THE OCEAN-CONTINENT BOUNDARY OFF THE WESTERN CONTINENTAL-MARGIN OF IBERIA .1. CRUSTAL STRUCTURE AT 40-DEGREES 30'N

被引:84
作者
WHITMARSH, RB [1 ]
MILES, PR [1 ]
MAUFFRET, A [1 ]
机构
[1] UNIV PARIS 06, DEPT GEOL DYNAM, F-75230 PARIS 05, FRANCE
关键词
continental margin; Iberia; North Atlantic; ocean–continent boundary; seismic structure;
D O I
10.1111/j.1365-246X.1990.tb01788.x
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The western continental margin of the Iberian peninsula has the characteristics of a rifted non‐volcanic margin with half‐graben and tilted fault blocks seen in several places. The ocean–continent boundary (OCB) is therefore expected to be where thinned continental crust and oceanic crust are juxtaposed, as at many similar margins worldwide. It is particularly useful to locate the OCB off western Iberia in order to constrain the pre‐rift fit of North America to Iberia and, by implication, the shape of the proto‐Bay of Biscay. The fit is only marginally constrained by sea‐floor spreading magnetic anomalies because anomaly 34 is believed to be far to the west of the OCB and it is even possible that all older oceanic crust was created during the Cretaceous constant polarity interval. The best way to distinguish oceanic crust from thinned continental crust appears to be the crustal seismic velocity structure. Therefore in 1986 a series of seismic refraction lines was shot parallel to, and normal to, the continental margin. These lines enabled us to bracket the location of the OCB. A further constraint on the location was obtained by modelling an east–west magnetic profile which included the enigmatic J‐anomaly. This anomaly can be explained as either just pre‐anomaly MO or as part of the Cretaceous constant polarity interval, depending on whether spreading began about 127 or after 118 Myr ago, respectively. The evidence favours the former explanation. Lastly the depth to acoustic basement was contoured from a compilation of seismic reflection profiles. This indicated a new fracture zone at 41°15'N which offsets the OCB. A few key reflection profiles also suggest that the OCB can be identified by an abrupt landward step‐down in acoustic basement. We conclude that the OCB in the eastern Iberia Abyssal Plain lies between 12°10’ and 12°30'W and has a trend just east of north. This westerly location is consistent with recent estimates of the location of the OCB off the Grand Banks but brings into question the proposed location at about 11°W of the OCB in the Tagus Abyssal Plain. Copyright © 1990, Wiley Blackwell. All rights reserved
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页码:509 / +
页数:1
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