Archaeoseismology and Palaeoseismology in the Alpine ... - Tierra
Archaeoseismology and Palaeoseismology in the Alpine ... - Tierra
Archaeoseismology and Palaeoseismology in the Alpine ... - Tierra
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CONCLUSIONS<br />
Analysis of <strong>the</strong> 1798 photographs recollected on <strong>the</strong><br />
Guadalquivir Diapiric Ridge <strong>and</strong> <strong>the</strong> Cadiz Contornite<br />
Channel <strong>in</strong> <strong>the</strong> Gulf of Cadiz has allowed to identify 5861<br />
chimneys ly<strong>in</strong>g scattered <strong>in</strong> dense concentrations over <strong>the</strong><br />
seabed. The fallen chimneys present a regular spatial<br />
distribution <strong>in</strong> a NW‐SE direction. The basal morphology<br />
of <strong>the</strong>m shows common characteristics of an angular<br />
breakage associated with flexo‐traction processes. These<br />
characters are very significant because <strong>the</strong>y are a strong<br />
<strong>in</strong>dication for <strong>the</strong> seismic orig<strong>in</strong> of chimneys rupture.<br />
On <strong>the</strong> basis of <strong>the</strong> geological characteristics of <strong>the</strong> area<br />
<strong>and</strong> <strong>the</strong> mechanical properties of <strong>the</strong> carbonate chimneys<br />
it has been determ<strong>in</strong>ed from ground motion prediction<br />
equations a first order approximation to <strong>the</strong> most likely<br />
seismic scenario. We have particularly looked at two<br />
different scenarios: (A) an earthquake produced by a fault<br />
located right under <strong>the</strong> chimneys field (Rjb=0 km) with a<br />
m<strong>in</strong>imum Mw 7.2; <strong>and</strong>, (B) an earthquake located about 6<br />
km far from <strong>the</strong> chimneys field with a Mw=7.8<br />
earthquake. Probably this fault was <strong>the</strong> Guadalquivir Bank<br />
Fault, that present a NE‐SW trend <strong>and</strong> it is very close of<br />
<strong>the</strong> study area.<br />
Acknowledgements: We thank all those who participated <strong>in</strong> <strong>the</strong><br />
research cruises of <strong>the</strong> TASYO project, especially <strong>the</strong> Ma<strong>in</strong><br />
Researches of TASYO project, Luis Somoza (Instituto Geológico y<br />
M<strong>in</strong>ero de España, IGME) <strong>and</strong> Victor Díaz‐del‐Río (Instituto<br />
Español de Oceanografía, IEO) <strong>and</strong> <strong>the</strong> capta<strong>in</strong>s <strong>and</strong> crews of <strong>the</strong><br />
research vessel R/V Cornide de Saavedra. This research was<br />
funded by <strong>the</strong> Spanish Mar<strong>in</strong>e Science <strong>and</strong> Technology Program,<br />
under <strong>the</strong> CONTOURIBER Project CTM2008‐06399‐C04‐01/MAR.<br />
It is also a contribution to <strong>the</strong> project CONSOLIDER‐INGENIO<br />
2010 CSD2006‐0041‐TOPOIBERIA.<br />
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