![]() ![]() This triggers our anti-spambot measures, which are designed to stop automated systems from flooding the site with traffic. ![]() Some unofficial phone apps appear to be using GameFAQs as a back-end, but they do not behave like a real web browser does.Using GameFAQs regularly with these browsers can cause temporary and even permanent IP blocks due to these additional requests. If you are using Maxthon or Brave as a browser, or have installed the Ghostery add-on, you should know that these programs send extra traffic to our servers for every page on the site that you browse.The most common causes of this issue are: There is a fourth column, then ignore that column.Your IP address has been temporarily blocked due to a large number of HTTP requests. ![]() The format of these data are year, day-of-year, and slip in mm. In addition, there is a table listing the estimates of theĪmplitude and phase of the O1 and M2 tides calculated as a function of The ReadMe file contains the lists of offsets and data removed forĪnalysis. More data exist, but have not been archived. None of these GTSM instrumentsĬurrently work after more than 20 years of continuous operation.įor the DTM instruments, the data are complete through the end ofĢ019. These GTSM instrumentsĪre identified with a 3 letter code. Gauge data for the DTM instruments are notįor the GTSM instruments, the data are complete. Offsets due to valve resets, for the Carnegie, DTM Outliers due to telemetry problems, instrument visits, and etc Data are provided in two modes 1) Cleaned strain data and 2)Ĭlean strain data adjusted for the Earth Tide and atmospheric pressureĬhanges. We provide both the extensometer and the tensor strainĬhanges. These data can be combined into tensor strain based upon analysis using Since these instruments have at least 3 extensometers, Terrestial Magnetism (DTM) and the other is a three or 4 component We are providing data for two different instruments, one is Of 0.001 part per million) as a function of time for instruments inĬalifornia. The data listed below are measures of changes in tensor strain (units Of the O1 and M2 tides calculated as a function of time for the strainmeter. In addition, there is a table listing the estimates of the amplitude and phase The ReadMe file contains the lists of offsets and data removed for analysis. (not scaled to units of pressure) are also provided.ĭata are complete through the end of 2019. DataĪre provided in two modes 1) Cleaned strain data and 2) Clean strain dataĪdjusted for the Earth Tide and atmospheric pressure changes. Offsets due to valve resets have been removed. Outliers due to telemetry problems, instrument visits, andĮtc have been removed. (units of 0.001 part per million) as a function of time for instruments The data listed below are measures of changes in volumetric strain More information can be found in the USGS Open File Report:Ĭreepmeter measurements in California from 1966 through 1988įor information on 5 sites along the Hayward Fault (cpp, ctm, coz, ![]() Is a fourth column, then ignore that column. The 1-day data files will include older data. The 10-minute and 1-day sampled data often do not cover the same Note that at some sites, there exists both 10 minute and 1-day sampledĭata. However, for the most recent observations, that is, within the pastĢ weeks, they have not always been reviewed and, if needed, edited. For sites with telemetry, the data are uploaded to this webpageĭaily. For each site, the available dataĪre listed. For other creepmeters without telemetry,īelow is a list of creepmeters, from North to South, located on the SanĪndreas, Hayward, and Calaveras Faults. In addition, periodic measurements are made manually for comparison with Minutes and are sent via satellite telemetry to Menlo Park for analysis. The change in length of the wire (or the change in distance between theįor many of the creepmeters, the measurements are made once every 10 A displacement transducer (LVDT) measures The invar wire oriented roughly a 30 degree angleįrom the local trace of the fault. The main fault trace liesīetween the two piers. Creepmeters consist of two piers separated byĪbout 30 meters and connected by an invar wire. The data listed below are measures of surface fault slip (scaled in mm)Īs measured by creepmeters. ![]()
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