2020
DOI: 10.1016/j.jastp.2020.105231
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Variations of global thunderstorm activity derived from the long-term Schumann resonance monitoring in the Antarctic and in the Arctic

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Cited by 15 publications
(40 citation statements)
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“…Higher magnitudes can be identified in the years near the solar maxima and smaller ones near the solar minimum (see Figures 3C-J). This observation had been noted earlier for the total horizontal magnetic field by Koloskov et al (2020). To take a closer look at this phenomenon we have removed the yearly averages from the VRN records for each (H NS , H EW ) field component and plotted the residuals (ΔI) in Figure 4.…”
Section: Long-term Variationssupporting
confidence: 69%
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“…Higher magnitudes can be identified in the years near the solar maxima and smaller ones near the solar minimum (see Figures 3C-J). This observation had been noted earlier for the total horizontal magnetic field by Koloskov et al (2020). To take a closer look at this phenomenon we have removed the yearly averages from the VRN records for each (H NS , H EW ) field component and plotted the residuals (ΔI) in Figure 4.…”
Section: Long-term Variationssupporting
confidence: 69%
“…Here we note only that data segments with distorted SR spectra were removed from the VRN and SOU databases before averaging. From the VRN station an extended dataset of the spectral intensity at 11 Hz (between the first and second resonance peaks) is also presented (Koloskov et al, 2020). Later in this study we show that a substantial portion of long-term SR intensity variations are related to changes in the quality factor (Q-factor) of the Earth-ionosphere cavity, which characterizes the rate of energy dissipation at a given resonance mode (Madden and Thompson, 1965;Kulak et al, 2003a).…”
Section: Sr Datamentioning
confidence: 74%
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