We evaluate spatial coverage, as indicated by variance explained by AMPS grid cells corresponding to observing locations, and perform the analysis separately for East Antarctica, West Antarctica, and the Antarctic Peninsula. Preliminary results for the whole continent show that the temperature correlation length scales are larger in winter (April-September) when compared to summer (October-March), and that the opposite is true for surface pressure. Observing stations vary in the amount variance they explain throughout the continent, especially for temperature. Some have a large spatial influence but the signal is not isotropic. We find that there are large gaps in spatial coverage at daily time scales, in particular for temperature observations. Although still incomplete, coverage improves substantially at longer time scales. In addition to identifying gaps in the coverage by the existing network, we conclude by identifying the specific location where one new observation would add the most value to the network. A companion abstract (Hryniw et al.) describes data denial experiments that are used to evaluate the value of existing stations.