Schumann resonances observed using Poynting vector spectra

We present the results of a Schumann resonance monitoring campaign held at Lehta observatory, Karelia, Russia during July–August, 1998. Three electromagnetic (EM) field components were recorded simultaneously: the vertical electric and two orthogonal magnetic fields. This paper demonstrates advantag...

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Veröffentlicht in:Journal of atmospheric and solar-terrestrial physics 1999-07, Vol.61 (10), p.751-763
Hauptverfasser: Belyaev, G.G, Schekotov, A.Yu, Shvets, A.V, Nickolaenko, A.P
Format: Artikel
Sprache:eng
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Zusammenfassung:We present the results of a Schumann resonance monitoring campaign held at Lehta observatory, Karelia, Russia during July–August, 1998. Three electromagnetic (EM) field components were recorded simultaneously: the vertical electric and two orthogonal magnetic fields. This paper demonstrates advantages of the Poynting vector (PV) technique when studying the space–time dynamics of the worldwide thunderstorm activity from a single observatory. Analysis of the diurnal PV patterns revealed a night-time peak in African thunderstorm activity. This maximum occurs around 02:00–03:00 UT and reaches 1/3 of regular afternoon level. The Schumann resonance structure was discovered in the spectra of the wave arrival angles.
ISSN:1364-6826
1879-1824
DOI:10.1016/S1364-6826(99)00027-9