Accurate timing is also needed to shift and combine the signals from the various dishes.
> often be achieved to within a couple of meters using google maps and a sat image of your back yard.
Position accuracy requirements are fractions of the wavelength being observed. So for this 11.2 GHz dish (26.8 mm), the position of the dish needs to be known to much better than 2mm.
In practice this can be done by observing a bright source with a well-known sky position and then solving for the antenna positions. Aspects of this are discussed in Memo 503 from the Atacama Large Millimeter Array Memo series. http://legacy.nrao.edu/alma/memos/html-memos/alma503/memo503...