Y. Ricard et al., THE 3-DIMENSIONAL SEISMOLOGICAL MODEL A-PRIORI CONSTRAINED - CONFRONTATION WITH SEISMIC DATA, J GEO R-SOL, 101(B4), 1996, pp. 8457-8472
We compare the predictions of an a priori model of the upper mantle wi
th seismic observations of surface waves and eigenmodes. The S-Dimensi
onal Seismological Model A Priori Constrained (3SMAC) has been develop
ed by Nataf and Ricard [1996]. It is based on the interpretation-by ge
odynamicists of the near surface layers of the Earth; on distributions
of temperature, pressure, and composition as a function of depth; and
then on estimates of seismic parameters (density, velocities, attenua
tions) from solid state laboratory measurements as a function of tempe
rature and pressure. The 3SMAC predictions are confronted with observa
tions consisting of phase velocities for Love and Rayleigh waves in th
e period range of 70-250 s [Montagner and Tanimoto, 1990]. We first sh
ow that tomographic inversions applied to 3SMAC synthetics induce a st
rong smoothing of the heterogeneities. This casts doubt on the meaning
of the spectra of mantle heterogeneities revealed by tomography We th
en show that most of the Love and Rayleigh fundamental mode observatio
ns for periods less than 200 s are satisfactorily predicted by 3SMAC.
The major differences come from the seismic velocities under the Red S
ea and Southeast China, which are much slower than what is estimated f
rom 3SMAC, as well as those under Greenland, which are not as fast as
the other cratonic areas. Because the lithosphere is thinner than 100
km under oceans and thinner than 300 km under continents in 3SMAC, we
suggest that the existence of deeper lithospheric anomalies as propose
d in many tomographic models is mostly due to a spurious effect of the
inversion rather than implied by surface wave data. Half of the varia
nce of the degree 2 anomaly mapped by low-degree eigenmode observation
s can be explained by lithospheric velocity structures. The other half
is highly correlated with the distribution of deep slabs, but its amp
litude is a factor of 3 or 4 larger than that predicted by 3SMAC. The
lithospheric anomalies present a degree 6 pattern well correlated with
the distribution of hotspots even when the thermal anomalies that cou
ld be associated with plumes are not included in 3SMAC. Our results em
phasize the importance of giving very close attention to ''surface cor
rections'' in tomographic models.