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Rupture kinematics of 2020 January 24 Mw6.7 Doǧanyol-Sivrice, Turkey earthquake on the East Anatolian Fault Zone imaged by space geodesy

  • Diego Melgar*
  • , Athanassios Ganas
  • , Tuncay Taymaz
  • , Sotiris Valkaniotis
  • , Brendan W. Crowell
  • , Vasilis Kapetanidis
  • , Varvara Tsironi
  • , Seda Yolsal-Çevikbilen
  • , Taylan Öcalan
  • *Bu çalışma için yazışmadan sorumlu yazar
  • University of Oregon
  • Institute of Geodynamics
  • University of Washington
  • National and Kapodistrian University of Athens
  • University of Patras
  • Yildiz Technical University

Araştırma sonucu: Dergiye katkıMakalebilirkişi

72 Atıf (Scopus)

Özet

Here, we present the results of a kinematic slip model of the 2020 Mw 6.7 Doǧanyol-Sivrice, Turkey Earthquake, the most important event in the last 50 yr on the East Anatolian Fault Zone. Our slip model is constrained by two Sentinel-1 interferograms and by 5 three-component high-rate GNSS (Global Navigation Satellite System) recordings close to the earthquake source. We find that most of the slip occurs predominantly in three regions, two of them at between 2 and 10 km depth and a deeper slip region extending down to 20 km depth. We also relocate the first two weeks of aftershocks and find a distribution of events that agrees with these slip features. The HR-GNSS recordings suggest a predominantly unilateral rupture with the effects of a directivity pulse clearly seen in the waveforms and in the measure peak ground velocities. The slip model supports rupture propagation from northeast to southwest at a relatively slow speed of 2.2 km s-1 and a total source duration of ∼20 s. In the absence of near-source seismic stations, space geodetic data provide the best constraint on the spatial distribution of slip and on its time evolution.

Orijinal dilİngilizce
Sayfa (başlangıç-bitiş)862-874
Sayfa sayısı13
DergiGeophysical Journal International
Hacim223
Basın numarası2
DOI'lar
Yayın durumuYayınlandı - 1 Kas 2020

Bibliyografik not

Publisher Copyright:
© 2020 The Author(s). Published by Oxford University Press on behalf of The Royal Astronomical Society.

Finansman

Athanassios Ganas and Vassilis Kapetanidis thank 'HELPOS- Hellenic Plate Observing System' (MIS 5002697) which is cofinanced by Greece and the European Union (European Regional Development Fund). TT and SY-Ç thank Istanbul Technical University Research Fund, the National Scientific and Technological Research Council of Turkey (TUBITAK), Turkish Academy of Sciences (TUBA) in the framework forYoung ScientistAward Program (TUBA-GEBIP), the Science Academy Chamber-Turkey (BAGEP), and the Alexander von Humboldt Foundation Research Fellowship Award for providing computing facilities and other relevant computational resources through Humboldt-Stiftung Follow-Up Programme.

Finansörler
Istanbul Technical University Research Fund
National Scientific and Technological Research Council of Turkey
Science Academy Chamber-Turkey
TUBA
TUBA-GEBIP
Alexander von Humboldt-Stiftung
European Commission
Türkiye Bilimsel ve Teknolojik Araştirma Kurumu
Türkiye Bilimler Akademisi
European Regional Development Fund

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