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Study of the Average Ion Mass of the Dayside Magnetospheric Plasma

机译:Study of the Average Ion Mass of the Dayside Magnetospheric Plasma

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The investigation of heavy ions dynamics and properties in the Earth's magnetosphere is still an important field of research as they play an important role in several space weather aspects. We present a statistical survey of the average ion mass in the dayside magnetosphere made comparing plasma mass density with electron number density measurements and focusing on both spatial and geomagnetic activity dependence. Field line resonance frequency observations across the European quasi-Meridional Magnetometer Array, are used to infer the equatorial plasma mass density in the range of magnetic L-shells 1.6–6.2. The electron number density is derived from local electric field measurements made on Van Allen Probes using the Neural-network-based Upper-hybrid Resonance Determination algorithm. The analysis is conducted separately for the plasmasphere and the plasmatrough during favorable periods for which both the plasma parameters are observed simultaneously. We found that throughout the plasmasphere the average ion mass is ?1 amu for a wide range of geomagnetic activity conditions, suggesting that the plasma mainly consist of hydrogen ions, without regard to the level of geomagnetic activity. Conversely, the plasmatrough is characterized by a variable composition, highlighting a heavy ion mass loading that increases with increasing levels of geomagnetic disturbance. During the most disturbed conditions, the average radial structure shows a broad maximum around 3–4 Earth radii, probably correlated with the accumulation of oxygen ions near the plasmapause. Those ions are mostly observed in the post-dawn and pre-dusk longitudinal sectors.
机译:重离子动力学和调查在地球的磁气圈仍然是属性扮演着一个重要的研究领域在几个空间天气方面的重要作用。我们提出一个统计调查的平均离子质量的光面的磁气圈比较等离子体质量密度和电子数密度测量和关注空间和地磁活动的依赖。场线共振频率的观察整个欧洲quasi-Meridional磁强计数组,用于推断赤道等离子体质量密度的磁L-shells1.6 - -6.2。从当地电场测量了范艾伦辐射探测器使用神经元网络Upper-hybrid共振确定算法。分析分开进行的等离子体层和plasmatrough期间有利的时期的等离子体同时参数观察。在整个等离子体层平均离子质量是什么? 1为范围广泛的地磁阿姆河活动条件,这表明等离子体主要是由氢离子,不考虑地磁活动水平。plasmatrough的特点是一个变量成分,突出重离子质量加载水平的增加而增加地磁扰动。干扰条件下,平均径向环绕地球3 - 4显示了一个广泛的最大的结构半径,可能与积累氧离子等离子体层顶附近。主要是观察到的post-dawn pre-dusk纵向行业。

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