On the growth of normal faults and the existence of flats and ramps along the El Asnam active fold and thrust system
- Creators
-
Avouac, J. P.
- Meyer, B.
- Tapponnier, P.
Abstract
The combination of detailed topographic leveling on the southwest segment of the El Asnam thrust fault with existing seismic and geologic data implies that the geometry of this fault involves shallow dipping flats and steep ramps. The fault appears to be growing along strike toward the southwest end, where the main shock initiated in 1980. From a depth of about 10 km, the main thrust appears to ramp to the basement-Cenozoic cover interface on a plane striking N40°E and dipping 50°–55° to the northwest. Along the southwest segment where folding has not yet developed, the thrust continues steeply through the Cenozoic cover to the near surface where it flattens, causing normal faulting. Along the central and northeast segments, which display a more evolved fold structure, the deep thrust probably flattens at a depth of 5–6 km, into a decollement along the Cenozoic-Jurassic interface before ramping to the surface. The Sara El Marouf and Kef El Mes anticlines have thus formed as fault propagation folds. Normal faults at Beni Rached probably branch with the thrust to maintain kinematic compatibility between the deep ramp and decollement. The greater separation (∼7 km) between the normal faults at Beni Rached and the thrust where it crosses Oued Cheliff than along the southwest segment (∼1 km) reflects the greater depth of the ramp to flat bend. We infer that the September 9, 1954, earthquake activated only the central deep segment of the main thrust together with the Beni Rached normal faults, while that of October 10, 1980, activated the whole system of flat decollements, ramp thrusts and compatibility normal faults. Further complexities of the faulting in map view are related to changes of strike of the thrust (in particular north of Oued Cheliff).
Additional Information
© 1992 American Geophysical Union. Received September 7, 1990; revised April 23, 1991. Accepted June 4, 1991. This work was supported by the Institut National des Sciences de l'Univers (INSU) and by the Centre de Recherche d'Astronomie, d'Astrophysique et de Geophysique (CRAAG). We thank M. Meghraoui for his help in the field and D. Hatzfeld for providing the aftershocks files. We also thank B. Slemmons, who drew attention to the small width of the aftershocks zone under 6 km, one anonymous referee for constructive reviews, and Rolando Armijo for discussions. An early draft benefited from Ross Stein's comments. Special thanks are due to Guy Aveline for the illustration. This is IPGP contribution 1190.Attached Files
Published - Avouac_MeyerTectonics_1992.pdf
Files
Name | Size | Download all |
---|---|---|
md5:ed68d2bbf846a21b1f6d31e9a66918de
|
782.8 kB | Preview Download |
Additional details
- Eprint ID
- 33966
- Resolver ID
- CaltechAUTHORS:20120910-114313483
- Institut national des sciences de l'Univers (INSU)
- Centre de Recherche d'Astronomie, d'Astrophysique et de Geophysique (CRAAG)
- Created
-
2012-09-10Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Seismological Laboratory, Division of Geological and Planetary Sciences (GPS)
- Other Numbering System Name
- IPGP
- Other Numbering System Identifier
- 1190