Atmospheric Planetary Waves at Ionospheric Heights Measured at the Moscow Observatory (IZMIRAN)

Pub Date : 2023-12-25 DOI:10.1134/s0001433823060087
S. A. Riabova, S. L. Shalimov
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Abstract

The variations of the ionospheric current in the lower ionosphere and the plasma density of the upper ionosphere have been studied based on the monitoring of the horizontal component of the geomagnetic field induction and height-frequency sounding of the critical frequency of the ionosphere F layer at the Moscow Observatory. It is shown that, in the spectra of time variations of the geomagnetic field and the critical frequency of the F2 layer in the range of planetary waves in winter, there are both harmonics associated with solar activity and harmonics corresponding to quasi-5-, 10-, and 16-day planetary waves. The involvement of geomagnetic field registration data for a 20-year time interval (from 2001 to 2020) have made it possible to identify more subtle effects, namely, the harmonics associated with the modulation effect of longer period variations and tidal effects are identified.

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莫斯科天文台(IZMIRAN)测量到的电离层高度的大气行星波
摘要 在莫斯科天文台监测地磁场感应水平分量和电离层 F 层临界频率高频探测的基 础上,研究了电离层下部电离层电流和电离层上部等离子体密度的变化。研究表明,在冬季行星波范围内的地磁场和 F2 层临界频率的时间变化频谱中,既有与太阳活动有关的谐波,也有与准 5 天、10 天和 16 天行星波相对应的谐波。20 年时间间隔(从 2001 年到 2020 年)的地磁场登记数据的参与使我们有可能确定更微妙的效应,即确定与较长周期变化的调制效应和潮汐效应有关的谐波。
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