Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004geoji.157..251h&link_type=abstract
Geophysical Journal International, Volume 157, Issue 1, pp. 251-264.
Astronomy and Astrophysics
Astronomy
11
Lithosphere, Random Medium, Scattering, Seismic Coda
Scientific paper
An energy-flux model (EFM) and a teleseismic fluctuation wavefield method (TFWM) have been applied to interpret the teleseismic P coda observed at three temporary and two permanent networks in northern and central Europe. The aim is to determine the small-scale random structure of the lithosphere below the receivers. Various subsets of these data have been exploited previously with one of the two methods. The main objectives here are:
In the Baltic shield, Rhenohercynian belt, Ardenne and Brabant mountains, eastern Rhenish massif, Eifel, Hunsrück mountains, Lorraine, Frankonian Jura and massif Central scattering predominantly occurs in the crust. For the frequency range from 0.5 to 5 Hz correlation lengths of 1-7 km and rms velocity fluctuations of 3-7 per cent are obtained. For the Rhenohercynian belt (RH) and the N-German basin RMS velocity fluctuations and correlation lengths could not be resolved. The data from the N-German basin (NB) cannot be explained by scattering within the crust only.
Smallest scattering Q was found in the N German basin (Qs~ 100 at 1 Hz) and largest scattering Q in the Baltic shield (Qs~ 450 at 2-3 Hz). For the Frankonian Jura only a Gaussian ACF can fit the Q-1s values. The data from the eastern Rhenish massif also indicate a random medium with Gaussian ACF. For all other subregions we cannot distinguish between exponential or Gaussian ACF for the random medium structure.
Hock Silke
Korn Matthias
Ritter Joachim R. R.
Rothert Elmar
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