@article{d0276410a2424318bb6b3db8af546e35,
title = "Strain Field Associated With a Component of Divergent Motion Along the Southern Dead Sea Fault: Insights From Magnetic Fabrics",
abstract = " In order to reconstruct the strain field along the southern segment of the Dead Sea Fault (DSF) plate boundary, we analyzed the magnetic fabrics of carbonate rocks, outcropping along it. The magnetic fabrics provide a microstructural indicator that help to approximate the principal strain directions in the rocks. Our analysis includes ~900 cores from 58 sampling localities, along ~400 km of the southern DSF. We measured the magnetic fabrics of (1) pure calcite-bearing limestones that consist diamagnetic fabrics and (2) chalks with composite fabrics, which we further separated into diamagnetic and paramagnetic subfabrics, using measurements of Anisotropy of Magnetic Susceptibility at low temperatures. The results show that 87% of the diamagnetic fabrics and subfabrics are of tectonic origin. The orientations of the maximum Anisotropy of Magnetic Susceptibility axes (K 3 axes) approximately align with the maximum horizontal shortening directions along the southern segment of the DSF, differ from the remote stress direction, and are largely parallel to the main trace of the DSF. This parallelism is not related to local variations in the geometry of the faults. We suggest that the deflection of the maximum horizontal shortening parallel to the transform plate boundary is a kinematic consequence of the Sinai-Arabia relative plate motion, which expresses a component of divergence along the southern segment of the DSF. We conclude that magnetic fabrics of carbonate rocks are sensitive and reliable microstructural indicators for determination of the strain field along major fault systems.",
keywords = "Dead Sea fault, LT-AMS, anisotropy of magnetic susceptibility (AMS), magnetic fabrics, tectonics, transform faults",
author = "R. Issachar and T. Levi and S. Marco and R. Weinberger",
note = "Funding Information: This study was supported by grants from the Israel Science Foundation 1245/11 and 868/17 to R.W., Israel Science Foundation Center of Excellence grant 1436/14 to S.M., the Israeli Ministry of Energy, and the Naomi Foundation through the Tel Aviv University GRTF Program. We wish to thank the Institute for Rock Magnetism (IRM) for hosting and supporting RI during the course of this study; especially we wish to thank Mike Jackson, Dario Bilardello, and Andrea Biedermann for fruitful discussions and help. The IRM is funded by the NSF Instruments and Facilities program and by the University of Minnesota. We thank Ron Shaar and Yael Ebert for their kind collaboration and help. The assistance in the field of Daniel Zvi, Ran Benyamin, Asaf Ido, Iyad Swaed, Oria Vanunu, and Misha Kitin is highly appreciated. We thank Yehudit Harlavan for her help in analyzing the geochemical data. We thank two anonymous reviewers for providing constructive and very helpful reviews. All the data used for this study are accessible by contacting the authors at ranissachar@gmail.com and available online at https://figshare.com. Funding Information: This study was supported by grants from the Israel Science Foundation 1245/11 and 868/17 to R.W., Israel Science Foundation Center of Excellence grant 1436/14 to S.M., the Israeli Ministry of Energy, and the Naomi Foundation through the Tel Aviv University GRTF Program. We wish to thank the Institute for Rock Magnetism (IRM) for hosting and sup porting RI during the course of this study; especially we wish to thank Mike Jackson, Dario Bilardello, and Andrea Biedermann for fruitful discussions and help. The IRM is funded by the NSF Instruments and Facilities program and by the University of Minnesota. We thank Ron Shaar and Yael Ebert for their kind collaboration and help. The assistance in the field of Daniel Zvi, Ran Benyamin, Asaf Ido, Iyad Swaed, Oria Vanunu, and Misha Kitin is highly appreciated. We thank Yehudit Harlavan for her help in analyzing the geochemical data. We thank two anonymous reviewers for providing constructive and very helpful reviews. All the data used for this study are accessible by contacting the authors at ranis-sachar@gmail.com and available online at https://figshare.com. Publisher Copyright: {\textcopyright}2018. American Geophysical Union. All Rights Reserved.",
year = "2019",
month = jan,
day = "1",
doi = "10.1029/2018TC005168",
language = "English",
volume = "38",
pages = "335--353",
journal = "Tectonics",
issn = "0278-7407",
publisher = "Wiley-Blackwell",
number = "1",
}