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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Global features of Kelvin-Helmholtz waves at the magnetopause for northward interplanetary magnetic field
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Global features of Kelvin-Helmholtz waves at the magnetopause for northward interplanetary magnetic field

机译:全球Kelvin-Helmholtz波的特性磁层为向北行星际磁场

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摘要

[1] We investigate the global features of Kelvin-Helmholtz waves (KHW) at the low-latitude magnetopause for constant northward interplanetary magnetic field conditions, using global magnetohydrodynamic simulations. The root-integrated power (RIP) of X component of bulk velocity is employed to analyze the magnetopause mode of KHW along the boundary layer. The RIP distribution of the outer KHW is much broader than that of the inner one, and the maximum amplitude of global KHW occurs near the dawn/dusk terminator regions. In the dayside magnetopause, the phase of the waveform at middle latitudes leads to that at low latitudes, while the situation reversed in the nightside. The global evolution of KHW phases is a representation of an interesting feature that the axis of the Kelvin-Helmholtz vortex aligns with the geomagnetic field lines. We suggest that the reported features may also exist in other KHW active regions with flow-sheared plasma.
机译:[1]我们调查的全球特性Kelvin-Helmholtz波在低纬度(KHW)磁层持续向北行星际磁场条件下,使用全球磁流体动力模拟。root-integrated权力(RIP)的X分量速度是用来分析磁层沿边界KHW模式层。更广泛的内部,全球最大振幅的KHW附近发生黎明或黄昏终结者的地区。磁层,在中间阶段的波形纬度导致,在低纬度地区,在阴面形势逆转。是一个全球KHW的进化阶段表示的一个有趣的特性Kelvin-Helmholtz涡与轴地磁场线。也可能存在于其他KHW报告功能活跃的地区flow-sheared等离子体。

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