Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003geoji.154..196n&link_type=abstract
Geophysical Journal International, Volume 154, Issue 1, pp. 196-204.
Astronomy and Astrophysics
Astronomy
13
8° Discontinuity, Scattering, Seismic Modelling, Seismic Waves, Synthetic Seismograms, Upper Mantle
Scientific paper
Detailed interpretation of upper-mantle scattered waves recorded in the 800-1400 km offset range of four reversed `peaceful nuclear explosion' seismic sections along the 3500 km long profile Kraton in Russia has revealed an ~85 km thick seismically inhomogeneous low-velocity zone below the 8° discontinuity at ~100 km depth. The scattered waves make up a wave train of high amplitude that decreases in duration from ~8 s at 800 km offset to ~4 s at 1400 km offset. 2-D elastic finite-difference modelling of the seismic wavefield has previously shown that the inhomogeneous zone from ~100 to ~185 km depth may be described by continuous, random velocity fluctuations represented by an exponential medium with a horizontal correlation length of 5-10 km, a vertical correlation length of <5 km and a standard deviation of ~2 per cent of the average background velocity value. Here, we demonstrate that other proposed velocity fluctuations in the lower crust and in the uppermost mantle from the Moho to ~100 km depth cannot explain the observed scattered phases. Our study shows that upper-mantle velocity fluctuations below the 8° discontinuity at 100 km depth are needed in order to explain the observed seismic wavefield, and that they lead to scattering that is significantly different from the scattering caused by the fluctuations at shallower levels.
Levander Alan
Nielsen Lars
Solodilov Leonid N.
Thybo Hans
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