This is a copy of an extended abstract, ISAG (International Symposium on Andean Geodynamics) meeting in Barcelona, Catalunya, Sept. 2005. A newer  article is: 

Brasse, H. & Eydam, D. (2008): Electrical conductivity beneath the Bolivian Orocline and its relation to subduction processes at the South American continental margin, J. Geophys. Res., 113, B07109, doi:10.1029/2007JB005142.

 

The mantle wedge in the Bolivian orocline in the view of deep electromagnetic soundings

Heinrich Brasse, Fachrichtung Geophysik, FU Berlin, Malteserstr. 74-100, D-12249 Berlin, Germany

 

KEY WORDS: electrical conductivity, magnetotellurics, mantle wedge, central Andes

 

ABSTRACT

Long-period electromagnetic soundings were carried out in the central Andes on a profile from the Eastern Cordillera south of La Paz over the Altiplano and the volcanic arc until the Longitudinal Valley in Northern Chile south of Arica. Besides the asymmetric Cenozoic, well-conducting basin structures in the central part of the high plateau, a major anomaly was found in the upper mantle which is tentatively interpreted as imaging fluid- and melt-related processes due to fluid release from the downgoing slab. The reasons for the unexpectedly high conductivities and the position well east of the actual volcanic arc will be discussed in this contribution.

 

The MT experiment

Motivated by earlier findings of a large zone of high electrical conductivity below the southern Altiplano (Ancorp profile, cf. Brasse et al. 2002) a comparative magnetotelluric (MT) study was performed in 2002 (continued in 2004) along a profile extending from the Eastern Cordillera over the central Altiplano and the Western Cordillera until the forearc in North Chile (Fig. 1). Spacing between stations was on the average 10 km and data were recorded in a period range from 10-20.000 s, yielding approximate penetration depths from 5-200 km, depending on sub­soil conductivity. The profile direction is approx. 45° and thus roughly perpendicular to the strike of main struc­tural features in this area of the Bolivian orocline as well as to the contour lines of the Wadati-Benioff zone, inferred from Cahill and Isacks (1992). Topography and unaccessibility prohibited the continuation of the profile further into the Eastern Cordillera; in addition the sharp rise of the Western Cordillera Escarpment led to a, although minimal, gap in the profile. Distortion effects and deviations from two-dimensionality are low for most stations with the particular exception of sites PAT and OBS (near Patacamaya geomagnetic observatory), where the Coniri fault connects with the Laurani fault, and the forearc sites in North Chile.

Fig. 1: Shaded relief map of the western central Andes (based on SRTM-90m data) showing locations of recently measured MT sites in the Bolivian Orocline. The profile line is a great circle projection of the sites, while dotted lines mark the depth to the Wadati-Benioff zone after Cahill and Isacks (1992).

 

PRELIMINARY 2-D MODELING AND FIRST INTERPRETATION ATTEMPTS

It is a lucky and not often encountered circumstance that induction vectors, derived from purely magnetic transfer functions (the ratio of vertical to horizontal field variations Bz/Bh), point in the direction of the profile over much of the study area (again with exception of North Chile), permitting a 2-D interpretation of the data set at least over the whole Altiplano. This direction is also corroborated by a multi-site, multi-frequency strike analysis of MT transfer functions, employing a code by McNeice and Jones (2001). A 2-D inversion code (Rodi and Mackie 2001) was applied using a homogeneous halfspace as a starting model, incorporating also the well conducting Pacific Ocean as a-priori structure. The data inverted for were the magnetic transfer functions with addition of magnetotelluric responses sensu strictu (apparent resistivities and phases). By adapting respective error bounds the weight of phase data (reflecting the actual induction process) was enhanced during inversion; effects due to static distortion of apparent resistivity curves could thus be minimized. Numerous inversion tests were performed, including variation of starting models, inversion of TE, TM mode and Bz data separately and jointly, calculation of trade-off curves, sensitivity studies, etc.

The expectation concerning conductive structures below the Altiplano was to find a similar HCZ in the deeper crust as below the Ancorp profile at 21°S. The resulting model, however, looks strikingly different (Fig. 2). Near the surface the Cenozoic Corque Basin appears as a highly conductive, asymmetric structure (e.g., Hérail et al. 1997) together with adjacent minor basins. This was already reported by Ritz et al. (1991) who carried out a similar experiment; the depth range of their interpretation was limited to the crust, however, owing to the limited frequency range and the unavailability of vertical field transfer functions.

Fig. 2: Resistivity model from 2-D inversion. A - A' - A'': Corque and minor basins, B: deep crustal magma chamber below W. Cordillera?, C: imperpeable upper crustal block, D: Eastern Cordillera block (analog to Dorbath et al. 1993, Dorbath and Granet 1996), E: mantle wedge, F: rise of fluids/melts. Question marks refer to areas of low resolution and/or three-dimensionality. Data in the forearc were not taken into account.

 

The most spectacular feature of the model is a very good conductor in the upper mantle below the Altiplano at depths of approx. 120 km. From there a slightly less conductive structure is observed, rising to middle crust. A similar, but oblique and even less conductive branch reaches and underlies the western margin of the volcanic arc. A resistive block is modelled in the upper crust; also the margins of the model are resistive (i.e., below the forearc and the Eastern Cordillera), but naturally these resistivities are not well resolved due to lacking data coverage.

Although one might expect to image the mantle wedge as a good conductor, several of its features are surprising:

a) Conductivities are so high (in the order of 1 S/m) that a melt rate of at least 5% is needed. This contradicts many assumptions based, e.g., on seismological studies. Perhaps more saline fluids (usually thought to be more conductive then partial melt itself) then previously thought are involved. These high conductivies could, however, also be an effect caused by the 2-D approximation.

b) The shape resembles a dyke-like structure; this is, however, not well resolved and other geometries are possible, leaving the general characteristics concerning depth and position untouched.

c) The position of the conductor (in course agreement with a low-velocity zone detected by Dorbath and Granet 1996) well to the east of the volcanic arc is not in accordance with standard subduction scenarios. It must be taken into account, however, that we observe a momentary image only and that volcanism in this particular study area has recently been much less active then elsewhere in the Andes. One may speculate that we observe the initiazation of a new magmatic event or the feeding of a deep crustal magma reservoir similar to the one detected below the southern Altiplano.

 

ACKNOWLEDGMENTS

The Bolivian part of this study was carried out during my stay as guest lecturer at the Universidad Mayor de San Andrés (UMSA), La Paz, funded by the German Academic Exchange Service (DAAD). The help of F. Ticona and D. Eydam made the field campaigns a success. I thank E. Ricaldi (UMSA), H. Wilke (Universidad Católica del Norte, Antofagasta) and the German Embassy La Paz for logistical support, and the National Park authorities of Bolivia and Chile for the permit to work in Sajama and Lauca National Parks, respectively.

REFERENCES

Brasse, H., Lezaeta, P., Rath, V., Schwalenberg, K., Soyer, W., and Haak, V. (2002): The Bolivian Altiplano conductivity anomaly, J. Geophys. Res., 107 (B5), 10.1029/ 2001JB000391.

Cahill, T.A. and Isacks, B.L. (1992): Seismicity and the shape of the subducted Nazca Plate, J. Geophys. Res., 97 (B12), 17503-17529.

Dorbath, C., Granet, M., Poupinet, G., and Martinez, C. (1993): A teleseismic study of the Altiplano and the Eastern Cordillera in northern Bolivia: New constraints on a lithospheric model, J. Geophys. Res., 98 (B6), 9825-9844.

Dorbath, C. and Granet, M. (1996): Local earthquake tomography of the Altiplano and the Eastern Cordillera of northern Bolivia, Tectonophysics, 259, 117-136.

Hérail, G., Rochat, P., Baby, P., Aranibar, O., Lavenu, A., and Mascle, G. (1997): El Altiplano Norte de Bolivia, evolución geológica terciaria. In: R. Charrier, P. Aceituno, M. Castro, A. Llanos and L.A. Raggi (Eds.), El Altiplano: ciencia y conciencia en los Andes, Actas 2. Simposio Internacional Estudios Altiplánicos, Arica 1993. Universidad de Chile, Santiago de Chile, pp. 33-44.

McNeice, G.W. & Jones, A.G. (2001): Multi-site, multi-frequency tensor decomposition of magnetotelluric data, Geophysics, 66, 158-173.

Ritz, M., Bondoux, F., Hérail, G. and Sempere, T. (1991): A magnetotelluric survey in the northern Bolivian Altiplano, Geophys. Res. Lett., 18, 475-478.

Rodi, W. and Mackie, R.L. (2001): Nonlinear conjugate gradients algorithm for 2-D mag­neto­telluric inversions, Geophysics, 66, 174-187.