The intraplate velocities based on CEGRN observations will be compared at the non-reference permanent sites where the ITRF 2000 velocities are available.
OBSERVATIONS OF CEGRN FROM 1994 TO 2005 AND THE EPOCH NETWORK SOLUTIONS
The number of observed stations included in CEGRN was gradually increased.
Summary with characteristics of solutions of eight epoch CEGRN observing campaigns processed at Slovak University of Technology is given in Tab.
Results of individual CEGRN epoch observations are obtained in the form of vector geocentric coordinates [X.
The estimated parameters--geocentric coordinates of CEGRN sites are denoted as Y and the respective site velocities as [v.
CEGRN EPOCH VELOCITIES AND THEIR COMPARISON WITH VELOCITIES OBTAINED FROM PERMANENT OBSERVATIONS
This criterion meets IGS stations BOR1, GRAZ, KOSG, MATE, WTZR, ONSA and ZIMM, which were included in CEGRN epoch campaign processing.
The distribution of CEGRN intraplate horizontal velocities can be roughly characterized by three regional groupings: