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Introduction to Acoustics

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found from<br />

�<br />

LW = Lp + 10 log A<br />

+ 4.34<br />

A0<br />

A<br />

S<br />

�<br />

+ 10 log 1 + Sc<br />

�<br />

8Vf<br />

� �<br />

427 273<br />

−25 log<br />

400 273 + θ<br />

� �<br />

B<br />

− 6<br />

B0<br />

dB re 10 −12 W , (23.31)<br />

where LW is the band sound power level of the sound<br />

source under test, Lp is the band space-averaged sound<br />

pressure level of the sound source under test, A is the<br />

equivalent absorption area of the room, given by:<br />

A = 55.26<br />

� �<br />

V<br />

,<br />

c Trev<br />

V is the room volume, Trev is the reverberation time for<br />

the particular band, A0 is the reference absorption area,<br />

S is the <strong>to</strong>tal surface area of the room, f is the midband<br />

frequency of the measurement, c is the speed of sound<br />

at temperature θ in ◦C, B is the atmospheric pressure,<br />

with B0 = 1.013 × 105 Pa, V0 = 1m3 , T0 = 1s.<br />

Diffuse sound fields can be obtained in labora<strong>to</strong>ry<br />

reverberation rooms. Sufficiently close engineering<br />

approximations <strong>to</strong> diffuse-field conditions can be obtained<br />

in rooms that are fairly reverberant and irregularly<br />

shaped. When these environments are not available or<br />

when it is not possible <strong>to</strong> move the noise source under<br />

test, other techniques valid for the in situ determination<br />

of sound power level may be used and are described later<br />

in this section.<br />

Non-steady and impulsive noises are difficult <strong>to</strong> measure<br />

under reverberant-field conditions. Measurements<br />

on such noise sources should be made under free-field<br />

conditions.<br />

Sound Power Determination<br />

in an Ordinary Room<br />

The sound pressure field in an ordinary room such as<br />

an office or labora<strong>to</strong>ry space that has not been designed<br />

for acoustical measurements is neither a free-field nor<br />

a diffuse field. Here the relationship between the sound<br />

intensity and the mean-square pressure is more complicated.<br />

Instead of measuring the mean-square pressure,<br />

it is usually more advantageous <strong>to</strong> use a sound intensity<br />

analyzer that measures the sound intensity directly<br />

(Sect. 23.1.8). By sampling the sound intensity at defined<br />

locations in the vicinity of the source, the sound<br />

power level of the source can be determined. A standard<br />

for the in situ determination of sound power is also<br />

available, and is described below.<br />

Noise 23.2 Noise Sources 973<br />

Source Directivity<br />

Most sources of sound [23.15, 16] of practical interest<br />

are directional <strong>to</strong> some degree. If one measures the sound<br />

pressure level in a given frequency band a fixed distance<br />

away from the source, different levels will generally be<br />

found for different directions. A plot of these levels in<br />

polar fashion at the angles for which they were obtained<br />

is called the directivity pattern of the source.<br />

The directivity fac<strong>to</strong>r Qθ is defined as the ratio of the<br />

mean-square sound pressure, p2 θ , at angle θ and distance<br />

r from an actual source radiating W and the mean-square<br />

sound pressure p2 S at the same distance from a nondirectional<br />

source radiating the same acoustic power W.<br />

Alternatively, Qθ is defined as the ratio of the intensity<br />

in the direction of propagation W/m2 at angle θ and distance<br />

r from an actual source <strong>to</strong> the intensity at the same<br />

distance from a nondirectional source, both sources radiating<br />

the same sound power W. It must be assumed<br />

that the directivity fac<strong>to</strong>r is independent of distance from<br />

the source.<br />

The directivity index DIθ of a sound source on a rigid<br />

plane (radiating in<strong>to</strong> hemispherical space) at angle θ and<br />

for a given frequency band is computed from<br />

DIθ = Lpθ −〈Lp〉H + 3dB, (23.32)<br />

where Lpθ is the sound pressure level measured a distance<br />

r and angle θ from the source, and 〈Lp〉H is the<br />

sound pressure level of the space-averaged mean-square<br />

pressure averaged over a test hemisphere of radius r (and<br />

area 2πr 2 ) centered on and surrounding the source.<br />

The 3 dB in this equation is added <strong>to</strong> 〈Lp〉H because<br />

the measurement was made over a hemisphere<br />

instead of a full sphere. The reason for this is that the<br />

intensity at radius r is twice as large if a source radiates<br />

in<strong>to</strong> a hemisphere as compared <strong>to</strong> a sphere. That<br />

is, if a nondirectional source were <strong>to</strong> radiate uniformly<br />

in<strong>to</strong> hemispherical space, DIθ = DI = 3 dB. Equations<br />

are available for sound radiation in<strong>to</strong> a sphere and in<strong>to</strong><br />

a quarter sphere [23.15, 16].<br />

23.2.2 International Standards for the<br />

Determination of Sound Power<br />

The International Organization for Standardization<br />

(ISO) has published a series of international standards,<br />

the ISO 3740 series [23.17], which describes several<br />

methods for determining the sound power levels of noise<br />

sources. Table 23.3 summarizes the applicability of each<br />

of the basic standards of the ISO 3740 series. The most<br />

important fac<strong>to</strong>r in selecting an appropriate noise mea-<br />

Part G 23.2

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