Electron acceleration behind a wavy dipolarization front

被引:0
作者
Mingyu Wu
Quanming Lu
Martin Volwerk
Rumi Nakamura
Tielong Zhang
机构
[1] Harbin Institute of Technology,CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Science
[2] University of Science and Technology of China,Space Research Institute
[3] Austrian Academy of Science,undefined
来源
Astrophysics and Space Science | 2018年 / 363卷
关键词
Dipolarization front; Electron acceleration; Betatron acceleration;
D O I
暂无
中图分类号
学科分类号
摘要
In this paper, with the in-situ observations from the Time History of Events and Macroscale Interactions during Substorms (THEMIS) probes we report a wavy dipolarization front (DF) event, where the DF has different magnetic structures and electron distributions at different y\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$y$\end{document} positions in the Geocentric Solar Magnetospheric (GSM) coordinates. At y∼2.1RE\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$y \sim2.1R_{E}$\end{document} (RE\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$R_{E}$\end{document} is the radius of Earth), the DF has a relatively simple structure, which is similar to that of a conventional DF. At y∼3.0RE\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$y \sim3.0R_{E}$\end{document}, the DF is revealed to have a multiple DF structure, where the plasma exhibits a vortex flow. Such a wavy DF could be the results of the interchange instability. The different structure of such a wavy DF at different sites has a great effect on electron acceleration. Fermi acceleration can occur at the site of the DF with a simple or multiple DF structure, while betatron acceleration as a local process has the contribution to energetic electrons only at the site of the DF with a simple structure.
引用
收藏
相关论文
共 61 条
[1]  
Angelopoulos V.(2008)undefined Space Sci. Rev. 141 5-34
[2]  
Angelopoulos V.(1992)undefined J. Geophys. Res. 97 4027-365
[3]  
Ashour-Abdalla M.(2011)undefined Nat. Phys. 7 360-264
[4]  
Auster H.U.(2008)undefined Space Sci. Rev. 141 235-3616
[5]  
Birn J.(2011)undefined J. Geophys. Res. 116 3604-6027
[6]  
Nakamura R.(2014)undefined J. Geophys. Res. Space Phys. 119 6023-1765
[7]  
Panov E.V.(2011)undefined Geophys. Res. Lett. 38 1759-2530
[8]  
Hesse M.(2013)undefined Geophys. Res. Lett. 40 22-6025
[9]  
Birn J.(2010)undefined Geophys. Res. Lett. 37 2516-10,105
[10]  
Runov A.(2015)undefined J. Geophys. Res. Space Phys. 120 6019-6300