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Mechanics of Fluids

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3. dp/dz =−ϱg. (Since the pressure varies only in the vertical (z) direction,<br />

the partial derivative in eqn 2.2 may give way to the full derivative.)<br />

To determine the pressure at any point in a fluid in equilibrium, eqn 2.2<br />

must be integrated:<br />

�<br />

p = −ϱgdz<br />

Evaluation <strong>of</strong> the integral is not possible, however, unless the variation <strong>of</strong> ϱ<br />

with z known.<br />

2.2.1 The equilibrium <strong>of</strong> a fluid <strong>of</strong> constant density<br />

Since for all practical differences in height the variation <strong>of</strong> g is negligible,<br />

integration <strong>of</strong> eqn 2.2 for a homogeneous fluid <strong>of</strong> constant density gives<br />

p + ϱgz = constant (2.3)<br />

This result is valid throughout a continuous expanse <strong>of</strong> the same fluid since,<br />

in deriving eqn 2.2, no restriction at all was placed on the value <strong>of</strong> θ.<br />

The value <strong>of</strong> the constant in eqn 2.3 is determined by the value <strong>of</strong> p at a<br />

point where z is specified. If the fluid is a liquid with a horizontal free surface<br />

at which the pressure is atmospheric (pa) this free surface may be taken<br />

as the datum level z = 0. For equilibrium <strong>of</strong> the surface the pressure immediately<br />

below it must equal that immediately above it, and so the pressure<br />

in the liquid at the surface is pa. Then, for a point at a depth h below the<br />

surface, h =−z (since h is measured downwards whereas z is measured<br />

upwards) and, from eqn 2.3,<br />

Variation <strong>of</strong> pressure with position in a fluid 45<br />

p = pa + ϱgh (2.4)<br />

The pressure therefore increases linearly with the depth, whatever the shape<br />

<strong>of</strong> any solid boundaries may be.<br />

Equation 2.4 shows that the pressure at a point in a liquid in equilibrium<br />

is due partly to the weight <strong>of</strong> the liquid. Thus atmospheric pressure is usually<br />

effective, even if indirectly, on all surfaces, and over the differences <strong>of</strong> height<br />

normally encountered it is sensibly constant. Consequently it is <strong>of</strong>ten simpler<br />

to regard atmospheric pressure as the zero <strong>of</strong> the pressure scale. A pressure<br />

expressed relative to atmospheric pressure is known as a gauge pressure.<br />

Equation 2.4 then reduces to p = ϱgh. As we shall see in Section 2.3, this<br />

relation forms the basis <strong>of</strong> a number <strong>of</strong> methods <strong>of</strong> measuring pressure.<br />

The direct proportionality between gauge pressure and h for a fluid <strong>of</strong><br />

constant density enables the pressure to be simply visualized in terms <strong>of</strong><br />

the vertical distance h = p/ϱg. The quotient p/ϱg is termed the pressure<br />

head corresponding to p. So useful is the concept <strong>of</strong> pressure head that it<br />

is employed whether or not an actual free surface exists above the point<br />

in question. For a liquid without a free surface, as for example in a closed<br />

pipe, p/ϱg corresponds to the height above the pipe to which a free surface<br />

would rise if a small vertical tube <strong>of</strong> sufficient length and open to atmosphere<br />

– known as a piezometer tube – were connected to the pipe (Fig. 2.2).<br />

Fig. 2.2

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