Note that Bernoulli and mass balance provide two equations: \frac{p_{1}}{\rho }=gz_{1}+\frac{1}{2}\nu ^{2}_{1}=\frac{p_{2}}{\rho }+gz_{2}+\frac{1}{2}\nu ^{2}_{2}, \nu _{1}A_{1}=\nu _{2}A_{2}, which can be used to solve for the two velocities, \nu_{1} and \nu_{2}, along a straight horizontal streamline s in a steady, converging, ideal flow, with A_{1} and A_{2} known. To do so, however, we must independently compute or measure the pressures p_{1} and p_{2}. Assuming a negligible gravitational field, determine if the pressure gauges in Fig. 8.9 can be used to determine the pressures along the center streamline.