Abstract
By using P and S wave receiver functions and P and S wave travel time residuals, we have found velocity models for 16 seismograph stations in Eastern Anatolia. Our study is focused mainly on the mantle lithosphere, asthenosphere and transition zone. The volcanism and uplift of the Eastern Anatolia Plateau are thought to be related to the Bitlis slab break off and delamination of the continental lithosphere. Sinking cold slab and lithospheric drips can reduce temperature in the mantle transition zone (MTZ) by up to a few hundred degrees C. However, our analysis of seismic data provides no robust evidence of significant cooling of the transition zone. In the mantle immediately above the 410-km discontinuity there is a pronounced low S wave velocity layer that may be a source of the volcanism in the study region. Another low velocity layer is present at the base of the MTZ. The obtained S wave velocity models of the upper mantle can be divided into three groups. In the first group, the lithosphere—asthenosphere boundary (LAB) is at a depth of ~ 60 km. In the second group, the LAB is at a depth from 90 to 100 km. In the third group, the mantle lithosphere is practically absent. On a scale of our analysis there is no clear correspondence between the obtained mantle velocity models and the volcanism (< 23 Ma) exposed at the surface. Only the models of the first group are well represented in the neighboring Central Anatolian Plateau.
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Acknowledgements
This study was conducted in the framework of a joint project supported by the Scientific and Research Council of Turkey (TÜBİTAK, project no. 111Y190) and as part of a state contract of IPE RAS (project no. 12_05_91373_ST_a).The seismic data are obtained from KOERI (Kandilli Observatory and Earthquake Research Institute) and from ETSE (Eastern TurkeySeismic Experiment) where seismograms are provided by IRIS-DMC. The Rayleigh wave dispersion curves are provided by the Center for Imaging the Earth’s Interior, University of Colorado, Boulder, US. The seismograms were analyzed by the Seismic Handler software by K. Stammler. Some figures were plotted with the GMT software tools by Wessel and Smith 1998. Authors appreciate help from Yusuf Arif Kutlu during the TÜBİTAK project management. We dedicate this study to our team member Grigory Kosarev, who recently passed away.
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Fig.1s.
The same as in Fig.3 but for stations ERZN and PTK. (PDF 1443 KB)
Fig.2s.
Effect of the teleseismic residuals for stations MALT and SVRC. Posterior distributions of the free model parameters Vp, Vs and Vp/Vs are shown by color code. The velocities of the IASP91 model and limits of the search are shown by black and red lines, respectively; the medians are shown by dash lines. The LAB is marked by red arrow. The statistics of the modeled receiver functions are shown by the same color code; the actual receiver functions are shown by dash lines. The data with and without the teleseismic residuals are shown on the left-hand side and right-hand side respectively. (PDF 2139 KB)
Fig.3s.
Effects of starting models for station AGRB. Posterior distributions of the free model parameters Vp, Vs and Vp/Vs are shown by color code. The velocities of the IASP91 model and limits of the search are shown by black and red lines, respectively; the medians are shown by dash lines. The LAB is marked by the red arrow. The statistics of the modeled receiver functions are shown by the same color code; the actual receiver functions are shown by dash lines. The four final models differ by the starting models in the inversion procedure. (PDF 2005 KB)
Fig.4s.
The same as in Fig. 2s, but for station MALT. (PDF 2135 KB)
Fig.5s.
Effects of the fixed velocities at the depth of 300 km. Posterior distributions of the free model parameters Vp, Vs and Vp/Vs are shown by color code. The velocities of the IASP91 model and limits of the search are shown by black and red lines, respectively. The medians are shown by dash lines. The LAB is marked by the red arrow. The statistics of the modeled receiver functions are shown by the same color code; the actual receiver functions are shown by dash lines. The left-hand side model differs from the right-hand side one by the values of the fixed velocities at a depth of 300 km. The IASP91 model is on the left-hand side. 8.8 km/s and 4.8 km/s for Vp and Vs are on the right-hand side. (PDF 1692 KB)
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Erduran, M., Oreshin, S., Vinnik, L. et al. Mantle lithosphere, asthenosphere and transition zone beneath Eastern Anatolia. J Seismol 26, 265–281 (2022). https://doi.org/10.1007/s10950-022-10074-z
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DOI: https://doi.org/10.1007/s10950-022-10074-z