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首页> 外文期刊>Annales Geophysicae >The relationship between small-scale and large-scale ionospheric electron density irregularities generated by powerful HF electromagnetic waves at high latitudes
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The relationship between small-scale and large-scale ionospheric electron density irregularities generated by powerful HF electromagnetic waves at high latitudes

机译:高纬度强HF电磁波产生的小尺度和大尺度电离层电子密度不规则性之间的关系

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Satellite radio beacons were used in June 2001 to probe the ionosphere modified by a radio beam produced by the EISCAT high-power, high-frequency (HF) transmitter located near Tromso (Norway). Amplitude scintillations and variations of the phase of 150- and 400-MHz signals from Russian navigational satellites passing over the modified region were observed at three receiver sites. In several papers it has been stressed that in the polar ionosphere the thermal self-focusing on striations during ionospheric modification is the main mechanism resulting in the formation of large-scale (hundreds of meters to kilometers) nonlinear structures aligned along the geomagnetic field (magnetic zenith effect). It has also been claimed that the maximum effects caused by small-scale (tens of meters) irregularities detected in satellite signals are also observed in the direction parallel to the magnetic field. Contrary to those studies, the present paper shows that the maximum in amplitude scintillations does not correspond strictly to the magnetic zenith direction because high latitude drifts typically cause a considerable anisotropy of small-scale irregularities in a plane perpendicular to the geomagnetic field resulting in a deviation of the amplitude-scintillation peak relative to the minimum angle between the line-of-sight to the satellite and direction of the geomagnetic field lines. The variance of the logarithmic relative amplitude fluctuations is considered here, which is a useful quantity in such studies. The experimental values of the variance are compared with model calculations and good agreement has been found. It is also shown from the experimental data that in most of the satellite passes a variance maximum occurs at a minimum in the phase fluctuations indicating that the artificial excitation of large-scale irregularities is minimum when the excitation of small-scale irregularities is maximum.
机译:2001年6月,卫星无线电信标被用来探测由位于特罗姆瑟(挪威)附近的EISCAT高功率,高频(HF)发射器产生的无线电波所改造的电离层。在三个接收站观测到经过修改区域的俄罗斯导航卫星的150-MHz和400-MHz信号的幅度闪烁和相位变化。在几篇论文中,已经强调指出,在电离层的极地电离层中,热自聚焦在条纹上是形成沿地磁场(磁场(磁场)天顶效应)。还要求在与磁场平行的方向上观察到由卫星信号中检测到的小范围(数十米)不规则引起的最大影响。与那些研究相反,本论文表明振幅闪烁的最大值并不严格与磁天顶方向相对应,因为高纬度漂移通常会在垂直于地磁场的平面上引起相当大的各向异性,导致小范围的不规则性,从而导致偏差振幅闪烁峰相对于卫星视线与地磁场线方向之间的最小夹角的角度。这里考虑对数相对幅度波动的方差,这在此类研究中是有用的量。将方差的实验值与模型计算进行比较,并且发现了良好的一致性。从实验数据还可以看出,在大多数卫星通过的情况下,相位波动中的方差最大值最小,这表明当小规模不规则的激发最大时,大型不规则的人工激发最小。

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