http://www.seipub.org/des
Development in Earth Science Volume 2, 2014
Association of Seismic Activity with Solar Cycle and Geomagnetic Activity Tamara Gulyaeva Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, IZMIRAN, Kaluzskoe Sh. 4, Troitsk, 142190 Moscow, Russia gulyaeva@izmiran.ru Abstract The long-term relationship is investigated between the occurrence of earthquakes with magnitude from 5.0 to 10.0 (M5+), the solar cycle and geomagnetic activity for a period from 1964 to 2013. It is found that the global number of earthquakes tends to grow towards the solar cycle minimum characterized by the sunspot number, SSN, and solar radio flux F10.7. The trend of anti-correlation between the global earthquake occurrence and the phase of the solar cycle is expressed analytically in terms of SSN and F10.7 and applied for prediction of earthquakes number, EQN, based on SSN prediction. The occurrence of EQN in the South magnetic hemisphere relative to that in the North hemisphere is about 1.5 times greater the both irrespective of season. It is shown that zones of enhanced seismic activity are located in the Pacific Ocean at longitudes between 120 to 210E and magnetic latitudes from 40S to 40N with dominant earthquake occurrence in the sub-equatorial region of the South hemisphere. Taking advantage of monitoring the equatorial ring current variations with geomagnetic disturbance storm time Dst index, relevant catalogue of 1305 geomagnetic Dst storms during 1964-2013 is produced and compared with seismic activity. It is found that 13% of earthquakes M5+ occur during Dst storm times showing an enhanced seismic activity at the growing branch of phase of the solar cycle which is permanent feature of the geomagnetic activity. Keywords Earthquake; Seismology; Solar Activity; Geomagnetic Storm
Introduction It is recognized that there are pre-earthquake phenomena comprised of the local magnetic field variations, electromagnetic emissions at the different frequency ranges, excess radon emanation from the ground, changes in water chemistry, water condensation in the atmosphere leading to haze, fog or clouds, atmospheric gravity waves rising up to the ionosphere, changes in the ionospheric Total Electron Content (TEC) and the F2 layer peak electron density
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(Gokhberg et al., 1983; Biagi et al., 2001; Hayakawa et al., 2010; Freund, 2013). The seismic-ionospheic theories and lithosphere–atmosphere–ionosphere models explain the earthquake-ionosphere coupling processes by electromagnetic wave propagation, acoustic gravity wave, atmospheric electricity and geochemical channel (Pulinets, 2009; Harrison et al., 2010; Namgaladze et al., 2012; Freund, 2013). The ionosphere precursors of earthquakes and the magnetosphere storm effects on seismic events are widely investigated (Pulinets and Boyarchuk, 2004; Liu et al., 2004; Zhao et al., 2008; Karatay et al., 2010; Namgaladze et al., 2012; Komjathy et al., 2013; Le et al., 2011, 2013; Pohunkov et al., 2013; He et al., 2014). Though the earthquake affects the surrounding space within the restricted area (of 100 to 4,000 km radius), the prolonged effects and frequency of occurrence of the earthquakes may have cumulative effects on the ionosphere structure and variability (Rishbeth, 2006; Astafyeva et al., 2009; Gulyaeva et al., 2014a). The solar electromagnetic radiation, particularly, at wavelengths of solar X-rays (XUV) is absorbed by the Earth’s upper atmosphere producing the ionosphere plasma. The XUV fluctuates regularly and irregularly over timescales from minutes (flares) and roughly 27 days (solar rotation) to decades (11-year solar cycle), with amplitudes varying up to more than 1000 times (Liu et al., 2011). Though it is difficult to distinguish between pure seismic precursors in the ionosphere from geomagnetic storm effects (Karatay et al., 2010; He et al., 2014), the post-earthquake phenomena are well observed and found over the local areas of high seismic activity providing opportunity to make study of both temporal and spatial earthquake-ionosphere associations (Rishbeth, 2006; Pohunkov et al., 2013). While the ionosphere precursors and post-event effects of the particular earthquakes or series of seismic events has been intensely studied (Le et al., 2011; Namgaladze et al., 2012), a possible linkage of