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首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Determining the drift velocity of ionospheric irregularities by analyzing three mutually orthogonal projections of the HF radio signal field vector
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Determining the drift velocity of ionospheric irregularities by analyzing three mutually orthogonal projections of the HF radio signal field vector

机译:通过分析HF无线电信号场矢量的三个相互正交的投影来确定电离层不规则性的漂移速度

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摘要

This paper presents results of an experimental verification of our earlier suggested spectral-polarization method of measuring the interference pattern velocity by analyzing three mutually orthogonal projections of the radio signal field vector using a single receiving antenna. The measurements were made on an HF radio path about 100 km in length, with a simultaneous monitoring of the ionospheric situation using an oblique-incidence sounding chirp-ionosonde. In an effort to eliminate multipath effects, in the analysis we used nighttime intervals, for which a stable one-mode reflected radio signal was observed. It is shown that the proposed method gives the mean values of the azimuth and zenith angle which differ by no more than 2 to 5 deg from calculated values. Mean values of the velocity of travelling ionospheric disturbances (of order 50 m/s) and propagation directions (north-westward changing to northward by the morning hours) obtained for these time intervals are consistent with existing published data.
机译:本文介绍了对我们较早提出的频谱偏振方法进行实验验证的结果,该方法通过使用单个接收天线分析无线电信号场矢量的三个相互正交的投影来测量干涉图样速度。测量是在大约100公里长的HF无线电路径上进行的,同时使用斜入射测深chi探空仪同时监视电离层情况。为了消除多径效应,我们在分析中使用了夜间间隔,针对该间隔观察到了稳定的单模反射无线电信号。结果表明,所提出的方法给出的方位角和天顶角平均值与计算值相差不超过2至5度。在这些时间间隔内获得的电离层扰动速度的速度(约50 m / s)和传播方向(从西北向北改变为早晨,向北方向)的平均值与现有公布的数据一致。

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