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arXiv 1808.05034physics.space-ph
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IMF $\mathit{B}_{y}$如何在北向IMF $\mathit{B}_{z}$和特征时标期间引入局部$\mathit{B}_{y}$分量

How the IMF $\mathit{B}_{y}$ Induces a Local $\mathit{B}_{y}$ Component During Northward IMF $\mathit{B}_{z}$ and Characteristic Timescales

P. Tenfjord, N. Østgaard, S. Haaland, K. Snekvik, K. M. Laundal, J. P. Reistad, R. Strangeway, S. E. Milan, M. Hesse, A. Ohma

摘要:

利用Lyon-Fedder-Mobarry全球磁流体动力学模型,研究了行星际磁场(IMF)$\mathit{B}_{y}$分量在IMF $\mathit{B}_{z}$ $>$ 0.我们描述了如何在这些条件下磁层$\mathit{B}_{y}$组件上引起闭合场线的演变。从昼侧波瓣重联开始,新重联磁力线上的磁张力使两半球之间的开放磁通量不对称地重新分配。这导致在叶中的不对称的磁能密度。诱导剪切流以恢复平衡,这些流是有效诱导局部$\mathit{B}_{y}$分量的流。我们显示的径向依赖性的诱导$\mathit{B}_{y}$和比较结果的诱导$\mathit{B}_{y}$在向南IMF条件。我们还显示了在北向IMF $\mathit{B}_{z}$期间,内磁层对IMF $\mathit{B}_{y}$反转的响应和重构时间。本文对七颗地球静止运行环境卫星在不同的当地时间对IMF $\mathit{B}_{y}$的正负反转进行了磁场测量的叠加历元分析。我们发现,诱导的$\mathit{B}_{y}$响应在16分钟内的国际货币基金组织$\mathit{B}_{y}$在弓形冲击的到来,它完全重新配置在47分钟内。

英文摘要:

We use the Lyon-Fedder-Mobarry global magnetohydrodynamics model to study the effects of the interplanetary magnetic field (IMF) $\mathit{B}_{y}$ component on the coupling between the solar wind and magnetosphere-ionosphere system when IMF $\mathit{B}_{z}$ $>$0. We describe the evolution of how a magnetospheric $\mathit{B}_{y}$ component is induced on closed field lines during these conditions. Starting from dayside lobe reconnection, the magnetic tension on newly reconnected field lines redistribute the open flux asymmetrically between the two hemispheres. This results in asymmetric magnetic energy density in the lobes. Shear flows are induced to restore equilibrium, and these flows are what effectively induces a local $\mathit{B}_{y}$ component. We show the radial dependence of the induced $\mathit{B}_{y}$ and compare the results to the induced $\mathit{B}_{y}$ during southward IMF conditions. We also show the response and reconfiguration time of the inner magnetosphere to IMF $\mathit{B}_{y}$ reversals during northward IMF $\mathit{B}_{z}$. A superposed epoch analysis of magnetic field measurements from seven Geostationary Operational Environmental Satellite spacecraft at different local times both for negative-to-positive and positive-to-negative IMF $\mathit{B}_{y}$ reversals is presented. We find that the induced $\mathit{B}_{y}$ responds within 16 min of the arrival of IMF $\mathit{B}_{y}$ at the bow shock, and it completely reconfigures within 47 min.

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