Features of the HF Signal Propagation on Oblique Sounding Paths During Solar and Magnetic Activity in September 2017

被引:4
|
作者
Uryadov, V. P. [1 ,2 ]
Vybornov, F., I [1 ]
Pershin, A., V [1 ]
机构
[1] NI Lobachevsky State Univ Nizhny Novgorod, Radiophys Res Inst, Nizhnii Novgorod, Russia
[2] Polyot, Nizhnii Novgorod, Russia
关键词
FREQUENCY; DOPPLER;
D O I
10.1007/s11141-019-09956-z
中图分类号
TM [电工技术]; TN [电子技术、通信技术];
学科分类号
0808 ; 0809 ;
摘要
We present the results of studying the influence of solar and magnetic activity in September 2017 on the HF signal characteristics on subauroral and midlatitude paths. A connection between the ionospheric effects caused by the magnetic storm and the magnetic disturbance intensity is established. It is shown that the formation of a strong sporadic E-s layer in the auroral ionosphere during a magnetic storm makes it possible to use the propagation mode with reflection from E-s in the interests of HF communication to neutralize the effects of the negative phase of the storm and absorption growth when unfavorable conditions for the F-mode propagation with reflection from the upper ionosphere occur.
引用
收藏
页码:85 / 98
页数:14
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