The San Andreas Fault Observatory at Depth: Recent Site Characterization Studies and the 2.2-Km-Deep Pilot Hole

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The San Andreas Fault Observatory at Depth: Recent Site Characterization Studies and the 2.2-Km-Deep Pilot Hole Steve Hickman and Bill Ellsworth (USGS) Mark Zoback (Stanford University) and the Pre-EarthScope SAFOD Science Team

San Andreas Fault Observatory at Depth (SAFOD) Pacific Plate North American Plate The central scientific objective of SAFOD is to study directly the physical and chemical processes that control deformation and earthquake generation within an active platebounding fault zone.

7.9

San Andreas Fault Observatory at Depth: Project Overview and Science Goals Test fundamental theories of earthquake mechanics: Determine structure and composition of the fault zone. Measure stress, permeability and pore pressure conditions in situ. Determine frictional behavior, physical properties and chemical processes controlling faulting through laboratory analyses of fault rocks and fluids. Establish a long-term observatory in the fault zone: Characterize 3-D volume of crust containing the fault. Monitor strain, pore pressure and temperature during the cycle of repeating microearthquakes. Observe earthquake nucleation and rupture processes in the near field.

Parkfield Experiment Observe the build-up and release of stresses on the San Andreas Fault through multiple earthquake cycles. GOALS Test the feasibility of short-term earthquake prediction. Measure near-fault shaking during earthquake rupture, and learn how to predict the amplification of shaking caused by different soil types for improving building codes and designs.

SAFOD Source: Jessica Murray Felix Waldhauser & Bill Ellsworth

Examples of Repeating Earthquakes

Pilot Hole Stage I: Drilling, Sampling and Downhole Measurements Rotary drill to 2.2 km, collecting drill cuttings and bottom-hole core. Wireline logging for physical properties, fracture geometry, stress directions and temperature. Hydraulic fracturing stress test and fluid sampling at bottom. Stage 2: Downhole Monitoring Install temporary 3-component seismic array inside hole. Conduct surface seismic surveys, while recording downhole. Instrument hole for long-term monitoring of pore pressure, strain, temperature and seismic activity. SAFOD Pilot Hole Goals Provide technical information about drilling conditions prior to SAFOD. Measure stress, fluid pressure and heat flow adjacent to the fault zone. Record surface sources during seismic experiments in 2002 and 2003. Facilitate precise location of target earthquakes for SAFOD. Test seismic, pressure, and strain monitoring instruments for SAFOD. Calibrate physical properties from surface geophysical surveys. Reveal nature and extent of fluid/rock interaction adjacent to fault zone.

Electrical Imaging Reveals Distribution and Orientation of Faults and Fractures Ultrasonic Imaging Reveals Stress-Induced Breakouts That Yield Stress Orientation

Temperature Log From the Pilot Hole (Aug 6) Preliminary heat flow: 85 mw/m 2 Background: 65-85 mw/m 2 From Colin Williams

Installing the Pilot Hole Seismic Array

Pilot Hole Array: M 3.8 Earthquake on 9/4/02 (17 km to SE) Depth 850 m Depth 2100 m 0 2 4 6 8 10 Time, seconds Vertical components

Seismic Calibration Shots Conducted in October 2002

Explosion 5 Km west of SAFOD

All components of EarthScope must work together in the planning, execution and interpretation of experiments aimed at understanding the SAFOD crustal volume. SAFOD PBO USArray InSAR Integrated physics-based models for faulting and earthquake generation along the San Andreas Fault that combine measurements made in the drill hole with crustal-scale measurements of the displacement field, seismic velocity, density, conductivity and other properties.

Drilling of Main SAFOD Hole in 2004(?) SAFOD is an open experiment. Monitoring data from the observatory will be freely available to all without restriction.