
USNO Global VLBI Solution crf2006cPresented here is the U.S. Naval Observatory's crf2006c global solution. Parameterization of this solution follows that of the International Celestial Reference Frame (ICRF) solution (Ma et al. 1998, AJ, 116, 516) and its extensions (Fey et al. 2004, AJ, 127, 3587) but includes several analysis changes, the most important of which are 1) using the Niell Mapping Function to model the troposphere, 2) more frequent estimation of troposphere gradients (once every 6 hours instead of once every 24 hours as was done for the ICRF), 3) a priori mean gradients computed from a GSFC Data Assimilation Office model for meteorological data from 199095, and 4) 5 degree elevation cutoff (versus 6 degree cutoff as was done for the ICRF). The solution also includes the most recent data and 9.5 years of VLBA RDV experiments (RDV01 to RDV57). Similar to the ICRF solution, the primary geodetic parameters, the station positions, were estimated separately for each session in the solution. Station motions within a day, from solid Earth tides and ocean loading, were derived from unadjusted a priori models. The adjusted "arc" parameters (i.e., parameters that depend only on the data from an individual experiment and are estimated separately for each epoch of observation) included: positions of sources with identified excessive apparent motion or random variation; celestial pole offsets in ecliptic longitude and obliquity to account for errors in the standard precession/nutation models; positions of the stations; the rate of UT1 relative to a good a priori time series; twentyminute piecewise linear continuous troposphere parameters; tropospheric gradients in the eastwest and northsouth directions, linear in time, estimated once every 6 hours; quadratic clock polynomials for the gross clock behavior; sixtyminute piecewise linear continuous clock parameters; and necessary nuisance parameters such as clock jumps and baseline clock offsets. The remaining parameters, including source positions, were adjusted as invariant, or "global," quantities (i.e., parameters that are dependent on all data sets and are carried from step to step resulting in a single estimate derived from the combined data of all experiments in the solution). The resultant global SOLVE solution includes most available VLBI observations at 8.4 GHz (Xband) and 2.2 GHz (Sband) from 1979 August 3 through 2006 October 5. This includes a total of 4053 diurnal sessions encompassing 4,889,588 measurements of group delay and delay rate. The weighted rootmeansquare residuals of the solution were 23.873 ps in delay and 80.941 fs/s in delay rate. The SOLVE batch control file crf2006c_02.cnt.gz was used to generated this solution with an output spool file crf2006c_02.spl.gz (~20.2 MByte). Tabulated below are the global and session values for the solution. Source and Station PositionsPositions of 713 sources were estimated as global parameters. Positions for an additional 188 sources (including 2 radio stars) were estimated for each session independently as "arc" parameters. A total of 82 sources with either no good observations or with bad data were excluded from the solution. Positions of all 130 stations were estimated as local (session) parameters. Plots.
Tabulated data.
^{*}Note: the complete set of 901 source positions can be obtained by downloading these two files. The positions for the local sources are weighted mean positions. The position uncertainties for the local sources are the weighted rootmeansquare deviations from the weighted mean positions. Earth Orientation ParametersDaily nutation offsets in longitude and obliquity were estimated for each session separately. Tabulated data.
ComparisonsShown below are comparisons of the USNO crf2006c source positions with the ICRF, ICRFExt.1, ICRFExt.2 and USNO crf2006b source positions. The weighted rms differences are at the end of the difference tables. In the vector difference plots, green indicates a less than 3sigma position difference, orange indicates a 35 sigma difference and red indicates a greater than 5sigma difference. Note that the sigmas are based on the inflated errors for the ICRF and ICRFExt.1 comparisons. The sigmas are based on the formal errors for the ICRFExt.2 and the USNO frame comparisons. Tabulated data and plots.
Position Time SeriesTo assess the position stability of the sources observed in more than one session, eight additional solutions were made with identical parameterization and data as for crf2006c_02. In each of these solutions, one eighth of the sources were estimated as "arc" parameters. The remaining sources were treated as "global." The SOLVE BATCH control files for these additional solutions are available here ( crf2006c_01_pts1.cnt.gz, crf2006c_01_pts2.cnt.gz, crf2006c_01_pts3.cnt.gz, crf2006c_01_pts4.cnt.gz, crf2006c_01_pts5.cnt.gz, crf2006c_01_pts6.cnt.gz, crf2006c_01_pts7.cnt.gz, crf2006c_01_pts8.cnt.gz ). Daily nutation offsets in longitude and obliquity were estimated for each session separately. Nutation offsets are presented in the following tables. Tabulated data.
Position time series plots and associated statistics tables are presented below. In the plots, green indicates a less than 3sigma difference from the weighted mean position, orange indicates a 35 sigma difference and red indicates a greater than 5sigma difference. The blue curves in the plots represent a 1year running weighted average (boxcar smoothing). Tabulated statistics and plots.
Below is a comparison of the source "arc" positions with their global positions. The weighted rms differences are at the end of the difference table. In the vector difference plot, green indicates a less than 3sigma position difference, orange indicates a 35 sigma difference and red indicates a greater than 5sigma difference. Note that the sigmas are based on the formal errors.
