Investigation of the Reaction of Schumann Resonances to Short Transient Geophysical Events Under the Influence of Atmospheric Electromagnetic Noise

The interference of electromagnetic signals from lightning discharges in the frequency range below 100 Hz is the source of a global electromagnetic phenomenon in the Earth's atmosphere known as the Schumann resonance (SR). Changes in the parameters of SR signals caused by geophysical disturbanc...

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Veröffentlicht in:Journal of geophysical research. Atmospheres 2022-08, Vol.127 (16), p.n/a
Hauptverfasser: Poklad, Yu. V., Ryakhovsky, I. A., Gavrilov, B. G., Ermak, V. M., Kozakova, E. N., Achkasov, N. S.
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Sprache:eng
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Zusammenfassung:The interference of electromagnetic signals from lightning discharges in the frequency range below 100 Hz is the source of a global electromagnetic phenomenon in the Earth's atmosphere known as the Schumann resonance (SR). Changes in the parameters of SR signals caused by geophysical disturbances make it possible to study the state and dynamics of the lower ionosphere. When calculating the SR parameters, there are problems associated with the impact of electromagnetic interference of natural and anthropogenic origin. The main natural sources of interference are signals associated with the radiation of nearby lightning discharges, as well as the influence of the Alfvén ionospheric resonator. The paper presents a new method for calculating the SR parameters, which makes it possible to find the spectra distorted by interference, mention above, and exclude them from further processing. The developed technique significantly increased the temporal resolution of the obtained data on the frequency and amplitude of the SR. Due to this, it became possible to study the influence of fast heliogeophysical disturbances (such as solar X‐ray flares) on the lower ionosphere and, as a consequence, on the parameters of the SR. An analysis of the experimental data made it possible to establish a linear dependence of the SR frequency on the logarithm of the X‐ray flux in the range up to 0.2 nm during a class X solar flare. Key Points A new method for calculating the parameters of Schumann resonance (SR) significantly reduces the impact of electromagnetic interference The developed technique increased the temporal resolution of the SR frequency and amplitude data The new technique made it possible to establish the dependence of the SR frequency on the X‐ray flux with a wavelength of less than 0.2 nm
ISSN:2169-897X
2169-8996
DOI:10.1029/2022JD036820