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  5. High-resolution seismic tomography across the 1980 (Ms 6.9) Southern Italy earthquake fault scarp
 
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High-resolution seismic tomography across the 1980 (Ms 6.9) Southern Italy earthquake fault scarp

Author(s)
Improta, L.  
Dipartimento di Fisica, Università di Napoli, Napoli, Italia  
Zollo, A.  
Dipartimento di Fisica, Università di Napoli, Napoli, Italia  
Bruno, P. P.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia  
Herrero, A.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione OV, Napoli, Italia  
Villani, F.  
Dipartimento di Scienze della terra, Università di Napoli, Napoli, Italia  
Language
English
Status
Published
Peer review journal
Yes
Journal
Geophysical Research Letters  
Issue/vol(year)
30/10-1494 (2003)
Date Issued
2003
DOI
10.1029/2003GL017077, 2003
URI
https://www.earth-prints.org/handle/2122/2045
Subjects
04. Solid Earth::04.06. Seismology::04.06.07. Tomography and anisotropy  
Subjects

computational methods...

tomography

paleoseismology

seismic hazard assess...

fractures and faults

surface faulting

Abstract
A high-resolution multi-fold wide-angle seismic
survey carried out across the Irpinia fault, Southern Italy,
yields new information about the shallow structure of this
normal fault that was reactivated in 1980. The fault zone is
imaged to a depth of about 60 m by using a non-linear
tomographic technique that is specially designed to image
strongly heterogeneous media. Results confirm the location
of the fault, as previously inferred by a trench excavated in
soft soils, and clearly delineates a 30–35 m step in the
bedrock. This single step is indicative of a narrow fault
zone, which corresponds upward to warped soils exposed in
the trench, thus demonstrating that the near-surface warping
is directly related to a brittle faulting in the bedrock.
Assuming that the vertical slip rate yielded by paleoseismic
data (0.25–0.35 mm/yr) has been constant since the fault’s
inception, the latter should date back to about 100–140 kys
ago. Such a young age may explain why the Irpinia fault is
not associated with evident, large-scale geomorphic
indicators of its activity.
References
Amato, A., and P. Montone, Present day stress field and active tectonics in
southern peninsular Italy, Geophys. J. Int., 130, 519– 534, 1997.

Ascione, S., A. Cinque, L. Improta, and F. Villani, Late quaternary faulting
within the Southern Apennines seismic belt: New data from the Mt. Mar-zano
area (Southern Italy), Quaternary Int., 99-101-102, 27– 41, 2003.

D’Addezio, G., D. Pantosti, and G. Valensise, Paleoearthquakes along the
Irpinia fault at the Pantano di San Gregorio Magno (southern Italy),
Quaternario, 4(1a), 121– 136, 1991.

Dolan, J. F., and T. L. Pratt, High resolution seismic reflection profiling of
the Santa Monica fault zone, West Los Angeles, California, Geophys.
Res. Lett., 24(16), 2051– 2054, 1997.

Guadagno, F. M., and C. Nunziata, Seismic velocity of fractured carbonate
rocks (Southern Apennines Italy), Geophys. J. Int., 113, 739– 746, 1993.

Herrero, A., L. Improta, A. Zollo, P. Dell’Aversana, and S. Morandi, 2-D
Nonlinear traveltime tomography by multi-scale search: Imaging an over-thrust
structure in the Southern Apennines, AGU 2000 Fall Meeting, Eos
Trans. AGU, 81, 418, 910, 2000.

Improta, L., A. Zollo, A. Herrero, M. R. Frattini, J. Virieux, and
P. Dell’Aversana, Seismic imaging of complex structures by non-linear
traveltime inversion of dense wide-angle data: Application to a thrust belt,
Geophys. J. Int., 151, 264–278, 2002.

Jackson, J. A., and D. P. McKenzie, The relationship between plate motions
and seismic moment tensor, and the rates of active deformation in the
Mediterranean and Middle East, Geophys. J., 93, 45– 73, 1988.

Mazzotti, A. P., E. Stucchi, G. L. Fradelizio, L. Zanzi, and P. Scandone,
Seismic exploration in complex terrains: A processing experience in the
Southern Apennines, Geophysics, 65(5), 1402–1417, 2000.

Miller, K. C., S. H. Harder, D. C. Adams, and T. O’Donnell, Integrating
high-resolution refraction data into near-surface seismic reflection data
processing and interpretation, Geophysics, 63, 1339– 1347, 1998.

Morey, D., and G. T. Schuster, Paleoseismicity of the Oquirrh fault, Utah,
from shallow seismic tomography, Geophys. J. Int., 138, 25–35, 1999.

Pantosti, D., and G. Valensise, Faulting mechanism and complexity of the
November 23, 1980, Campania-Lucania earthquake, inferred from sur-face
observations, J. Geophys. Res., 95(15), 319– 341, 1990.

Pantosti, D., D. P. Schwartz, and G. Valensise, Paleoseismolgy along the
1980 surface rupture of the Irpinia fault: Implications for earthquake
recurrence in the Southern Apennines, Italy, J. Geophys. Res., 98(B4),
6561– 6577, 1993.

Podvin, P., and I. Lecomte, Finite difference computation of traveltimes in
very contrasted velocity model: A massively parallel approach and its
associated tools, Geophys. J. Int., 105, 271–284, 1991.

Schwartz, D. P., and K. J. Coppersmith, Fault behavior and characteristic
earthquake: Examples from the Wasatch and San Andreas fault zones,
J. Geophys. Res., 89, 5681– 5698, 1984.
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