HR: 16:30h
AN: S32E-03 [PDF]
TI: Long-period mantle structure from Earth's free oscillation spectra
AU: * Deuss, A
EM: arwen.deuss@earth.ox.ac.uk
AF: University of Oxford, Department of Earth Sciences
Parks Road, Oxford, OX1 3PR
United Kingdom
AU: Woodhouse, J H
EM: john.woodhouse@earth.ox.ac.uk
AF: University of Oxford, Department of Earth Sciences
Parks Road, Oxford, OX1 3PR
United Kingdom
AB:
Models of the Earth's long period three dimensional structure are obtained from the study of the splitting of Earth's free
oscillation spectra. These data place important constraints on the aspherical compressional and shear wave velocity
structure, and in addition has the capability to provide information on aspherical density structure. In general, {\it
splitting functions} are measured from the normal mode spectra using a least squares inversion. These splitting functions are
linearly dependent upon the aspherical velocity and density structure and are then used in a second least squares inversion
to obtain tomographic velocity models. Many recent tomographic models, including S20RTS, have used splitting functions in
addition to body wave and surface wave data. In principle, normal mode spectra could also be inverted directly to get
tomographic models.
In order to use splitting functions, it has been assumed that modes are isolated and therefore can be studied in the
self-coupling approximation or that only small groups of modes need to be coupled. We will show that for many modes, this
represents a poor approximation compared to full coupling, where large groups of modes are coupled. This implies that it is
actually not accurate enough to use splitting functions.
In order to access the influence of the splitting function approximation on the long period structure in tomographic models,
we have performed tests for a data set of normal mode spectra of recent large earthquakes, including the Bolivia and Kuril
Island events of 1994. We will show the different tomographic models obtained from a two-step inversions using splitting
functions compared with a one-step direct inversion of the normal mode spectra. We will also show the difference between a
direct inversion of normal spectra using the self coupling approximation versus the group coupling approximation.
DE: 7200 SEISMOLOGY
DE: 7207 Core and mantle
DE: 7255 Surface waves and free oscillations
DE: 7260 Theory and modeling
DE: 8180 Tomography
SC: Seismology [S]
MN: 2003 Fall Meeting