Abstract
Some basic conceptions of relativistic reference systems are given. The conventional solar-system barycentric reference system (B-system) and the conventional geocentric reference system (G-system) are discussed. It is suggested that the harmonic conditions be used in the definition of the B-system and the G-system be defined by the B-system and the coordinate transformation given by eqs (3–2), (3–3) and (3–4).
Publisher
Cambridge University Press (CUP)