Abstract.
We present the first full interferometric simulations of galaxy clusters
containing radio plasma bubbles as observed by the proposed Q band
receiver system
for the ALMA telescope. We discuss the observational requirements for
detecting
intracluster substructure directly from the SZ signal and the advantages
of these observations
over those made with the current generation of SZ survey instruments.
Keywords : instrumentation: interferometers - radiation
mechanisms: general - galaxies: clusters