交变电场存在下离子回旋电磁波与高能粒子相互作用的环形分布

IF 0.6 Q4 ASTRONOMY & ASTROPHYSICS Journal of Astronomy and Space Sciences Pub Date : 2022-06-01 DOI:10.5140/jass.2022.39.2.67
K. N. Shukla, J. Kumari, R. S. Pandey
{"title":"交变电场存在下离子回旋电磁波与高能粒子相互作用的环形分布","authors":"K. N. Shukla, J. Kumari, R. S. Pandey","doi":"10.5140/jass.2022.39.2.67","DOIUrl":null,"url":null,"abstract":"The elements that impact the dynamics and collaborations of waves and particles\n in the magnetosphere of planets have been considered here. Saturn’s internal\n magnetosphere is determined by substantiated instabilities and discovered to be an\n exceptional zone of wave activity. Interchanged instability is found to be one of the\n responsible events in view of temperature anisotropy and energization processes of\n magnetospheric species. The generated active ions alongside electrons that constitute\n the populations of highly magnetized planets like Saturn’s ring electron current are\n taken into consideration in the current framework. The previous and similar method of\n characteristics and the perturbed distribution function have been used to derive\n dispersion relation. In incorporating this investigation, the characteristics of\n electromagnetic ion cyclotron wave (EMIC) waves are determined by the composition of\n ions in plasmas through which the waves propagate. The effect of ring distribution\n illustrates non-monotonous description on growth rate (GR) depending upon plasma\n parameters picked out. Observations made by Cassini found appropriate for modern study,\n have been applied to the Kronian magnetosphere. Using Maxwellian ring distribution\n function of ions and detailed mathematical formulation, an expression for dispersion\n relation as well as GR and real frequency (RF) are evaluated. Analysis of plasma\n parameters shows that, proliferating EMIC waves are not developed much when propagation\n is parallelly aligned with magnetosphere as compared to waves propagating in oblique\n direction. GR for the oblique case, is influenced by temperature anisotropy as well as\n by alternating current (AC) frequency, whereas it is much affected only by AC frequency\n for parallel propagating waves.","PeriodicalId":44366,"journal":{"name":"Journal of Astronomy and Space Sciences","volume":null,"pages":null},"PeriodicalIF":0.6000,"publicationDate":"2022-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"Interaction of Ion Cyclotron Electromagnetic Wave with Energetic Particles in the\\n Existence of Alternating Electric Field Using Ring Distribution\",\"authors\":\"K. N. Shukla, J. Kumari, R. S. Pandey\",\"doi\":\"10.5140/jass.2022.39.2.67\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The elements that impact the dynamics and collaborations of waves and particles\\n in the magnetosphere of planets have been considered here. Saturn’s internal\\n magnetosphere is determined by substantiated instabilities and discovered to be an\\n exceptional zone of wave activity. Interchanged instability is found to be one of the\\n responsible events in view of temperature anisotropy and energization processes of\\n magnetospheric species. The generated active ions alongside electrons that constitute\\n the populations of highly magnetized planets like Saturn’s ring electron current are\\n taken into consideration in the current framework. The previous and similar method of\\n characteristics and the perturbed distribution function have been used to derive\\n dispersion relation. In incorporating this investigation, the characteristics of\\n electromagnetic ion cyclotron wave (EMIC) waves are determined by the composition of\\n ions in plasmas through which the waves propagate. The effect of ring distribution\\n illustrates non-monotonous description on growth rate (GR) depending upon plasma\\n parameters picked out. Observations made by Cassini found appropriate for modern study,\\n have been applied to the Kronian magnetosphere. Using Maxwellian ring distribution\\n function of ions and detailed mathematical formulation, an expression for dispersion\\n relation as well as GR and real frequency (RF) are evaluated. Analysis of plasma\\n parameters shows that, proliferating EMIC waves are not developed much when propagation\\n is parallelly aligned with magnetosphere as compared to waves propagating in oblique\\n direction. GR for the oblique case, is influenced by temperature anisotropy as well as\\n by alternating current (AC) frequency, whereas it is much affected only by AC frequency\\n for parallel propagating waves.\",\"PeriodicalId\":44366,\"journal\":{\"name\":\"Journal of Astronomy and Space Sciences\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.6000,\"publicationDate\":\"2022-06-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Astronomy and Space Sciences\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.5140/jass.2022.39.2.67\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Astronomy and Space Sciences","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.5140/jass.2022.39.2.67","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 1

摘要

这里考虑了影响行星磁层中波和粒子的动力学和协同作用的因素。土星的内部磁层是由证实的不稳定性决定的,并被发现是一个特殊的波活动区域。从磁层物质的温度各向异性和能量化过程来看,发现交换不稳定性是导致磁层不稳定的原因之一。在当前的框架中,考虑到产生的活性离子和电子构成了像土星环这样的高磁化行星的电子电流。利用先前和类似的特性法和摄动分布函数推导了色散关系。结合这项研究,电磁离子回旋波(EMIC)波的特性是由等离子体中离子的组成决定的,等离子体通过这些离子传播。环形分布的影响表明,随着选取的等离子体参数的不同,生长速率(GR)呈现非单调的变化。卡西尼号的观测发现适合于现代研究,已应用于克罗尼亚磁层。利用离子的麦克斯韦环分布函数和详细的数学公式,给出了色散关系、GR和实频率(RF)的表达式。对等离子体参数的分析表明,与斜向传播相比,沿磁层平行方向传播时,扩散电磁波的发展程度较低。斜向波的GR受温度各向异性和交流频率的影响,而平行波的GR仅受交流频率的影响。
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
Interaction of Ion Cyclotron Electromagnetic Wave with Energetic Particles in the Existence of Alternating Electric Field Using Ring Distribution
The elements that impact the dynamics and collaborations of waves and particles in the magnetosphere of planets have been considered here. Saturn’s internal magnetosphere is determined by substantiated instabilities and discovered to be an exceptional zone of wave activity. Interchanged instability is found to be one of the responsible events in view of temperature anisotropy and energization processes of magnetospheric species. The generated active ions alongside electrons that constitute the populations of highly magnetized planets like Saturn’s ring electron current are taken into consideration in the current framework. The previous and similar method of characteristics and the perturbed distribution function have been used to derive dispersion relation. In incorporating this investigation, the characteristics of electromagnetic ion cyclotron wave (EMIC) waves are determined by the composition of ions in plasmas through which the waves propagate. The effect of ring distribution illustrates non-monotonous description on growth rate (GR) depending upon plasma parameters picked out. Observations made by Cassini found appropriate for modern study, have been applied to the Kronian magnetosphere. Using Maxwellian ring distribution function of ions and detailed mathematical formulation, an expression for dispersion relation as well as GR and real frequency (RF) are evaluated. Analysis of plasma parameters shows that, proliferating EMIC waves are not developed much when propagation is parallelly aligned with magnetosphere as compared to waves propagating in oblique direction. GR for the oblique case, is influenced by temperature anisotropy as well as by alternating current (AC) frequency, whereas it is much affected only by AC frequency for parallel propagating waves.
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 Astronomy and Space Sciences
Journal of Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
1.30
自引率
20.00%
发文量
0
审稿时长
12 weeks
期刊介绍: JASS aims for the promotion of global awareness and understanding of space science and related applications. Unlike other journals that focus either on space science or on space technologies, it intends to bridge the two communities of space science and technologies, by providing opportunities to exchange ideas and viewpoints in a single journal. Topics suitable for publication in JASS include researches in the following fields: space astronomy, solar physics, magnetospheric and ionospheric physics, cosmic ray, space weather, and planetary sciences; space instrumentation, satellite dynamics, geodesy, spacecraft control, and spacecraft navigation. However, the topics covered by JASS are not restricted to those mentioned above as the journal also encourages submission of research results in all other branches related to space science and technologies. Even though JASS was established on the heritage and achievements of the Korean space science community, it is now open to the worldwide community, while maintaining a high standard as a leading international journal. Hence, it solicits papers from the international community with a vision of global collaboration in the fields of space science and technologies.
期刊最新文献
Structural Design of Planar Synthetic Aperture Radar (SAR) Antenna for Microsatellites Preliminary Characterization of Secondary Illumination at Shackleton Crater Permanently Shadowed Region from ShadowCam Observations and Modeling Search for Dark Photon in e+e− → A′A′ Using Future Collider Experiments Preparation of Contingency Trajectory Operation for the Korea Pathfinder Lunar Orbiter ShadowCam Instrument and Investigation Overview
×
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