Authors: Alexander P. Yefremov
In the framework of six-dimensional quaternionic theory of relativity (a short review is given) non-inertial frames are reasonably described: uniformly accelerated observer on rectilinear trajectory and arbitrary accelerated observer on circular orbit. The results are used to derive exact Thomas precession formula and calculate change of position of Jupiter's satellite observed from Earth, an integral cinematic effect for frames with variable relative velocity.
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[v1] 25 Feb 2007
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