PROBLEMS OF GEOCOSMOS

Proceedings of the 7th International Conference "Problems of Geocosmos" (St. Petersburg, Russia, 26-30 May 2008)
ABOUT NON-LINEAR DYNAMICS APPLIED TO DEPTH FRACTURES,
CONRTOLLING HIGH SEISMICITY AREAS IN DAGHESTAN
A.M. Boykov
Institute of Geothermal Problems of Daghestan Scientific Centre of RAS, Makchatchkala, 367030,
Russia, e-mail: buamama@yandex.ru
Abstract. Seismogenerating fractures are revealed in the surface temperature field by means of
anomalies of heat space survey. These anomalies are rather the processes of preparing for the
earthquakes. Our heat model of subvertical inter block zone for analysis of seismogene dynamics
corresponds Foothills fracture, which controls zones of high seismicity. Geological characteristics
of this fault correspond in details to a well-known seismodynamic model I.A.Volodin. This model
as well as the Foothills fracture, contains a zone of narrow plates, alternating with the fissures. The
fracture-resonator is the source of non-linear diffraction of Fraunhofer regarding the waveguide
seismic field. The seismic activation, whose source is the fracture-resonator of the seismic energy
is added by prolonged actions of seismic pulses in the limits of influence of the earthquakes
centers zones. The heat cosmic survey in the regime of observation is perfectly able, as it follows
from the given above, to have a sense of forcast. Therefore it is reasonable to carry it out with
these purposes in the Daghestan region in the future.
Seismogenerating fractures are revealed in the surface temperature, field by means of anomalies of heat
space survey (See fig.1). These anomalies are rather the processes of preparing for the earthquakes. These
Fig.1. Fragment of the map of the Caucasus earthquakes epicenters (the author – A.A.Godzikovskaya –
February 21, 2001). The black arrow points the disposition of the anomaly fragment of the cosmic survey
radiation temperatures, which we used to calculate the width of the Foothills fracture. (The anomaly extents
along the route of the Foothills fracture. The cosmic survey was made at night 21.07.98 at 3:07 Moscow
Time. The survey data processing was done by the method of lower frequency filtration with radius
R=0,7 km. The smoothing of the obtained data was done by the Gauss method – in the area from the centre
of picsel).
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