MUD VOLCANO FIELD SEAWARD OF THE BARBADOS ACCRETIONARY COMPLEX - A DEEP-TOWED SIDE SCAN SONAR SURVEY

被引:98
作者
HENRY, P
LEPICHON, X
LALLEMANT, S
FOUCHER, JP
WESTBROOK, G
HOBART, M
机构
[1] IFREMER, DEPT GEOSCI MARINES, F-29263 PLOUZANE, FRANCE
[2] COLUMBIA UNIV, LAMONT DOHERTY GEOL OBSERV, PALISADES, NY 10964 USA
[3] UNIV BIRMINGHAM, SCH EARTH SCI, BIRMINGHAM B15 2TT, W MIDLANDS, ENGLAND
来源
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS | 1990年 / 95卷 / B6期
关键词
D O I
10.1029/JB095iB06p08917
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A 30km2 diapiric field has been identified near 13°50′N up to 12km seaward of the deformation front of the Barbados accretionary complex. This field has been active for 200 000yr and that it is a transient feature triggered by the seaward propagation of the high pore fluid pressure associated with the decollement beneath the accretionary complex. The venting results in the formation of a stiff carbonate crust and of large subsiding basins around the mud pies. Continuous active fluid explusions through these structures indicates that an efficient piping system still connects them to the zone of anomalously high pore pressure below the protodecollement. -from Authors
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页码:8917 / 8929
页数:13
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