Lithospheric low-velocity zones associated with a magmatic segment of the Tanzanian Rift, East Africa
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Geophysical Journal International
Abstract
Rifting in a cratonic lithosphere is strongly controlled by several interacting processes including
crust/mantle rheology, magmatism, inherited structure and stress regime. In order to better
understand how these physical parameters interact, a 2 yr long seismological experiment has
been carried out in the North Tanzanian Divergence (NTD), at the southern tip of the eastern
magmatic branch of the East African rift, where the southward-propagating continental rift is
at its earliest stage.We analyse teleseismic data from 38 broad-band stations ca. 25 km spaced
and present here results from their receiver function (RF) analysis. The crustal thickness and
Vp/Vs ratio are retrieved over a ca. 200 × 200 km2 area encompassing the South Kenya
magmatic rift, the NTD and the Ngorongoro-Kilimanjaro transverse volcanic chain. Cratonic
nature of the lithosphere is clearly evinced through thick (up to ca. 40 km) homogeneous crust
beneath the rift shoulders. Where rifting is present, Moho rises up to 27 km depth and the
crust is strongly layered with clear velocity contrasts in the RF signal. The Vp/Vs ratio reaches
its highest values (ca. 1.9) beneath volcanic edifices location and thinner crust, advocating
for melting within the crust. We also clearly identify two major low-velocity zones (LVZs)
within the NTD, one in the lower crust and the second in the upper part of the mantle. The
first one starts at 15–18 km depth and correlates well with recent tomographic models. This
LVZ does not always coexist with high Vp/Vs ratio, pleading for a supplementary source of
velocity decrease, such as temperature or composition. At a greater depth of ca. 60 km, a midlithospheric
discontinuity roughly mimics the step-like and symmetrically outward-dipping
geometry of the Moho butwith amore slanting direction (NE–SW) compared to theNS rift. By
comparison with synthetic RF, we estimate the associated velocity reduction to be 8–9 per cent.
We relate this interface to melt ponding, possibly favouring here deformation process such
as grain-boundary sliding (EAGBS) due to lithospheric strain. Its geometry might have been
controlled by inherited lithospheric fabrics and heterogeneous upper mantle structure. We
evidence that crustal and mantle magmatic processes represent first order mechanisms to ease
and locate the deformation during the first stage of a cratonic lithospheric breakup.

