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Multiple-Mode Interference and Phase Standard Deviation of VLF Wave Propagation in an Anisotropic Earth–Ionosphere Waveguide

机译:各向异性地球-电离层波导中VLF传播的多模干扰和相位标准偏差

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In this paper, the multiple-mode interference (MMI) and phase standard deviation of very low frequency (VLF) wave propagation in an anisotropic earth–ionosphere waveguide are treated analytically. The phase stability of a VLF wave is dependent on the characteristics of each propagable mode, such as the excitation factor, the attenuation rate, the phase velocity, as well as their derivatives with respect to the effective ionosphere height. Computations show that the phase stability in the multiple-mode zone is much poorer than that in the single-mode zone, and the phase standard deviations evaluated considering the ionospheric anisotropy are more consistent with the measured data. It is also found that there exist pronounced directional differences in the interference distributions, and the effect of MMI is weakened as the geomagnetic inclination angle increases. By comparison of the phase standard deviation and the field strength, we find that the maxima of the phase standard deviation coincide with the minima of the field strength. Moreover, the MMI zone is much broader in nighttime than in daytime, and in an anisotropic waveguide, the interference will present evident aggregation at certain heights.
机译:本文对各向异性地球电离层波导中的多模干扰(MMI)和甚低频(VLF)波传播的相位标准偏差进行了分析处理。 VLF波的相位稳定性取决于每种可传播模式的特性,例如激发因子,衰减率,相速度及其相对于有效电离层高度的导数。计算表明,多模态区的相位稳定性比单模区差得多,考虑电离层各向异性评估的相位标准偏差与实测数据更加一致。还发现干扰分布中存在明显的方向差异,并且随着地磁倾斜角的增加,MMI的作用减弱。通过比较相位标准偏差和场强,我们发现相位标准偏差的最大值与场强的最小值一致。此外,夜间的MMI区比白天的宽得多,并且在各向异性波导中,干涉将在某些高度出现明显的聚集。

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