The PI's request funds to analyze the dynamics of fault interaction between the San Jacinto (SJFZ)and southernmost San Andreas (SAFZ) fault zones in southern California. They seek to address whether there has been a decrease in the slip rate along the Indio segment of the SAFZ related to the birth and continued maturation of the SJFZ, and/or whether these two fault zones alternatively assume dominant roles in accommodating relative plate motion across the region over any time scales. These questions have proven difficult to address with any one geological/geophysical technique or data type. They will therefore employ an integrated, cross-disciplinary approach to investigate the evolution, present-day behavior,and dynamics of these active faults. Specifically, the PI's propose to:

- Investigate trade-offs between fault model parameter estimates derived from geodetic observations. They will use the SCEC and SCIGN data sets together with inverse elastic fault models and more realistic visco-elastic finite element forward models to perform resolution and covariance analyses to explore the trade-offs between slip rate, locking depth, creep, and seismic cycle effects on these faults. They will (1)determine marginal confidence bounds on the range of present-day boundary conditions on fault evolution models, and (2)determine what improvements in geodetic coverage (e.g.,PBO station locations and station density)will be necessary in order to further narrow the class of admissible fault evolution models.

-Investigate the relative importance of, and feedbacks between, fault zone geometry, and lithospheric rheology by numerical simulations using a 3-D visco-elastic finite element modeling approach. Their investigations will include an assessment of how the presence of the restraining bend in the SAFZ affects partitioning of strain between the SJFZ and SAFZ, how the eastern California shear zone affects this partitioning, and whether there are resolvable differences in fault zone strength between the SAFZ and the SJFZ.

- Determine the age of offset alluvial deposits using cosmogenic dating techniques which were not available ten years ago, at the present-day precision. The order-of-magnitude increase in precision of the offset alluvial fan ages will allow the PI's to discriminate between competing models for fault zone evolution over the 10 to 100 ka time scale. These new cosmogenic dating measurements will be made at no additional cost under this proposal. Rather, funds to cover the costs of this component of our research are anticipated from Deutsche Forschungsgesellschaft (DFG proposal pending, Prof. Friedrich, P.I.).

- Construct a model for the co-evolution of the SJFZ and SAFZ incorporating an aggregation of new and existing displacement history data sets across a broad range of time scales for both fault zones, as well as dynamical considerations. Our integrated approach will provide a more comprehensive test of fault slip dependence between these fault systems than any individual technique could possibly provide on its own.

The strength of our proposal is that our multidisciplinary research will be coordinated by the over-riding goal of testing competing hypotheses for the evolution of this complex fault system.

Agency
National Science Foundation (NSF)
Institute
Division of Earth Sciences (EAR)
Type
Standard Grant (Standard)
Application #
0441371
Program Officer
Stephen S. Harlan
Project Start
Project End
Budget Start
2004-08-01
Budget End
2005-08-31
Support Year
Fiscal Year
2004
Total Cost
$16,535
Indirect Cost
Name
University of Arizona
Department
Type
DUNS #
City
Tucson
State
AZ
Country
United States
Zip Code
85721