Schumann resonances observed using Poynting vector spectra

Details Schumann resonances observed using Poynting vector spectra Schumann resonances observed using Poynting vector spectra

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jastp..61..751b&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 61, Issue 10, p. 751-763.

Physics

11

Scientific paper

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.

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