The processing of EPN benchmark test campaign at the GNSS data analysis centre of the Main Astronomical Observatory of the NAS of Ukraine

2012 ◽  
Vol 18 (4(77)) ◽  
pp. 59-65
Author(s):  
O.A. Khoda ◽  
2014 ◽  
Vol 49 (3) ◽  
pp. 137-150
Author(s):  
M. Ishchenko

Abstract For the first time, a homogeneous coordinate solution in the IGS05 reference frame and the values of the zenith tropospheric refraction for the GPS weeks 935-1399 (from December 12, 1997 to November 4, 2006) were obtained at the GNSS Data Center Analysis of the Main Astronomical Observatory NAS of Ukraine. The obtained solution is devoid of effects, brought by changes in the methods of processing models, a priori data and software (absolute phase center model combinations of antenna-dome instead of relative models, model of ocean loading FES2004 instead of GOT00.2_PP, the elevations cut-off angle 3° instead of 10°, etc. were used). To estimate the quality of the solution, a comparison with the international combined solutions using the Helmert transformation was carried out. The RMS of direct station coordinate differences and correlation coefficients between the solutions estimated by the Main Astronomical Observatory, European GNSS Permanent Network and International GNSS Service are presented. The obtained results allow making the conclusion that the solution obtained at the GNSS Data Center Analysis of the Main Astronomical Observatory shows a good quality and agrees well with other solutions.


1990 ◽  
Vol 141 ◽  
pp. 156-156 ◽  
Author(s):  
M. M. Medvedsky

The software for the reduction of the VLBI observations of the Main Astronomical Observatory of the Ukrainian Academy of Science is described.Our program complex has three parts:1) calculation of geometrical delay τ,2) calculation of required corrections to values of τ,3) data analysis procedures.This software has been tested using the NGS VLBI data for the obtaining of corrections to the ERP. The parameters of the clock were derived. Our results were compared with similar results, which were published by Shanghai observatory (China) and IRIS bulletin.The differences between our results and the data given in the IRIS bulletin are within 5 mas, and for UT are within 0.1 ms.


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