Seismic anisotropy reveals focused mantle flow around the Calabrian slab (Southern Italy)

被引:68
|
作者
Baccheschi, P. [1 ]
Margheriti, L.
Steckler, M. S.
机构
[1] Ist Nazl Geofis & Vulcanol, CNT, I-00143 Rome, Italy
[2] Ist Nazl Geofis & Vulcanol, CNT, Grottaminarda, Italy
[3] Lamont Doherty Earth Observ, Palisades, NY USA
关键词
D O I
10.1029/2006GL028899
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
SKS splitting at the Calabrian subduction zone, with delay times (delta t) up to 3s, reveals the presence of a strong anisotropic fabric. Fast directions (phi) are oriented NNE-SSW in the Calabrian Arc ( C. A.) and rotate NNW-SSE to the north following the arcuate shape of the subducting plate. We interpret the trench-parallel phi as local-scale mantle flow driven by the retrograde motion of the slab; the absence of trench perpendicular f below the Southern Apennines (S. A.) excludes the presence of a seismically detectable return flow at its NE edge. This may be due to the relative youth and limited width of the S. A. slab tear. A possible return flow is identified farther north at the boundary of the S. A. and Central Apennines. Different and weaker anisotropy is present below the Apulian Platform ( A. P.). This implies that the influence of the slab rollback in the sub-slab mantle is limited to less then 100 km from the slab.
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页数:6
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