Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009geoji.178.1021h&link_type=abstract
Geophysical Journal International, Volume 178, Issue 2, pp. 1021-1027.
Astronomy and Astrophysics
Astronomy
12
Seismicity And Tectonics, Cratons, Africa
Scientific paper
The southern African Plateau is marked by anomalously high elevations, reaching 1-2 km above sea level, and there is much debate as to whether this topography is compensated by a lower mantle source or by elevated temperatures in the upper mantle. In this study, we use S-wave receiver functions (SRFs) to estimate the lithospheric thickness and sublithospheric mantle velocity structure beneath the Kaapvaal craton, which forms the core of the Plateau. To fit the SRF data, a low-velocity zone (LVZ) is required below a ~160-km-thick lithospheric lid, but the LVZ is no thicker than ~90 km. Although the lid thickness obtained is thinner than that reported in previous SRF studies, neither the lid thickness nor the shear velocity decrease (~4.5%) associated with the LVZ is anomalous compared to other cratonic environments. Therefore, we conclude that elevated temperatures in the sublithospheric upper mantle contribute little support to the high elevations in this region of southern Africa.
Dirks Paul H. G. M.
Durrheim Raymond J.
Hansen Samantha E.
Julia Jordi
Nyblade Andrew A.
No associations
LandOfFree
Upper-mantle low-velocity zone structure beneath the Kaapvaal craton from S-wave receiver functions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Upper-mantle low-velocity zone structure beneath the Kaapvaal craton from S-wave receiver functions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Upper-mantle low-velocity zone structure beneath the Kaapvaal craton from S-wave receiver functions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-832750