|
Read Full Article (file size: 2719949 bytes) Cited by
GEOPHYSICAL RESEARCH LETTERS,
VOL. 30, NO. 10,
1531,
doi:10.1029/2002GL016436,
2003
Upper mantle P wave velocity structure and transition zone thickness beneath the Arabian Shield
Margaret H. Benoit
Department of Geosciences, Penn State University, University Park, Pennsylvania, USA
Andrew A. Nyblade
Department of Geosciences, Penn State University, University Park, Pennsylvania, USA
John C. VanDecar
Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC, USA
Harold Gurrola
Department of Geosciences, Texas Tech University, Lubbock, Texas, USA
Abstract
We use P wave tomography and receiver function analysis to place new constraints on the nature of the thermal anomaly in the
upper mantle beneath the Arabian Shield. A broad, low velocity anomaly is found in the upper mantle characterized by a strong
lateral velocity gradient, with a peak to peak anomaly of at least 4–6% extending from the Red Sea eastward into the interior
of the shield. The lowest velocities are found under the region adjacent to the Red Sea where elevations are more than 1 km
higher than elsewhere in the Arabian Shield. We infer that large lateral temperature variations exist beneath the Arabian
Shield associated with the higher elevations near the Red Sea. Receiver function stacks of P to S conversions from the 410
and 660 km discontinuities do not indicate thinning of the transition zone, suggesting that the broad, low velocity anomaly
is likely confined to depths shallower than 410 km.
Received 10
October
2002;
accepted 21
February
2003;
published 27
May
2003.
Index Terms: 7218 Seismology: Lithosphere and upper mantle; 8121 Tectonophysics: Dynamics, convection currents and mantle plumes; 8180 Tectonophysics: Tomography.
Read Full Article (file size: 2719949 bytes) Cited by
Citation: Benoit, M. H., A. A. Nyblade, J. C. VanDecar, and H. Gurrola
(2003),
Upper mantle P wave velocity structure and transition zone thickness beneath the Arabian Shield,
Geophys. Res. Lett.,
30(10),
1531,
doi:10.1029/2002GL016436.
Copyright 2003 by the American Geophysical Union.
|