REGIONAL MAGMA FLOW IN SILLS OF THE KAROO LIP, SOUTH AFRICA
Magnetic fabrics, such as the anisotropy of magnetic susceptibility (AMS), provide an effective and accurate mean to determine magma flow direction in mafic intrusive rocks. A previous study had shown that the AMS fabric is a reliable proxy for magma flow as long as samples are collected from the upper chilled margin of a sill. The central part of sills is more complex due to interference caused by thermal convection and inverse magnetic fabrics. Oriented core samples were collected from 30 sills and yielded 1598 specimens for AMS measurements. The low-field magnetic susceptibility Km ranges widely from about 100 to 20,000 microSI, while the degree of anisotropy P' ranges from 1.01 to 1.10. Thermomagnetic experiments reveal that the main magnetic carrier is titanomagnetite with variable ulvöspinel content and pseudo-single domain grain size.
Our results show that magma flow followed a main NW-SE direction in the Karoo Basin. The AMS axes are consistent with the nearly horizontal attitude of the sill in 23 out of 30 sills, with subvertical K3 axes. In 5 out of 30 sills, K3 axes are subhorizontal, with scattered directional data and are considered anomalous AMS fabrics. K1 axes are systematically subhorizontal and mark the magma flow direction. This regional scale flow pattern indicates that the Karoo LIP maximum magma flow was not located under the Drakensberg basalts, which are the thickest part of the Karoo volcanic pile. Instead the center of magmatic activity was most likely located to the NW of the Karoo Basin, somewhere in what is today Namibia.