Typical Signal Flow Diagram ............................................................................................................7-1
Amplifier and Loudspeaker Power Ratings ......................................................................................7-5
Wire Gauges and Line Losses .........................................................................................................7-5
Constant Voltage Distribution Systems (70-volt lines)......................................................................7-6
Low Frequency Augmentation—Subwoofers ...................................................................................7-6
Case Study A: A Speech and Music System for a Large Evangelical Church..................................7-9
Case Study B: A Distributed Sound Reinforcement System for a Large Liturgical Church ..............7-12
Case Study C: Specifications for a Distributed Sound System Comprising a Ballroom,
Small Meeting Space, and Social/Bar Area ...............................................................................7-16
Bibliography
Sound System Design Reference Manual
Preface to the 1999 Edition:
This third edition of JBL Professional’s Sound System Design Reference Manual is presented in a new
graphic format that makes for easier reading and study. Like its predecessors, it presents in virtually their
original 1977 form George Augspurger’s intuitive and illuminating explanations of sound and sound system
behavior in enclosed spaces. The section on systems and case studies has been expanded, and references
to JBL components have been updated.
The fundamentals of acoustics and sound system design do not change, but system implementation
improves in its effectiveness with ongoing developments in signal processing, transducer refinement, and
front-end flexibility in signal routing and control.
As stated in the Preface to the 1986 edition: The technical competence of professional dealers and
sound contractors is much higher today than it was when the Sound Workshop manual was originally
introduced. It is JBL’s feeling that the serious contractor or professional dealer of today is ready to move away
from simply plugging numbers into equations. Instead, the designer is eager to learn what the equations really
mean, and is intent on learning how loudspeakers and rooms interact, however complex that may be. It is for
the student with such an outlook that this manual is intended.
John Eargle
January 1999
i
Sound System Design Reference Manual
Chapter 1: Wave Propagation
Sound System Design Reference Manual
Wavelength, Frequency, and Speed of
Sound
Sound waves travel approximately 344 m/sec
(1130 ft/sec) in air. There is a relatively small velocity
dependence on temperature, and under normal
indoor conditions we can ignore it. Audible sound
covers the frequency range from about 20 Hz to 20
kHz. The wavelength of sound of a given frequency
is the distance between successive repetitions of the
waveform as the sound travels through air. It is given
by the following equation:
wavelength = speed/frequency
or, using the common abbreviations of c for speed
f
for frequency, and λ for wavelength:
,
λ = c/f
Period
(T) is defined as the time required for
one cycle of the waveform. T = 1/f.
For f = 1 kHz, T = 1/1000, or 0.001 sec, and
λ = 344/1000, or .344 m (1.13 ft.)
The lowest audible sounds have wavelengths
on the order of 10 m (30 ft), and the highest sounds
have wavelengths as short as 20 mm (0.8 in). The
range is quite large, and, as we will see, it has great
bearing on the behavior of sound.
The waves we have been discussing are of
course
speech and music signals. Figure 1-1 shows some of
the basic aspects of sine waves. Note that waves of
the same frequency can differ in both amplitude and
in phase angle. The amplitude and phase angle
relationships between sine waves determine how
they combine, either acoustically or electrically.
sine waves
, those basic building blocks of all
Figure 1-1. Properties of sine waves
1-1
Sound System Design Reference Manual
Combining Sine Waves
Referring to Figure 1-2, if two or more sine
wave signals having the same frequency and
amplitude are added, we find that the resulting signal
also has the same frequency and that its amplitude
depends upon the phase relationship of the original
signals. If there is a phase difference of 120°, the
resultant has exactly the same amplitude as either
of the original signals. If they are combined in phase,
the resulting signal has twice the amplitude of either
original. For phase differences between l20° and
240°, the resultant signal always has an amplitude
less than that of either of the original signals. If the
two signals are exactly 180° out of phase, there will
be total cancellation.
In electrical circuits it is difficult to maintain
identical phase relationships between all of the sine
components of more complex signals, except for the
special cases where the signals are combined with
a 0° or 180° phase relationship. Circuits which
maintain some specific phase relationship (45°, for
example) over a wide range of frequencies are fairly
complex. Such wide range, all-pass phase-shifting
networks are used in acoustical signal processing.
When dealing with complex signals such as
music or speech, one must understand the concept
of
coherence
through a high quality amplifier. Apart from very small
amounts of distortion, the output signal is an exact
. Suppose we feed an electrical signal
replica of the input signal, except for its amplitude.
The two signals, although not identical, are said to
be highly coherent. If the signal is passed through a
poor amplifier, we can expect substantial differences
between input and output, and coherence will not be
as great. If we compare totally different signals, any
similarities occur purely at random, and the two are
said to be non-coherent.
When two non-coherent signals are added, the
rms
(root mean square) value of the resulting signal
can be calculated by adding the relative powers of
the two signals rather than their voltages. For
example, if we combine the outputs of two separate
noise generators, each producing an rms output of
1 volt, the resulting signal measures 1.414 volts rms,
as shown in Figure 1-3.
Figure 1-3. Combining two random noise generators
1-2
Figure 1-2. Vector addition of two sine waves
Sound System Design Reference Manual
Combining Delayed Sine Waves
If two coherent wide-range signals are
combined with a specified time difference between
them rather than a fixed phase relationship, some
frequencies will add and others will cancel. Once the
delayed signal arrives and combines with the original
signal, the result is a form of “comb filter,” which
alters the frequency response of the signal, as
shown in Figure 1-4. Delay can be achieved
electrically through the use of all-pass delay
networks or digital processing. In dealing with
acoustical signals in air, there is simply no way to
avoid delay effects, since the speed of sound is
relatively slow.
Figure 1-4A. Combining delayed signals
Figure 1-4B. Combining of coherent signals with constant time delay
1-3
Sound System Design Reference Manual
A typical example of combining delayed
coherent signals is shown in Figure 1-5. Consider
the familiar outdoor PA system in which a single
microphone is amplified by a pair of identical
separated loudspeakers. Suppose the loudspeakers
in question are located at each front corner of the
stage, separated by a distance of 6 m (20 ft). At any
distance from the stage along the center line, signals
from the two loudspeakers arrive simultaneously.
But at any other location, the distances of the two
loudspeakers are unequal, and sound from one must
arrive slightly later than sound from the other. The
illustration shows the dramatically different frequency
response resulting from a change in listener position
of only 2.4 m (8 ft). Using random noise as a test
signal, if you walk from Point B to Point A and
proceed across the center line, you will hear a
pronounced swishing effect, almost like a siren. The
change in sound quality is most pronounced near the
center line, because in this area the response peaks
and dips are spread farther apart in frequency.
Figure 1-5. Generation of interference effects (comb filter response) by a split array
1-4
Figure 1-6. Audible effect of comb filters shown in Figure 1-5
Sound System Design Reference Manual
Subjectively, the effect of such a comb filter is
not particularly noticeable on normal program
material as long as several peaks and dips occur
within each one-third octave band. See Figure 1-6.
Actually, the controlling factor is the “critical
bandwidth.” In general, amplitude variations that
occur within a critical band will not be noticed as
such. Rather, the ear will respond to the signal power
contained within that band. For practical work in
sound system design and architectural acoustics, we
can assume that the critical bandwidth of the human
ear is very nearly one-third octave wide.
In houses of worship, the system should be
suspended high overhead and centered. In spaces
which do not have considerable height, there is a
strong temptation to use two loudspeakers, one on
either side of the platform, feeding both the same
program. We do not recommend this.
Diffraction of Sound
Diffraction refers to the bending of sound waves
as they move around obstacles. When sound strikes
a hard, non-porous obstacle, it may be reflected or
diffracted, depending on the size of the obstacle
relative to the wavelength. If the obstacle is large
compared to the wavelength, it acts as an effective
barrier, reflecting most of the sound and casting a
substantial “shadow” behind the object. On the other
hand, if it is small compared with the wavelength,
sound simply bends around it as if it were not there.
This is shown in Figure 1-7.
An interesting example of sound diffraction
occurs when hard, perforated material is placed in
the path of sound waves. So far as sound is
concerned, such material does not consist of a solid
barrier interrupted by perforations, but rather as an
open area obstructed by a number of small individual
objects. At frequencies whose wavelengths are small
compared with the spacing between perforations,
most of the sound is reflected. At these frequencies,
the percentage of sound traveling through the
openings is essentially proportional to the ratio
between open and closed areas.
At lower frequencies (those whose wavelengths
are large compared with the spacing between
perforations), most of the sound passes through the
openings, even though they may account only for 20
or 30 percent of the total area.
Figure 1-7. Diffraction of sound around obstacles
1-5
Sound System Design Reference Manual
Effects of Temperature Gradients on
Sound Propagation
If sound is propagated over large distances
out of doors, its behavior may seem erratic.
Differences (gradients) in temperature above ground
level will affect propagation as shown in Figure 1-8.
Refraction of sound refers to its changing direction
as its velocity increases slightly with elevated
temperatures. At Figure 1-8A, we observe a situation
which often occurs at nightfall, when the ground is
still warm. The case shown at B may occur in the
morning, and its “skipping” characteristic may give
rise to hot spots and dead spots in the listening area.
Effects of Wind Velocity and Gradients
on Sound Propagation
Figure 1-9 shows the effect wind velocity
gradients on sound propagation. The actual velocity
of sound in this case is the velocity of sound in still
air plus the velocity of the wind itself. Figure 1-10
shows the effect of a cross breeze on the apparent
direction of a sound source.
The effects shown in these two figures may be
evident at large rock concerts, where the distances
covered may be in the 200 - 300 m (600 - 900 ft)
range.
Figure 1-8. Effects of temperature gradients on sound propagation
Figure 1-9. Effect of wind velocity gradients on sound propagation
1-6
Effects of Humidity on Sound
Propagation
Contrary to what most people believe, there
is more sound attenuation in dry air than in damp air.
The effect is a complex one, and it is shown in
Figure 1-11. Note that the effect is significant only
at frequencies above 2 kHz. This means that high
frequencies will be attenuated more with distance
than low frequencies will be, and that the attenuation
will be greatest when the relative humidity is 20
percent or less.
Sound System Design Reference Manual
Figure 1-10. Effect of cross breeze on apparent direction of sound
Figure 1-11. Absorption of sound in air vs. relative humidity
1-7
Sound System Design Reference Manual
Chapter 2: The Decibel
Sound System Design Reference Manual
Introduction
In all phases of audio technology the decibel is
used to express signal levels and level differences in
sound pressure, power, voltage, and current. The
reason the decibel is such a useful measure is that it
enables us to use a comparatively small range of
numbers to express large and often unwieldy
quantities. The decibel also makes sense from a
psychoacoustical point of view in that it relates
directly to the effect of most sensory stimuli.
Power Relationships
Fundamentally, the
common logarithm of a power ratio:
For convenience, we use the
one-tenth bel. Thus:
decibel = 10 log (P1/P0)
The following tabulation illustrates the
usefulness of the concept. Letting P0 = 1 watt:
bel
is defined as the
bel = log (P1/P0)
decibel
, which is simply
signal. The convenience of using decibels is
apparent; each of these power ratios can be
expressed by the same level, 10 dB. Any 10 dB level
difference, regardless of the actual powers involved,
will represent a 2-to-1 difference in subjective
loudness.
We will now expand our power decibel table:
P1 (watts)Level in dB
10
1.251
1.602
23
2.54
3.155
46
57
6.38
89
1010
This table is worth memorizing. Knowing it, you
can almost immediately do mental calculations,
arriving at power levels in dB above, or below, one
watt.
P1 (watts)Level in dB
10
1010
10020
100030
10,00040
20,00043
Note that a 20,000-to-1 range in power can be
expressed in a much more manageable way by
referring to the powers as levels in dB above one
watt. Psychoacoustically, a ten-times increase in
power results in a level which most people judge to
be “twice as loud.” Thus, a 100-watt acoustical signal
would be twice as loud as a 10-watt signal, and a
10-watt signal would be twice as loud as a 1-watt
Here are some examples:
1. What power level is represented by 80
watts? First, locate 8 watts in the left column and
note that the corresponding level is 9 dB. Then,
note that 80 is
Thus:
2. What power level is represented by 1
milliwatt? 0.1 watt represents a level of minus 10 dB,
and 0.01 represents a level 10 dB lower. Finally,
0.001 represents an additional level decrease of 10
dB. Thus:
10 times
–10 – 10 – 10 =
8, giving another 10 dB.
9 + 10 =
19 dB
–30 dB
2-1
Sound System Design Reference Manual
3. What power level is represented by 4
milliwatts? As we have seen, the power level of 1
milliwatt is –30 dB. Two milliwatts represents a level
increase of 3 dB, and from 2 to 4 milliwatts there is
an additional 3 dB level increase. Thus:
–30 + 3 + 3 =
–24 dB
4. What is the level difference between 40 and
100 watts? Note from the table that the level
corresponding to 4 watts is 6 dB, and the level
corresponding to 10 watts is 10 dB, a difference of 4
dB. Since the level of 40 watts is 10 dB greater than
for 4 watts, and the level of 80 watts is 10 dB greater
than for 8 watts, we have:
6 – 10 + 10 – 10 =
–4 dB
We have done this last example the long way,
just to show the rigorous approach. However, we
could simply have stopped with our first observation,
noting that the dB level difference between 4 and 10
watts, .4 and 1 watt, or 400 and 1000 watts will
always be the same, 4 dB, because they all
represent the same power ratio.
The level difference in dB can be converted
back to a power ratio by means of the following
equation:
Power ratio = 10
dB/10
For example, find the power ratio of a level
difference of 13 dB:
Power ratio = 10
13/10
= 10
1.3
= 20
Voltage, Current, and Pressure
Relationships
The decibel fundamentally relates to power
ratios, and we can use voltage, current, and pressure
ratios as they relate to power. Electrical power can
be represented as:
P = EI
P = I2Z
P = E2/Z
Because power is proportional to the square of
the voltage, the effect of
quadruple
the power:
As an example, let E = 1 volt and Z = 1 ohm.
Then, P = E2/Z = 1 watt. Now, let E = 2 volts; then,
P = (2)2/1 = 4 watts.
The same holds true for current, and the
following equations must be used to express power
levels in dB using voltage and current ratios:
dB level = 10 log
dB level = 10 log
doubling
the voltage is to
(2E)2/Z = 4(E)2/Z
2
E
1
20 log
=
E
0
2
I
1
=
I
0
20 log
E
1
, and
E
0
I
1
.
I
0
The reader should acquire a reasonable skill in
dealing with power ratios expressed as level
differences in dB. A good “feel” for decibels is a
qualification for any audio engineer or sound
contractor. An extended nomograph for converting
power ratios to level differences in dB is given in
Figure 2-1.
Figure 2-1. Nomograph for determining power ratios directly in dB
2-2
Sound pressure is analogous to voltage, and
levels are given by the equation:
P
dB level = 20 log
1
.
P
0
Sound System Design Reference Manual
The normal reference level for voltage, E0, is
one volt. For sound pressure, the reference is the
extremely low value of 20 x 10
-6
newtons/m2. This
reference pressure corresponds roughly to the
minimum audible sound pressure for persons with
normal hearing. More commonly, we state pressure
in
pascals
(Pa), where 1 Pa = 1 newton/m2. As a
convenient point of reference, note that an rms
pressure of 1 pascal corresponds to a sound
pressure level of 94 dB.
We now present a table useful for determining
levels in dB for ratios given in voltage, current, or
sound pressure:
Voltage, Current or
Pressure RatiosLevel in dB
10
1.252
1.604
26
2.58
3.1510
412
514
6.316
818
1020
This table may be used exactly the same way
as the previous one. Remember, however, that the
reference impedance, whether electrical or
acoustical, must remain fixed when using these
ratios to determine level differences in dB. A few
examples are given:
If we simply compare input and output voltages,
we still get 0 dB as our answer. The
voltage gain
is in
fact unity, or one. Recalling that decibels refer
primarily to power ratios, we must take the differing
input and output impedances into account and
actually compute the input and output powers.
Input power =
Output power =
T 10 log
600
15
E
2
Z
= 10 log 40 = 16 dBhus,
=
E
Z
2
1
600
=
watt
1
15
Fortunately, such calculations as the above are
not often made. In audio transmission, we keep track
of operating levels primarily through voltage level
calculations in which the voltage reference value of
0.775 volts has an assigned level of 0 dBu. The
value of 0.775 volts is that which is applied to a 600ohm load to produce a power of 1 milliwatt (mW). A
power level of 0 dBm corresponds to 1 mW. Stated
somewhat differently, level values in dBu and dBm
will have the same numerical value only when the
load impedance under consideration is 600 ohms.
The level difference in dB can be converted
back to a voltage, current, or pressure ratio by
means of the following equation:
Ratio = 10
dB/20
1. Find the level difference in dB between 2
volts and 10 volts. Directly from the table we observe
20 – 6 =
14 dB
.
2. Find the level difference between 1 volt and
100 volts. A 10-to-1 ratio corresponds to a level
difference of 20 dB. Since 1-to-100 represents the
product of
two
such ratios (1-to-10 and 10-to-100),
the answer is
20 + 20 = 40 dB.
3. The signal input to an amplifier is 1 volt, and
the input impedance is 600 ohms. The output is also
1 volt, and the load impedance is 15 ohms. What is
the gain of the amplifier in dB? Watch this one
carefully!
For example, find the voltage ratio
corresponding to a level difference of 66 dB:
voltage ratio = 10
66/20
= 10
3.3
= 2000.
2-3
Sound System Design Reference Manual
Sound Pressure and Loudness Contours
We will see the term dB-SPL time and again in
professional sound work. It refers to sound pressure
levels in dB above the reference of 20 x 10-6 N/m2.
We commonly use a
measure SPL. Loudness and sound pressure
obviously bear a relation to each other, but they are
not the same thing. Loudness is a subjective
sensation which differs from the measured level in
certain important aspects. To specify loudness in
scientific terms, a different unit is used, the
Phons and decibels share the same numerical value
only at 1000 Hz. At other frequencies, the phon scale
deviates more or less from the sound level scale,
depending on the particular frequency and the
sound pressures; Figure 2-2 shows the relationship
between phons and decibels, and illustrates the
well-known Robinson-Dadson equal loudness
contours. These show that, in general, the ear
becomes less sensitive to sounds at low frequencies
as the level is reduced.
sound level meter
(SLM) to
phon
.
When measuring sound pressure levels,
weighted response may be employed to more closely
approximate the response of the ear. Working with
sound systems, the most useful scales on the sound
level meter will be the A-weighting scale and the
linear scale, shown in Figure 2-3. Inexpensive sound
level meters, which cannot provide linear response
over the full range of human hearing, often have no
linear scale but offer a C-weighting scale instead. As
can be seen from the illustration, the C-scale rolls off
somewhat at the frequency extremes. Precision
sound level meters normally offer
in addition to linear response. Measurements made
with a sound level meter are normally identified by
noting the weighting factor, such as: dB(A) or dB(lin).
Typical levels of familiar sounds, as shown in
Figure 2-4, help us to estimate dB(A) ratings when a
sound level meter is not available. For example,
normal conversational level in quiet surrounds is
about 60 dB(A). Most people find levels higher than
100 dB(A) uncomfortable, depending on the length of
exposure. Levels much above 120 dB(A) are
definitely dangerous to hearing and are perceived as
painful by all except dedicated rock music fans.
A, B,
and C scales
2-4
Figure 2-2. Free-field equal loudness contours
Sound System Design Reference Manual
Figure 2-3. Frequency responses for SLM weighting characteristics
Figure 2-4. Typical A-weighted sound levels
2-5
Sound System Design Reference Manual
Inverse Square Relationships
When we move away from a
sound out of doors, or in a
free field
SPL falls off almost exactly 6 dB for each doubling of
distance away from the source. The reason for this is
shown in Figure 2-5. At A there is a sphere of radius
one meter surrounding a point source of sound P
representing the SPL at the surface of the sphere. At
B, we observe a sphere of twice the radius, 2 meters.
The area of the larger sphere is
smaller one, and this means that the acoustical
power passing through a small area on the larger
sphere will be
one-fourth
that passing through the
same small area on the smaller sphere. The 4-to-1
power ratio represents a level difference of 6 dB, and
the corresponding sound pressure ratio will be 2-to-1.
A convenient nomograph for determining
inverse square losses is given in Figure 2-6. Inverse
square calculations depend on a theoretical point
source in a free field. In the real world, we can
point source
, we observe that
four times
that of the
of
1
closely approach an ideal free field, but we still must
take into account the factors of finite source size and
non-uniform radiation patterns.
Consider a horn-type loudspeaker having a
rated sensitivity of 100 dB, 1 watt at 1 meter. One
meter from where? Do we measure from the mouth
of the horn, the throat of the horn, the driver
diaphragm, or some indeterminate point in between?
Even if the measurement position is specified, the
information may be useless. Sound from a finite
source does not behave according to inverse square
law at distances close to that source. Measurements
made in the “near field” cannot be used to estimate
performance at greater distances. This being so, one
may well wonder why loudspeakers are rated at a
distance of only 1 meter.
The method of rating and the accepted
methods of measuring the devices are two different
things. The manufacturer is expected to make a
number of measurements at various distances under
free field conditions. From these he can establish
2-6
Figure 2-5. Inverse square relationships
Figure 2-6. Nomograph for determining inverse square losses
Sound System Design Reference Manual
that the measuring microphone is far enough away
from the device to be in its
calculate the imaginary point from which sound
waves diverge, according to inverse square law. This
point is called the
accurate field measurements have been made, the
results are converted to an equivalent one meter
rating. The rated sensitivity at one meter is that SPL
which would be measured if the inverse square
relationship were actually maintained that close to
the device.
Let us work a few exercises using the
nomograph of Figure 2-6:
1. A JBL model 2360 horn with a 2446 HF driver
produces an output of 113 dB, 1 watt at 1 meter.
What SPL will be produced by 1 watt at 30 meters?
We can solve this by inspection of the nomograph.
Simply read the difference in dB between 1 meter
and 30 meters: 29.5 dB. Now, subtracting this from
113 dB:
2. The nominal power rating of the JBL model
2446 driver is 100 watts. What maximum SPL will be
produced at a distance of 120 meters in a free field
when this driver is mounted on a JBL model 2366
horn?
There are three simple steps in solving this
problem. First, determine the inverse square loss
from Figure 2-6; it is approximately 42 dB. Next,
determine the level difference between one watt and
100 watts. From Figure 2-1 we observe this to be 20
dB. Finally, note that the horn-driver sensitivity is 118
dB, 1 watt at 1 meter. Adding these values:
Calculations such as these are very
commonplace in sound reinforcement work, and
qualified sound contractors should be able to make
them easily.
acoustic center
113 – 29.5 = 83.5 dB
118 – 42 + 20 = 96 dB-SPL
far field
, and he can also
of the device. After
Adding Power Levels in dB
Quite often, a sound contractor will have to
add power levels expressed in dB. Let us assume
that two sound fields, each 94 dB-SPL, are
combined. What is the resulting level? If we simply
add the levels numerically, we get 188 dB-SPL,
clearly an absurd answer! What we must do in effect
is convert the levels back to their actual powers, add
them, and then recalculate the level in dB. Where
two levels are involved, we can accomplish this
easily with the data of Figure 2-7. Let D be the
difference in dB between the two levels, and
determine the value N corresponding to this
difference. Now, add N to the
original values.
As an exercise, let us add two sound fields, 90
dB-SPL and 84 dB-SPL. Using Figure 2-7, a D of 6
dB corresponds to an N of about 1 dB. Therefore, the
new level will be 91 dB-SPL.
Note that when two levels differ by more than
about 10 dB, the resulting summation will be
substantially the same as the higher of the two
values. The effect of the lower level will be negligible.
higher
of the two
Reference Levels
Although we have discussed some of the
common reference levels already, we will list here all
of those that a sound contractor is likely to
encounter.
In acoustical measurements,
measured relative to 20 x 10-6 Pa. An equivalent
expression of this is .0002 dynes/cm2.
In broadcast transmission work, power is often
expressed relative to 1 milliwatt (.001 watt), and such
levels are expressed in
The designation
one watt. Thus, 0 dBW = 30 dBm.
In signal transmission diagrams, the
designation
.775 volts.
dBu
indicates voltage levels referred to
dBm
dBW
refers to levels relative to
SPL
is always
.
Figure 2-7. Nomograph for adding levels expressed in dB.
Summing sound level output of two sound sources where D is their output difference in dB.
N is added to the higher to derive the total level.
2-7
Sound System Design Reference Manual
In other voltage measurements,
dBV
refers to
levels relative to 1 volt.
Rarely encountered by the sound contractor will
be acoustical power levels. These are designated
dB-PWL, and the reference power is 10
-12
watts. This
is a very small power indeed. It is used in acoustical
measurements because such small amounts of
power are normally encountered in acoustics.
Peak, Average, and
rms
Signal Values
Most measurements of voltage, current, or
sound pressure in acoustical engineering work are
given as
rms
(root mean square) values of the
waveforms. The rms value of a repetitive waveform
equals its equivalent DC value in power
transmission. Referring to Figure 2-8A for a sine
wave with a peak value of one volt, the rms value is
.707 volt, a 3 dB difference. The average value of the
waveform is .637 volt.
For more complex waveforms, such as are
found in speech and music, the peak values will be
considerably higher than the average or rms values.
The waveform shown at Figure 2-8B is that of a
trumpet at about 400 Hz, and the spread between
peak and average values is 13 dB.
In this chapter, we have in effect been using
rms values of voltage, current, and pressure for all
calculations. However, in all audio engineering
applications, the time-varying nature of music and
speech demands that we consider as well the
instantaneous values of waveforms likely to be
encountered. The term
headroom
refers to the extra
margin in dB designed into a signal transmission
system over its normal operating level. The
importance of headroom will become more evident
as our course develops.
2-8
Figure 2-8. Peak, average, and rms values.
Sinewave (A); complex waveform (B).
Sound System Design Reference Manual
Chapter 3: Directivity and Angular
Coverage of Loudspeakers
Introduction
Proper coverage of the audience area is one of
the prime requirements of a sound reinforcement
system. What is required of the sound contractor is
not only a knowledge of the directional
characteristics of various components but also how
those components may interact in a multi-component
array. Such terms as directivity index (DI), directivity
factor (Q), and beamwidth all variously describe the
directional properties of transducers with their
associated horns and enclosures. Detailed polar
data, when available, gives the most information of
all. In general, no one has ever complained of having
too much directivity information. In the past, most
manufacturers have supplied too little; however,
things have changed for the better in recent years,
largely through data standardization activities on the
part of the Audio Engineering Society.
Some Fundamentals
Assume that we have an omnidirectional
radiator located in free space and that there is a
microphone at some fixed distance from it. This is
shown in Figure 3-1A. Let the power radiated from
the loudspeaker remain constant, and note the SPL
at the microphone. Now, as shown in B, let us place
a large reflecting boundary next to the source and
again note the SPL at the microphone. At high
frequencies (those whose wavelengths are small
compared to the size of the reflecting boundary), the
increase in SPL will be 3 dB. The power that was
radiating into full space is now confined to half
space; thus, the doubling of power at the
microphone. Moving on to the example at C, we
place a dihedral (2-sided) corner next to the source.
Power that was confined to half-space now radiates
into quarter-space, and the SPL at the microphone
Figure 3-1. Directivity and angular coverage
3-1
Sound System Design Reference Manual
increases another 3 dB. Continuing on at D, we
place the sound source in a trihedral (3-sided)
corner, and we note an additional 3 dB increase as
sound power is radiated into one-eighth-space.
We could continue this exercise further, but our
point has already been made. In going from A to D in
successive steps, we have increased the
index
3 dB at each step, and we have doubled the
directivity factor
at each step.
directivity
We will now define these terms: Directivity
index is the level difference in intensity along a given
axis, and at a given distance, from a sound radiator
compared to the intensity that would be produced at
the same distance by an omnidirectional point source
radiating the same power. Directivity factor is the
ratio of the two intensities. Details are shown in
Figure 3-2. Directivity index (DI) and directivity factor
(Q) are related as follows:
DI = l0 log Q
DI/10
Q = 10
3-2
Figure 3-2. Directivity index and directivity factor
Figure 3-3. Illustration of Molloy’s equation
Sound System Design Reference Manual
The data of Figure 3-1 was generalized by
Molloy (7) and is shown in Figure 3-3. Here, note that
Dl and Q are related to the solid angular coverage of
a hypothetical sound radiator whose horizontal and
vertical coverage angles are specified. Such ideal
sound radiators do not exist, but it is surprising how
closely these equations agree with measured Dl and
Q of HF horns that exhibit fairly steep cut-off outside
their normal coverage angles.
As an example of this, a JBL model 2360
Bi-Radial horn has a nominal 900-by-400 pattern
measured between the 6 dB down points in each
plane. If we insert the values of 90° and 40° into
Molloy’s equation, we get DI = 11 and Q = 12.8. The
published values were calculated by integrating
response over 360° in both horizontal and vertical
planes, and they are Dl = 10.8 and Q = 12.3. So the
estimates are in excellent agreement with the
measurements.
For the JBL model 2366 horn, with its nominal
6 dB down coverage angles of 40° and 20°, Molloy’s
equation gives Dl = 17.2 and Q = 53. The published
values are Dl = 16.5 and Q = 46. Again, the
agreement is excellent.
Is there always such good correlation between
the 6 dB down horizontal and vertical beamwidth of a
horn and its calculated directivity? The answer is no.
Only when the response cut-off is sharp beyond the
6 dB beamwidth limits and when there is minimal
radiation outside rated beamwidth will the correlation
be good. For many types of radiators, especially those
operating at wavelengths large compared with their
physical dimensions, Molloy’s equation will not hold.
A Comparison of Polar Plots, Beamwidth
Plots, Directivity Plots, and Isobars
There is no one method of presenting
directional data on radiators which is complete in all
regards. Polar plots (Figure 3-4A) are normally
presented in only the horizontal and vertical planes.
A single polar plot covers only a single frequency, or
frequency band, and a complete set of polar plots
takes up considerable space. Polars are, however,
the only method of presentation giving a clear picture
of a radiator’s response outside its normal operating
beamwidth. Beamwidth plots of the 6 dB down
coverage angles (Figure 3-4B) are very common
because considerable information is contained in a
single plot. By itself, a plot of Dl or Q conveys
information only about the on-axis performance of a
radiator (Figure 3-4C). Taken together, horizontal and
vertical beamwidth plots and Dl or Q plots convey
sufficient information for most sound reinforcement
design requirements.
Figure 3-4. Methods of presenting directional information
3-3
Sound System Design Reference Manual
Isobars have become popular in recent years.
They give the angular contours in spherical
coordinates about the principal axis along which the
response is -3, -6, and -9 dB, relative to the on-axis
maximum. It is relatively easy to interpolate visually
between adjacent isobars to arrive at a reasonable
estimate of relative response over the useful frontal
solid radiation angle of the horn. Isobars are useful in
advanced computer layout techniques for
determining sound coverage over entire seating
areas. The normal method of isobar presentation is
shown in Figure 3-4D.
Still another way to show the directional
characteristics of radiators is by means of a family of
off-axis frequency response curves, as shown in
Figure 3-5. At A, note that the off-axis response
curves of the JBL model 2360 Bi-Radial horn run
almost parallel to the on-axis response curve. What
this means is that a listener seated off the main axis
will perceive smooth response when a Bi-Radial
constant coverage horn is used. Contrast this with
the off-axis response curves of the older (and
obsolete) JBL model 2350 radial horn shown at B. If
this device is equalized for flat on-axis response,
then listeners off-axis will perceive rolled-off HF
response.
Directivity of Circular Radiators
Any radiator has little directional control for
frequencies whose wavelengths are large compared
with the radiating area. Even when the radiating area
is large compared to the wavelength, constant
pattern control will not result unless the device has
been specifically designed to maintain a constant
pattern. Nothing demonstrates this better than a
simple radiating piston. Figure 3-6 shows the
sharpening of on-axis response of a piston mounted
in a flat baffle. The wavelength varies over a 24-to-1
range. If the piston were, say a 300 mm (12”)
loudspeaker, then the wavelength illustrated in the
figure would correspond to frequencies spanning the
range from about 350 Hz to 8 kHz.
Among other things, this illustration points out
why “full range,” single-cone loudspeakers are of
little use in sound reinforcement engineering. While
the on-axis response can be maintained through
equalization, off-axis response falls off drastically
above the frequency whose wavelength is about
equal to the diameter of the piston. Note that when
the diameter equals the wavelength, the radiation
pattern is approximately a 90° cone with - 6 dB
response at ±45°.
3-4
Figure 3-5. Families of off-axis frequency response curves
Sound System Design Reference Manual
The values of DI and Q given in Figure 3-6 are
the on-axis values, that is, along the axis of
maximum loudspeaker sensitivity. This is almost
always the case for published values of Dl and Q.
However, values of Dl and Q exist along
any
axis of
the radiator, and they can be determined by
inspection of the polar plot. For example, in Figure
3-6, examine the polar plot corresponding to
Diameter = λ. Here, the on-axis Dl is 10 dB. If we
simply move off-axis to a point where the response
has dropped 10 dB, then the Dl along that direction
will be 10 - 10, or 0 dB, and the Q will be unity. The
off-axis angle where the response is 10 dB down is
marked on the plot and is at about 55°. Normally, we
will not be concerned with values of Dl and Q along
axes other than the principal one; however, there are
certain calculations involving interaction of
microphones and loudspeakers where a knowledge
of off-axis directivity is essential.
Omnidirectional microphones with circular
diaphragms respond to on- and off-axis signals in a
manner similar to the data shown in Figure 3-6. Let
us assume that a given microphone has a diaphragm
about 25 mm (1”) in diameter. The frequency
corresponding to λ/4 is about 3500 Hz, and the
response will be quite smooth both on and off axis.
However, by the time we reach 13 or 14 kHz, the
diameter of the diaphragm is about equal to λ, and
the Dl of the microphone is about 10 dB. That is, it
will be 10 dB more sensitive to sounds arriving on
axis than to sounds which are randomly incident to
the microphone.
Of course, a piston is a very simple radiator —
or receiver. Horns such as JBL’s Bi-Radial series are
complex by comparison, and they have been
designed to maintain constant HF coverage through
attention to wave-guide principles in their design.
One thing is certain: no radiator can exhibit much
pattern control at frequencies whose wavelengths
are much larger than the circumference of the
radiating surface.
Figure 3-6. Directional characteristics of a circular-piston source
mounted in an infinite baffle as a function of diameter and λ.
3-5
Sound System Design Reference Manual
The Importance of Flat Power Response
If a radiator exhibits flat power response, then
the power it radiates, integrated over all directions,
will be constant with frequency. Typical compression
drivers inherently have a rolled-off response when
measured on a
Figure 3-7A. When such a driver is mounted on a
typical radial horn such as the JBL model 2350, the
on-axis response of the combination will be the sum
of the PWT response and the Dl of the horn. Observe
at B that the combination is fairly flat on axis and
does not need additional equalization. Off-axis
response falls off, both vertically and horizontally,
and the total power response of the combination will
be the same as observed on the PWT; that is, it rolls
off above about 3 kHz.
plane wave tube
(PWT), as shown in
Now, let us mount the same driver on a BiRadial uniform coverage horn, as shown at C. Note
that both on-and off-axis response curves are rolled
off but run parallel with each other. Since the Dl of
the horn is essentially flat, the on-axis response will
be virtually the same as the PWT response.
At D, we have inserted a HF boost to
compensate for the driver’s rolled off power
response, and the result is now flat response both on
and off axis. Listeners anywhere in the area covered
by the horn will appreciate the smooth and extended
response of the system.
Flat power response makes sense only with
components exhibiting constant angular coverage.
If we had equalized the 2350 horn for flat power
response, then the on-axis response would have
been too bright and edgy sounding.
3-6
Figure 3-7. Power response of HF systems
Sound System Design Reference Manual
The rising DI of most typical radial horns is
accomplished through a narrowing of the vertical
pattern with rising frequency, while the horizontal
pattern remains fairly constant, as shown in Figure
3-8A. Such a horn can give excellent horizontal
coverage, and since it is “self equalizing” through its
rising DI, there may be no need at all for external
equalization. The smooth-running horizontal and
vertical coverage angles of a Bi-Radial, as shown at
Figure 3-8B, will always require power response HF
boosting.
Measurement of Directional
Characteristics
Polar plots and isobar plots require that the
radiator under test be rotated about several of its
axes and the response recorded. Beamwidth plots
may be taken directly from this data.
DI and Q can be calculated from polar data by
integration using the following equation:
sin d
2
θθ
DI = 10 log
P
is taken as unity, and θ is taken in 10° increments.
Θ
π
∫
o
P
(
2
2
)
θ
The integral is solved for a value of DI in the
horizontal plane and a value in the vertical plane.
The resulting DI and Q for the radiator are given as:
DI
DI
DI =
hv
+
2
and
Figure 3-8. Increasing DI through narrowing
vertical beamwidth
Q = Q Q
⋅
nv
(Note: There are slight variations of this
method, and of course all commonly use methods
are only approximations in that they make use of
limited polar data.)
3-7
Sound System Design Reference Manual
Using Directivity Information
A knowledge of the coverage angles of an HF
horn is essential if the device is to be oriented
properly with respect to an audience area. If polar
plots or isobars are available, then the sound
contractor can make calculations such as those
indicated in Figure 3-9. The horn used in this
example is the JBL 2360 Bi-Radial. We note from the
isobars for this horn that the -3 dB angle off the
vertical is 14°. The -6 dB and -9 dB angles are 23°
and 30° respectively. This data is for the octave band
centered at 2 kHz. The horn is aimed so that its
major axis is pointed at the farthest seats. This will
ensure maximum reach, or “throw,” to those seats.
We now look at the -3 dB angle of the horn and
compare the reduction in the horn’s output along that
angle with the inverse square advantage at the
closer-in seats covered along that axis. Ideally, we
would like for the inverse square advantage to
exactly match the horn’s off-axis fall-off, but this is
not always possible. We similarly look at the
response along the -6 and -9 dB axes of the horn,
Figure 3-9. Off-axis and inverse square calculations
comparing them with the inverse square advantages
afforded by the closer-in seats. When the designer
has flexibility in choosing the horn’s location, a good
compromise, such as that shown in this figure, will be
possible. Beyond the -9 dB angle, the horn’s output
falls off so rapidly that additional devices, driven at
much lower levels, would be needed to cover the
front seats (often called “front fill” loudspeakers).
Aiming a horn as shown here may result in a
good bit of power being radiated toward the back
wall. Ideally, that surface should be fairly absorptive
so that reflections from it do not become a problem.
Directional Characteristics of Combined
Radiators
While manufacturers routinely provide data on
their individual items of hardware, most provide little,
if any, data on how they interact with each other. The
data presented here for combinations of HF horns is
of course highly wavelength, and thus size,
dependent. Appropriate scaling must be done if this
data is to be applied to larger or smaller horns.
In general, at high frequencies, horns will act
independently of each other. If a pair of horns are
properly splayed so that their -6 dB angles just
overlap, then the response along that common axis
should be smooth, and the effect will be nearly that of
a single horn with increased coverage in the plane of
overlap. Thus, two horns with 60° coverage in the
horizontal plane can be splayed to give 120°
horizontal coverage. Likewise, dissimilar horns can
be splayed, with a resulting angle being the sum of
the two coverage angles in the plane of the splay.
Splaying may be done in the vertical plane with
similar results. Figure 3-10 presents an example of
horn splaying in the horizontal plane.
3-8
Figure 3-10. Horn splaying for wider coverage
Loading...
+ 74 hidden pages
You need points to download manuals.
1 point = 1 manual.
You can buy points or you can get point for every manual you upload.