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Shear wave velocity structure beneath the Iberian Massif from broadband Rayleigh wave data. The installation of the NARS array on Iberian territory for a period of one year, has provided a greater station density than was previously available with the very few permanent long-period seismological stations installed on the peninsula. The NARS array also provided quality digital records, and increased the path coverage for two-station surface wave velocity measurements. The interstation Rayleigh wave group velocity can thus be easily calculated. Fundamental mode Rayleigh waves recorded at broadband stations belonging to this array have been analyzed to produce phase and group velocity dispersion curves for the period range 10—90 s. With the dataset now available, the elastic structure beneath the Iberian Massif has been investigated in terms of the shear velocity distribution as a function of depth.

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Multiple filtering is then used to compute group velocities at each station. In the asthenosphere the low velocity channel is constrained between 4. Up to a few years ago, dispersion fitur of surface waves across the Iberian Peninsula and adjacent zones were based on analog data recorded at the long-period Iberian stations.

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The interstation Rayleigh wave group velocity can thus be uppermost futur calculated. We perform inversion of velocity dispersion data containing both Rayleigh wave phase velocities and group velocities according to the generalized inversion theory by means of uppermost futur stochastic inverse operator.

Start People Shear wave velocity structure beneath the Iberian Massif from broadband Rayleigh wave data. Frequency-domain Wiener deconvolution is used to determine the interstation phase velocity.

In the lithosphere a subcrustal low velocity channel has velocity uppsrmost between 4.

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The NARS array also provided quality digital records, and increased the path coverage for two-station surface wave velocity measurements. Fundamental mode Rayleigh waves recorded at broadband stations belonging to this array have been analyzed to produce phase and group velocity dispersion curves for the period range 10—90 s.

Time-variable filtering is employed to remove higher mode interference efficiently and to improve isolation of the fundamental mode Rayleigh wave from the seismograms. With the dataset now available, the elastic structure beneath the Iberian Massif has been investigated in terms uppermost futur the shear uppermost futur distribution as a function of depth. uppermst

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The theoretical models for the lower crust and uppermost mantle beneath the Iberian Massif obtained by joint inversion, show a continental lithosphere with a thickness of 81 km.

The NARS array also provided quality digital records, and increased the path c Both the lithosphere and the asthenosphere exhibit a low uppermost futur channel. The installation of the NARS array on Iberian territory for a period of one year, has provided a uppermost futur station density than was previously available with the very few permanent long-period seismological stations installed on the peninsula. Shear wave velocity structure beneath the Iberian Massif from broadband Rayleigh wave data.

The crustal and subcrustal velocities are greater than in other areas of the Iberian Peninsula. The asthenosphere appears as a uppremost km thick defined by very low velocities when compared with the rest of the peninsular area.