The decade of the 1980’s saw many improvements in the quality of cinema sound. Dolby
Laboratories had begun the cinema sound revolution during the middle 1970’s with the introduction of
noise reduction and equalization of cinema loudspeaker systems. In 1981, JBL demonstrated the first
flat power response loudspeaker systems at the Academy of Motion Picture Arts and Sciences. In
1983, Lucasfilm introduced the
THX@
system, along with their program of cinema certification. As the
1980’s progressed, Dolby stereo optical sound tracks gained in favor, increasing the number of stereo
houses significantly. The application of Dolby Spectral Recording (SR) to cinema release prints
represented another step forward in sound quality.
By the mid
199Os,
three digital systems had been introduced into the cinema, Dolby SR-D.
Digital Theater Sound (DTS), and Sony Dynamic Digital Sound (SDDS). These systems have similar
digital performance characteristics, and they all provide analog stereo optical tracks for overall
compatibility and operational redundancy, should the digital portion of the system fail, or momentarily
go into a mute mode. DTS makes use of a synchronized CD-ROM for its digital program, while the
other two include the digital information on the print itself.
As new cinema complexes are being pianned and constructed, acoustical engineers are now
more than ever before being engaged to deal with problems of architectural acoustics and sound
isolation between adjacent exhibition spaces. More attention is being paid to the specification of
sound equipment and its careful integration into the cinema environment.
JBL has a strong commitment to the cinema sound market. We have become the
acknowledged leader in the field, and our products are routinely specified for major studios and
post-
production houses throughout the world. JBL continues its rapid pace in new product development
aimed at increasing performance levels in the cinema.
This manual has several goals. First, it will provide a background in basic systems concepts,
and then move on to acoustical considerations in the cinema. The subject of electroacoustical
specification will be discussed, as will the problems of mounting and aiming of the components.
Electrical interface and system checkout will be covered in detail. JBL believes that the more dealers
and installers know about the basics of sound in the cinema, the better will be the results of their work
in all areas.
II. BASIC SYSTEM CONCEPTS
A. Analog Film Formats
There are two film sizes for theatrical exhibition: 35 mm and 70 mm. The most common
projection image aspect ratios (horizontal vs. vertical) for 35 mm can be either 1.851 (“flat”) or
(“scope”). Seventy mm prints are normally projected at a ratio of
2.2:1.
The advantages of 70 mm
2.35:1
have, in the past, been the availability of six magnetic tracks and large image area. The cost of a 70
mm print is quite high, and these prints have normally been made in limited quantities for exhibition in
premier houses in large metropolitan locations. Today, the general practice with 70 mm is to use three
channels behind the screen (left, center, and right) and a single surround channel feeding multiple
page
2
loudspeakers. Options are to use the two remaining magnetic tracks for subwoofer signals and/or split
(dual channel) surrounds.
The 35 mm format was modified during the 1950’s to handle four magnetic tracks: three screen
channels and a single surround channel. At the same time, the standard monophonic variable area
optical track was maintained. Figures IA and B show the channel layout for both 70 mm and 35 mm
magnetic standards. At present, the 35 mm magnetic standard is no longer in general use.
A. 70
mm
0.35
mm
A
I
’
MAGNETiC
STRIPING
Figure 1. 70mm six-track magnetic format (A); 35mm four-track magnetic format (B)
Figure 2A. 35mm Dolby Stereo Optical format
page
3
I
rOUTPUTS
--QL
-_o
C
--_o R
-_o
SURROUNDS
0
SUBWOOFER
I
LT
RTO
INPUTS ----
0
ADAPTIVE
MATRIX
*
+
c
MASTER
LEVEL
CONTROL
I
AUDIO
DELAY
-
i kHz
LOW-PASS
FILTER
-
Figure 28. Block diagram of the Dolby Stereo Optical playback matrix
B~TYPE
NR
DECODER
Today, the Dolby Stereo Optical system is virtually a standard format on non-digital 35 mm
film. In this process, the dual bilateral variable area optical sound tracks, which were formerly
modulated with a monophonic signal, are now modulated in stereo, as shown in Figure 2A. Recording
on the two sound tracks is accomplished through a matrix, which accepts inputs for the three screen
channels and the single surround channel. The signals intended primarily for the left and right screen
loudspeakers are fed to the left and right channels. Program material intended for the center screen
loudspeaker, including most on-screen dialog, is fed to both stereo channels in phase. The in-phase
relationship between the stereo channels triggers the playback matrix to steer that information
primarily to the center screen loudspeaker, through a combination of gain control and altering of
separation coefficients within the matrix. In a similar manner, information intended for the surround
channels is fed to both stereo channels so that there is a 180” phase relationship between them. This
phase relationship triggers the playback matrix to steer that information primarily to the surround
loudspeaker array.
Figure 2B shows details of the playback matrix used in Dolby Stereo Optical soundtracks. The
surround channel is delayed relative to the other channels so that, by the precedence (or
Haas)
effect,
the surround channel will not dominate the perceived sound field in the middle and back of the house.
The reason for this is that the matrix output contains certain “leakage” signals that may be disturbing to
a listener if such signals were to be heard from the surround loudspeakers. in practice, the surround
channel is delayed with respect to the screen channels so that the most distant listener in the cinema
will hear that channel delayed by a minimum of 20 milliseconds. Since the ear will “lock in” on earlier
arrival sounds, localization will be maintained in the direction of the screen for all patrons, while effects
intended only for the surround channel will be
problem is further addressed by rolling off the response of the surround channel above about 7
clearly heard from the surround loudspeakers. This
kHz.
B. Digital Film Formats
The Dolby SR-D format, introduced in 1992, is shown in Figure 3A. It has exactly the same
optical sound tracks as shown in Figure 2A with the addition of digital information located in the
otherwise unused space between sprocket holes. This new digital format provides the usual three
screen channels plus a split surround pair and a single low frequency (subwoofer) channel limited to
100 Hz. This is commonly referred to as a “5.1’ channel system and uses an elaborate perceptual
encoding process known as AC-3.
Figure 3B shows the format used in DTS. Here we see only the stereo optical tracks and a
sync channel for maintaining control of the associated CD ROM player.
Figure 3C shows the format used with SDDS. In addition to the stereo optical tracks, there are
two digital tracks, one at each edge of the film.
Like Dolby SR-D, DTS and SDDS make use of perceptual encoding methods for reducing the
amount of digital data required for system operation. DTS and SDDS support the 5.1 channel format
used in most cinemas, but SDDS also supports as many as 5 screen channels for special
applications.
All digital formats discussed here have a fall-back (failsafe) mode in which the analog tracks
will be used in case of failure of the digital portion of the systems.
C. A- and B-chains
For convenience in defining responsibilities for system specification and alignment, the
playback chain is customarily broken down into the A-chain and the B-chain, as shown in Figure 4.
The A-chain is comprised of the preamplifiers (optical or magnetic), light source (optical), magnetic
heads, solar cells (optical), associated equalization (signal de-emphasis), and noise reduction and
directional decoding required for flat electrical output at the end of that chain. For digital reproduction,
a digital optical reader is used and the digital signal is fed to a digital-to-analog conversion system.
The analog A-chain is shown in Figure
4A,
and the digital A-chain is shown at B. The B-chain,
including split surround channels, is shown at C.
FILM
SIGNAL OUT
--$-I_
___)
‘I’
LAMP
SCREEN CHANNEL
I1
of31
SOLAR
I
h
i
CELL
Figure 4A.
--)
PREAMP
--)
Block diagram of analog A-chain
NOISE
REDUCTION
SIGNAL OUT
-
Figure 48. Block diagram of digital A-chain
MASTER
FADER
SURROUND CHANNEL
il Of
2)
SUB CHANNEL
,:,pg
A
1 3 OCTAVE
EO
_,,
Figure 4C. Block diagram of B-chain with split surrounds
The B-chain is comprised of one-third octave equalization, dividing networks (low- or high-level),
power amplification, and loudspeakers. JBL Professional products are used extensively used in the
chain of the system.
D. Evolving Dynamic Range Requirements in the Cinema
Figure 4D shows details of the headroom requirements of current and future cinema formats.
According to Dolby Laboratories, the level of dialog in the cinema will remain as it currently is, while
the added headroom will be used primarily for more realistic peak levels for sound effects and music.
Depending on specific signal content, the peak level capability of Dolby SR analog tracks can be 3
greater in the mid-band than with Dolby A, rising to about 9 dB at the frequency extremes. The digital
formats can provide 12 dB headroom relative to Dolby A, with overall characteristics that are flat over
the frequency band. This peak capability translates into acoustical levels, on a per-channel basis, of
103 dB-SPL in the house. All of the loudspeaker systems discussed in this manual will meet these
new specifications, consistent with the size of the cinema for which the systems will be specified.
dE
110
100
B-
dB
SO
80
-1
16K
tiz
Figure 40.
1K
2K
:r(
375
63
125
253500
Peak power levels
(Al
A-type.
(8) SF?. (CI SR.D
8K
Dynamic range requirements for Dolby-A, Dolby SR and Dolby SR-D formats
E. Integration of Loudspeakers into the Acoustical Environment
In order to present a clear picture of the interaction of loudspeakers and the acoustical
environment, we will begin with the previous era in cinema loudspeaker design. Through the end of
the
1970’s,
way designs composed of multicellular or radial high-frequency horns and hybrid horn/reflex
the loudspeaker systems which were current in the cinema were the tried and true
two-
low-
frequency systems. These systems had been developed by Bell Laboratories as far back as the
1930’s,
and the versions used until just a few years ago were essentially the same as has been
developed and refined by Lansing and Hilliard (1). These systems were well engineered in terms of
efficiency, ruggedness, and low distortion, given the acoustical performance demands of the day.
Their designers had also successfully coped with the problems of frequency division and arrival time
page
7
differences between high and low frequency sections. The chief weakness of these systems was their
lack of uniform coverage. System design stressed output conversion efficiency, because of the small
power amplifiers available at the time.
Figure 5A shows the on- and off-axis curves of a typical horn/reflex system, while polar
response of a typical multicellular horn is shown at B. Note that the off-axis response of the
low-
frequency system falls off considerably at higher frequencies. The typical reverberant room response
of a system composed of these elements is shown at C. Note here the double hump, which indicates
that the total power output of the system is far from uniform. At the same time, however, the on-axis
response of the system may be fairly flat, when measured under non-reflective conditions.
A. Off-axis response of ported horn system
C. Reverberant (power) response of a cinema system composed of
elements similar to those shown in Figures 5A and 58
-
-
I
I
c5
8.
Polar characteristics of a 2 x 5 multicellular horn
( -Ii:
'25
.Hi
+1c
+5
c
-5
I
-
-
I-
--
-
I
4
-
-
-
I
I
'5
3
I
3'5 63
I
Mulhcellular horn (2 x 5) 1000 Hz verticalMulticellular horn (2 x 5) 2000 Hz vertical
(soliu);
(so/id); horizontal (dashed)
Figure 5.
horizontal (dashed)
Theatre equalization of old-style cinema system
Multicellular horn (2 x 5) 10
(solid); horizontal (dashed)
If any attempt is made to equalize the response of this system in the cinema, then the response along
the major axis of the system will be anything but flat. This is precisely the problem which Dolby
Laboratories encountered when they introduced equalization into cinemas during the 1970’s.
Page 8
kHz
vertical
F. Power Response and Power-Flat Systems
The discrepancy between on-axis and reverberant room response in the older systems was
solved with the introduction of a new family of systems based on uniform coverage high-frequency
horns and simple ported low-frequency enclosures. Figure 6A shows the horizontal off-axis response
of the JBL 4648A low-frequency system. Note that the response is uniform below 500 Hz over a wide
angle. At 6B we show the vertical off-axis response of the 4648A system. Note that the response
begins to narrow just below 200 Hz. The net result of this pattern narrowing in the horizontal and
vertical planes is that they make a good match for the pattern control of the JBL 2360A horn at the
normal crossover frequency of 500 Hz.
Figure 6C shows the off-axis response curves for the 2360A Bi-Radial horn, coupled to a JBL
2446J high-frequency driver which has been equalized for flat power response. Note that the off-axis
curves are essentially parallel, indicating that the horn produces a solid radiation angle which is
uniform with respect to frequency. The need for equalization of the compression driver comes as a
result of the natural high frequency roll-off which occurs in high frequency drivers above about 3.5
kHz.
This frequency is known as the “mass break point” and is a function of diaphragm mass and
various electrical and magnetic constants in the design of the driver.
When the 4648A or 4638 low-frequency system and the 2360/2446 combination are integrated
into a full range system for cinema use, the -6 dB beamwidth above 500 Hz is smoothly maintained at
90” in the horizontal plane and 40” in the vertical plane out to 12.5
kHz.
At lower frequencies, the
system’s coverage broadens, eventually becoming omnidirectional in the range below 100 Hz.
A
I3
-
Figure 6.
1
(A) Horizontal response; (B) Vertical response; (C) Off-axis response of a JBL 236OA horn
equalized for
flar
power response
When the system described above is equalized in a typical cinema environment, both direct
sound and reverberant sound can be maintained quite smoothly, as shown in Figure 7A. The system’s
reverberant response is proportional to its power output, or to its power response, and the matching of
the system’s on-axis and power response indicate that the reflected sound field in the cinema will
have the same spectral characteristics as the direct sound from the loudspeaker. When this condition
exists, sound reproduction, especially dialog, will sound extremely natural. (The frequency response
contour shown in Figure 78 is the so-called “X-curve” recommended for cinema equalization, as
specified in
IS0
Document 2969.)
-
ON
*xis
---
POWER
RESPONSE
RESWNSE
UNEOUALIZED
Figure 7.
Cinema equalization of power flat systems
JBL pioneered the concept of flat power response in the cinema
EQUALIZED
(2,3).
It has become the
guiding principle in much of JBL’s product design, and it has been adopted by the industry at large.
G. Coverage Requirements for Proper Stereo Reproduction
In the cinema, it is expected that all patrons will be able to appreciate convincing stereo
reproduction. By contrast, standard two-channel stereo in the home environment often imposes strict
limitations on where the listener must sit in order to perceive correct stereo imaging. The factor that
makes the big difference in the cinema is the presence of the center channel. Not only does the
center loudspeaker lock dialog into the center of the screen, it further reduces the amount of common
mode information the left and right channels must carry, thus making it possible for listeners far from
the axis of symmetry to hear the three channels with no ambiguity or tendency for the signal to
“collapse” toward the nearer loudspeaker. In the Dolby stereo matrix, the same convincing effect is
largely maintained through gain coefficient manipulation during playback.
Ideally, each patron in the house should be within the nominal horizontal and vertical coverage
angles of
all
the high-frequency horns. This requirement can usually be met by using horns with a
nominal 90” horizontal dispersion and by toeing in the left and right screen loudspeakers. In very wide
houses, the spreading of high frequencies above approximately 5
kHz,
as they pass through the
screen at high off-axis angles, actually helps in providing the desired coverage.
Another desirable condition is maintaining levels as uniformly as possible throughout the
house. We have found that aiming the screen systems, both high- and low-frequency, toward the back
wall helps in this regard, by offsetting normal inverse square losses with the on-axis “gain” of the
screen systems. Measurements made at the Goldwyn Theater of the Academy of Motion Picture Arts
and Sciences in Beverly Hills, California, show that, over most of the frequency range, front-to-back
levels in the house are maintained within a range of 5
elements toward the audience would produce front-to-back level variations of up to 10 to 12
dB.
By contrast, aiming the high-frequency
dB.
An
important requirement here is that the back wall of the cinema be as absorptive as possible. If the rear
wall is not highly absorptive, then tilt the high frequency loudspeakers down, with the horn’s axis
pointing at the seating area two-thirds of the way back in the house.
This performance is seen in Figure 8. At A, we show in plan view the direct field coverage
given by a JBL 2360 horn aimed at the absorptive back wall of a large theater with sloped floor.
Coverage at 2
kHz
is within a range of
+/- 3dB,
front to back. If the horn is aimed downward to a point
two-thirds the distance from front to back, the coverage is as shown at B, and coverage at the rear of
the house is compromised. The coverage given by one of the outside horns, aimed at the rear wall, is
shown at C. It is customary to toe in the left and right systems toward the center, whether or not the
screen itself is curved, and the aim is to provide adequate coverage for all patrons, with response
maintained within a total range of 6
dB.
Figure 8.(A) Direct field coverage at
n
2kHz,
aimed at rear wall; (B) Same, horn aimed 2/3 distance front to back;
(C) Coverage of single outside horn.
-
page
11
The surround ensemble of loudspeakers, if properly specified, can easily produce a sound
field that is uniform throughout the back two-thirds of the house, and level variations can often be held
within a range of 2 to 3
dB.
Details of surround system specification will be covered in a later section.
L
When all of the above points are properly addressed, the sound in a cinema can approach that
which we take for granted in a post-production screening facility
director intended it to sound. It is only when such details as these have been carefully worked out that
the effects intended by the sound mixer can be appreciated by the viewing audience.
-
which is, after all, how the picture
.-.
III. ACOUSTlCAL
CONSIDERATIONS
A. Noise Criterion (NC) Requirements
The usual sources of noise in a cinema, outside of the patrons themselves, are air handling
and transmission of noise from the outside. In the case of multiplex installations, there can be leakage
from adjacent cinemas as well. Not much can be done about a noisy audience, but it is true that at the
post-production.stage,
encountered in the
mixing engineers take into account certain masking noise levels which may be
field
and even do the final mix under simulated noisy conditions (4).
63
125
2%
94
FREOUEW
Figure 9. Noise Criterion (NC)
octave
band
IK
(Hz)
data
2ll
wrves,
.(*
xa
FREOUENCV
1K
(Hz)
4K
Figure 10. Sound Transmission Curves
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