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  Terrestrial Reference System

Under these hypothesis, the general transformation of the cartesian coordinates of any point close to the Earth from a TRS (1) to a TRS (2) will be given by a tri-dimensional similarity (T1,2 is a translation vector, λ1,2 a scale factor and R1,2 a rotation matrix):

  \begin{displaymath}
\lambda = \Vert ec E_i \Vert_{i=1,2,3}nd{displaymath} (2)

This concept can be generalized in the frame of a relativistic background model such as Einstein's General Relativity, using the spatial part of a local cartesian frame.

  1. Conventional Terrestrial Reference System (CTRS).

Such a system designates the set of all conventions, algorithms and constants which determine the estimation of coordinates of points in a specific ideal TRS.

  1. Conventional Terrestrial Reference Frame (CTRF).

A Conventional Terrestrial Reference Frame is defined as a set of physical points with precisely determined coordinates in a specific coordinate system as a realization of an ideal Terrestrial Reference System. Two types of frames are currently distinguished (this is also valid for celestial references), namely dynamical or kinematical ones, depending whether a dynamical model is applied in the determination process of these coordinates, or not.

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