Broad accommodation of rift-related extension recorded by dyke intrusion in Saudi Arabia
AuthorsPallister, John S.
McCausland, Wendy A.
Zahran, Hani M.
El-Hadidy, Salah Y.
Stewart, Ian C F
Lundgren, Paul R.
White, Randal A.
Moufti, Mohammed Rashad H
KAUST DepartmentCrustal Deformation and InSAR Group
Earth Science and Engineering Program
Environmental Science and Engineering Program
Physical Sciences and Engineering (PSE) Division
Permanent link to this recordhttp://hdl.handle.net/10754/561537
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AbstractThe extensive harrat lava province of Arabia formed during the past 30 million years in response to Red Sea rifting and mantle upwelling. The area was regarded as seismically quiet, but between April and June 2009 a swarm of more than 30,000 earthquakes struck one of the lava fields in the province, Harrat Lunayyir, northwest Saudi Arabia. Concerned that larger damaging earthquakes might occur, the Saudi Arabian government evacuated 40,000 people from the region. Here we use geologic, geodetic and seismic data to show that the earthquake swarm resulted from magmatic dyke intrusion. We document a surface fault rupture that is 8 km long with 91 cm of offset. Surface deformation is best modelled by the shallow intrusion of a north-west trending dyke that is about 10 km long. Seismic waves generated during the earthquakes exhibit overlapping very low- and high-frequency components. We interpret the low frequencies to represent intrusion of magma and the high frequencies to represent fracturing of the crystalline basement rocks. Rather than extension being accommodated entirely by the central Red Sea rift axis, we suggest that the broad deformation observed in Harrat Lunayyir indicates that rift margins can remain as active sites of extension throughout rifting. Our analyses allowed us to forecast the likelihood of a future eruption or large earthquake in the region and informed the decisions made by the Saudi Arabian government to return the evacuees. © 2010 Macmillan Publishers Limited. All rights reserved.
SponsorsThis work is the result of a joint effort of the Saudi Arabian Geological Survey (SGS), and the US Geological Survey (USGS), conducted with the assistance of the US Consulate, Jeddah, Saudi Arabia. We thank many SGS colleagues (too numerous to list individually here) who participated in field and laboratory work and contributed to the success of the crisis response. We also acknowledge support to the Volcano Disaster Assistance Program provided by USAID's Office of Foreign Disaster Assistance and the USGS Volcano Hazards Program, and we thank SGS President Z. Nawab for facilitating our work together. Original Envisat radar raw data are copyrighted by the European Space Agency (ESA) and were provided by ESA. We also acknowledge the Nature Geoscience reviewers and editor Whitchurch, whose contributions substantially improved this paper.