By assumption, the analysis of the time series should be referred to
topocentric coordinates (horizontal components N, E and vertical component U).
The quality is measured in terms of standard deviations of the topocentric coordinates ([delta]e, [delta]n, [delta]u).
The validation process is carried out by computing the standard deviations of the rover position error ([[sigma].sub.n], [[sigma].sub.e], [[sigma].sub.u]) of topocentric coordinates. A single number, [[sigma].sub.[rho]], is assigned and the corresponding state is obtained.
All of the Cartesian coordinates (X,Y,Z) provided by the systems and determined manually in ITRF2008 datum were then converted to the local
topocentric coordinates (north, east and up) and differences for all components were calculated as reads by Equation 4.
You can calculate an ephemeris for any interval in astrometric, geocentric, rectangular, or
topocentric coordinates and then display it on screen, save it as a file on disk, or print it.
From practical reasons the spatial Cartesian coordinates X, Y, Z are transformed into geodetic coordinates B, L, h, and eventually into local
topocentric coordinates n, e, u.