Geomagnetic Pulsations, Blackout and Low-Latitude Aurorae Associated with Power Magnetic Storm

V. Parkhomov, A. Mikhalev, Konstantin Ratovskyi
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Abstract

The research analyzed the regularities of the dynamics of geomagnetic pulsation regimes in the frequency range 0.002–5 Hz, the generation of which reflects the interaction with the Earth's magnetosphere of the solar filament ejected by a powerful solar flare of 3B. We compared the dynamics of the change in the types and modes of geomagnetic pulsations with the dynamics of the atmosphere glow in two spectral lines and the total ionospheric absorption of radio waves. The study developed a possible model of the observed phenomenon.
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与强磁暴相关的地磁脉动、停电和低纬度极光
研究分析了0.002 ~ 5 Hz频率范围内地磁脉动的动力学规律,其产生反映了3B强太阳耀斑抛射的太阳细丝与地球磁层的相互作用。我们将地磁脉动的类型和模式变化的动力学与大气两谱线辉光的动力学和电离层对无线电波的总吸收进行了比较。这项研究为观察到的现象提出了一个可能的模型。
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