Searcharxiv⌕ Search

arXiv · physics/0305099

Dynamical system analysis and forecasting of deformation produced by an earthquake fault

Abstract

We present a method of constructing low-dimensional nonlinear models describing the main dynamical features of a discrete 2D cellular fault zone, with many degrees of freedom, embedded in a 3D elastic solid. A given fault system is characterized by a set of parameters that describe the dynamics, rheology, property disorder, and fault geometry. Depending on the location in the system parameter space we show that the coarse dynamics of the fault can be confined to an attractor whose dimension is significantly smaller than the space in which the dynamics takes place. Our strategy of system reduction is to search for a few coherent structures that dominate the dynamics and to capture the interaction between these coherent structures. The identification of the basic interacting structures is obtained by applying the Proper Orthogonal Decomposition (POD) to the surface deformations fields that accompany strike-slip faulting accumulated over equal time intervals. We use a feed-forward artificial neural network (ANN) architecture for the identification of the system dynamics projected onto the subspace (model space) spanned by the most energetic coherent structures. The ANN is trained using a standard back-propagation algorithm to predict (map) the values of the observed model state at a future time given the observed model state at the present time. This ANN provides an approximate, large scale, dynamical model for the fault.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Marian Anghel, Yehuda Ben-Zion, Ramiro Rico-Martinez. 2003-05-22. Dynamical system analysis and forecasting of deformation produced by an earthquake fault. https://doi.org/10.1007/s00024-004-2547-9

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Supershear Rupture Indicator in Near-fault Particle Motion

Earthquake rupture propagation speed is an essential source parameter that fundamentally controls hazard and risk. In this paper, we develop and demonstrate the capability of a single near-fault seismic record in delineating earthquake rupture speed by inspecting displacement particle motion. We apply this method to near-fault strong-motion data in M7+ strike-slip earthquakes and identify diverse particle-motion signatures associated with subshear rupture, supershear rupture, supershear transition, initial rupture expansion, and potential multiple rupture fronts. This study highlights the value of near-fault observations for determining rupture speed.

physics.geo-ph↗

Extracting and Characterizing Near-Fault Effects from Strong Motion Observations of the 2022 Chishang Earthquake Sequence

Accurately characterizing near-fault ground motions, particularly permanent tectonic displacements and velocity pulses associated with rupture directivity, is essential for seismic hazard assessment and infrastructure design. However, conventional ground-motion processing can distort or remove these characteristics. This study extends existing baseline correction methods by synchronously processing all three components of strong-motion recordings to preserve near-fault effects. The proposed methodology is applied to 59 recordings from the 2022 M 6.5 Guanshan foreshock and M 6.9 Chishang mainshock in Taiwan. Comparison with nearby Global Navigation Satellite System (GNSS) observations demonstrates that the method reliably captures the amplitude and orientation of permanent tectonic displacements. Analysis of the processed recordings reveals pronounced velocity pulses and permanent displacements, with the largest peak-to-peak velocities concentrated along the direction of rupture propagation. A classification framework is also introduced to distinguish fling-step pulses from dynamic velocity pulses. The results indicate that fling-step pulses typically occur early in the ground shaking, whereas dynamic pulses span a broader temporal range. Furthermore, the spatial distribution and orientation of near-fault effects are consistent with bridge damage documented during post-earthquake reconnaissance. The resulting dataset provides ground-motion time histories that preserve near-fault characteristics for seismic hazard assessment and engineering applications.

physics.geo-ph↗

Shallow lunar fractures dominate the long-lasting seismic coda

Lunar seismic records are characterized by long-lasting spindle-shaped coda, which has long been considered to be caused by strong velocity contrasts in a continuous-medium lunar crust; however, simulated waveforms could not well match the observation even with unrealistically strong velocity contrasts, demonstrating its mechanism still unsolved. Here we propose a novel model of coda wave generation with random fractures in the lunar crust, where vacuum fractures prevent seismic wave propagation as insulating boundaries, causing strong persistent reverberation in terms of total reflection among fractures. Our model can easily reproduce the typical characteristics of observed Apollo data even using a limited number of simplified fractures in homogeneous matrix, with envelope correlations over 0.9, much higher than previous studies. Numerical simulations suggest that fractures in the uppermost ~1 km of the crust may dominate lunar seismic scattering. This model enables us to investigate the shallow lunar fracture system using seismic data and to suppress seismic coda for detecting critical phases reflected from deep interiors.

physics.geo-ph↗