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Reference Frame Errors

The IGS disseminates all data from the global network, globally consistent GPS orbits, and precise site coordinates. This has freed regional investigators from having to deploy fiducial networks or compute their own orbits, and has relieved concern about changing reference frames as fiducial sites change. Heflin et al [1994] now report daily global site position repeatabilities of about 14 mm (2 parts in 10). The published global reference frame is accurate absolutely to about 1 cm. There is still room for reference frame improvement as GPS moves towards sub-centimeter global geodesy. Analysts have long noted that orbit accuracy degrades when the satellites pass through the earth's shadow and have suspected mis-modeling of GPS thermal radiation [ Blewitt, 1993]. Bar-Sever et al [1995] uncovered a possibly root cause: unpredictable yaw variations when the satellite loses its sun sensor. They proposed inserting a 0.5 deg yaw bias in the satellite attitude control subsystem, which was adopted and instituted by the Air Force in June of 1994. Early results show a clear improvement in orbit accuracy during eclipse periods. Monument instability threatens the integrity of the reference frame and the authenticity of perceived geophysical signals. While of only modest concern for global measurements, site stability is a top priority for the SCIGN array in the Los Angeles Basin, which will feature 5--10 km site spacing and could detect strain rates of 0.2 mm/yr within one year. The SCIGN science team has set a provisional goal of 0.5 mm for long term monument stability. Such local effects as soil expansion from rainfall and slow churning can in principle perturb even robust monuments by millimeters over months or years [ D. Agnew, personal communication]. Land subsidence due to intensive water pumping can be on the order of centimeters per year. Even relatively benign areas may exhibit nontectonic subsidence at the millimeter level over a period of years from fluid extraction or as a result of drought [ Sylvester, 1992; Van Hasselt, 1992]. A focused effort is needed to probe site stability at the submillimeter level required by dense networks, and GPS may be an effective tool for the job. Elosegui et al [1993] report measurement precisions of about 0.1 mm on baselines of less than 100 m with just a few hours of data, consistent with results from JPL in the late 1980s and from Genrich and Bock [1992]. Long term GPS measurements on closely spaced monuments could answer some of the questions now being raised for the Los Angeles array.



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Next: Selective Availability and Up: Environmental Effects Previous: Ionospheric Effects



U.S. National Report to IUGG, 1991-1994
Rev. Geophys. Vol. 33 Suppl., © 1995 American Geophysical Union