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首页> 外文期刊>Experimental astronomy >IMPALAS: Investigation of MagnetoPause Activity using Longitudinally-Aligned Satellites-a mission concept proposed for the ESA M3 2020/2022 launch
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IMPALAS: Investigation of MagnetoPause Activity using Longitudinally-Aligned Satellites-a mission concept proposed for the ESA M3 2020/2022 launch

机译:IMPALAS:使用纵向对准卫星调查磁悬浮活动-为ESA M3 2020/2022发射建议的任务概念

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The dayside magnetopause is the primary site of energy transfer from the solar wind into the magnetosphere, and modulates the activity observed within the magnetosphere itself. Specific plasma processes operating on the magnetopause include magnetic reconnection, generation of boundary waves, propagation of pressure-pulse induced deformations of the boundary, formation of boundary layers and generation of Alfvén waves and field-aligned current systems connecting the boundary to the inner magnetosphere and ionosphere. However, many of the details of these processes are not fully understood. For example, magnetic reconnection occurs sporadically, producing flux transfer events, but how and where these arise, and their importance to the global dynamics of the magnetospheric system remain unresolved. Many of these phenomena involve propagation across the magnetopause surface. Measurements at widely-spaced (Δ ~ 5 R _E) intervals along the direction of dayside terrestrial field lines at the magnetopause would be decisive in resolving these issues. We describe a mission carrying a fields and plasmas payload (including magnetometer, ion and electron spectrometer and energetic particle telescopes) on three identical spacecraft in synchronized orbits. These provide the needed separations, with each spacecraft skimming the dayside magnetopause and continuously sampling this boundary for many hours. The orbits are phased such that (i) all three spacecraft maintain common longitude and thus sample along the same magnetopause field line; (ii) the three spacecraft reach local midday when northern European ground-based facilities also lie near local midday, enabling simultaneous sampling of magnetopause field lines and their footprints.
机译:日间磁层绝顶是能量从太阳风传递到磁层的主要场所,并调节磁层自身内部的活动。在磁层顶上运行的特定等离子体过程包括磁重新连接,边界波的产生,压力脉冲引起的边界变形的传播,边界层的形成以及Alfvén波的产生以及将边界连接到内部磁层和磁场的场对准电流系统。电离层。但是,这些过程的许多细节尚未完全理解。例如,磁重新连接偶发地发生,产生磁通转移事件,但是这些事件的发生方式和位置以及它们对磁层系统整体动力学的重要性仍未解决。这些现象中的许多都涉及在磁更年期表面上的传播。沿磁层顶的日间地面磁力线方向以大间距(Δ〜5 R _E)进行测量对于解决这些问题具有决定性意义。我们描述了在同步轨道上的三个相同航天器上载有场和等离子体有效载荷(包括磁力计,离子和电子能谱仪以及高能粒子望远镜)的任务。这些提供了所需的间隔,每个航天器都会掠过白天的磁层顶并连续数小时对该边界进行采样。轨道的相位使(i)所有三个航天器保持共同的经度,并因此沿相同的磁更年期磁力线采样; (ii)当北欧地面基地设施也位于当地午间时,这三架航天器到达当地午间,从而可以同时采样磁层顶磁力线及其足迹。

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