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IUGG XXIV General Assembly July 2-13, 2007 Perugia, Italy<br />

(S) - <strong>IASPEI</strong> - International Association of Seismology and Physics of the Earth's<br />

Interior<br />

JSS009 Poster presentation 2056<br />

Day-time variations of foF2 connected to strong earthquakes<br />

Dr. Mikhail Rodkin<br />

Geophysical Center Russian Academy of Sciences <strong>IASPEI</strong><br />

Elena Liperovskaya, Vadim Bogdanov, Claudia-Veronica Meister, Victor Liperovsky<br />

In the present work, the authors continue their search for earthquake precursors and study of the<br />

behavior of some characteristic parameters of the ionosphere occurring during the earthquake<br />

preparation processes and after the earthquakes. The F-layer is the most dynamic regular layer of the<br />

ionosphere being considerably modified by different reasons. The foF2 frequency characterizing the<br />

maximum of the electron concentration in this layer is one of the parameters of the ionosphere that is<br />

regularly measured during vertical sounding experiments. Here the variability of the foF2 frequency<br />

connected with the strong earthquakes is investigated statistically, more than 100 events with<br />

magnitude M>6.0 are taken into examination. These earthquakes have a depth less than 80 km, and<br />

they happened at a distance less than 1000 km from the vertical sounding station. The used foF2<br />

frequency hourly data were registered at the stations: Wakkanai, Akita , Kokubunji, and Yamagawa ()<br />

since 1957 until 1990. The authors find an increase in the variability of the foF2 frequency at time scale<br />

1-2 hours during 5-10 days before the event and the decrease in the variability of the foF2 frequency<br />

since the day before until a few days after an earthquake. Analyzing the diurnal behavior of the effect,<br />

they find that it occurs at day-time in periodbetween 11 h and 15 h LT. Diurnal variability depends on<br />

the season, on 11-years Solar variations circle, and on geomagnetic variations. In the work we use the<br />

data recorded in time intervals with weak heliomagnetic disturbances (Wolf number below 100 and Σ<br />

Kp< 30). The amplitude of the modification may be larger than 10%, and the statistical reliability of the<br />

effect amounts to more than 0.95. No effect is obtained for the strong earthquakes with depths more<br />

than 80 km. Also, no effect is found for weaker earthquakes with M

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