磁暴恢复相后期超低频波观测分析

魏超; 戴磊

doi:10.11728/cjss2020.04.479

磁暴恢复相后期超低频波观测分析

doi: 10.11728/cjss2020.04.479

魏超^1,2,
戴磊¹

1. 中国科学院国家空间科学中心北京 100190;
2. 中国科学院大学北京 100049

基金项目:

国家自然科学基金项目（41874175，41574161，41731070，41574159）和中国科学院空间科学先导专项（二期）项目（XDA15052500，XDA15350201）共同资助

详细信息

作者简介:
魏超,E-mail:weichaojl@126.com

中图分类号: P353
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- 被引次数: 0
出版历程
- 收稿日期: 2019-04-09
- 修回日期: 2019-10-15
- 刊出日期: 2020-07-15

Observations of ULF Waves at the Late Recovery Phase of Magnetic Storm

WEI Chao^1,2,
DAI Lei¹

1 National Space Science Center, Chinese Academy of Sciences, Beijing 100190;
2 University of Chinese Academy of Sciences, Beijing 100049

摘要

摘要: 利用Radiation Belt Storm Probes（RBSP）和Magnetospheric Multiscale（MMS）的联合观测研究了2016年1月25日和2月22日的两个超低频（ULF）波动事件.这两个事件均发生在磁暴的恢复相后期，波动分布在晨侧与正午之间的区域.RBSP观测到的两次波动都发生在低L-shell（4.7～5.8），MMS观测到的两次波动都发生在高L-shell（8.0～14.2）.在高L-shell，超低频波偏振以环向波为主，沿磁力线方向为基频谐波.在低L-shell，超低频波偏振以径向波为主，沿磁力线方向为二次谐波.对内磁层（L<6）中的ULF波，通过比较∂f/∂w|μ,L和（dL）/（dW）（∂f）/（∂L）|μ,W的绝对值可知，bump-on-tail的离子分布和向地的离子相空间密度梯度通过N=1的弹跳共振，共同为波动的产生提供自由能.多重事例分析表明，在磁暴恢复相后期，约10keV的离子伴随着波动的存在而存在，并且为波动的产生提供自由能.
- 超低频波 /
- 空间分布 /
- Bump-on-tail /
- 密度梯度
Abstract: Two ULF wave events on 25 Jan. and 22 Feb. 2016 are studied by using the combined observations of Radiation Belt Storm Probes (RBSP) and Magnetospheric Multiscale (MMS). Both events occurred in the late recovery phase of the magnetic storm, and both fluctuations occurred in the area between morning and noon. The two events observed by RBSP occurred in the low L-shell (4.7~5.8), and the two events observed by MMS occurred in the high L-shell (8.0~14.2). In the high L-shell, the ULF wave is dominated by toroidal mode, and it is the first harmonic along the field line. In the low L-shell, the ULF wave is dominated by the poloidal wave, and it is the second harmonic along the field line. In addition, by comparing the absolute values of ∂f/∂w|μ,L and （dL）/（dW）（∂f）/（∂L）|μ,W, the bump-on-tail ion distribution and inward gradient of ion phase space density together provide free energy for the wave through N=1 bounce resonance. According to the analysis of these two cases, about 10keV ions exist with the waves and provide free energy for the generation of waves at the late recovery phase of the magnetic storm.
- ULF waves /
- Spatial distribution /
- Bump-on-tail /
- Gradient of density

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