  A network of synchronized detectors can increase the likelihood of
discovering the QCD axion, within the Axion Quark Nugget (AQN) dark matter
model. A similar network can also discriminate the X-rays emitted by the AQNs
from the background signal. These networks can provide information on the
directionality of the dark matter flux (if any), as well as its velocity
distribution, and can therefore test the Standard Halo Model. We show that the
optimal configuration to detect AQN-induced axions is a triangular network of
stations 100 km apart. For X-rays, the optimal network is an array of
tetrahedral units.
