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standard pressure p 0 (z), which is the horizontally averaged pressure at each height,
and a corresponding standard density ρ 0 (z), defined so that p 0 (z) and ρ 0 (z) are in
exact hydrostatic balance:
1
ρ 0
dp 0
dz ≡−
g
(2.26)
We may then write the total pressure and density fields as
p (x,y,z,t)
p(x, y, z, t)
=
p 0 (z)
+
(2.27)
ρ (x,y,z,t)
ρ(x, y, z, t)
=
ρ 0 (z)
+
where p and ρ are deviations from the standard values of pressure and density.
For an atmosphere at rest, p and ρ would thus be zero. Using the definitions of
(2.26) and (2.27) and assuming that ρ 0 is much less than unity in magnitude so
that (ρ 0 +
=
ρ 1
0
ρ ) 1
(1 -ρ 0 ), we find that
∂z p 0 +
p
1
ρ
∂p
∂z
1
0 +
g
=−
g
ρ )
ρ
ρ 0
ρ g
(2.28)
∂p
∂z
∂p
∂z
1
ρ 0
dp 0
dz
1
ρ 0
=−
+
For synoptic scale motions, the terms in (2.28) have the magnitudes
δP
ρ 0 H
∂p
∂z
ρ g
ρ 0
1
ρ 0
10 1 ms -2 ,
10 1 ms -2
Comparing these with the magnitudes of other terms in the vertical momentum
equation (Table 2.2), we see that to a very good approximation the perturbation
pressure field is in hydrostatic equilibrium with the perturbation density field so that
∂p
∂z +
ρ g
=
0
(2.29)
Therefore, for synoptic scale motions, vertical accelerations are negligible and
the vertical velocity cannot be determined from the vertical momentum equation.
However, we show in Chapter 3 that it is, nevertheless, possible to deduce the
vertical motion field indirectly.
2.5
THE CONTINUITY EQUATION
We turn now to the second of the three fundamental conservation principles, con-
servation of mass. The mathematical relationship that expresses conservation of
mass for a fluid is called the continuity equation . This section develops the con-
tinuity equation using two alternative methods. The first method is based on an
Eulerian control volume, whereas the second is based on a Lagrangian control
volume.
 
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