Email this article Features of the HF Signal Propagation on Oblique Sounding Paths During Solar and Magnetic Activity in September 2017
- Authors: Uryadov V.P.1,2, Vybornov F.I.1, Pershin A.V.1
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Affiliations:
- Radiophysical Research Institute, N. I. Lobachevsky State University of Nizhny Novgorod
- Polyot, a research and production enterprise
- Issue: Vol 62, No 2 (2019)
- Pages: 85-98
- Section: Article
- URL: https://journals.rcsi.science/0033-8443/article/view/243947
- DOI: https://doi.org/10.1007/s11141-019-09956-z
- ID: 243947
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Abstract
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 Es layer in the auroral ionosphere during a magnetic storm makes it possible to use the propagation mode with reflection from Es 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.
About the authors
V. P. Uryadov
Radiophysical Research Institute, N. I. Lobachevsky State University of Nizhny Novgorod; Polyot, a research and production enterprise
Email: vybornov@nirfi.unn.ru
Russian Federation, Nizhny Novgorod; Nizhny Novgorod
F. I. Vybornov
Radiophysical Research Institute, N. I. Lobachevsky State University of Nizhny Novgorod
Author for correspondence.
Email: vybornov@nirfi.unn.ru
Russian Federation, Nizhny Novgorod
A. V. Pershin
Radiophysical Research Institute, N. I. Lobachevsky State University of Nizhny Novgorod
Email: vybornov@nirfi.unn.ru
Russian Federation, Nizhny Novgorod
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