Elsevier

Gondwana Research

Volume 89, January 2021, Pages 168-176
Gondwana Research

Receiver function investigation of crustal structure in the Malawi and Luangwa rift zones and adjacent areas

https://doi.org/10.1016/j.gr.2020.08.015Get rights and content

Highlights

  • Crustal thickness and Vp/Vs of the Malawi rift zone (MRZ) and nearby areas are mapped

  • A crustal stretching factor of about 1.05–1.08 is revealed beneath the non-volcanic MRZ

  • High Vp/Vs (≥ 1.81) beneath the southern MRZ may indicate crustal partial melting

  • Infiltration of magma-derived CO2 may cause the observed low Vp/Vs in northern MRZ

  • Normal crustal thickness and Vp/Vs suggest a complete recovery of Luangwa rift

Abstract

Stacking over 2300 P-to-S receiver functions recorded by 33 SAFARI (Seismic Arrays for African Rift Initiation) broadband seismic stations that we installed in the vicinity of the Malawi and Luangwa rift zones (MRZ and LRZ, respectively) reveals significant variations of crustal thickness (32.8–46.3 km) and Vp/Vs (1.69–1.85). The resulting crustal stretching factor is about 1.05–1.08 for the MRZ, which is approximately 10–40% lower than that observed in the mature segments of the East African Rift System (EARS). The low stretching factor is consistent with the general absence of volcanism in the MRZ, and the relatively high Vp/Vs (≥ 1.81) beneath the southern MRZ, when combined with observations from previous studies, indicate the possible existence of crustal partial melting, elevated temperatures or fluid-filled deep crustal faults that are likely associated with lithospheric stretching. In sharp contrast with the southern MRZ, low Vp/Vs measurements in the range of 1.69–1.72 are observed along the western boundary of the northern MRZ, which could be attributable to the infiltration of magma-derived CO2 into the crust. The LRZ shows negligible crustal thinning and a Vp/Vs that is comparable to the globally averaged value for continental crust, suggesting a complete post-rifting recovery of crustal properties in terms of crustal thickness and VpVs.

Introduction

A typical continental rift is a fault-bounded narrow valley where the entire lithosphere has been pulled apart under extension (Sengor and Burke, 1978; Gregory, 1894). As an archetypal example of continental rifts, the East Africa Rift System (EARS), which extends from the northern Red Sea to the southern terminus of the Malawi rift zone (MRZ), is an ideal natural laboratory for investigating rifting mechanisms and the characteristics of continental rifts in various stages. Relative to most of the other segments of the EARS, the Cenozoic MRZ of the EARS and the nearby Paleozoic-Mesozoic Luangwa Rift Zone (LRZ; Ebinger et al., 2017) have been less adequately investigated. Consequently, the magnitude and extent of crustal deformation, the existence of partial melting or mafic intrusion in the crust, and important characteristics such as the depth penetration and possible CO2 infiltration (Roecker et al., 2017) of the seismically active boundary faults, remain enigmatic.

Laboratory investigations of crustal rock samples (Holbrook et al., 1992) suggest that under average crustal temperature and pressure conditions, felsic, intermediate, and mafic rocks have Vp/Vs values of smaller than 1.76, between 1.76 and 1.81, and greater than 1.81, respectively. The existence of crustal partial melting can lead to a higher Vp/Vs due to a greater reduction of Vs than Vp (Greenfield et al., 2016). Similarly, intensive intrusion of mantle materials into the crust can also increase the bulk crustal Vp/Vs (Christensen, 1996). An increasing number of mineral physical and observational studies have suggested that CO2 released from the mantle through deep and steep lithospheric faults can significantly reduce crustal Vp/Vs (Julian et al., 1998; Lee et al., 2016; Parmigiani et al., 2016; Roecker et al., 2017). Specifically, it has been suggested that CO2 can decrease Vp through its strong effect on the pore-fluid compressibility of porous crustal rocks, and consequently, reduce the crustal Vp/Vs (Ito et al., 1979; Mavko and Mukerji, 1995). Therefore, observations of Vp/Vs values that are below the normal felsic rock value of 1.76 may suggest the presence of magma-derived CO2, as well as the existence of lithospheric faults acting as conduits for the CO2 (Lee et al., 2016).

In this study, we measure spatial variations of crustal thickness and Vp/Vs using P-to-S receiver functions (RFs) recorded at 33 broadband seismic stations (Gao et al., 2013), to unveil crustal characteristics and possible effects of CO2 infiltration and partial melting on crustal Vp/Vs beneath the MRZ and LRZ and adjacent areas.

Section snippets

Tectonic setting

The Cenozoic MRZ is the southernmost segment of the magma-poor western branch of the EARS. It separates the Nubian plate and the Rovuma microplate (Fig. 1) and originated approximately 25 Ma (Roberts et al., 2012). The Rungwe Volcanic Province located at the northern tip of the rift zone is the only volcanic province within the MRZ (Ebinger et al., 1993). Kinematic GPS studies (Saria et al., 2014; Stamps et al., 2018) indicated that the spreading rate between the Nubian plate and the Rovuma

Data and methods

The teleseismic (epicentral distance ranging from 30° to 100°) data used in the study were recorded by 33 stations (Fig. 1) that we installed in Malawi, Mozambique, and Zambia over a 2 year period (2012–2014) as a component of the SAFARI (Seismic Arrays for African Rift Initiation; Gao et al., 2013) project. One of these stations (Q05MS) is a combination of two nearby stations Q05MJ and Q05ML. To balance the quality and quantity of the selected data, a variable cut-off magnitude (Mc) was set by

Results

Robust P-to-S arrivals are obtained from the migrated RFs (Fig. 4, Fig. 5), enabling reliable determinations of crustal thickness and Vp/Vs beneath the vast majority of the stations.

Constraints on crustal magmatic intrusion and partial melting beneath the MRZ

In this study, a relatively flat Moho (39.4 ± 2.7 km) was found under most stations in the MRZ including the central and southern parts of the MRZ. The average crustal thickness observed beneath the Mozambique Belt and SIB are 41.9 ± 2.8 km and 43.6 ± 0.8 km, respectively, which are consistent with the ≥40 km results from a recent ANT study (Wang et al., 2019). Therefore, along the rift-orthogonal profile, the crustal thickness in the MRZ is 2–3 km thinner than the surrounding orogenic belts (

Conclusions

Crustal thickness and Vp/Vs beneath 33 SAFARI stations located along two profiles in the vicinity of the MRZ and LRZ were imaged by stacking 2307 high-quality RFs. The crustal thickness measurements are generally consistent with sparsely spaced previous measurements. The new observations show that relative to the adjacent orogenic belts, the crust beneath the MRZ is thinned by about 3 km. This low magnitude crustal stretching is consistent with the absence of volcanisms in the main portions of

CRediT authorship contribution statement

M.S. wrote the paper with help from all the co-authors. S.G., K.L., and Y.Y. wrote the computer programs and provided financial supports.

Declaration of competing interest

The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

Acknowledgments

We thank the IRIS DMC for archiving the data used in the study, and the Portable Array Seismic Studies of the Continental Lithosphere Instrument Center for providing equipment and logistical support. All the data used in the study were obtained from the IRIS DMC (last accessed: August 2018; doi:https://doi.org/10.7914/SN/XK_2012). Field assistance provided by Cory Reed, Shane Ingate, Patrick R. N. Chindandali, Belarmino Massingue, Hassan Mdala, and Daniel Mutamina, as well as by various

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