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arXiv 2609.35098physics.space-phastro-ph.EPastro-ph.SRphysics.comp-phphysics.plasm-ph

地球磁层边界太阳风电荷交换的光谱特性:MHD与测试粒子模拟

Spectral Properties of Solar Wind Charge Exchange from Earth's Magnetospheric Boundaries: MHD and Test Particle Simulations

A. Ramachandran, R. T. Desai, H. L. Norman, Y. Tong, D. Bewicke, S. Nitti, J. A. Carter, J. P. Eastwood, J. P. Chittenden

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中文总结 AI 辅助

本文通过Gorgon MHD与XIM粒子模拟,研究地球磁层边界SWCX的X射线发射,发现磁鞘和尖点增强发射及磁层顶betatron加速相关发射,为SMILE等X射线观测提供预测。

中文摘要 AI 辅助

太阳风电荷交换(SWCX)机制,即高电荷态重太阳风离子与中性原子相互作用产生X射线,为观测太阳-地球系统中能量和动量的大尺度输运提供了机会。在本研究中,我们利用Gorgon全球磁流体动力学(MHD)模拟结合我们称之为磁层X射线成像(XIM)框架的动力学粒子模拟,模拟了来自地球外边界SWCX信号。XIM预测的发射率与MHD模型的预测一致,产生了来自磁鞘和尖点区域的增强发射,但存在若干明显差异。与MHD相比,XIM在磁鞘中显示出增强的结构化,并沿磁层顶出现与betatron加速相关的显著增强发射。结果还显示了物种特异性的空间变化,这些变化与太阳风中预期的相对丰度和离子特异性属性相比有所不同。这些模拟为地球外边界SWCX的潜在动力学提供了新的见解,可用于理解空间X射线天文台(如最近发射的SMILE任务)可能观测到的现象。

英文摘要

The Solar Wind Charge Exchange (SWCX) mechanism, where X-rays can be generated through interactions between heavy, highly charged solar wind ions and neutral atoms, offers an opportunity to observe the large-scale transfers of energy and momentum through the Sun-Earth system. In this study, we simulate SWCX signatures from Earth's outer boundaries using Gorgon global magnetohydrodynamic (MHD) simulations combined with kinetic particle-based simulations which we call the X-ray Imaging of the Magnetosphere (XIM) framework. The XIM-predicted emissivities agree with the predictions of the MHD model, producing enhanced emissions from the magnetosheath and cusp regions, but several differences are apparent. Compared with MHD, XIM shows enhanced structuring in the magnetosheath and notable enhanced emissions along the magnetopause associated with betatron acceleration. The results also evidence species-specific spatial variations, which are shown to vary compared to anticipated relative abundances in the solar wind and ion-specific properties. These simulations provide new insights into the underlying dynamics of SWCX at the Earth's outer boundaries, which can be used to understand what might be observed using X-ray observatories in space, such as the recently launched SMILE mission.

发表机构

  • University of Warwick(华威大学)
  • Imperial College London(伦敦帝国学院)
  • University of Leicester(莱斯特大学)
  • Space Park Leicester(莱斯特太空公园)

机构由 AI 辅助整理,请以论文原文为准。

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