中文版 | English
题名

Formation of Electron Butterfly Pitch Angle Distributions in Saturn's Magnetosphere Due To Scattering by Equatorial ECH Waves

作者
通讯作者Cao, Xing; Ni, Binbin
发表日期
2023-10-16
DOI
发表期刊
ISSN
0094-8276
EISSN
1944-8007
卷号50期号:19
摘要
["The features of electron pitch angle distributions (PADs) often imply different physical mechanisms in planetary magnetospheres. We report a simultaneous equatorial electrostatic electron cyclotron harmonic (ECH) wave event with butterfly PADs of electrons at L similar to 7.6-9 observed by the Cassini spacecraft. Via calculating the bounce-averaged electron diffusion rates, we found that Saturnian ECH waves can resonate with similar to 10 eV to several keV electrons at <60 degrees pitch angles at time scales from similar to 10 (-8) to 10(-4) s(-1). Simulations show that the formation of similar to 100 eV to similar to 1 keV electron butterfly PADs are mainly caused by the pitch angle scattering of electrons at low pitch angles (<30 degrees) and the momentum scattering at intermediate pitch angles of similar to 30 degrees-45 degrees, though previous studies suggested the adiabatic transport is the dominated mechanism. Additionally, our results successfully reproduce the variation of peak pitch angles (alpha(p)) and phase space density ratios between alpha(90 degrees) and alpha(p) with L-shell.","Plain Language Summary Charged particles present different pitch angle distributions (PADs) due to different physical mechanisms in Saturn's magnetosphere. Butterfly PADs have local minimum at similar to 90 degrees pitch angle, which are commonly observed in Saturn's magnetosphere for electrons over a wide energy range from similar to 100 eV to several MeV. Previous studies proposed that the adiabatic transport dominates the transformation from the electron field-aligned PADs of similar to 100 eV-several keV to the butterfly shapes in Saturn's magnetosphere. In our study, we report a simultaneous electrostatic electron cyclotron harmonic (ECH) wave event with the butterfly PADs of electrons at L similar to 7.6-9 observed by the Cassini spacecraft. Via calculating the bounce-averaged electron diffusion rates of ECH waves and simulating the evolution of electron phase space densities (PSDs), we find that the formation of similar to 100 eV to similar to 1 keV electron butterfly PADs is mainly caused by the scattering of electrons induced by ECH waves. Our simulation results successfully reproduce the variation of peak pitch angle (alpha(p)) and PSD ratios between alpha(90 degrees) and alpha(p) with L-shell. These results would improve the current understanding of the electron dynamics in Saturn's magnetosphere and shed light on understanding the plasma environment of the outer planets and exoplanets."]
关键词
相关链接[来源记录]
收录类别
SCI ; EI
语种
英语
重要成果
NI论文
学校署名
其他
资助项目
This work was supported by the NSFC Grants 42188101, 42025404, and 42241143, the B-type Strategic Priority Program of the Chinese Academy of Sciences (Grant XDB41000000), the National Key Ramp;D Program of China (2022YFF0503700 and 2022YFF0503900), the Fu["42188101","42025404","42241143"] ; NSFC[XDB41000000] ; B-type Strategic Priority Program of the Chinese Academy of Sciences["2022YFF0503700","2022YFF0503900"] ; National Key Ramp;D Program of China[2042022kf1012]
WOS研究方向
Geology
WOS类目
Geosciences, Multidisciplinary
WOS记录号
WOS:001074653600001
出版者
EI入藏号
20234114871484
EI主题词
Cyclotrons ; Magnetosphere ; Phase space methods ; Planets
EI分类号
Atmospheric Properties:443.1 ; Extraterrestrial Physics and Stellar Phenomena:657.2 ; Magnetism: Basic Concepts and Phenomena:701.2 ; Mathematics:921 ; Particle Accelerators:932.1.1
ESI学科分类
GEOSCIENCES
来源库
Web of Science
引用统计
成果类型期刊论文
条目标识符http://sustech.caswiz.com/handle/2SGJ60CL/583008
专题理学院_地球与空间科学系
作者单位
1.Wuhan Univ, Sch Elect Informat, Dept Space Phys, Wuhan, Peoples R China
2.CAS Ctr Excellence Comparat Planetol, Hefei, Peoples R China
3.Harbin Inst Technol, Inst Space Sci & Appl Technol, Shenzhen, Peoples R China
4.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
5.Max Planck Inst Solar Syst Res, Gottingen, Germany
6.Univ Hong Kong, Dept Earth Sci, Hong Kong, Peoples R China
7.Southern Univ Sci & Technol, Dept Earth & Space Sci, Shenzhen, Peoples R China
推荐引用方式
GB/T 7714
Long, Minyi,Cao, Xing,Ni, Binbin,et al. Formation of Electron Butterfly Pitch Angle Distributions in Saturn's Magnetosphere Due To Scattering by Equatorial ECH Waves[J]. GEOPHYSICAL RESEARCH LETTERS,2023,50(19).
APA
Long, Minyi.,Cao, Xing.,Ni, Binbin.,Lou, Yuequn.,Yao, Zhonghua.,...&Wu, Siyuan.(2023).Formation of Electron Butterfly Pitch Angle Distributions in Saturn's Magnetosphere Due To Scattering by Equatorial ECH Waves.GEOPHYSICAL RESEARCH LETTERS,50(19).
MLA
Long, Minyi,et al."Formation of Electron Butterfly Pitch Angle Distributions in Saturn's Magnetosphere Due To Scattering by Equatorial ECH Waves".GEOPHYSICAL RESEARCH LETTERS 50.19(2023).
条目包含的文件
条目无相关文件。
个性服务
原文链接
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
导出为Excel格式
导出为Csv格式
Altmetrics Score
谷歌学术
谷歌学术中相似的文章
[Long, Minyi]的文章
[Cao, Xing]的文章
[Ni, Binbin]的文章
百度学术
百度学术中相似的文章
[Long, Minyi]的文章
[Cao, Xing]的文章
[Ni, Binbin]的文章
必应学术
必应学术中相似的文章
[Long, Minyi]的文章
[Cao, Xing]的文章
[Ni, Binbin]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
[发表评论/异议/意见]
暂无评论

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。