ANISOTROPY OF MAGNETIC-SUSCEPTIBILITY IN THE PONTA-GROSSA DYKE SWARM (BRAZIL) AND ITS RELATIONSHIP WITH MAGMA FLOW DIRECTION

被引:89
作者
RAPOSO, MIB
ERNESTO, M
机构
[1] Instituto Astronômico e Geofísico, University of São Paulo, 01065-970 São Paulo
基金
巴西圣保罗研究基金会;
关键词
D O I
10.1016/0031-9201(94)02970-M
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
Measurements of anisotropy of magnetic susceptibility (AMS) in 95 mafic dykes (mainly tholeiites 10-200 m in width) from the Mesozoic Ponta Grossa swarm, Southern Brazil, revealed two main types of magnetic fabric. Type I fabric (plane K1-K2 parallel to the dyke plane) represents magma flow within the dykes, whereas Type II (plane K1-K3 parallel to the dyke plane) is compatible with a fabric pattern reflecting vertical compaction of the magma column. Fabric Type I dominates (51% of the dykes) within the swarm, whereas Type II (38% of the dykes) concentrates mainly in the western region where the dykes intrude sediments. Considering the dykes with Type I fabrics, it is concluded that 58% of the dykes were fed by horizontal or sub-horizontal (K1 inclinations less than 30-degrees) magmatic flow, and 42% were fed by inclined to vertical (K1 inclinations more than 30-degrees) magma flow. The latter are more frequent in the southeastern part of the swarm, suggesting a magma source close to this area, although there may have been other sources in other regions where dykes with inclined flow and distinct chemical characteristics are also found.
引用
收藏
页码:183 / 196
页数:14
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