Hi, all,
I sense some confusion here between an "initial synchronization" and keeping clocks at different locations (perhaps in a curved spacetime, and/or undergoing acceleration), which are exchaning time signals, running at carefully adjusted rates so that they continue to remain "in synch" over a substantial period of time.
lalbatros said:
Just one more short comment.
the GPS system is always re-synchronising all the atomic clocks in the system
This isn't quite right. The GPS satellite clocks are set to run slow by "the basic GPS correction factor" (the frequency shift for "Hagihara observers" exchanging time signals with observers on the surface of an isolated nonrotating spherically symmetric massive object, which works out to 38 microseconds per day) precisely to avoid the procedure lalbatros imagines. On top of this, from time to time small corrections are made from the control center to deal with stuff which is impossible to predict far in advance, like solar wind buffeting of the satellites, but the point is that if the satellite clocks were not set to run slow as just described, the corrections needed to keep everything in synch would
not be small. That would be a serious problem, so they are set to run slow by the precise factor obtained from the above mentioned gtr model.
See
http://www.arxiv.org/abs/gr-qc/0507121 and http://relativity.livingreviews.org/Articles/lrr-2003-1/index.html for two readable expositions of "relativistic corrections" to the GPS.
Note that the GPS is basically designed using Newtonian theory (for the astrodynamics) plus Maxwell's theory of EM (i.e. in flat spacetime, for the signals) overlaid with somewhat cumbersome corrections, which is obviously not a very pretty way of thinking about this. But there is nothing to prevent one from designing a spacetime charting/navigation satellite beaconing system which is inherently relativistic. There has been considerable interest of this lately, because it leads to a little-noticed revolution in the history of ideas, the first self-consistent timekeeping/locating schemes. That is, in traditional coordinatizations of the Earth, topological considerations ensure awkward and ugly coordinate singularites like the International Date Line, the Earth (not to mention the solar system) is plenty large enough that the finite speed of light and other relativistic effects becomes very noticeable, and calendars based on quasiperiodic astronometric phenomena are notoriously difficult to maintain over long periods. All of these problems are obviated by the relativistic satellite beaconing scheme of Bartolome Coll; see for example
http://www.arxiv.org/abs/gr-qc/0606044