On Spatial Structuring of the F2 Layer Studied by the Satellite Radio Sounding of the Ionosphere Disturbed by High-Power HF Radio Waves
We present the results of studying the characteristics of the artificial plasma structures excited in the ionospheric F 2 region modified by high-power HF radio waves. The experiments were carried out at the Sura heating facility using satellite radio sounding of the ionosphere. The plasma density p...
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Veröffentlicht in: | Radiophysics and quantum electronics 2018-01, Vol.60 (8), p.609-617 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | We present the results of studying the characteristics of the artificial plasma structures excited in the ionospheric F
2
region modified by high-power HF radio waves. The experiments were carried out at the Sura heating facility using satellite radio sounding of the ionosphere. The plasma density profile was reconstructed with the highest possible spatial resolution for today, about 4 km. In a direction close to the magnetic zenith of the pump wave, the following phenomena were observed: the formation of a cavity with a 15% lower plasma density at the altitudes of the F
2
layer and below; the formation of an area with plasma density increased by 12% at altitudes greater than 400 km. With a long-term quasiperiodic impact of the pump wave on the ionosphere, wavy large-scale electron-density perturbations (the meridional scale λ
x
≈ 130 km and the vertical scale λ
z
≈ 440 km) are also formed above the Sura facility. These perturbations can be due to the plasma density modulation by an artificial acoustic-gravity wave with a period of 10.6 m, which was formed by the heat source inside a large-scale cavity with low plasma density; there is generation of the electron density irregularities for the electrons with ΔN
e
/N
e
≈ 3% in the form of layers having the sizes 10–12 km along and about 24 km across the geomagnetic field, which are found both below and above the F
2
-layer maximum. The mechanisms of the formation of these plasma structures are discussed. |
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ISSN: | 0033-8443 1573-9120 |
DOI: | 10.1007/s11141-018-9831-5 |