黄靖^1,2,,
倪彬彬^1,2,,,
付松¹,
顾旭东^1,2,
曹兴¹,
项正¹,
王琦¹,
罗琼¹,
何颖¹,
闫玲¹,
王敬之¹
1. 武汉大学电子信息学院空间物理系, 武汉 430072
2. 澳门科技大学月球与行星科学实验室-中国科学院月球与深空探测重点实验室伙伴实验室, 澳门 519020

基金项目: 国家自然科学基金（41674163，41574160，41474141，41704162），中国博士后科学基金（2018T110792，2018M632908）与澳门科技大学月球与行星科学实验室-中国科学院月球与深空探测重点实验室伙伴实验室开放课题共同资助


详细信息

作者简介: 黄靖, 女, 1993年生, 硕士研究生, 从事木星磁层动力学与波粒相互作用研究.E-mail:jinghuang123@whu.edu.cn

通讯作者: 倪彬彬, 男, 教授, 主要从事磁层辐射带物理与空间波粒相互作用方面的研究.E-mail:bbni@whu.edu.cn

中图分类号: P353

收稿日期:2018-12-10
修回日期:2019-01-24
上线日期:2019-03-05

Analysis of whistler waves in the Jovian magnetosphere based on data from JUNO WAVES Instrument

HUANG Jing^1,2,,
NI BinBin^1,2,,,
FU Song¹,
GU XuDong^1,2,
CAO Xing¹,
XIANG Zheng¹,
WANG Qi¹,
LUO Qiong¹,
HE Ying¹,
YAN Ling¹,
WANG JingZhi¹
1. Department of Space Physics, School of Electronic Information, Wuhan University, Wuhan 430072, China
2. Lunar and Planetary Science Laboratory, Macau University of Science and Technology-Partner Laboratory of Key Laboratory of Lunar and Deep Space Exploration, Chinese Academy of Sciences, Macau 519020, China


More Information

Corresponding author: NI BinBin,E-mail:bbni@whu.edu.cn

MSC: P353

--> Received Date: 10 December 2018
Revised Date: 24 January 2019
Available Online: 05 March 2019


摘要
摘要:等离子体波的空间分布在木星磁层高能电子动力学过程中起着重要的作用.现有大多数对木星磁层哨声波的观测仅限于|λ|≤ 15°的磁纬范围内，但是最新的JUNO卫星WAVES仪器提供的波动数据使得更高纬度、更广区域范围内的等离子体波动分布研究成为可能.本文通过对JUNO卫星WAVES仪器数据进行分析处理，详细研究了木星磁层哨声波的空间分布特性.观测表明，存在位于高L_J、高磁纬的木星磁层哨声波，它们广泛分布于距木星中心距离35~75个木星半径、磁纬为|λ|≤ 30°的空间区域.分析研究发现，WAVES仪器观测的木星磁层哨声波幅度一般为几个pT，远小于地球磁层哨声波的强度.木星磁层哨声波幅会随着L_J的增大缓慢增加，也会随着磁纬的减小趋向平缓变化.基于以上观测事实，本文利用指数幂函数分别拟合得到木星磁层哨声波幅随L_J和磁纬变化的经验模型.该模型将有助于精确理解哨声波对木星磁层高能电子动力学过程的重要影响.
关键词: 木星磁层/
JUNO卫星/
哨声波/
统计分析

Abstract:Spatial distributions of plasma waves play an essential role in the dynamics of Jovian magnetospheric electrons. Despite that most previous observations of whistler waves in the Jovian magnetosphere are limited to|λ|≤ 15° of the magnetic equator, the data availability from JUNO WAVES instrument provides good opportunity to capture plasma waves over a broader range of latitude and distance. By using the datasets obtained from JUNO WAVES instrument, the spatial distribution features of whistler waves in the Jovian magnetosphere are studied in detail. The observations indicate that whistler waves occur widely in the region between 35~75 R_J (the Jupiter's radius) within 30° of the magnetic equator. The average amplitude of whistler waves in the Jovian magnetosphere is generally at the level of several pT, weaker than that in the terrestrial magnetosphere. Whistler wave intensities at Jupiter are also found to exhibit a tendency of slow increase with increasing L_J and gradual stability with decreasing magnetic latitude. Based on these observational results, we implement fits of exponential power-law function to develop an empirical model of the variation of Jovian whistler wave amplitude with L_J and magnetic latitude, which can be used readily to contribute to improved understanding of the importance of whistler waves to the dynamical variations of high energy electrons in the Jovian magnetosphere.
Key words:Jovian magnetosphere/
JUNO/
Whistler waves/
Statistical analysis



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