Hemispheric asymmetry in the near-Venusian magnetotail during solar maximum

S. D. Xiao; T. L. Zhang; W. Baumjohann

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Hemispheric asymmetry in the near-Venusian magnetotail during solar maximum

机译：near-Venusian半球不对称磁尾在太阳能最大

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摘要

During solar minimum the near-Venusian magnetotail exhibits a hemispheric asymmetry in the cross-tail field distribution. It implies that the magnetic field lines in the -E hemisphere are wrapped more tightly around Venus than in the +E hemisphere. Therefore, a strong field reversal region occurs in the magnetotail, which is prone to the magnetic reconnection. Since the Venus magnetotail is formed due to the solar wind interaction with the ionosphere and the ionosphere is modulated by the solar activity, it is interesting to study the solar cycle dependence of the induced magnetosphere. Here we statistically examine the Venus Express magnetotail data during solar maximum. We find that the magnetic field configuration asymmetry in Venus magnetotail is very much similar to that during solar minimum. The hemispheric asymmetry in the magnetotail persists through the whole solar cycle and magnetic reconnection in the near-Venusian magnetotail might occur during solar minimum as well as solar maximum conditions.

机译：在太阳活动极小期near-Venusian磁尾展品的半球不对称cross-tail场分布。的磁场线- e半球包裹得更紧金星比+ E半球。地区发生在磁尾,倾向磁重联。由于太阳风磁尾形成与电离层和交互电离层是太阳活动的调制,它有趣的是研究太阳活动周期依赖的感应磁场。统计检查金星快车在太阳能最大磁尾的数据。的磁场不对称配置在金星磁尾非常相似在太阳能最低。通过整个磁尾的存在太阳周期中磁场重联near-Venusian磁尾期间可能发生太阳活动极小期以及太阳能最大条件。

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《Journal of Geophysical Research, A. Space Physics: JGR》 |2016年第5期|4542-4547|共6页
作者
S. D. Xiao; T. L. Zhang; W. Baumjohann;
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作者单位

Space Research Institute, Austrian Academy of Sciences, Graz, Austria;

CAS Key Laboratory of Geospace Environment, University of Science and Technology of China, Hefei, China;

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正文语种英语
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关键词
MAGNETOTAIL; magnetic reconnection; field linesolar cyclesSolar maximumSolar Energy;

机译：linesolar磁尾;磁重联;字段cyclesSolar maximumSolar能源;

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Hemispheric asymmetry in the near-Venusian magnetotail during solar maximum

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