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Present-day dynamic and residual topography in Central Anatolia

  • Ebru Şengül Uluocak*
  • , Russell Pysklywec
  • , Oğuz H. Göğüş
  • *Bu çalışma için yazışmadan sorumlu yazar
  • Canakkale Onsekiz Mart University
  • University of Toronto

Araştırma sonucu: Dergiye katkıMakalebilirkişi

31 Atıf (Scopus)

Özet

The Central Anatolian orogenic plateau is represented by young volcanism, rapid plateau uplift and distinctive (past and active) tectonic deformation. In this study, we consider observational data in terms of regional present-day geodynamics in the region. The residual topography of Central Anatolia was derived to define the regional isostatic conditions according to Airy isostasy and infer the potential role of 'dynamic topography'. 2-D thermomechanical forward models for coupled mantle-lithosphere flow/deformation were conducted along an N-S directional profile through the region (e.g. northern/Pontides, interior and southern/Taurides). These models were based on seismic tomography data that provide estimates about the present-day mantle thermal structure beneath the Anatolian plate. We compare the modelling results with calculated residual topography and independent data sets of geological deformation, gravity and high surface heat flow/widespread geothermal activity. Model results suggest that there is ~1 km of mantle flow induced dynamic topography associated with the sublithospheric flow driven by the seismically inferred mantle structure. The uprising mantle may have also driven the asthenospheric source of volcanism in the north (e.g. Galatia volcanic province) and the Cappadocia volcanic province in the south while elevating the surface in the last 10 Myr. Our dynamic topography calculations emphasize the role of vertical forcing under other orogenic plateaux underlain by relatively thin crust and low-density asthenospheric mantle.

Orijinal dilİngilizce
Sayfa (başlangıç-bitiş)1515-1525
Sayfa sayısı11
DergiGeophysical Journal International
Hacim206
Basın numarası3
DOI'lar
Yayın durumuYayınlandı - 1 Eyl 2016

Bibliyografik not

Publisher Copyright:
© The Authors 2016. Published by Oxford University Press on behalf of The Royal Astronomical Society.

Finansman

ACKNOWLEDGEMENTS Authors acknowledge support from TUBITAK Visiting Scientist fellowship programme. RP acknowledges funding from an NSERC Discovery Grant. Numerical calculations were done using a modified version of the SOPALE (2000) software. The SOPALE modelling code was originally developed by Phillip Fullsack at Dalhousie University with Chris Beaumont and his Geodynamics group. We thank the anonymous reviewers and Laurent Husson for their useful comments and contributions to the manuscript.

Finansörler
TUBITAK
Natural Sciences and Engineering Research Council of Canada

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