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      Near-source high-rate GPS, strong motion and InSAR observations to image the 2015 Lefkada (Greece) Earthquake rupture history

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          Abstract

          The 2015/11/17 Lefkada (Greece) earthquake ruptured a segment of the Cephalonia Transform Fault (CTF) where probably the penultimate major event was in 1948. Using near-source strong motion and high sampling rate GPS data and Sentinel-1A SAR images on two tracks, we performed the inversion for the geometry, slip distribution and rupture history of the causative fault with a three-step self-consistent procedure, in which every step provided input parameters for the next one. Our preferred model results in a ~70° ESE-dipping and ~13° N-striking fault plane, with a strike-slip mechanism (rake ~169°) in agreement with the CTF tectonic regime. This model shows a bilateral propagation spanning ~9 s with the activation of three main slip patches, characterized by rise time and peak slip velocity in the ranges 2.5–3.5 s and 1.4–2.4 m/s, respectively, corresponding to 1.2–1.8 m of slip which is mainly concentrated in the shallower (<10 km) southern half of the causative fault. The inferred slip distribution and the resulting seismic moment (M 0 = 1.05 × 10 19 N m) suggest a magnitude of M w 6.6. Our best solution suggests that the occurrence of large ( M w  > 6) earthquakes to the northern and to the southern boundaries of the 2015 causative fault cannot be excluded.

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                Author and article information

                Contributors
                antonio.avallone@ingv.it
                Journal
                Sci Rep
                Sci Rep
                Scientific Reports
                Nature Publishing Group UK (London )
                2045-2322
                4 September 2017
                4 September 2017
                2017
                : 7
                : 10358
                Affiliations
                [1 ]Istituto Nazionale di Geofisica e Vulcanologia, Centro Nazionale Terremoti, Via di Vigna Murata 605, Rome, 00143 Italy
                [2 ]Istituto Nazionale di Geofisica e Vulcanologia, sezione di Roma1, Via di Vigna Murata 605, Rome, 00143 Italy
                [3 ]ISNI 0000 0000 9463 1022, GRID grid.424955.b, Institute of Engineering Seismology and Earthquake Engineering (ITSAK-EPPO), ; P.O. Box 53, FInikas, Thessaloniki, 55102 Greece
                [4 ]Ecole Normale Supérieure, PSL Research University, Laboratoire de Géologie - UMR CNRS 8538, 24 Rue Lhomond, Paris, 75005 France
                [5 ]National Observatory of Athens, Institute of Geodynamics, P.O. Box 20048, Athens, 11810 Greece
                Author information
                http://orcid.org/0000-0002-0264-2897
                http://orcid.org/0000-0002-4144-3794
                http://orcid.org/0000-0002-0958-2129
                http://orcid.org/0000-0001-7378-0712
                http://orcid.org/0000-0002-0169-9197
                http://orcid.org/0000-0003-2863-3662
                http://orcid.org/0000-0001-6805-6295
                http://orcid.org/0000-0002-1937-3283
                Article
                10431
                10.1038/s41598-017-10431-w
                5583176
                28871096
                e80fed46-15f2-4a9e-bf6f-b4d29706b3e4
                © The Author(s) 2017

                Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 23 September 2016
                : 9 August 2017
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