aus00002.eops.txt Technical description of solution aus00002 1. Purpose of solution: Session EOP 2. Analysis Center: GEOSCIENCE AUSTRALIA (AUS) 3. Short narrative description of solution: Observational VLBI time delays ( IRIS-A/NEOS-A) since 07-Feb-1983 have been analyzed for this solution. Reductional model is realised in accordance with IERS Conventions (2000) except recommended precession/nutation model. Celestial reference frame was fixed to Geoscience Australia solution 2002 (ga2002a). Terrestrial reference frame - daily station coordinates have been estimated under NNR and NNT constraints. All stations for 24-hour session are used for the constraints exception the TIGOCONC VLBI site. Associated velocity field is used for station coordinates calculation. All parameters under estimation have been adjusted using Kalman filter technique. Tropospheric gradients have been considered as constant parameters. 4. Estimated parameters: a. celestial frame: No b. terrestrial frame: Yes c. Earth orientation: X, Y, UT1-UTC, dpsi, deps d. zenith troposphere: Random walk process e. troposphere gradients: Estimates as a constant parameters f. station clocks: Offset as a random walk process, rate as a constant except sessions when the clock rate is considered as a random walk process for separate stations g. baseline clocks: No h. other: No 5. Celestial reference frame: a. a priori source positions: ga2002a ICRF solution b. source positions adjusted in solution: No e. solution identification or reference: ga2002a 6 - Terrestrial reference frame: a. a priori station positions: ga2002a ITRF solution exception TIGOCONC, SVETLOE and GILCREEK after 03-Nov-2003 b. a priori station velocities: ga2002a ITRF solution exception TIGOCONC, SVETLOE and GILCREEK after 03-Nov-2003 c. reference epoch: 1997.0 d. station positions/velocities adjusted in solution: station positions adjusted on daily basis l. solution identification or reference: ga2002a 7. Earth orientation: a. a priori precession model: IAU(1976) b. a priori nutation model: IAU(1980) c. a priori short-period tidal variations in x, y, UT1: IERS Conventions (2000) - model by R.Eanes d. EOP estimation: X, Y, UT1-UTC, dpsi, deps every session 8. A priori geophysical models: a. troposphere: Niell mapping function for dry and wet delays b. solid Earth tide: IERS Conventions 2000, except re-instating for permanent tides. c. ocean loading: IERS Conventions 2000 d. atmosphere loading: no applied 9. Data type: delays 10. Data editing: Only data with zero quality flag in NGS format are used 11. Data weighting: Observations with elevation less than 5 degrees to be divided by sin(elevation). Observations with elevation more than 5 degrees are not weighted as a rule, but Kalman filter approach checks a quality of every observation and downweights it in case of bad result. 12. Standard errors reported: Formal errors are derived from Kalman filter adjustment 13 Software: OCCAM 5.1 14. Other information: For new station TIGOCONC in Chile the following apriori coordinates for initial epoch 1997.0 have been adopted The stations is not used for NNT and NNR constraints. X = 1492054.032 m Y = -4887960.972 m Z = -3803541.438 m For new station SVETLOE in Russia the following apriori coordinates for initial epoch 1997.0 have been adopted. X = 2370173.964 m Y = 1562442.580 m Z = 5529969.035 m Gilcreek after the seismic event 03-Nov-2002 has the following shift for apriori coordinates. dX = -36 mm dY = -58 mm dZ = -37 mm Moreover, exponential model has been applied for post-seismic effect approximation ---------------------------------------------------------------------- Dr. Oleg A.Titov Tel: +61-2-62499064 Project officer Fax: +61-2-62499929 Geoscience Australia PO Box 378, Canberra, ACT, 26102, Australia e-mail: Oleg.Titov@ga.gov.au