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An Automatic Detection Algorithm Applied to Fast Magnetosonic Waves With Observations of the Van Allen Probes

机译:一种自动检测算法应用于VAN艾伦探针的快速磁性波

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摘要

Fast magnetosonic (MS) waves can play an important role in the evolution of the inner magnetosphere. However, there is still not an effective method to quantitatively identify such waves for observations of the Van Allen Probes reasonably. In this paper, we used Van Allen Probes data from 18 September 2012 to 30 September 2014 to find a more comprehensive automatic detection algorithm for fast MS waves through statistical analysis of the major properties, including the planarity, ellipticity, and wave normal angle of whole fluctuations using the singular value decomposition method. According to a control variate method, we find an obvious difference between fast MS waves and other waves in the statistical distribution of their major properties. After eliminating the influence of background noises, by excluding fluctuations at L < 1.8, we set up an automatic detection algorithm applied to fast MS waves, that is, smaller than 0.2 for the absolute value of wave ellipticity, larger than 70° for the wave normal angle, with frequency range of 2 Hz to 1.5 f_(LHR) (f_(LHR) is the local lower hybrid resonance frequency). Finally, we have checked the planarity to verify availability of this method and tested this completely automatic method on the Van Allen Probes data and found some results consistent with previous studies. Inside the plasmapause, we found that there is a more obviously favorable occurrence of MS waves at dusk sector with increasing magnetic latitudes.
机译:快速磁性(MS)波可以在内磁层的演变中发挥重要作用。然而,仍然没有一种有效的方法来定量地识别这种波,用于合理地观察范例探针。在本文中,我们在2012年9月18日至2014年9月30日之前使用了Van Allen探针数据,以通过对主要性质的统计分析找到一种更全面的自动检测算法,包括全部性质的统计分析,包括整体的平面,椭圆度和波正常角度使用奇异值分解方法的波动。根据控制变化方法,我们在其主要性质的统计分布中发现快速MS波和其他波之间的明显差异。在消除背景噪声的影响之后,通过排除L <1.8的波动,我们设置了一个自动检测算法,其应用于快速MS波,对于波椭圆形的绝对值小于0.2,对于波浪大于70°正常角度,频率范围为2 Hz至1.5 f_(lhr)(f_(lhr)是局部较低的混合谐振频率)。最后,我们已经检查了平面性以验证此方法的可用性,并在Van Allen探针数据上测试了这种完全自动方法,发现一些结果与以前的研究一致。在近视之内,我们发现,随着磁纬度的增加,黄昏扇区的MS波有更明显有利的发生。

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