratio R between ECH and whistler waves tends to increase with a higher hot electron proportion n h / n e ${n}_{h}/{n}_{e}$ , lower temperature anisotropy A $A$ , and higher ratio of plasma frequency to electron cyclotron frequency f pe / f ce ${f}_{\text{pe}}/{f}_{\text{ce}}$ . However, it shows little dependence on the size of loss-cone width β $\beta $ and parallel temperature T ${T}_{\mathit{{\Vert} }}$ . This study not only supports that the suppression of ECH waves by whistler waves is a common phenomenon but also provides some new insights into understanding the global distribution of ECH waves in the Earth's magnetosphere.

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
×
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