Alexandria Digital Research Library

Kinematic Earthquake Sources of High and Low Frequencies and Their Relation to Earth Structure

Author:
Yano, Tomoko Elizabeth
Degree Grantor:
University of California, Santa Barbara. Geological Sciences
Degree Supervisor:
Chen Ji and Toshiro Tanimoto
Place of Publication:
[Santa Barbara, Calif.]
Publisher:
University of California, Santa Barbara
Creation Date:
2012
Issued Date:
2012
Topics:
Geophysics
Keywords:
Wave propagation
Transient deformation
Earthquake dynamics
Surface waves and free oscillations
Earthquake source observations
Seismic tomography
Genres:
Online resources and Dissertations, Academic
Dissertation:
Ph.D.--University of California, Santa Barbara, 2012
Description:

In this thesis, we studied the earthquake process from a dual perspective: i.e. modeling the complex Earth medium and the earthquake dislocations at the source. These two fundamental aspects define the ground motion. Existing kinematic source models are essentially based on the low frequencies contained in the seismic signals (< 1 Hz). Due to our limited knowledge of the Earth medium, the high frequencies in the seismic signals are difficult to be modeled properly. In order to optimize our understanding of the complex earthquake rupture process, a synthesis of both the Earth medium and source model is required.

For modeling the complex Earth medium, we developed a tomographic method that exploits the ellipticity of the fundamental Rayleigh wave (ZH ratio). This method enables us to constrain the shear-wave velocity in a narrower target depth range than conventional methods. The ZH ratio method has been applied to the crust and upper mantle beneath the GEOSCOPE stations. The results show that low-velocity zones exist beneath some stations near hotspots.

The ZH ratio was applied to the L'Aquila basin area to constrain the shallow velocity structure prior to a kinematic source inversion of the 2009 L'Aquila earthquake. Because of differences in the slip models derived from seismological or geodetic data, we introduced a new strategy to differentiate between slip that occurs co-seismically and that occurs as early post-seismic afterslip. The results suggest that the co-seismic rupture was followed by a slow-slip event with significant moment release in the first day.

Lastly, we discussed the development of a back-propagation method to map high-frequency spatial-temporal seismic wave radiation sources onto the fault plane. The new approach considers the free surface reverberations and the fault geometry while existing methods doesn't. Based on results from a synthetic test, we demonstrate that the new back-propagation method is better than existing back-projection method because it not only can locate the spatial-temporal locations of the target sources but also can fairly well recover their amplitudes.

Physical Description:
1 online resource (134 pages)
Format:
Text
Collection(s):
UCSB electronic theses and dissertations
ARK:
ark:/48907/f3d798ck
ISBN:
9781267934512
Catalog System Number:
990039503640203776
Rights:
Inc.icon only.dark In Copyright
Copyright Holder:
Tomoko Yano
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