EOP and Station Positions Determined with OCCAM Package

Details EOP and Station Positions Determined with OCCAM Package EOP and Station Positions Determined with OCCAM Package

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ivsg.conf..350s&link_type=abstract

International VLBI Service for Geodesy and Astrometry 2000 General Meeting Proceedings, edited by Nancy R. Vandenberg and Karen

Astronomy and Astrophysics

Astronomy

Scientific paper

The preliminary results of EOP [Pole coordinates, UT1 and corrections to nutation angles (Zvçb and &)] and station positions determination from NEOS-A, CORE-A, CORE-B and IRIS-A observation programs using package OCCAM version 3.5 in IAA RAS are reported in this paper. The EOP series for period 1984—1999 were obtained from these four programs. Comparison of the series with EOP(IERS)C04 shows both bias and rate in Xp pole coordinate arise from one in IRIS-A series. Station positions were estimated for every observational session. Station positions at epoch 1997.0 and velocities for 23 stations were derived from station positions time series by LSM estimations.

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