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A multidisciplinary investigation of the Notträsk Gabbro, northern Sweden

 

作者: Lennart Widenfalk,   Sten-ÅKe Elming,   Thomas Enmark,  

 

期刊: Geologiska Föreningen i Stockholm Förhandlingar  (Taylor Available online 1985)
卷期: Volume 107, issue 2  

页码: 109-126

 

ISSN:0016-786X

 

年代: 1985

 

DOI:10.1080/11035898509452623

 

出版商: Taylor & Francis Group

 

关键词: Gabbro;geology;geophysics;petrophysics;nickel;sulfide;magnetometry;gravity;palaeomagnetism;cumulate;Notträsk;northern Sweden;N6550 N6550 E2150 E2150

 

数据来源: Taylor

 

摘要:

The differentiated, sulfide-bearing gabbro near the city of Boden in northern Sweden has been investigated in order to get a plausible model for its formation, shape and age. The gabbro is associated with a major fault system along which several intrusive bodies occur. The largest of these has been traversed by a gravimetric, magnetometric and geological profile. The investigated intrusion is undeformed and oval-shaped and covers some 20 km2. The outer parts of the body consist of a norite in contact with older meatasediments and granites of varying age. Inside the norite occurs a magnetite-rich gabbro, which forms a ring around the centre of the massif, which in turn consists of leucogabbro-olivine gabbro. Fe, Ti and K are low in the centre where Mg and Cr have their highest contents. Impregnations of sulfides and a massive pyrrhotite vein with some 1 % Ni are located in the norite. A number of intrusion models have been tested by computer modelling combining gravimetric and magnetic field data. The most probable model seems to be a funnel-shaped body pointing downwards. The different gabbro types dip steeply inwards indicating vertical zones rather than horizontal. Palaeomagnetic measurements show that the intrusion has a similar orientation of magnetization as other gabbros of the Haparanda series in northern Sweden (1800–1900 Ga, Rb-Sr). Furthermore, the pole distributions show that the rock cooled slowly, which may indicate that the present outcrop is a deep part of an eroded intrusion. The massif is supposed to have been formed by a diapiric re-emplacement of primary horizontal cumulates formed in the sequence olivine gabbro-leucogabbro-magnetite-bearing gabbro-norite.

 

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