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Basics of Fluid Mechanics, 2014a

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4.3. PRESSURE AND DENSITY IN A GRAVITATIONAL FIELD 85<br />

density is a function <strong>of</strong> the depth. For constant bulk modulus, it was shown in “Fundamentals<br />

<strong>of</strong> Compressible Flow” by this author that the speed <strong>of</strong> sound is given by<br />

√<br />

B T<br />

c =<br />

(4.VII.a)<br />

ρ<br />

Calculate the time it take for a sound wave to propagate perpendicularly to the surface<br />

to a depth D (perpendicular to the straight surface). Assume that no variation <strong>of</strong><br />

the temperature exist. For the purpose <strong>of</strong> this exercise, the salinity can be completely<br />

ignored.<br />

Solution<br />

The equation for the sound speed is taken here as correct for very local point. However,<br />

the density is different for every point since the density varies and the density is a<br />

function <strong>of</strong> the depth. The speed <strong>of</strong> sound at any depth point, x, is to be continue<br />

??????????????<br />

B T<br />

c =<br />

=<br />

√ ρ 0 B T<br />

B T − gρ 0 z<br />

√<br />

B T − gρ 0 z<br />

ρ 0<br />

The time the sound travel a small interval distance, dz is<br />

dτ =<br />

dz<br />

√<br />

BT − gρ 0 z<br />

ρ 0<br />

(4.VII.b)<br />

(4.VII.c)<br />

The time takes for the sound the travel the whole distance is the integration <strong>of</strong> infinitesimal<br />

time<br />

⎧ - D<br />

t =<br />

⎪⎭<br />

- 0<br />

dz<br />

√<br />

BT − gρ 0 z<br />

The solution <strong>of</strong> equation (4.VII.d) is<br />

t = √ ρ 0<br />

(2 √ B T − 2 √ )<br />

B T − D<br />

ρ 0<br />

(4.VII.d)<br />

(4.VII.e)<br />

The time to travel according to the standard procedure is<br />

t =<br />

√ D = D √ ρ 0<br />

√<br />

BT BT<br />

ρ 0<br />

The ratio between the corrected estimated to the standard calculation is<br />

√ ( √<br />

ρ0 2 BT − 2 √ B T − D )<br />

correction ratio =<br />

D √ ρ 0<br />

√<br />

BT<br />

(4.VII.f)<br />

(4.VII.g)

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