Open Journal of Earthquake Research
Vol.08 No.04(2019), Article ID:96299,12 pages
10.4236/ojer.2019.84015

Lower Ionospheric Turbulence Variations during the Intense Tectonic Activity of October, 2018 at Zakynthos Area, Greece

Michael E. Contadakis1, Dimitrios N. Arabelos1, George S. Vergos1, Emmanuel M. Scordilis2

1Department of Geodesy and Surveying, Aristotle University of Thessaloniki, Thessaloniki, Greece

2Department of Geophysics, Aristotle University of Thessaloniki, Thessaloniki, Greece

Copyright © 2019 by author(s) and Scientific Research Publishing Inc.

This work is licensed under the Creative Commons Attribution International License (CC BY 4.0).

http://creativecommons.org/licenses/by/4.0/

Received: October 17, 2019; Accepted: November 8, 2019; Published: November 11, 2019

ABSTRACT

In this paper we investigate the ionospheric turbulence from TEC observations before and during the intense seismic activity of October of 2018 at Zakynthos area (λ = 20.51˚E, φ = 37˚34'N), (Main shock: ML 6.6, 60.6 km SW of Zakynthos). The Total Electron Content (TEC) data of 5 Global Positioning System (GPS) stations of the EUREF network, which are being provided by IONOLAB (Turkey), were analyzed using Discrete Fourier Analysis in order to investigate the TEC variations. The results of this investigation indicate that the High-Frequency limit fo, of the ionospheric turbulence band content, increases as the site and the moment of the earthquake occurrence are approaching, pointing to the earthquake locus. We conclude that the LAIC mechanism through acoustic or gravity wave could explain this phenomenology.

Keywords:

Seismicity, Lower Ionosphere, Ionospheric Turbulence, Brownian Walk

1. Introduction

It is generally accepted that the original cause of the earth surface perturbation is the increasing stress and the rapture of the rocks at the earthquake preparation area where radon release takes place. The coupling of radon with the atmosphere at the earth surface results in the increase of the Ionization, Temperature [1], Electromagnetic field and disturbances in the air electrical conductivity. This perturbation is transmitted to the Ionosphere by some LAIC Mechanism. The proposed possible hypothesis on the mechanism of coupling between lithospheric activity and ionosphere is Transmission through the: 1) Chemical channels [2], 2) Atmospheric oscillation (or acoustic) channels [3] and (3) Electromagnetic channels [2] [3]. Finally, a hypothesis of electrostatic channel has been proposed by Freund [4] on the basis of positive hole charge carriers release in crustal rocks, alongside electrons. When the positive holes arrive at the Earth’s surface, they can cause massive ionization of the air molecules and positive surface potential. Subsequently, these perturbations are transmitted to Ionosphere. From all these hypothesis for the LAIC mechanism, we believe that the hypothesis of the Atmospheric oscillation (or acoustic) channel [3] is the most suitable for the explanation of our observations so far [5] [6] [7], since the observed frequency band of the suggested Gravity waves of our work complies with the observed frequency bands of the Internal Atmospheric Gravity waves (Acoustic standing waves) by Horie et al. [8] and Molchanov et al. [9] [10]. Thus according to the LAIC mechanism through Acoustic channel, Acoustic or Gravity waves affect the turbulence of the lower ionosphere. Subsequently the produced disturbance starts to propagate in the ionosphere’s waveguide as gravity wave. The inherent frequencies of the acoustic or gravity wave range between 0.003 Hz (period 5 min) and 0.0002 Hz (period 83 min), which according to Molchanov et al. [9] [10] correspond to the frequencies of the turbulent produced by tectonic activity during the earthquake preparation period. During this propagation, the higher frequencies are progressively damped. Thus, observing the frequency content of the ionospheric turbidity we will observe a decrease of the higher limit of the turbidity frequency band. Our investigations so far, on the occasion of strong earthquakes approve this view. Never the less, since the approval of the theoretical view depends mainly on the compliance of the observational results to the theoretical clues, further observational results are always welcome.

In this paper we investigate the ionospheric turbulence from TEC observations before and during the intense seismic activity of October of 2018 at Zakynthos area (λ = 20.51˚E, φ = 37˚34'N), (Main shock: ML 6.6, 60.6 km SW of Zakynthos). The Total Electron Content (TEC) data of 5 Global Positioning System (GPS) stations of the EUREF network, which are being provided by IONOLAB (Turkey), were analyzed using Discrete Fourier Analysis in order to investigate the TEC variations [2] [3] [4].

2. Seismotectonic Information

On October 26, 2018 (22:54 GMT) a strong (ML = 6.6) shallow (h~10 km) earthquake occurred ~50 km off the SW coast of Zakynthos Island, southern Greece (37.34˚N, 20.51˚E). The main shock was followed by an aftershock sequence that lasted for almost three months.

Strong earthquakes have occurred in the broader region in the past with magnitudes up to 7.2 (Table 1, Figure 1). Their generation is related to significant regional seismic faults, characterizing the NW edge of the Hellenic Trench and showing dextral strike slip faulting with thrust component (typical fault plane solution: Az = 38, Dip = 61, Rake = 174; [11] ). However, remarkable thrust

Figure 1. Epicenters of all known strong (M ≥ 6.0) earthquakes that occurred in the wider region since 1900 (see Table 1). http://www.isc.ac.uk/.

Table 1. All known strong (M ≥ 6.5) shallow (h < 60 km) earthquakes that occurred since 1900 in the broader region of the seismic sequence under study (Information from Papazachos and Papazachou, 2003 and from the online bulletin of ISC, http://www.isc.ac.uk/).

faults, striking NW-SE are also met in the same region (to the SW of Zakynthos Island) with typical fault plane solution: Az = 309, Dip = 23, Rake = 101 [11]. The fault plane solution of the main shock of October (the two nodal planes, NP1 and NP2, according to GCMT, have Az = 13˚, Dip = 24˚, Rake = 165˚ and Az = 117˚, Dip = 84˚, Rake = 66˚, respectively; https://www.globalcmt.org/CMTsearch.html), assumes that both the above seismic faults could be responsible for its generation.

The main shock was followed by a remarkable number of aftershocks, the strongest of which occurred four days later (on October 30, 15:12 GMT) with ML = 5.4, while within the same day and a few hours earlier (02:59 GMT), another strong aftershock with similar magnitude (ML = 5.3) occurred, with its epicenter very close to that of the main shock. Table 2 and the map of Figure 2 give information on the aftershock activity during the first four months after the occurrence of the main shock.

Figure 2. Seismic activity SE of Zakynthos Isl. (southern Greece) during the period October 25, 2018-February 28, 2019. Red star denotes the epicenter of the main shock (October 25, 2018; 22:54 UTC; ML = 6.6). (Data from: http://geophysics.geo.auth.gr/the_seisnet/WEBSITE_2005/catalogs_en.html, http://www.gein.noa.gr/services/current_catalogue.php and http://bbnet.gein.noa.gr/HL/seismicity/catalogues/real-time-catalogue.

Table 2. A list of the strongest (M ≥ 5.0) earthquakes which occured in the broader area of Zakynthos around the time of the main shock occurence (Information from http://geophysics.geo.auth.gr/ss/bulletins.html and http://bbnet.gein.noa.gr/HL/seismicity/catalogues/real-time-catalogue).

3. TEC Variation over Mid Latitude in Europe

In the following we investigate the variations of TEC [2] [12] over the broader area of Mediterranean before and during the intense seismic activity of October, 2018 at Zakynthos area (λ = 20.51˚E, φ = 37˚34'N), (Main shock: ML 6.6, 60.6 km SW of Zakynthos). To this purpose we use the TEC estimates provided by IONOLAB (http://www.ionolab.org) [13] (Arikan et al. 2009) for 5 mid latitude GPS stations of EUREF which cover epicentre distances from the active areas ranging from 496.7 km to 2164.3 km, for the time periods between 15/07/2018 to 15/11/2018. The selected GPS stations have about the same latitude and are expected to be affected equally from the Equatorial Anomaly as well as from the Auroral storms. Table 3 displays the 5 EUREF stations while Figure 3 displays the locus of the five GPS stations and the main shocks.

IONOLAB system provides comparison graphs of its TEC estimations with the estimations of the other TEC providers of IGS in its site. In this work only TEC estimations in perfect accordance among all providers were used. The TEC values are given in the form of a Time Series with a sampling gap of 2.5 minute. The IONOLAB TEC estimation system uses a single station receiver bias estimation algorithm, IONOLAB-BIAS, to obtain daily and monthly averages of receiver bias and is successfully applied to both quiet and disturbed days of the ionosphere for station position at any latitude. In addition, TEC estimations with high resolution are also possible [13]. Figure 4 display the TEC variation over the 5 EUREF stations for the time periods between 25/09/2018 to 25/11/2018.

Figure 3. The locus of the five GPS stations and the main shocks.

Table 3. Distance of GPS stations from the epicenter of the earthquake.

Figure 4. The TEC variation over the 5 EUREF stations for the time period between 25/09/2018 to 25/11/2018.

4. Fast Fourier Transform Analysis

The Power Spectrum of TEC variations will provide information on the frequency content of them. Apart of the well known and well expressed tidal variations, for which the reliability of their identification can be easily inferred by statistical tests, small amplitude space-temporal transient variations cannot have any reliable identification by means of a statistical test. Nevertheless looking at the logarithmic power spectrum we can recognize from the slope of the diagram whether the contributed variations to the spectrum are random or periodical. If they are random the slope will be 0, which correspond to the white noise, or −2 which correspond to the Brownian walk noise, otherwise the slope will be different, the so called Fractal Brownian walk [14]. This means that we can trace the presence of periodical variations in the logarithmic power spectrum of TEC variations. As an example, Figure 5 displays the logarithmic power spectrum of TEC variations over the GPS station of Mate at the days of 23 to 25/10/2018. It is seen that the slope of the diagram up to the log(f) = −2.2, is −2. This means that for higher frequencies the TEC variation is random noise. On the contrary the variation of TEC for lower frequencies contains not random variations i.e. turbulent. So we conclude that the upper frequency limit fo of the turbulent band is 738.6 μHz. Or, equivalently, the lower period limit Po of the contained turbulent is 22.563 minutes.

5. Results and Discussion

Figure 6 and Figure 7 display the variation with epicentral distance of TEC turbulence frequency band upper limit fo and of lower Period limit Po, respectively, over the selected EUREF GPS stations for the day of the shocks, i.e. 25 of Oktober, 2018 and for a seismically “quiet” day, the 8 of November 2018. It is

Figure 5. The logarithmic power spectrum of TEC variations over the GPS station of Mate around the days of 23-25/10/2018. Where log(f) is the logarithm of the turbulent frequency and log(P) is the logarithm of the Power spectrum density.

Figure 6. Variation of TEC turbulence frequency upper limit fo over the GPS Stations with the epicentral distance, at 25/10/2018 i.e. the day of the main earthquake (blue) and at 08/11/2018, an aseismic day.

Figure 7. Variation of TEC turbulence Period lower limit Po over the GPS Stations with the epicentral distance, at 25/10/2018 i.e. the day of the main earthquake (blue) and at 08/11/2018, an aseismic day (red).

shown that at the day of the earthquake a strong dependence of the upper frequency fo (lower period Po) limit of the Ionospheric turbulent content with the epicentral distance is observed. In particular, the closer of the GPS station to the active area the higher frequency fo/lower period Po limit is. This dependence is not shown at the “quiet” day. As it is seen from Figure 6 and Figure 7, the upper frequency limit, fo, and lower period limit, Po, of the turbulence band in quiet days, or at remote GPS stations during the days of seismic activity, range between 400 - 200 μHz or equivalently 41.5 - 83 min. A brief statistic of our data for the quiet days give mean values: Mean (fo) = 372.7 ± 75 μHz and Mean (Po) = 44.71 ± 8.25 min. These frequencies are in the range of the observed Acoustic Gravity Waves on the occasions of strong earthquakes, which are: periods of 30 to 100 min [9] [10] or 20 to 80 min [8].

Figure 8 and Figure 9 show the variation of the upper frequency fo and of the lower period Po, limits of ionospheric turbulence content over the nearest to the active area Orid GPS station while Figure 10 and Figure 11 show the variation of the upper frequency fo and of the lower period Po, limits of ionospheric turbulence content over the most remote to the active area Yebes GPS station. In the same figures the occurrence times of strong earthquakes (M > 5.0) are shown with arrows. It is seen that at the days of strong earthquakes the ionospheric turbulence upper frequency limit, fo, increases (or the lower period limit, Po, decreases). These results indicate time and space convergence of increasing turbulence frequency band upper limit fo to the earthquakes occurrence.

Figure 8. Variation of TEC turbulence frequency upper limit fo over the GPS Station of Orid, with the epicentral distance.

Figure 9. Variation of TEC turbulence Period lower limit over the GPS Station of Orid. The arrows show the occurrence of strong earthquakes (M > 5.0).

Figure 10. Variation of TEC turbulence frequency upper limit over the GPS Station of Yebes, with the epicentral distance. The arrows show the occurrence of strong earthquakes (M > 5.0).

Figure 11. Variation of TEC turbulence Period lower limit over the GPS Station of Yebes, with the epicentral distance. The arrows show the occurrence of strong earthquakes (M > 5.0).

Hobara et al. [15] in a study on the ionospheric turbulence in low latitudes concluded that the attribution of the turbulence to earthquake process and not to other sources, i.e. solar activity, storms etc. is not conclusive. Nevertheless in our case, the steady monotonic, time and space, convergence of the frequency band upper limit fo increment, to the occurrence of the East Aegean strong earthquakes is a strong indication that the observed turbulence is generated by the respective earthquakes preparation processes.

The qualitative explanation of this phenomenology can be offered on the basis of the LAIC: Tectonic activity during the earthquake preparation period produces anomalies at the ground level which propagate upwards in the troposphere as Acoustic or Standing gravity waves [16] [17]. These Acoustic or Gravity Waves affect the turbulence of the lower ionosphere, where sporadic Es-layers may appear too [18], and the turbulence of the F layer. Subsequently, the produced disturbance starts to propagate in the ionosphere’s waveguide as gravity wave and the inherent frequencies of the acoustic or gravity waves can be traced on TEC variations [i.e. the frequencies between 0.003 Hz (period 5 min) and 0.0002 Hz (period 100 min)], which, according to Molchanov et al. [9] [10] and Horie et al. [8] correspond to the frequencies of the turbulent induced by the LAIC coupling process to the ionosphere. As we move far from the disturbed point, in time or in space, the higher frequencies (shorter wavelength) variations are progressively attenuated. It has to be noted that the original cause of the earth surface perturbation is the increasing stress and the rapture of the rocks at the earthquake preparation area where radon release takes place. The coupling of radon with atmosphere at the earth’s surface results to the increase the ionization, temperature [1], electromagnetic field and to disturbances in the air electrical conductivity. This perturbation is transmitted to the Ionosphere by some LAIC Mechanism. The proposed possible hypothesis on the mechanism of coupling between lithospheric activity and ionosphere is transmission through the: 1) chemical channels [2], 2) atmospheric oscillation (or acoustic) channels [3] and 3) electromagnetic channels [2] [3]. Finally, a hypothesis of electrostatic channel has been proposed by Freund [4] on the basis of positive hole charge carriers release in crustal rocks, alongside electrons. When the positive holes arrive at the Earth’s surface, they can cause massive ionization of the air molecules and positive surface potential. Subsequently these perturbations are transmitted to Ionosphere. From this hypothesis for the LAIC mechanism, we believe that the hypothesis of the atmospheric oscillation (or acoustic) channel [3] is most suitable for the explanation of our observations, since the observed frequency band of the suggested gravity waves of this work comply with the observed frequency bands of the Internal Atmospheric Gravity waves (Acoustic standing waves) by Horie et al. [8] and Molchanov et al. [9] [10], as it is already mentioned.

6. Conclusion

The results of our investigation, on the case of the recent East Aegean tectonic activity, indicate that the High-Frequency limit fo, of the ionospheric turbulence content, increases as we are getting closer to the site and the time of the earthquake occurrence, pointing to the earthquake location. We conclude that the LAIC mechanism through acoustic or gravity wave could explain this phenomenology. That is, tectonic activity during the earthquake preparation period produces anomalies at the ground level which propagate upwards in the troposphere as Acoustic or Standing gravity waves. These Acoustic or Gravity waves affect the turbulence of the lower ionosphere, where sporadic Es-layers may appear, too, as well as the turbulence of the F layer. Subsequently, the produced disturbance starts to propagate in the ionosphere’s wave guide. Thus observing the frequency content of the ionospheric turbulence we will observe a decrease of the higher limit of the turbulence frequency band, as a result of the differential frequency attenuation of the propagating waves.

Conflicts of Interest

The authors declare no conflicts of interest regarding the publication of this paper.

Cite this paper

Contadakis, M.E., Arabelos, D.N., Vergos, G.S. and Scordilis , E.M. (2019) Lower Ionospheric Turbulence Variations during the Intense Tectonic Activity of October, 2018 at Zakynthos Area, Greece. Open Journal of Earthquake Research, 8, 255-266. https://doi.org/10.4236/ojer.2019.84015

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