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Comment on “Zemmouri earthquake rupture zone (Mw 6.8, Algeria): Aftershocks sequence relocation and 3D velocity model” by A. Ayadi et al.
Jacques Déverchère, Bernard Mercier de Lépinay, A. Cattaneo, Pierre Strzerzynski, Eric Calais, Anne Domzig, Rabah Bracene

Comment on “Zemmouri earthquake rupture zone (Mw 6.8, Algeria): Aftershocks sequence relocation and 3D velocity model” by A. Ayadi et al.

Science & Mathematics Published 2010 Verification Pending

Overview & Synopsis

Although often difficult to characterize, the relationship between a seismic rupture, its aftershock sequence, and cumulative subsurface or surface faulting or folding is an important challenge to modern seismology and seismotectonics. Among other benefits, it helps document fault length, slip, and magnitude relationships, reconstruct the evolution of the rupture process through historical and prehistorical times and identify the complexity of the deformation in its path toward the surface. This approach is a prerequisite to any seismic hazard assessment but is particularly difficult for faults whose surface trace projects offshore. A specific effort to identify and quantify the source parameters of large earthquakes in coastal areas is therefore needed, not only in subduction zones but also in areas of slow rate and/or diffuse deformation.

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Document Information

Document Title Comment on “Zemmouri earthquake rupture zone (Mw 6.8, Algeria): Aftershocks sequence relocation and 3D velocity model” by A. Ayadi et al.
Author / Organization Jacques Déverchère, Bernard Mercier de Lépinay, A. Cattaneo, Pierre Strzerzynski, Eric Calais, Anne Domzig, Rabah Bracene
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2010
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-20789
Original Source Link Visit Source Page on hal.science »