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The blazars provide a considerable opportunity to peer into the workingswithin a few tens of parsecs of the central engine in AGN. This considerableopportunity involves significant challenges as different macroscopic dynamicalprocesses and microscopic physical processes operating at different locationscan be responsible for the observed emission. In this proceedings article Ireview recent theoretical and numerical results relevant to dynamics inside theblazar zone, review the particle acceleration processes capable of producingthe high energy particles required by the observed emission, discuss some ofthe progress made at the microphysical level, and consider what recent TeV andradio observations of M87 can tell us about the blazar zone.

M87 and the Dynamics and Microphysics inside the Blazar Zone