XMM1 Middle Mountain Creepmeter Electronics for this instrument were changed on March 7, 1996. Scale factor to coverting DCP counts to RL slip in mm was changed from 142 to 133. Cleaned data below has this change included; However, there may be a slight offset in the data which has not necessarily been taken-out. The Sept 28, 2004 Parkfield Earthquake caused the wire to stretch beyond the limits of the micrometer. (ie, the meter 'pegged') Released tension on wire by feeding 68mm from the anchor end; Micrometer read -0.7mm It appears the both the 'Big Creep' counter gauge and electronics worked through the EQ. Examination of the differences between the micrometer and telemetry values indicate that the calibration of this meter is not correct. In particular, the data from 1993 to 1996 (and perhaps the period between 1986 and 1988) indicate a mis-calibration. The equipment change in 1996 is documented above. Finally, the post-Parkfield EQ data indicate another change in calibration; but there was no equipment change. We will investigate this, soon. Sept-October 2005; The wire had lots of friction due to that 6 inch diameter conduit pulling apart from slip on the fault; the pull-apart allowed for the soil to cave-in and covered the wire. The wire was replaced and the conduit was patched. May 2007; swap-out electronics and DCP for a new version; Telemetry voltage range now 0-5v; scale factor is now 147 counts(mv) per mm fault slip (creep). Note --- (Aug 2022) The data from ~June 2021 and the present suggest that site is not detecting creep --- rate has been 0mm/yr -- expect something like 10 mm/yr rate 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)