Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001geoji.145..579w&link_type=abstract
Geophysical Journal International, Volume 145, Issue 3, pp. 579-592.
Astronomy and Astrophysics
Astronomy
22
Scattering, Seismic Coda, Seismology, Volcanic Structure
Scientific paper
The seismic structure of the stratovolcano Merapi (Java, Indonesia) was studied using an active seismic experiment. Three 3km long seismic profiles each consisting of up to 30 three-component seismometers with an interstation distance of 100m were built up in an altitude range between 1000 and 2000m above sea level. The detailed study of the seismic properties of the propagation media in active volcanic regions is important to understand the natural seismic signals used for eruption forecasting. The seismic experiment at Merapi therefore concentrates on the heterogeneous structure within a radius of 5km from the active dome, where the sources of most of the natural volcanic seismic events are located. The cone of Merapi volcano consists of different materials changing on a small scale due to the layering of eruptive material. Additionally, the topography of the erosion valleys leads to an irregular deposition, which cannot be described by a simple 1-D layering. These inhomogeneities have a strong influence on seismic signals. The direct P and S waves are attenuated quickly and show only small amplitudes on seismograms. The energy lost from the direct waves, however, is not changed into heat but scattered and can be observed as seismic coda following the direct waves. The observed seismograms show a spindle-like amplitude increase after the direct P phase. This shape of the envelope can be explained by the diffusion model. According to this model there are so many strong inhomogeneities that the direct wave can be neglected and all energy is concentrated in multiple scattered waves. Besides the envelope, the coherence and polarization properties of the wavefield also indicate strong scattering. Only the first onset shows coherence over a station spacing of 100m, whereas the late phases carrying the major part of the energy are mainly incoherent. The horizontal components of the seismograms have larger amplitudes than the vertical component, but within the horizontal plane the polarization is almost arbitrary, corresponding to waves arriving from scatterers located arbitrarily in space. As a result of the inversion using the diffusion model we obtain values of the S-wave scattering attenuation coefficient, ɛs, and the S-wave intrinsic absorption coefficient, ɛi. In the frequency range of 4-20Hz used in this study the scattering attenuation is at least one order of magnitude larger than the intrinsic absorption (ɛs>>ɛi). The mean free path of S waves is as low as 100m (ɛs-1~100m). The scattering coefficient is independent of frequency (ɛs~f0.0), whereas the coefficient of intrinsic attenuation increases with increasing frequency (ɛi~f1.6). The natural seismic signals at Merapi volcano show similar characteristics to the artificial shots. The first onsets have only small amplitudes and the energy maximum arrives delayed compared to the direct waves. Therefore, these signals appear to be strongly affected by multiple scattering also.
Lühr Birger-G.
Wegler Ulrich
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