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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 />

JSS013 Oral Presentation 2220<br />

Crust and upper mantle anisotropy in the Central Alborz Region<br />

Dr. Ahmad Sadidkhouy<br />

Seismology Institute of Geophysics, Tehran University<br />

Gholam Javan Doloei<br />

During the last 3 decades, the determination of anisotropy is a subject of interest for seismologists. In<br />

this study, we investigated anisotropy by shear wave splitting of Ps and SKS phases on broadband and<br />

short period seismograms. When a shear wave propagates through an anisotropic medium, energy is<br />

partitioned into orthogonally polarized fast and slow shear waves. This property is referred to as shear<br />

wave splitting. In this study we used shear wave splitting of Moho Ps and SKS phases from teleseismic<br />

to identify and estimate the shear wave anisotropy in the crust and upper mantle of the Alborz region<br />

(IRAN). The use of Moho Ps phase to study anisotropy is potentially valuable since it is one of the few<br />

ways to isolate the lower crust in the study of anisotropy. The SKS phase is a good tool for determining<br />

of anisotropy because in an isotropic medium, there is no SKS energy on the transverse component so<br />

that the presence of transverse energy indicates the rate of anisotropy. In this study, we selected<br />

teleseismic events ( & for shear wave splitting of Ps method and for shear wave splitting of SKS<br />

method) which were recorded in 3 broadband seismic stations, DAMV, CHTH and THKV (International<br />

Institute of Earthquake Engineering and Seismology (IIEES)) and also 6 short period seismic stations,<br />

FIR, DMV, AFJ, SHR, MHD and GZV (Institute of Geophysics, Tehran University, (IGTU)) for determining<br />

anisotropy parameters in crust and upper mantle of the Alborz region. The majority of receiver functions<br />

showed two different Ps phases before Moho Ps on radial component. We believed in that the first Ps<br />

phase is generated in the upper crust (h

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