电离层人工气辉区域总电子含量空间分布图的绘制方法

I. Nasyrov, D. Kogogin, A. Shindin, S. Grach, R. Zagretdinov, A. Beletsky, V. Emeljanov
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引用次数: 0

摘要

在SURA设施强射电辐射干扰电离层实验中,提出了在光谱红线(λ = = 630 nm)上绘制电离层人工气辉区域总电子含量(TEC)空间分布图的方法。为了测试该方法,选择了2016年8月29日18:40至20:10 UTC的测量时段,即电离层和天气条件略有变化,并允许同时从两个空间分离的地点(SURA设施附近的Vasilsursk和位于SURA设施以东约170公里的Magnitka)对电离层的人工气光进行光学测量。通过同时进行的光学测量,绘制了人造气辉的三维投影面积,并确定了受SURA设施强射电辐射刺激的电离层扰动区的空间位置。绘制电离层扰动区域电子密度分布的空间格局的方法是基于对无线电路径“导航卫星-地面接收站”的TEC变化的联合分析,这些接收站位于距离SURA设施约160公里半径内的全球导航卫星系统的一些接收站。利用该方法,可以得到电离层扰动区不同空间截面上的电子密度变化值。利用所考虑的方法对实验数据进行了联合分析,结果表明,在强无线电波场中,沿磁力线形成了具有复杂结构的扰动区。电子密度增加的等离子体不均匀性发生在电子浓度降低的区域边界。在扰动区边界处,即电子密度增加和减少区域之间的差值∆N e /N e可能达到10%。扰动区的大小是沿地球磁力线⊥≈45 ÷ 60公里,沿地球磁力线⊥(cid:107) (cid:38) 70公里。
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The Method of Plotting a Spatial Distribution Pattern of the Total Electron Content in the Region of Artificial Airglow of the Ionosphere
The method of plotting a spatial distribution pattern of the total electron content (TEC) in the region of artificial airglow of the ionosphere in the red line of the optical spectrum ( λ = = 630 nm) was developed during the experiments on disturbances of the ionosphere by powerful radio emission of the SURA facility. To test the method, a measurement session on August 29, 2016 from 18:40 to 20:10 UTC, i.e., when the ionospheric and weather conditions varied slightly and allowed simultaneous optical measurements of the artificial airglow of the ionosphere from two spatially separated sites (Vasilsursk near the SURA facility and Magnitka lying ∼ 170 km East of the SURA facility), was selected. As a result of the simultaneous optical measurements, the area of artificial airglow was plotted in a three-dimensional projection and the spatial position of the disturbed region of the ionosphere stimulated by the powerful radio emission of the SURA facility was determined. The method of plotting a spatial pattern of the electron density distribution in the disturbed region of the ionosphere is based on a joint analysis of variations in the TEC on the radio paths “navigation satellite – ground receiving site” for a number of receiving stations of the global navigation satellite systems located within a radius of ∼ 160 km from the SURA facility. By using this method, the values of electron density variations for different spatial cross-sections of the disturbed region of the ionosphere can be obtained. The joint analysis of the experimental data carried out with the help of the method under consideration showed that in the field of the powerful radio wave a disturbed region with the complex structure formed along the magnetic field lines. Plasma inhomogeneities with an increased electron density occurred at the boundaries of the region with a reduced electron concentration. The difference ∆ N e /N e at the boundaries of the disturbed region, i.e., between the regions with increased and decreased electron density, might reach 10%. The size of the disturbed region is l ⊥ ≈ 45 ÷ 60 km across and l (cid:107) (cid:38) 70 km along the Earth’s magnetic field lines.
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