Tomographic inversion of P-wave velocity and Q structures beneath the Kirishima volcanic complex, southern Japan, based on finite difference calculations of complex traveltimes
T. Tomatsu et al., Tomographic inversion of P-wave velocity and Q structures beneath the Kirishima volcanic complex, southern Japan, based on finite difference calculations of complex traveltimes, GEOPHYS J I, 146(3), 2001, pp. 781-794
We estimate the P-wave velocity and attenuation structures beneath the Kiri
shima volcanic complex, southern Japan, by inverting the complex traveltime
s (arrival times and pulse widths) of waveform data obtained during an acti
ve seismic experiment conducted in 1994. In this experiment, six 200-250 kg
shots were recorded at 163 temporary seismic stations deployed on the volc
anic complex. We use first-arrival times for the shots, which were hand-mea
sured interactively. The waveform. data are Fourier transformed into the fr
equency domain and analysed using a new method based on autoregressive mode
lling of complex decaying oscillations in the frequency domain to determine
pulse widths for the first-arrival phases. A non-linear inversion method i
s used to invert 893 first-arrival times and 325 pulse widths to estimate t
he velocity and attenuation structures of the volcanic complex. Wavefronts
for the inversion are calculated with a finite difference method based on t
he Eikonal equation, which is well suited to estimating the complex travelt
imes for the structures of the Kirishima volcano complex, where large struc
tural heterogeneities are expected. The attenuation structure is derived us
ing ray paths derived from the velocity structure. We obtain 3-D velocity a
nd attenuation structures down to 1.5 and 0.5 km below sea level, respectiv
ely. High-velocity pipe-like structures with correspondingly low attenuatio
n are found under the summit craters. These pipe-like structures are interp
reted as remnant conduits of solidified magma. No evidence of a shallow mag
ma chamber is visible in the tomographic images.