CRR1 Carr Ranch creepmeter Site defunct since 5/10/15 due to wire binding/conduit caved due to fault offset; remediated Feb. 2018; Has "CalTech" style electronics Sensor failed on Feb 10 1998; sensor removed. Change in scale factor in 1998 To reconcile micrometer and telemetry data, the telemetry data from Dec 2, 1999 through Feb 21, 2000 was deleted and 5.9 mm of "slip" was added to the telemetry data to match (approximately) the micrometer measurements. Telemetry data from Dec 2, 1999 through Feb 21, 2000 appeared noisy; notes about apparent solution were either not made or lost. 2004 Parkfield (Sept 28) 'pegged' the creepmeter; loosen wire at creepmeter and let 35 mm of wire slide to get a micrometer measurement of 25.1mm April 2007 DCP was swapped out for new one; electronics remain the same as output is 0 to 1 volt. Scale factor change of ratio 1000/409.6 Scale factor is now 146.6 counts(mv) per mm fault slip (creep). General Notes: FAULT CREEP DATA FROM PARKFIELD The following data represent real-time measurments of fault slip across the San Andreas fault or its "south-west" trace near Parkfield, CA. Creepmeters consists of 2 piers separated by about 30 meters and connected by an invar wire. The main fault-trace lies between the 2 piers. The wire is at roughly a 30 degree angle from the local trace of the fault. A displacement tranducer measures the change in length of the wire (or the change in distance between the piers). These measurements are made once every 10 minutes and are telemetred to Menlo Park. In addition, micrometer measurements are periodically made by "hand". The telemetred creep data are reconciled with the micrometer measurements. The data have been reconciled with the micrometer measurements and then decimated to daily measurements and scaled to represent fault slip in mm. The data provided here has been processed such that telemetry glitches have been removed, data edited for electronic and other problems, offsets due to resets of the instrument have been removed, and the telemetried data have been reconciled with the Micrometer measurements. Please note that when computing secular rates and other statistics that the assumption of data independence (ie gaussian distributed data) is NOT correct. For starters, the statistics of the data are a mixture of random-walk and white (gaussian) noise. You'll need to construct the appropriate data covariance matrix to account for these noise sources. Otherwise, if you let your standard least squares routine compute the secular rate and its standard error, that error bar will most likely be too small relative to the true estimate of standard error. Because the pier are installed at shallow depths (2-3 meters), these piers will tilt in responce to rainfall. ONE NEEDS TO EXAMINE RAINFALL RECORDS WHEN INTERPRETING THESE CREEP MEASUREMENTS. Many people have contributed to this project including: Robert Burford Sandy Schultz Kate Breckinridge Rich Liechti For questions, contact John Langbein (langbein@usgs.gov) or Andy Snyder (asnyder@usgs.gov)