Polar motion and length of day determination from satellite laser rangingThe kinematic and dynamic models used in obtaining the GSFC MERIT solution (using data from satellite laser ranging) for the x and y coordinates of the earth's rotation pole and the excess length-of-day (LOD) are discussed together with the analysis technique. Comparisons of the GSFC polar motion time series with the time series from the Bureau International de l'Heure shows small but consistent systematic differences (4.6 milliarcsec rms about a mean offset of 1 milliarcsec in the x component, and 2.9 milliarcsec rms about a 21 milliarcsec offset in the y component). A comparison with the data of the National Geodetic Survey's IRIS network shows departures of 2.5 milliarcsec rms about the mean for the x component and 2.0 milliarcsec rms for the y component. The precision of the GSFC earth orientation is estimated to be better than 1 milliarcsec for polar motion and 0.1 msec for excess LOD.
Document ID
19870048862
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Smith, David E. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Christodoulidis, Demosthenes C. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Torrence, Mark H. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Klosko, Steven M. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Dunn, Peter J. (EG&G Washington Analytical Services Center Inc., Lanham, MD, United States)