The Bulk Flow Velocity and Acceleration of the Inner Jet in M87

A high sensitivity, 7mm Very Long Baseline Array image of M\,87 is analyzed in order to estimate the jet velocity within 0.65 mas point origin. The captured a signal noise, double-ridged, counter-jet extending $\sim 1$ from nucleus. After defining conditions and requirements that justify approximate time averaged bilateral symmetry, continuous set Lorentz transformations are found map double-ridged intensity profile into profile. mapping realized by uniformly accelerating flow with intrinsic 0.27$c at 0.4 (a de-projected distance 0.38 lt-yrs) $0.38$c 0.61 Since field derived global surface brightness does not depend on motion enhanced features, it most likely bulk as opposed pattern velocity. This interpretation corroborated fact distribution apparent velocities previously identified individual features (from literature) nucleus consistent local hydrodynamic shocks being advected visible inner constraint can potentially break degeneracies between numerical simulations designed replicate both annulus was imaged Event Horizon Telescope well base jet.