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Electromagnetic Ion Cyclotron Waves in the High Altitude Cusp: Polar Observations

机译:高海拔尖峰中的电磁回旋加速器波:极地观测。

摘要

High-resolution magnetic field data from the Polar Magnetic Field Experiment (MFE) show that narrow band waves at frequencies approximately 0.2 to 3 Hz are a permanent feature in the vicinity of the polar cusp. The waves have been found in the magnetosphere adjacent to the cusp (both poleward and equatorward of the cusp) and in the cusp itself. The occurrence of waves is coincident with depression of magnetic field strength associated with enhanced plasma density, indicating the entry of magnetosheath plasma into the cusp region. The wave frequencies are generally scaled by the local proton cyclotron frequency, and vary between 0.2 and 1.7 times local proton cyclotron frequency. This suggests that the waves are generated in the cusp region by the precipitating magnetosheath plasma. The properties of the waves are highly variable. The waves exhibit both lefthanded and right-handed polarization in the spacecraft frame. The propagation angles vary from nearly parallel to nearly perpendicular to the magnetic field. We find no correlation among wave frequency, propagation angle and polarization. Combined magnetic field and electric field data for the waves indicate that the energy flux of the waves is guided by the background magnetic field and points downward toward the ionosphere.
机译:来自极地磁场实验(MFE)的高分辨率磁场数据显示,频率约为0.2至3 Hz的窄带波是极尖附近的永久特征。在邻近尖端的磁层(尖端的向极和赤道方向)以及尖端本身中都发现了波。波的发生与伴随着增强的等离子体密度的磁场强度的降低相吻合,表明磁石场等离子体进入了尖端区域。波的频率通常由局部质子回旋加速器频率定标,并且在局部质子回旋加速器频率的0.2到1.7倍之间变化。这表明,由于析出的磁石等离子体在波峰区域产生了波。波浪的属性变化很大。这些波在航天器框架中同时表现出左旋和右旋极化。传播角从几乎平行于磁场到几乎垂直于磁场变化。我们发现波频率,传播角度和极化之间没有相关性。波的磁场和电场数据的组合表明,波的能量通量受背景磁场引导,并向下指向电离层。

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