A useful theoretical equation for computing the relation between pressure, velocity, and altitude in a steady flow of a nearly inviscid, nearly incompressible fluid with negligible heat transfer and shaft work^5 is the Bernoulli relation, named after Daniel Bernoulli, who published a hydrodynamics textbook in 1738:
p_0 = p + \frac{1}{2} \rho V^2 + \rho gZ (1)
where p_0 = stagnation pressure
p = pressure in moving fluid
V = velocity
ρ = density
Z = altitude
g = gravitational acceleration
^5That’s an awful lot of assumptions, which need further study in Chap. 3.
(a) Show that Eq. (1) satisfies the principle of dimensional homogeneity, which states that all additive terms in a physical equation must have the same dimensions. (b) Show that consistent units result without additional conversion factors in SI units. (c) Repeat (b) for BG units.