W. Spakman et al., TRAVEL-TIME TOMOGRAPHY OF THE EUROPEAN MEDITERRANEAN MANTLE DOWN TO 1400 KM, Physics of the earth and planetary interiors, 79(1-2), 1993, pp. 3-74
The 3-D P-wave velocity structure of the mantle below Europe, the Medi
terranean region and a part of Asia Minor is investigated. This study
is a considerable extension of an earlier tomographic experiment that
was limited to imaging upper-mantle structure only. Here, the Earth's
volume under study encompasses the mantle to a depth of 1400 km, and w
e increase the number of International Seismological Centre (ISC) data
for inversion by a factor of four by taking more years of observation
, and by including data from teleseismic events. The most important de
parture from the earlier study is that we do not use the Jeffreys-Bull
en model as a reference model, but an improved radially symmetric velo
city model, the PM2 model, which is appropriate for the European-Medit
erranean mantle. Our inversion procedure consists of two steps. First,
the radial model PM2 is determined from the ISC delay times by a nonl
inear trial-and-error inversion of the data. As opposed to the Jeffrey
s-Bullen model, the new reference model has a high-velocity lithospher
e, a low-velocity zone, and seismic discontinuities at depths of 400 a
nd 670 km. Next, the ISC data arc corrected for effects related to the
change in reference model and inverted for 3-D heterogeneity relative
to the PM2 model. We follow this two-step approach to attain a better
linearizable tomographic problem in which ray paths computed in the P
M2 model provide a better approximation of the actual ray paths than t
hose computed from the Jeffreys-Bullen model. Hence, the two-step sche
me leads to a more credible application of Fermat's Principle in linea
rizing the tomographic equations. Inversion results for the 3-D hetero
geneity are computed for both the uncorrected ISC data and for the PM2
data. The data fit obtained in the two-step approach is slightly bett
er than in the inversion of ISC data (using the Jeffreys-Bullen refere
nce model). A comparison of the tomographic results demonstrates that
the PM2 data inversion is to be preferred. To assess the spatial resol
ution an analysis is given of hit count patterns (sampling of the mant
le by ray paths) and results of sensitivity tests with 3-D synthetic v
elocity models. The spatial resolution obtained varies with position i
n the mantle and is studied both in map view and in cross-section. In
the well-sampled regions of the mantle the spatial resolution for larg
er-scale structure can (qualitatively) be denoted as reasonable to goo
d, and at least sufficient to allow interpretation of larger-scale ano
malies. A comparison is made of the results of this study with indepen
dent models of S-velocity heterogeneity obtained in a number of invest
igations, and with a prediction of the seismic velocity structure of t
he mantle computed from tectonic reconstructions of the Mediterranean
region. In the context of this comparison, interpretations of large-sc
ale positive anomalies found in the Mediterranean upper mantle in term
s of subducted lithosphere are given. Specifically addressed are subdu
ction below southern Spain, below the Western Mediterranean and Italy,
and below the Aegean. In the last region a slab anomaly is mapped dow
n to depths of 800 km.