Abstract

Atmospheric electromagnetic waves created by global lightning activity contain information about electrical processes of the inner and the outer Earth. Large signal-to-noise ratio events are particularly interesting because they convey information about electromagnetic properties along their path. We introduce a new methodology to automatically detect and characterize lightning-based waves using a time–frequency decomposition obtained through the application of continuous wavelet transform. We focus specifically on three types of sources, namely, atmospherics, slow tails and whistlers, that cover the frequency range 10 Hz to 10 kHz. Each wave has distinguishable characteristics in the time–frequency domain due to source shape and dispersion processes. Our methodology allows automatic detection of each type of event in the time–frequency decomposition thanks to their specific signature. Horizontal polarization attributes are also recovered in the time–frequency domain. This procedure is first applied to synthetic extremely low frequency time-series with different signal-to-noise ratios to test for robustness. We then apply it on real data: three stations of audio-magnetotelluric data acquired in Guadeloupe, oversea French territories. Most of analysed atmospherics and slow tails display linear polarization, whereas analysed whistlers are elliptically polarized. The diversity of lightning activity is finally analysed in an audio-magnetotelluric data processing framework, as used in subsurface prospecting, through estimation of the impedance response functions. We show that audio-magnetotelluric processing results depend mainly on the frequency content of electromagnetic waves observed in processed time-series, with an emphasis on the difference between morning and afternoon acquisition. Our new methodology based on the time–frequency signature of lightning-induced electromagnetic waves allows automatic detection and characterization of events in audio-magnetotelluric time-series, providing the means to assess quality of response functions obtained through processing.

Highlights

  • Natural variation of the magnetic field in the frequency range 1 Hz to 10 kHz mainly originates from global lightning activity, with about 45 lightning strikes per second (Christian et al 2003)

  • We propose a new methodology: Automatic Detection of Electromagnetic Waves (ADEM), to automatically detect EM waves in the frequency range 10 Hz–10 kHz

  • We focus on three types of EM waves, atmospherics, slow tails and whistlers, all of which are well represented in the analysed time-series, providing an excellent basis for testing ADEM

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Summary

INTRODUCTION

Natural variation of the magnetic field in the frequency range 1 Hz to 10 kHz mainly originates from global lightning activity, with about 45 lightning strikes per second (Christian et al 2003). As whistlers, follow magnetic field lines from one hemisphere to the other through the magnetosphere Analysis of such waves’ properties supplies information about electric and atmospheric processes of the Earth. AMT data acquired in November 2012 in Guadeloupe, French Overseas Territories They exhibit interesting features of typical EM waves. It is located 8 km off the lava dome and 600 m off the Soufriere Volcano Observatory This station was composed by 50 m electric dipole for NS and EW measurements and MFS06 induction coils (using chopper off) to measure the magnetic field. We focus on three types of EM waves, atmospherics, slow tails and whistlers, all of which are well represented in the analysed time-series, providing an excellent basis for testing ADEM

Atmospherics
Slow tails
Whistlers
METHODS
Detection and characterization of EM waves
First criterion of significant amplitude
Polarization attributes
Test on synthetic data
Frequency content and occurrence
Characterization
Findings
Discussion—AMT impedance tensor and atmospheric activity
Full Text
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