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Open Session - SWISS GEOSCIENCE MEETINGs

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Figure 1. Transtensional to extensional brittle evolution of the Lepontine dome with relative chronology between the different states of<br />

stress recorded, showing a rotation of around 90° of the extensional axes. Mean direction of σ3 axes calculated from previous studies on<br />

brittle deformation in the extended Central Alps are reported as follow: Bi: Bistacchi and Massironi (2000); Ch: Champagnac et al (2006); Ci:<br />

Ciancaleoni and Marquer (2008); Gr: Grosjean et al (2004).<br />

REFERENCES<br />

Allanic, C., et al. (2006), A paleo-seismogenic Lepontine dome? New insights from pseudotachylytes-generating faults,<br />

Geochimica et Cosmochimica Acta, Vol. 70 (18), Suppl. 1, p9 Goldschmidt conf. Melbourne.<br />

Bistacchi, A., and Massironi M. (2000), Post-nappe brittle tectonics and kinematic evolution of the north-western Alps: an<br />

integrated approach, Tectonophysics, 327, 267-292.<br />

Champagnac, J. D., Sue, C., Delacou, B., Burkhard, M. (2006), Miocene orogen-parallel extension in the inner Western Alps<br />

revealed by dynamical fault analyses, Tectonics, 25, 1-26.<br />

Ciancaleoni, L., and Marquer D. (2008), Late Oligocene to early Miocene lateral extrusion at the eastern borders of the<br />

Lepontine dome of the Central Alps (Bergell and Insubric areas, Eastern Central Alps), Tectonics, 27, TC4008, doi:10.1029/<br />

2007TC002196, 2008.<br />

Grosjean, G., Sue, C., Burkhard, M. (2004), Late Neogene brittle extension in the vicinity of the Simplon fault zone, central<br />

Alps, Switzerland., Eclogae Geologicae Helvetiae, 97, 33-46.<br />

1.2<br />

Origin of the magnetic anisotropy in a two marble lithologies from the<br />

Morcles Nappe shear zone<br />

Almqvist Bjarne*, Hirt Ann*, Herwegh Marco**<br />

*Institut für Geophysik, ETH Zurich, Schaffmattstrasse 30, CH-8093 Zurich (bjarne.almqvist@mag.ig.erdw.ethz.ch)<br />

**Institut für Geologie, Universität Bern, Baltzerstrasse 1-3, CH-3012 Bern<br />

Anisotropy of magnetic susceptibility (AMS) arises from the sum of ferromagnetic (sensu lato), paramagnetic and diamagnetic<br />

minerals in a rock. The AMS is generally controlled by the ferromagnetic and paramagnetic phases, since these have the<br />

strongest magnetic susceptibility. However, when the ferromagnetic contribution to the AMS is negligible, it may be possible<br />

to separate the paramagnetic and diamagnetic fabrics using high-field magnetic-torque measurements at room temperature<br />

and 77K. This is illustrated in a study of two marble lithologies from the Morcles Nappe shear zone. The AMS of the marbles<br />

are compared with that of a set of quartzites from the Navia-Alto Sil slate belt in northwestern Spain, which have been studied<br />

using the same technique.<br />

From the room temperature AMS studied in a weak magnetic field it is possible to distinguish each marble based on its bulk<br />

susceptibility and degree of anisotropy. Texture mapping using electron backscatter diffraction (EBSD) shows that the AMS<br />

is controlled by the microtexture of the marbles. High-field AMS measurements, performed at 77K, produce an anisotropy<br />

that is in some cases more than 100 times stronger than that measured at room temperature, indicating that paramagnetic<br />

phases contribute to the total AMS. Separation of the paramagnetic and diamagnetic fabrics shows an inversion of the AMS<br />

ellipsoid, from oblate and triaxial shapes at room temperature to strongly prolate shape at 77K. This is commonly seen in<br />

marbles from the shear and root zones of the Morcles Nappe, and can be attributed to the presence paramagnetic cations<br />

(e.g. Fe 2+ and Mn 2+ ) in the calcite crystal lattice (Figure 1). Further texture mapping together with determination of the chemical<br />

composition of the calcites and secondary phases in the marbles should help identify the origin of their magnetic<br />

anisotropy.<br />

In contrast, the diamagnetic quartzites have similar bulk susceptibility as the marbles, but are only a few times more anisotropic<br />

at low temperature as compared to the room temperature measurements. This suggests that the quartzites have an<br />

AMS with a significantly lower paramagnetic contribution, and that the inherent AMS of the quartzite is less than that of<br />

the marble.<br />

13<br />

Symposium 1: Structural Geology, Tectonics and Geodynamics

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