A. Vuan et al., S-wave velocity models in the Scotia Sea Region, Antarctica, from nonlinear inversion of Rayleigh waves dispersion, PUR A GEOPH, 154(1), 1999, pp. 121-139
More than 60 events recorded by four recently deployed seismic broadband st
ations around Scotia Sea, Antarctica, have been collected and processed to
obtain a general overview of the crust and upper mantle seismic velocities.
Group velocity of the fundamental mode of Rayleigh waves in the period betw
een 10 s to 30-40 s is used to obtain the S-wave velocity versus depth alon
g ten different paths crossing the Scotia Sea region. Data recorded by two
IRIS (Incorporated Research Institutions for Seismology) stations (PMSA, EF
I) and the two stations of the OGS-IAA (Osservatorio Geofisico Sperimentale
-Instituto Antarctico Argentino) network (ESPZ, USHU) are used.
The Frequency-Time Analysis (FTAN) technique is applied to the data set to
measure the dispersion properties. A nonlinear inversion procedure, "Hedgeh
og," is performed to retrieve the S-wave velocity models consistent with th
e dispersion data.
The average Moho depth variation on a section North to South is consistent
with the topography, geological observations and Scotia Sea tectonic models
.
North Scotia Ridge and South Scotia Ridge models are characterised by simil
ar S-wave velocities ranging between 2.0 km/s at the surface to 3.2 km/s to
depths of 8 kms. In the lower crust the S-wave velocity increases slowly t
o reach a value of 3.8 km/s. The average Moho depth is estimated between 17
km to 20 km and 16 km to 19 km, respectively, for the North Scotia Ridge a
nd South Scotia Ridge, while the Scotia Sea, bounded by the two ridges, has
a faster and thinner crust, with an average Moho depth between 9 km and 12
km.
On other paths crossing from east to west the southern part of the Scotia p
late and the Antarctic plate south of South Scotia Ridge, we observe an ave
rage Moho depth between 14 km and 18 km and a very fast upper crust, compar
ed to that of the ridge. The S-wave velocity ranges between 3.0 and 3.6 km/
s in the thin (9-13 km) and fast crust of the Drake Passage channel. In con
trast the models for the tip of the Antarctic Peninsula consist of two laye
rs with a large velocity gradient (2.3-3.0 km/s) in the upper crust (6-km t
hick) and a small velocity gradient (3.0-4.0) in the lower crust (14-km thi
ck).