HR: 0800h
AN: S41A-0243 [Abstracts]
TI: Local Effects Observed on the Earth's Gravest Free Oscillations
AU: * Lambotte, S
EM: Sophie.Lambotte@eost.u-strasbg.fr
AF: IPGS-EOST, 5 rue Rene Descartes, Strasbourg, F-67084, France
AU: Rivera, L
EM: luis@sismo.u-strasbg.fr
AF: IPGS-EOST, 5 rue Rene Descartes, Strasbourg, F-67084, France
AU: Widmer-Schnidrig, R
EM: widmer@geophys.uni-stuttgart.de
AF: Black Forest Observatory (BFO), Heubach 206, Wolfach, D-77709, Germany
AB:
At tidal frequencies, recordings of closely-spaced horizontal seismometers, even if separated only by a few
meters, can present large discrepancies. These perturbations are due to local effects such as topography, local
geology or cavity effects (when instruments are installed in tunnels or cavities), which imply strain-tilt coupling.
These local effects are well observed in the Earth tide recordings and have been well understood since the 70s.
At very low frequencies (tide), the horizontal seismometers are mainly sensitive to tilt. As the frequency increases,
the inertial sensitivity becomes larger and competes with tilt, until at high frequency the local effects mentioned
above should
eventually disapear. The question arises then about the importance of such local effects in the seismic band (T
< 1h). This is the problem we address here by studying horizontal recordings of the Earth's normal modes from
co-located instruments. The gravest free oscillations of the Earth are excited by large earthquakes but are often
masked
by the high noise level induced by atmospheric activity. The long period recordings of the giant 2004 Sumatra
earthquake (Mw ~ 9.3) offer an excellent opportunity to study these local effects on the Earth's gravest free
oscillations (f < 1.2 mHz). In order to better understand the problem, we also compare the observations with
synthetic spectra that
include the modeling of Earth's global 3D structure. Using records from several seismic stations with high
signal/noise ratio, we demonstrate for the first time the presence of these local effects for the Earth's gravest free
oscillations. Our observations indicate that the fundamental modes are the most affected. These local effects can
be
characterized by 3 coefficients which express the coupling between the tilt and the strain field. For each station
and each instrument, we estimate a set of coefficients by comparing the numerical predictions with the
observations. Once estimated, these coefficients can be directly used to reduce the local effects in the normal
modes data. The
obtained coefficients for the free oscillations are comparable to those found in previous analyses at tidal
frequencies.
DE: 1734 Seismology
DE: 7255 Surface waves and free oscillations
SC: Seismology [S]
MN: 2007 Fall Meeting