ISS Alignment Notes ............................................................... 38
Figures
Figure 1
ISS Connection Diagram ......................................................... 44
Figure 2
ISS Ribbon Cable Bus............................................................. 45
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Issue 3, June 1990ISS User Guide
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Introduction
Your ISS was inspected and carefully
checked at the factory. We suggest, however, that you inspect the shipping cartons
and all contents for any damage.
If you do find damage, save the cartons and
all packing material and notify the shipper.
You are responsible for any shipping claims
that must be made.
The shipping carton will contain your ISS
mainframe, ISS circuit cards, ISS front
panel, ISS instruction manual, mainframe
instruction manual, warranty cards, and a
power cord. If any of these materials are
missing, contact your dealer or Studio
Technologies, Inc. immediately.
General Description
The Studio Technologies ISS Integrated
Simulator System is designed for use in
conjunction with MTS television broadcast
operations. The television broadcaster is
faced with the reality of having to broadcast
a combination of stereo and mono audio
material. Stereo simulators can greatly
improve the listeners appreciation of stereo TV. The ISS combines excellent stereo
simulation with advanced control circuitry
to provide superior audio and operational
performance.
Major Functions
The ISS provides several major functions:
Stereo Simulation: The ISS produces great
sounding simulated stereo. To create this
sound the ISS contains two stereo simulator circuit cards. These cards work together
to transform a mono signal into left and
right channel signals that give an excellent
stereo feel, while keeping the voice signals in the center. The ISS Type I simulator
card provides simulation over the entire
audio spectrum. The Type II simulator card
adds a specialized filter to give greater
simulation to all frequencies except those in
the voice band. The Type II card ensures
that excellent voice centering is maintained.
The simulated stereo is completely mono
compatible. The sound of the ISS is factory
optimized for the best overall performance.
Input/Output Circuitry: The input/output
circuitry of the ISS provides switch selectable 0, +4, or +8dBu operation to match
the requirements of most broadcast facilities. Careful circuit design provides excellent audio performance. The Transfer Relay
Assembly connects the audio input signals
directly to the audio output connectors in
the event of a system malfunction, power
failure, or operator request, thus ensuring
no interruption of broadcast audio.
Audio Control: A smooth electronic
crossfade circuit routes either the line inputs, or the outputs of the stereo simulator
cards to the ISS line outputs. Three crossfade speeds are used to ensure the appropriate action. The ISS has been designed
to provide the best simulated stereo sound
with the least obtrusive operation.
Remote Control Operation: Extensive features allow the operating status of the ISS
to be displayed and controlled remotely.
Relay contacts provide system status indication. These are also known as tally signals. Continuous or pulse logic level inputs
give the user complete control over the ISS
operating status.
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ISS
Mono/Stereo Recognition: The Recognition
Card determines the mono/stereo status
of the incoming left and right audio signals.
The Recognition Card contains circuitry
to determine if the incoming audio is two
channel mono, mono with signal on the left
channel only, or mono with signal on the
right channel only. Each condition can be
defeated by a switch. The circuitry has been
designed to minimize the chance of incorrect recognition, i.e., seeing a true stereo
input as mono, or vice versa.
Polarity Correction: ISS circuitry can monitor and correct 180 degree polarity reversals. The Polarity Correction Card ensures
that mono compatibility is maintained.
Design Criteria
We are pleased that you already have, or
will soon be purchasing an ISS. A great
deal of care and effort was put into developing this product. Our first design requirement was that the simulated stereo produced must sound very good. We, by all
means, love real stereo recordings, but
these, especially for TV broadcasters, are in
limited supply. The ISS provides the stereo
listener with a high quality, enhanced version of the mono source.
The second design criteria was to provide
the broadcaster with a set of features that
would allow complete interfacing into their
broadcast facility. We required that the
completed ISS have the operational characteristics to integrate easily with existing
facilities. We hope you share our enthusiasm about the ISS. Questions and comments can be directed to Gordon Kapes,
president of Studio Technologies. Your
praise or verbal thrashing is welcome!
Jim Cunningham designed the audio sections in the ISS. He is responsible for the
very effective stereo simulation method
used. Mitch Budniak designed most of the
logic circuitry and made suggestions that
added considerably to the overall reliability
of the ISS. The printed circuit cards were
designed by Fred Levine. Gordon Kapes
designed the overall architecture and coordinated the project.
Installation
Overview
In this section you will be:
Taking an ISS inventory
Mounting and powering the ISS
Mainframe
Connecting the audio signals
Connecting the remote control input
signals
Connecting to the status relay outputs
Configuring the circuit cards
Getting Ready
Carefully remove the ISS Mainframe from
the shipping carton. For protection, the
circuit cards are shipped installed in the
mainframe. Use your fingers to take out the
four front panel fasteners, allowing the front
panel to be removed. You can now take an
inventory:
An extender card can be purchased as an
option and may be part of your system. It
consists of 4 pieces: two ribbon cables and
two interface boards.
In some cases you may have purchased a
Tone Detection Card. It is an option and in
most cases will not be present.
Mounting
The ISS is rack-mountable, requiring three
standard rack spaces (5.25") in a standard
EIA 19.00" rack. Ensure that air flow is
maintained, especially on the right side
(when looking from the front) where the ISS
power supply section is located. A good
basic rule to remember is that most electronic equipment failures are power supply
related. Power supplies tend to generate
heat which, when not adequately dissipated, serve to cook the power supply,
drying out electrolytic capacitors and
stressing semiconductor junctions. Keeping
all equipment relatively cool will reduce the
likelihood of problems occurring.
Connecting the Unit to Power
The ISS may be operated from either nominal 115 or 230Vac, 50/60 Hz. Units selected
for 115V operation utilize a 0.75A 3AG
Slow-Blow fuse; 230V operation utilizes a
0.375A Slow-Blow fuse. Before connecting
the ISS to power, determine the actual line
voltage and check to see that the voltage
selector switch, visible through the square
cutout in the Transfer Relay Assembly, is
set to the appropriate voltage. If the voltage
selector switch is set for 230V, ensure that
the fuse, located adjacent to the voltage
selector switch, is 0.375A. PLEASE NOTE
THAT AN INCORRECT SETTING AND/OR
INCORRECT FUSE COULD SERIOUSLY
DAMAGE THE UNIT.
The ISS utilizes an IEC standard connector
to mate with the line cord. The line cord
supplied has a North American standard
plug at one end and an IEC connector at
the other. In non-North American applications, the plug must be cut off and an appropriate plug attached. The wire colors in
the line cord conform to the internationally
recognized CEE color code and should be
wired accordingly:
ConnectionWire Color
Neutral (N)Light Blue
Live (L)Brown
Protective Earth (E)Green/Yellow
Signal Connections
All signal connections to and from the ISS
are made via connectors located on the
back panel. Four, three pin XL-type connectors handle audio input and output signals;
female for input, male for output. One
25-pin male D-type subminiature connector
handles all remote control and status signals. Refer to Figure 1, located at the end
of this manual, for detailed connection
information.
Audio Signals
Left and right audio input and output connections must be made. For hum, noise,
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 7
ISS
and RF pickup rejection, shielded cable
must be used for the audio signals. Studio
Technologies uses the convention of pin 2
high, in honor of the European microphone
makers! In most cases, it is correct to
connect the shield lead to pin 1 of the XL
connectors. Pin 1 on the audio input and
output connectors are common with the ISS
Mainframe power supply ground, chassis
ground, and power cord ground leads.
Maintaining consistent left and right audio
input and output polarity is very important
for correct performance of the ISS.
If possible, use patch points on the input
and output signals of the ISS. Installation,
testing, and servicing procedures will be
greatly improved if the ISS is easily placed
on and off line. Make sure that the ISS can
be patched around while allowing test
signals to be sent to and returned from
the ISS.
The ISS audio input signals generally arrive
from the master control switcher, an STL,
leased telephone lines, etc. All audio processing (limiting, compressing, etc.) should
be performed prior to the audio getting to
the ISS. This helps to ensure that the ISS
simulated stereo remains mono compatible.
The source should be balanced and line
level. If the audio equipment contains audio
output transformers, load resistors matching the source impedance may need to be
inserted and soldered into the I/O card. In
many cases the value of the resistors would
be 600 ohms. Loading of the output transformers can prevent ringing of the audio
signals. The quality of the output transformers is the determining factor when deciding
whether to load or not to load. Bad transformers tend to need loading; good ones
generally do not. Refer to the Technical
Notes section of this manual for more
information on installing load resistors.
The ISS audio output signals usually go
directly to the transmitter, or to the transmitter via an STL or leased lines. The ISS
audio outputs are low impedance, electronically balanced, line level, direct coupled.
They are capable of driving virtually all line
inputs (low or high impedance, transformer
or transformerless). The ISS can even drive
150 ohm loads at high signal levels, not
bad huh!
The ISS uses electronically balanced input
and output circuitry. Best performance is
achieved if the equipment sending signal
to, and receiving signal from the ISS is
operating in a balanced mode. The ISS
input and output stages will operate correctly in an unbalanced mode, but selected
performance characteristics will be sacrificed. On the input side you will lose the
ability to reject common-mode signals that
balanced operation affords. On the output
side you will lose 6dB maximum output
level. This is not a technical fault but is
inherent in electronically balanced output
stages. If unbalanced input operation is
required, strap pin 3 to pin 1 on the male
connector that will mate with the ISS. Connect the unbalanced input signal high lead
to pin 2, and signal ground to pin 1. If
unbalanced output operation is required,
strap pin 3 to pin 1 on the female connector
that will mate with the ISS. Connect the
unbalanced output signal high lead to pin 2,
and signal ground to pin 1.
In most cases, transformer coupling between audio equipment is neither required,
nor desirable. If the equipment sending
signal to, or receiving signal from the
ISS requires the isolation given by a
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Page 8Studio Technologies, Inc.
ISS
transformer, but does not contain internal
transformers, external transformers can
be added. Refer to the Technical Notes
section of this manual for recommended
transformers.
Connecting the Remote Control Signals
Provision has been made for remotely
controlling a number of ISS functions.
These signals interface with the ISS via a
25-pin male D-type connector located on
the back panel. In most cases, the ISS will
be located some distance from the TV
master control point. It may be desirable to
control the ISSs operation using a telemetry system or switches connected via cable
pairs. The following is a description of the
remote control inputs:
Remote Control Enable: Activating this
allows use of the Remote Simulate from
Left and Remote Simulate from Right commands. Activating the Remote Control
Enable will override the commands from the
Recognition Card.
Remote Polarity Correction Function
Disable: Activating this command disables
the polarity correction function.
Low voltage, current limited logic type
signals are required for remote control
operation. Continuous or pulse (momentary) signals can be used. These logic
signals are usually nominally 5 or 12Vdc.
LED based optical couplers, located on the
ISS circuit cards, are utilized to eliminate
interfacing problems. The couplers require
current, rather than voltage or a contact
closure, to operate. The minimum current
required is 4mA; the maximum is 20mA. For
protection, 680 ohm resistors, located on
the ISS circuit boards, are in series with the
optical couplers. These resistors limit a
5Vdc signal to 4.5mA, and limit a 12Vdc
signal to 13mA. If higher DC voltages are
used, additional current limiting resistors,
connected in series with the remote control
inputs, are required. Failure to provide
current limiting will damage and/or shorten
the life of the opto couplers.
Remote Simulate from Left: This command
is only active when Remote Control Enable
is in effect. Remote Simulate from Left
allows you to place the ISS in the simulate
from the left channel mode.
Remote Simulate from Right: This command
is only active when Remote Control Enable
is in effect. Remote Simulate from Right
allows you to place the ISS in the simulate
from the right channel mode.
Remote I/O Bypass: Activating this command forces the relays on the Transfer
Relay Assembly to release, connecting the
audio input signals directly to the audio
output connectors. This electrically takes
the ISS out of the audio path.
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Studio Technologies, Inc.Page 9
Connecting to the Status Relay Outputs
Relay contacts indicating several ISS operating characteristics are provided for userdesignated functions. These contacts are
accessible via the 25-pin male D-type connector located on the back panel. These
can be extremely useful for local or remote
monitoring. An automation system can
watch for an error condition, or a master
control operator can monitor ISS operation
through a set of indicator lights. Dry (isolated) relay contacts are provided so that
virtually any monitoring scheme can be
implemented without interfering with ISS
operation due to ground loops, noise
pickup, etc. The following gives a description of the Status Relay Outputs.
ISS
ISS Remote Control Enabled: This contact
closes (shorts) when a Remote Control
Enable condition is in effect. This contact
gives acknowledgment of a valid Remote
Control Enable condition.
ISS Simulating from Left: This contact
closes (shorts) when the ISS is in the simulating from the left channel mode. This
contact closes any time the ISS is simulating from the left channel, whether due to
a Remote Simulate from Left command,
a command from the front panel controls,
or a command from the Recognition Card.
ISS Simulating from Right: This contact
closes (shorts) when the ISS is in the simulating from the right channel mode. This
contact closes any time the ISS is simulating from the right channel, whether due to
a Remote Simulate from Right command,
a command from the front panel controls,
or a command from the Recognition Card.
Polarity Correction Taking Place: This contact closes (shorts) when polarity correction
is taking place. You may want to let this
contact control an audible alerting device
in master control, a tape room, etc. The
audio source may need to be corrected,
or at least marked to show that a polarity
reversal is present.
Polarity Correction Function Disabled: This
contact closes (shorts) when a Remote
Polarity Correction Function Disable condition is in effect. This contact acknowledges
a valid Polarity Correction Function Disable
command.
Configuring and Installing the Circuit
Cards
Once the connections have been made, the
cards are ready to be configured. Do not
remove or insert any of the cards with the
mainframe power on. Do not hot install or
remove the cards! We will be working with
the cards in the order in which they are
housed in the cabinet: left to right, when
viewed from the front.
Mainframe card position 1 is on the left side
(viewed from the front); card position 9 is
on the right side.
The ISS mainframe is shipped with the
cards installed and the ribbon cable bus
attached. If you havent done so already,
carefully remove the ribbon cable bus from
all the cards. The connector on the front of
each card has latches that must be opened
for the ribbon cable bus connector to be
removed. Dont fear the ribbon cable bus!
It is fast, reliable, and easy to work with.
Once you are used to it, youll like it!
I/O Card: The ISS is designed to accept
nominal audio signal levels of 0, +4, or
+8dBu. The desired input and output levels
must be set using the two switches located
on the I/O Card. Remove the I/O Card from
mainframe position 1 (the far left position
when facing the front of the mainframe).
The INPUT LEVEL switch selects the nominal line input level for both channels. The
OUTPUT LEVEL switch sets the nominal
output level. Set these switches to match
your broadcast facilitys desired nominal
operating level. The A position corresponds
to 0dBu operation, the B position to +4dBu,
and the C position to +8dBu. The nominal
input and output levels do not have to be
the same. If input loading is required, refer
to the Technical Notes section of this
manual. After setting the switches, and
possibly installing load resistors, install the
card back into mainframe position 1. Remember, do not install this or any card
when the mainframe power is on.
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Type I Simulator Card: Remove the Type I
Simulator Card from mainframe position 2.
In addition to the identification label, this
card can be identified by the empty parts
locations on the circuit board. You will
observe a section in the middle of the board
where parts have not been inserted. There
are no switches to be set, or initial adjustments to be made on the Type I Simulator
Card. Confirm that single turn trim potentiometer R43 is set to the 50% rotation point,
i.e., halfway between fully clockwise and
fully counterclockwise. R43 is small and
basically round, and is located near the
front edge of the card. This pot was preset
at the factory but a visual check is a good
idea. DO NOT TOUCH ANY OTHER POTENTIOMETER ON THIS CARD OR FACTORY CALIBRATION MAY BE REQUIRED.
This card is now installed in mainframe card
position 2.
Polarity Correction Card: Remove the Polarity Correction Card from mainframe position
3. One switch must be set on the Polarity
Correction Card. This switch determines the
type of remote control signal that is going to
be used for the Remote Polarity Correction
Function Disable command. In the CONT
position a continuous signal will be applied.
In the PULSE position a momentary signal
will be applied. If you are not going to be
connecting a remote control signal the
switch should be in the CONT position. This
card is now installed in card position 3.
Type II Simulator Card: Remove the Type II
Simulator Card from mainframe position 4.
In addition to the identification label, this
card can be identified by the fact that,
unlike the Type I card, most of the components in the Type II printed circuit board
have been inserted. There are no switches
to be set, or initial adjustments to be made
on the Type II Simulator Card. Confirm that
single turn trim potentiometer R43 is set to
the 50% rotation point, i.e., halfway between
fully clockwise and fully counterclockwise.
This pot is in the same location, and is
labeled R43 on both the Type I and Type II
cards. This pot was preset at the factory
and should only require a visual confirmation of the correct setting. This card is now
installed in card position 4.
Crossfade Card: Remove the Crossfade
Card from mainframe card position 5. One
switch, INPUT, must be set on the Crossfade Card. This switch selects which audio
signal is connected to the card from the
ribbon cable bus. If, as is usual, the Polarity
Correction Card is installed, set the switch
to the B position. If, for reasons such as
repair, etc., the Polarity Correction Card is
not installed, set the switch to the A position. If a Tone Detection Card is present in
your system the INPUT switch is set to the
C position. This card is installed in card
position 5.
Recognition Card: Remove the Recognition
Card from mainframe card position 6. There
are two switches that must be set on the
Recognition Card. The INPUT switch selects which audio signal is connected to the
card from the ribbon cable bus. If, as is
usual, the Polarity Correction Card is installed, set the switch to the B position. If,
for reasons such as repair, etc., the Polarity
Correction Card is not installed, set the
switch to the A position. If a Tone Detection
Card is present in your system the INPUT
switch is set to the C position. The other
switch is a four position DIP type. This
switch decides which recognition modes
will be active. One, two, or all three modes
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ISS
can be turned on at the same time. Switch
position 1 controls if L=R is recognized as
mono. Place switch position 1 to ON if you
want a mono signal on both left and right to
be recognized as mono. Switch position 2
controls if a signal on the left channel only
will be recognized as mono. Place switch
position 2 to ON if left only is to be recognized as mono. Switch position 3 controls
if a signal on the right channel only will be
recognized as mono. Place switch position
3 to ON if right only is to be recognized as
mono. Remember that all three modes can
be, and in most cases will be, turned on at
once. Switch position 4 is not used and
should be left in the OFF position. Confirm
that the single turn trim potentiometer R10
is set to the 50% rotation point, i.e., halfway
between fully clockwise and fully counterclockwise. It is the only trim pot on the
Recognition Card. The pot was preset at
the factory, but a visual double check is
a good idea. This card is now installed in
card position 6.
Mode Select Card: Remove the Mode
Select Card from mainframe card position
7. One switch must be set on the Mode
Select Card. This switch determines the
type of remote control signals that are
going to be applied to the four remote
control inputs: Remote Control Enable,
Remote Simulate from Left, Remote Simulate from Right, and Remote I/O Bypass. In
the CONT position, continuous signals will
be applied. In the PULSE position, momentary signals will be applied. If remote control
signals are not going to be connected, the
switch should be set to the CONT position.
This card is now installed in card position 7.
Card Position 8: Card position 8 is reserved
for an option, the Tone Detection Card. This
card places the ISS in the electronic bypass
mode if a continuous, specific frequency
is detected. If your installation includes
this card, refer to the separately supplied
documentation for complete installation
instructions.
Card Position 9: Card position 9 is not
utilized at this time.
The Ribbon Cable Bus
Once the cards are configured and reinstalled, the ribbon cable bus can be installed, linking all the cards together. Start
with the I/O card, located in card position 1,
and work to the right. Orient the ribbon
cable bus so that the colored stripe, usually
red or blue, that indicates pin 1 will mate
with the top pins of the card connectors.
Mate the left most ribbon cable bus connector with the I/O Card connector. A mechanical key on the I/O Card prevents the ribbon
cable bus from being installed upside
down. Repeat this process for the remainder of the cards. Use the latches to secure
the ribbon cable bus connectors to the card
connectors.
For future reference note that the ribbon
cable bus can be removed or attached with
the mainframe power on or off. The ribbon
cable bus carries only audio and logic
signals. No damage will occur if one or
more of the cards are operated with their
respective ribbon cable bus connectors
disconnected. Remember that the cards
themselves cannot be hot plugged into,
or pulled out of, the mainframe.
Securing the Front Panel
Carefully place the front panel over the front
of the mainframe and secure using the four
screws.
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ISS
Using the ISS
In this section we will first review the controls and indicator lights on the ISS front
panel. Next we will run some basic tests on
the system and give you a feel for its operation.
I/O Card
One LED and one switch relate to the I/O
Card and its functions. When lit, the green
NORMAL LED indicates that the relays on
the Transfer Relay Assembly, located on the
back panel, are energized and that the
audio input and output signals are connected to the ISS circuitry. When the NORMAL LED is off, the relays on the Transfer
Relay Assembly de-energize, directly connecting the left line input to the left line
output, and the right line input to the right
line output. The NORMAL LED will not light
if a valid remote I/O Bypass command is
received, if the I/O switch is in the I/O
BYPASS position, or if a power supply
error is detected. A red LED on the Transfer
Relay Assembly mimics the operation of the
I/O cards LED. This LED is visible through
an access hole in the back panel.
When the I/O switch is in the I/O BYPASS
(down) position, the Transfer Relay Assembly is held in the I/O Bypass mode, removing the ISS from the audio path. In the
NORMAL (middle) position, the ISS will be
in the audio path but will ignore a remote
command to go into the I/O Bypass mode.
In the NORMAL + REMOTE (up) position,
a remote command to initiate I/O Bypass
will be executed.
Polarity Correction
Two LEDs and one switch relate to the
Polarity Correction Card and its functions.
When the red CORRECTING LED is lit, it
indicates that a polarity reversal has been
detected and is being corrected.
When the yellow REMOTE DISABLED LED
is lit, it indicates that the polarity correction
function is disabled via the remote control
input.
When the switch is in the DISABLE (down)
position, the polarity correction function has
been turned off. This is useful when testing
the ISS or related equipment. In the OPERATE (middle) position, the polarity correction function is active but the card will
ignore a remote control command to go
into the disable mode. In the OPERATE +
REMOTE (up) position, a remote command
to disable the polarity correction function
will be executed.
System Status
Three LEDs indicate the bypass/simulate
status of the ISS. When the green BYPASS
LED is lit, it indicates that the electronic
crossfade circuitry is routing the input audio
to the audio outputs; the stereo simulators
are not in the audio path. When the red SIM
LEFT LED is lit, it indicates that the left
audio input is being sent to the simulators
and the resulting simulated stereo signal is
being sent to the audio outputs. When the
red SIM RIGHT LED is lit, it indicates that
the right audio input is being sent to the
simulators and the resulting simulated
stereo signal is being sent to the audio
outputs.
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 13
ISS
Mode Select
One LED and two switches relate to the
Mode Select Card and its functions. When
lit, the yellow REMOTE LED indicates that
the ISS bypass/simulate status is being
controlled via remote control, indicating that
the remote manual mode is in effect.
The top switch, SYSTEM MODE, sets the
overall ISS operating mode. In the MANUAL
(down) position, the bypass/simulate status
is controlled by the lower switch. In the
AUTO (middle) position, the Recognition
Card will control the bypass/simulate status,
but a remote control override request is
ignored. In the AUTO + REMOTE (up)
position, the remote control override can
be used.
The lower switch, MANUAL, is active
when the SYSTEM MODE switch is in the
MANUAL (down) position. The MANUAL
switch selects bypass, and simulate from
the left input or simulate from the right input
operation.
A method of monitoring the ISS audio
outputs is also required, such as a set of
high quality audio speakers with an associated power amplifier. Set up the speakers
so that a good stereo image can be heard;
i.e., dont put them too far apartset them
up in a normal listening position. Set the
audio amplifier level controls to the OFF
position. Headphones are also a good
method of monitoring.
1)Check to ensure that audio is indeed
feeding the ISS.
2)Set the following ISS switches: I/O
switch to BYPASS, POLARITY CORRECTION switch to DISABLE, SYSTEM
MODE switch to MANUAL, and
MANUAL switch to BYPASS.
3)Push the ISS power switch to the ON
(in) position. The red LED located just
above the power switch should light.
Of the other LEDs, only the green
BYPASS LED on the Crossfade card
should be lit.
Initial Operation
The installation is over and youre somewhat familiar with the controls; now the fun
can begin as you see what the ISS can do.
You must first connect a source of audio to
the ISS inputs via your patch bay. A good
signal source would be left and right audio
from master control via an audio router; a
better signal would be a great sounding
compact disc run through a line amp to
come up to your required audio level! Do
not use sine waves, or other obscure nonprogram type signals in these tests. The
ISS was designed to work with actual program material!
Issue 3, June 1990ISS User Guide
Page 14Studio Technologies, Inc.
4)Raise the level of the audio amplifier
until your left and right test signals are
comfortably heard. You are listening to
the input signals connected directly to
the audio outputs via the Transfer Relay
Assembly.
5)It is a good idea to ensure that at the
start of our tests, audio input and output polarity has been correctly connected. To test this, feed the same
signal into the left and right inputs.
Sum the left and right audio outputs
and listen to the resulting mono signal.
You should not have any cancellation,
as this would indicate a 180 degree
reversal on an audio input or output.
ISS
The easiest way to listen to L+R is to
use an audio amplifier with a mono
button on it. Of course, you can always
use a scope to determine if the polarity
of the wiring or associated patch bay is
correct. Get this test over with now and
you wont have to worry about it later!
Be warned that a polarity reversal on
the same channels input and output
will not show up with this test. A
double flip could later lead to incorrect Polarity Correction Card or Recognition Card performance. After you have
confirmed the connection polarity you
should resume monitoring in stereo.
6)Place the I/O switch to the NORMAL
position. The green NORMAL LED on
the I/O Card should light; the red LED
on the Transfer Panel Assembly should
also light. You should hear audio at the
same level as heard in the previous
step. You are hearing audio through
the ISS circuitry! If the level does not
match, the most likely cause is an
incorrect INPUT LEVEL or OUTPUT
LEVEL switch setting on the I/O Card.
Recheck your switch settings.
7)Move the MANUAL switch to the SIM
LEFT position. The BYPASS LED will
fade out while the SIM LEFT LED will
light up. The audio you hear is stereo
simulated from the left input channel.
Listen to the left and right output signals
in mono. The simulated stereo effect
should drop out and you should hear a
faithful rendition of the left input signal.
If listening to the sum (L + R) of the ISS
outputs degrades the level and/or
quality of the audio you most likely have
a double flip, as was discussed in
step 5. This mono compatibility problem must be corrected NOW! Once you
confirm mono compatibility, move the
MANUAL switch back to the BYPASS
position. The output will fade from
simulated stereo back to the input
signals. Try simulating from the right
audio input by moving the MANUAL
switch to the SIM RIGHT position. Then
return the MANUAL switch to BYPASS.
8)Place the SYSTEM MODE switch to the
AUTO position. This lets the ISS mode
be controlled by the Recognition Card.
Remember, during system setup you
chose which of the three recognition
modes you wanted active. Most people
will have enabled all three modes, so
mono will be recognized as L=R, left
only, and right only.
Feed a stereo signal into audio inputs.
Remember, do not use sine waves as
your signal source. The BYPASS LED
should be lit.
Feed a mono signal into both the left
and right audio input. If you enabled
L=R is mono, the SIM LEFT LED will
light showing the ISS is simulating
stereo from the left input. If you did not
enable L=R is mono, then the ISS will
stay in the Bypass mode.
Feed a signal only into the left audio
input. If you enabled left only is mono,
the SIM LEFT LED will light showing the
ISS is simulating stereo from the left
input. If you did not enable left only is
mono, then the ISS will stay in the
Bypass mode.
Feed a signal only into the right audio
input. If you enabled right only is mono,
the SIM RIGHT LED will light showing
the ISS is simulating stereo from the
right input. If you did not enable right
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 15
ISS
only is mono, then the ISS will stay in
the Bypass mode.
9)Place the POLARITY CORRECTION
switch to the OPERATE position. The
CORRECTING LED should not be lit.
Feed signals into the left and right
audio inputs with the signals 180 degrees out of phase with each other.
This could be a mono or stereo signal
into both channels, 180 degrees out of
phase. The CORRECTING LED should
light when this condition is detected,
and will hold in the correcting mode
until signals with correct polarity are
presented on the inputs. The closer the
signals are to 180 degrees out of phase
with each other, the quicker the correction will take place. Mono signals 180
degrees out of phase and fed into the
left and right audio inputs will correct
very quickly. Audio material with lots of
stereo content, but 180 degrees out of
phase, will take longer to correct. Great
stereo signals are in a sense out of
phase between left and right; there is
lots of phase incoherence. The circuitry
has to cut through the valid phase
differences and find the error! To ensure that the input select switches are
correctly set on the Crossfade and
Recognition Cards, listen in mono to
the sum of the left and right outputs.
Feeding out of phase input signals,
listen to the output corrected and uncorrected. Uncorrected, you should
hear significant cancellation. Corrected,
you should hear the sum of left and
right in full fidelity.
10) If you have connected remote control
input signals, now is a good time to try
them out. Place the I/O switch to the
NORMAL + REMOTE position, making
the circuit accept a remote control
signal. Apply the Remote I/O Bypass
signal, either a continuous or momentary signal depending on your previously selected configuration. The I/O
NORMAL LED should go out and the
audio input signals will connect to the
audio output connectors. Either stop
the continuous signal, or again apply
the momentary signal. The NORMAL
LED should light again.
On the Polarity Correction Card, place
its switch in the OPERATE + REMOTE
position. Apply the Remote Polarity
Correction Function Disable signal,
either a continuous or momentary
signal depending on your previously
selected configuration. The REMOTE
DISABLE LED should light. Either stop
the continuous signal, or again apply
the momentary signal. The REMOTE
DISABLE LED should stop lighting.
Place the SYSTEM MODE switch to
AUTO + REMOTE, making the circuit
accept remote control signals. Apply
the Remote Control Enable signal,
either a continuous or momentary
signal depending on your previously
selected configuration. The REMOTE
LED should light. Apply a continuous or
momentary Remote Simulate from Left
signal. The system should immediately
go into the simulate from left channel
mode. Removing the continuous signal,
or again applying a momentary signal,
returns you to the Bypass mode. Try
applying the Remote Simulate from
Right command, then return to the
Bypass mode. Either stop the continuous signal, or again apply the momentary signal on the Remote Control
Enable input. The REMOTE LED should
Issue 3, June 1990ISS User Guide
Page 16Studio Technologies, Inc.
ISS
go out, making the Remote Simulate
from Left and Remote Simulate from
Right inputs inactive.
11) If you have connected the Status Relay
Outputs, you can test them now. Any
time the I/O NORMAL LED is not lit, the
ISS I/O Bypass Enabled relay contact
will close (short). The device connected
to this contact should indicate this
condition.
Any time the CORRECTING LED on the
Polarity Correction Card is lit, the Polarity Correction Taking Place relay contact will close (short). The device
connected to this contact should indicate this condition.
Any time the REMOTE DISABLE LED
on the Polarity Correction Card is lit,
the Polarity Correction Function Disabled relay contact will close (short).
The device connected to this contact
should indicate this condition.
Normal Operation
You should now feel confident that the ISS
has been carefully installed and tested, and
is ready to go to work in the exciting TV
business. (You remember excitement...
thats 3am Monday morning working on the
transmitter!) Seriously, if you have any
questions concerning the ISS, now is a
good time to give us at Studio Technologies a call. Otherwise, set the front panel
controls to your desired operating mode
and thats it. If one or more remote control
signals have been connected, be sure to
set the appropriate switches to allow remote operation. Youll most likely want the
SYSTEM MODE switch in either the AUTO
or the AUTO + REMOTE position.
Technical Notes
Definition of Level
Any time the SIM LEFT LED on the
SYSTEM STATUS section is lit, the ISS
Simulating from Left relay contact will
close (short). The device connected
to this contact should indicate this
condition.
Any time the SIM RIGHT LED on the
SYSTEM STATUS section is lit, the ISS
Simulating from Right relay contact will
close (short). The device connected
to this contact should indicate this
condition.
Any time the REMOTE LED on the
SYSTEM MODE section is lit, the ISS
Remote Control Enabled relay contact
will close (short). The device connected
to this contact should indicate this
condition.
Studio Technologies has opted to use the
dBu designation as it seems to be quite
rational. Using dBm was fine when all audio
line outputs were terminated with 600 ohm
loads. In this way, it is easy to say that
0dBm is 1 milliwatt dissipated in the known
load (i.e., 0dBm across 600 ohms will
measure 0.7746V). In contemporary situations, an audio output line is rarely terminated in 600 ohms; generally 5k ohms or
higher. The dBu designated is a better
reference because it refers to dB referenced
to 0.7746V, with no reference to load impedance. This takes into account todays
audio scene with load impedances varying
greatly. When the ISS specifications refer
to the maximum output level in dBu, this
would translate to dBm only when the
output is terminated with 600 ohms.
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 17
ISS
Transformer Coupling
As discussed in the Installation section of
this manual, there may be cases where
transformer isolation of the ISS audio input
and/or output signals may be required. As
the ISS has excellent electronically balanced
input and output circuitry, interfacing with
most other equipment should not require
transformer isolation except in the strangest
of cases. If you do find a case where you
need them, we suggest using transformers
from Jensen Transformers Inc., website:
www.jensentransformers.com. They make
excellent parts and we recommend their
JE-11-DMCF, a 600 to 600 ohm output type
transformer. This should give very good
results on both the input and output sides
of the ISS. If you want to splurge and go
for the premium transformer, you could
use their JE-11-BMCF; overkill but terrific
specs! Because of Jensens high quality,
load resistors do not have to be used.
Resistor Loading
Some broadcast operations as standard
practice load the outputs of audio equipment. This is not really necessary with the
design of contemporary audio equipment.
Current practice call for low source impedances and high input impedances; the ISS
follows this practice. Provision has been
made on the I/O Card for load resistors to
be added if required; resistor location R88
for the left input, R64 for the right input.
Carefully insert and solder your selected
resistors. Use diagonal cutters to clip the
excess resistor lead. Do not install load
resistors on the input connectorsonly
install them on the I/O Card. This ensures
that double loading will not occur in cases
where the Transfer Relay Assembly connects
the inputs directly to the outputs.
Output Load vs. Output Level
The I/O Card is user selectable for three
nominal operating levels. The input operating levels are measured in dBu and do not
have to take into account whether the inputs
are terminated (loaded) or not. The outputs
are a different matter. The output stage,
although excellent, is not completely stiff,
and will allow the nominal output level to
change slightly with different output load
impedances. The 0, +4, and +8dBu output
levels are stated under the assumption that
a 600 ohm termination will be present. The
nominal output level will change up to
0.5dB with a lower or higher load impedance, e.g. 150 or 20k ohms. This is to be
expected and should pose no operational
problem. Only a perfect line output stage
(if it can be found) will maintain an exactly
constant output level with a widely varying
load. This variance with load is constant
with frequency and does not effect frequency response linearity.
Signal Paths
All signals from the outside world come in
and go out via connectors on the Transfer
Relay Assembly. The Transfer Relay Assembly links with the mainframe via screw
terminal strips on the mainframe back
panel. The mainframe links with the cards
via 15-position card edge connectors.
Power (+15 and +24Vdc), signal ground,
and earth ground also come into each card
via the edge connectors. All inter-card
connections are made via a 20-conductor
ribbon cable bus. The ribbon cable bus
serves as the audio and logic signal highway between the cards. Cross talk is not a
problem as the signal level, type, and
physical positions were carefully chosen.
Issue 3, June 1990ISS User Guide
Page 18Studio Technologies, Inc.
ISS
The ISS utilizes an internal operating level
of 6dBu. This keeps adjacent positions in
the ribbon cable bus from significant coupling. The logic signals are asynchronous,
very low speed, and physically separated
from the audio signals. Power and ground
connection were kept off of the ribbon cable
bus to minimize the chance of current
(ground) loops. For your interest, Figure 2,
located at the end of this manual, describes
the signals that are carried on the ribbon
cable bus.
Crossfade Speed
We at Studio Technologies hope that the
crossfade times we have selected will be
right for you. If for some reason you have to
change one or more of the speeds, we will
now describe how to do it. The crossfade
circuitry is contained on the Crossfade
Card, and is discussed in depth in the
circuit description section of this manual.
Three crossfade speeds are used to optimize the audio output signal transition
between simulated and real stereo. Logic
circuitry on the Crossfade Card selects
which speed is appropriate for the operational situation. The SLOW speed is used
in two situations: the first is going from the
simulating stereo from left or right back to
a stereo input signal; the second is going
from a stereo input signal to simulated
stereo from left when there is a two channel
mono input signal. The FAST speed is used
when the input signal goes from a left and
right stereo input (not simulating) to left
input only, or right input only (going to
simulating stereo from left or right only
input). FAST is used so that the listener
hears only a minimal loss of left or right
channel audio, while the simulated stereo
is coming on line. The IMMEDIATE speed
is used whenever Remote Control Enable
is active. The ISS assumes that the remote
control input signals for Sim from Left and
Sim from Right are very precise and do not
require a time lag as a crossfade is performed. Note that the IMMEDIATE speed is
really just a fast crossfade. No audio clicks
are created during the transition.
The speeds are created in the Crossfade
Card circuitry using simple resistor/capacitor combinations. The SLOW speed is
created with resistor R7 and capacitor C7.
An analog switch adds resistor R9 in parallel with R7 to create the FAST speed. Another analog switch adds resistor R8 in
parallel with R7 to create the IMMEDIATE
speed. You can see that all three speeds
are based on the SLOW rate. Changing R7
will change all three speeds. Now do you
really want to change the SLOW speed?
Anyway, choose the speed(s) you want to
change.
If you want to change the SLOW speed,
remove R7 and increase its value if you
want a slower speed (longer RC time constant), or decrease its value if you want to
speed it up (shorter RC time constant).
Now check the FAST speed and see what
effect the new R7 value has made. If the
FAST speed is now not to your liking, remove R9 and replace it with a revised value.
Now check the IMMEDIATE speed. Adjusting R7 really shouldnt greatly effect the
IMMEDIATE speed, but if it does, remove
R8 and replace it with a revised value.
If SLOW is OK but you want to change the
FAST speed, remove R9 and increase its
value if you want a slower speed (longer
RC time constant), or decrease its value
if you want to speed it up (shorter RC time
constant).
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 19
ISS
If SLOW is OK but you want to change the
IMMEDIATE speed, remove R8 and increase its value if you want a slower speed
(longer RC time constant), or decrease its
value if you want to speed it up (shorter RC
time constant).
Recognition Card Adjustment
The Recognition Card recognition criteria
has been factory set for what we feel is
optimum performance. The Left Only and
Right Only recognition characteristics are
fixed by the design of the circuits. There is
no provision for changing their performance. The L=R recognition circuit does
contain a calibration trim pot. This pot, R10,
adjusts the sensitivity of the L=R recognition. The sensitivity determines when L=R
is recognized. It is factory set at 50% of
rotation. If you determine that stereo
signals are being recognized as L=R,
adjust R10 counterclockwise. This serves
to desensitize the circuit. If two channel
mono signals are not being recognized as
L=R, adjust R10 clockwise. This increases
the sensitivity of recognition. Be certain that
you really need to adjust this control. The
factory setting should give the best overall
performance.
Non-Standard Input and Output Levels
Studio Technologies designed the ISS to
match the audio operating levels of most
broadcast facilities. If you are the creative
type who likes to experiment, or the unlucky
one who inherited a station that has an
operating level different from 0, +4, or
+8dBu (ref. 0.7746V), dont despair. The 0,
+4, or +8 settings are used to optimize ISS
performance, and using a slightly different
operating level will make only minor differences in performance. If you are within two
dB of one of the ISSs preset levels, set
the input and output switches to the closest
value. If you are exactly in between two
of the choices, go for the lower one. An
example would be a station running +6.
Set the input and output levels for +4. If
you are running an operating level below
2 dB or above +10dB, contact Studio
Technologies for details on simple I/O
Card operating level modifications.
I/O Bypass versus Bypass
Frankly, when we named two ISS functions,
we inadvertently created a confusing situation. In this section we hope to clearly
explain just what we meant. Once you see
the similar names with different functions we
hope that long-term confusion will be minimized. As penance, the designers have
spent one weekend listening to the Greatest
Hits collections of Donnie and Marie, The
Turtles, and The Kingsmen. Extra time was
put in trying to figure out the actual words
to Louie Louie.
I/O Bypass: I/O Bypass is the name we
chose for a function performed by the I/O
Card and the Transfer Relay Assembly.
Relays on the Transfer Relay Assembly
connect the ISS audio inputs to the ISS
audio outputs in the event of a system
failure, operator request, or remote control
request. The I/O Bypass is a hard (relay
contact) bypassing of the ISS circuitry.
During normal ISS on-air operation, the
I/O Bypass mode will rarely be invoked.
Bypass: Bypass is the name we chose for
a function performed by the Crossfade
Card. When the ISS is in the Bypass mode
the crossfade circuit electronically connects
the left and right audio inputs to the left and
right audio outputs. This is an electronic, or
Issue 3, June 1990ISS User Guide
Page 20Studio Technologies, Inc.
ISS
soft bypass. The ISS will usually be in
this mode when stereo program material
is present on the left and right audio inputs.
When a Simulate from Left or Simulate from
Right command is given, the ISS mode will
change from Bypass to Sim from Left or
Sim from Right. During normal ISS on-air
operation, the state of the Bypass mode
will be changing in response to mono and
stereo input signals.
ISS Mainframe Grounding
The ISS mainframe contains two ground
circuits: earth and signal. Earth ground is
connected to all metal parts of the chassis,
the ground pin of the AC power connector,
pin 3 on each of the circuit card edge connectors serving the mainframe card slots,
and pin 1 of the four XL-type connectors.
Signal ground is the common point for the
power supplies and is connected to pins 4
and 11 on the mainframe card slots, and to
the relay driver circuitry on the Transfer
Relay Assembly. These grounds, electrically
isolated in the stock mainframe arrangement, are connected together via one point
in the ISS. This point is a jumper wire connecting pins 3 and 4 of edge connector P1
on the I/O Card. In most cases, this is the
preferred ground arrangement, insuring
safety and good shielding of the audio
signal wires. In certain cases it may be
desirable to isolate this ground. IN NO
CASE IS IT PERMISSIBLE TO FLOAT THE
CHASSIS FROM EARTH GROUND. This is
a safety ground and must connect via the
third wire of the power cord to an approved
ground. To isolate the signal ground from
the chassis, remove the previously mentioned jumper wire. Note this change on
your schematics for later reconnection if
required.
Remote Control Signals
One of the nicest features of the ISS is the
ability to control many functions remotely.
Two types of input signals can be used:
continuous or momentary. Switches on the
I/O Card, Polarity Correction Card, and
Mode Select Card set which type of signal
is to be recognized. Well consider a remote
control signal as a logic high whenever
current meeting the ISS specifications is
flowing into a remote control input. When
set for continuous, the remote control input
circuitry is enabled whenever a logic high
is present. When set for momentary, the
remote control input circuitry is leading
edge triggered. The transition from low to
high is considered a valid remote control
signal; a high to low transition is ignored.
Testing the ISS
Proof of performance tests on your broadcast facility commonly use sine waves of
different frequencies and levels to check
such things as frequency response, noise,
and distortion. Very unusual results can
occur if ISS performance tests are made
using sine wave or constant frequency
signals. These results are due to the way
the stereo simulator boards perform their
function, taking a mono input and delaying,
randomizing, and gyrating the signal into
a stereo image. Simulating stereo from a
fixed single frequency input will usually
result in different left and right output levels
that will appear to change randomly as the
input frequency is varied slightly. This is
completely normal and expected. Remember that the usual input signal to the simulator cards is a complex music, voice or other
natural sound. To get rational proof of
performance data, place the ISS in the
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 21
ISS
Bypass mode, putting the simulator cards
out of the broadcast chain. (This does not
mean removing the ISS from the audio path
by the use of the I/O Bypass mode!) If you
wish to check the ISS with the Stereo Simulator cards in the broadcast chain, you need
to use pink noise. The randomness of pink
noise will allow left verses right frequency
response observation. Studio Technologies
uses pink noise for testing the Stereo Simulator cards.
The Sound of the ISS
The ISS has been factory adjusted to give
what we feel is a very good overall simulated stereo sound. We spent a lot of time
doing listening tests with music, voice,
sound effects, and actual television audio
signals. If you feel you must adjust the ISS
stereo simulators, provisions have been
made for you to do so; trimmer potentiometers (trim pots) are buried behind the front
cover, but are accessible. The simulated
stereo is created by the two stereo simulator cards. The Type I Card is located in card
slot 2. The Type II Card is located in card
slot 4. Trim pot R43 on the Type I Simulator
Card controls the amount of simulation on
the full audio bandwidth. It is factory set at
50% of its rotation. Trim pot R43 on the
Type II Simulator Card controls the amount
of simulation over the upper and lower
portions of the audio band, but simulates
little on the voice band. It is factory set at
50% of its rotation. The outputs of the Type
I and Type II Simulator cards are combined
in the Crossfade Card to form the simulated
stereo signal you hear.
The following is a suggested procedure for
resetting the Stereo Simulator cards. You
should have a wide variety of sample program material available, especially mens
and womens voices and music with a very
wide frequency range. Remove the ISS front
panel by removing the four knurled screws.
Place the ISS in the SIM LEFT manual
mode. The trim pots to be adjusted are
located near the front of the simulators
cards. The cards do not have to be removed, nor the ISS power turned off, for
pot adjustment. However, you will need
a small screw driver and a little care. Turn
trim pots R43 on both simulator cards fully
counterclockwise. This turns off all stereo
simulation. Feed a voice signal into the ISS
left channel input. Listening in stereo to the
ISS left and right audio outputs, you should
hear the left input audio coming from both
the left and the right outputs, i. e., you
should be hearing two channel mono.
On the Type I Simulator Card, adjust R43
clockwise until an acceptable amount of
simulation is heard. Listen to make sure
that the voice does not sound overprocessed. Better too little simulation than
too much. Use the factory setting of 50%
pot rotation as a reference. Now feed a high
quality audio signal into the left input. By
high quality, we mean a music source that
has lots of low and high frequency content.
On the Type II Simulator Card, adjust R43
until your desired amount of simulated
stereo is heard. Listen carefully to the low
and high frequencies as this is where the
Type II Card is adding its affect. Switch
back to feeding voices and make sure they
still sound good. If they sound too affected,
adjust Type II R43 counterclockwise until
the voices again sound good. Go back to
the music, the simulated stereo should still
sound good. Confirm your settings by
doing listening tests with many different
audio signals, especially a wide variety of
voices. Once you are satisfied with your
settings, cut out this section of the manual
Issue 3, June 1990ISS User Guide
Page 22Studio Technologies, Inc.
ISS
and lock it in your desk. Practice saying to
everyone at your station, Gee, Id love to
let you adjust the ISS but its preset at the
factory.
Using the Extender Card Assembly
An Extender Card Assembly can be purchased to allow testing and maintenance of
individual ISS cards. Since signals connect
to an ISS card at both its front and back
edges, a rather unique extender arrangement has been devised. The Extender Card
Assembly consists of four parts: Extender
Cards 1 and 2, a 34-position ribbon extension cable, and a 20-position ribbon extension cable. To use the Extender Card
assembly:
1)If the ISS is currently on-air, arrange to
patch around the unit. Even though the
Transfer Relay Assembly can be used
to send the input audio to the audio
output connectors, it is better not to be
working on equipment when a minor
slip of the hand can result in on-air
errors. After patching around the ISS,
proceed.
2)Turn the ISS main power to the OFF
position.
3)Remove the ribbon cable bus from the
cards until the specific card to be serviced is disconnected. You dont have
to remove the entire ribbon cable bus.
4)Remove the card to be serviced.
6)Install Extender Card 1 with the attached 34-position ribbon extension
cable into the mainframe card slot
previously vacated by the card to be
serviced.
7)Reconnect the ribbon cable bus to
Extender Card 1 and to the other cards
that were previously detached.
8)Install one connector on the 20-position
ribbon extension cable into the connector marked P2 Extension on Extender
Card 1. (Extender 1 was just installed in
one of the mainframes card slots.) This
connector is directly above the connector that mates with the ribbon cable
bus. The colored stripe (usually red)
indicates pin 1 and should be mated
accordingly.
9)Install the other end of the 20-position
ribbon extension cable into connector
P2 on the card to be serviced. Ensure
that pin 1 is mated with pin 1.
10) Install the free end of the 34-position
ribbon extension cable to the connector
marked P1 Extension on Extender Card
2. Ensure pin 1 connects to pin 1.
11) Mate the card edge connector on
Extender Card 2 with edge card plug
P1 on the card under test. Ensure that
pin 1 mates with pin 1. The components
on the card under service and the test
points on Extender Card 2 should be
facing up.
5)Install either of the two connectors on
the 34-position ribbon extension cable
into the connector marked P1 Extension
on Extender Card 1 (the larger card).
The colored stripe (usually red) indicates pin 1 and should be mated accordingly.
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 23
12) Double check that all connectors are
mated correctly and pin 1 goes to pin 1
on all connectors.
13) Place the card (with the attached Extender Card 2) on a non-conducting
surface to protect the components from
accidental shorting.
ISS
14) You are now ready to turn the ISS
power switch to the ON position and
perform your required procedures.
Some minor cross talk or hum pickup
can occur due to the physical positions
of the ribbon cables connecting the
mainframe to the card being serviced.
Avoid placing the ribbon extension
cables (especially the 20-position) and
the card near strong magnetic fields
(such as near the ISS power supply)
that could induce hum or noise. Simply
moving the ribbon extension cable(s)
should clear up any major problems
encountered. The short interconnecting
distances on the actual ISS minimize
the chance of undesirable pickup under
operating conditions.
15) A service hint is to always begin testing
by checking the power supply voltages
that are easily accessed on the Extender Card 2 test points.
16) When storing the ribbon extension
cables, avoid sharp bends in the cable
which can cause permanent damage.
17) Feel free to call Studio Technologies
with any service or operation questions
you may have.
Technical Description
In this section, we will first review the ISS
system architecture. This will give an outline
of how the ISS relates to the outside world,
and how the circuit cards work together.
Then we will review the functionality and
circuitry contained on each ISS circuit card.
This information should greatly assist you in
understanding the operation of the ISS, as
well as providing a guide to troubleshooting
problems that may arise.
ISS System Architecture
As a complete unit, the ISS consists of a
mainframe, Transfer Relay Assembly, circuit
cards, ribbon cable bus, and front panel.
Studio Technologies chose to utilize a
commercially available powered mainframe.
By using a stock mainframe, the customer
benefits by getting the reliability that a
product built in quantity supplies; this
powered mainframe design is completely
field proven with thousands of units in
operation. The mainframe, manufactured by
dBx, Inc., includes a sophisticated power
supply and card slots for nine circuit cards.
The ISS circuit cards were designed to
mechanically and electrically interface into
this mainframe. Associated with each card
slot is a 10-position screw terminal strip
located on the mainframe back panel. All
connections to the Transfer Relay Assembly, i.e., audio signals, remote control
inputs, and status relay outputs, are made
via these screw terminal strips. Five connectors on the back of the Transfer Relay
Assembly interface the ISS with the outside
world. Connections are made between the
circuit cards using a ribbon cable bus
assembly. The ribbon cable bus assembly
consists of a length of 20-conductor flat
ribbon cable (commonly used in the computer industry) with eight 20-position sockets installed evenly along the length of the
ribbon cable. The sockets on the ribbon
bus connect with connectors located on
each of the ISS circuit cards. All connections on the ribbon cable bus go to every
card in the ISS. A circuit card uses only
those signals on the ribbon cable bus that
are needed. The signals on each of the 20
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ISS
positions of the ribbon cable are described
in Figure 2, located at the end of this
manual. As the 20 conductors on the ribbon
cable bus are .050" apart, care was taken
during the design phase to limit the chance
of cross talk occurring between adjacent
signal paths. This was achieved by two
means: signal path selection and limiting
signal level. Physical isolation was implemented by keeping the audio signals away
from control (logic) signals. The audio
signal levels are limited by the nominal
internal audio operating level of 6dBu.
Logic signal transitions are limited in number due to the non-synchronous design of
the system. No clock signals or reoccurring
logic transitions are produced within the
system.
I/O Card
There are four main sections of circuitry on
the I/O Card: ±18V power supplies,
undervoltage and I/O Bypass sensing and
control, line input, and line output.
+18V Power Supplies: With nominal input
and output levels of up to +8dBu, the input
and output audio circuitry on the I/O Card
requires ±18Vdc for excellent audio performance. Operation at lower power supply
rails, such as +15Vdc, will not provide
adequate peak signal levels; i.e., will give
inadequate headroom. The mainframe
provides ±15Vdc and ±24Vdc. The I/O
Card utilizes two integrated circuit type
voltage regulators (and supporting circuitry)
to reduce the ±24Vdc to ±18Vdc. As a
note, other sections of the I/O Card use the
±15Vdc and ±24Vdc.
Undervoltage Sensing and I/O Bypass: As a
product intended for continuous on-air duty,
major ISS failures must not take a stations
audio off the air. Relays on the Transfer
Relay Assembly act as a hard (mechanical) bypass switch. We call this the I/O
Bypass function. A control signal is generated by the I/O Card which controls the
Transfer Relay Assembly. When the ISS is
operating normally, the relays are held in
the energized state. The left and right line
input signals connect to the line input circuitry; the left and right line output circuitry
connects to the line output connectors.
When the I/O Card goes into the I/O Bypass
state, the transfer relays de-energize, connecting the line input signals to the line
output connectors. In this mode, the ISSs
line input and output circuitry is disconnected from the outside world.
The I/O Bypass function can occur because
of three reasons: an undervoltage condition
on one or more of the four power supply
voltages; a manually initiated command
from the front panel switch; or a command
via the remote control input.
A 5.1V zener diode provides a reference
voltage for the undervoltage sensing circuitry. This reference voltage is scaled and
connected to four sections of integrated
circuit voltage comparator. Two sections of
comparator monitor the mainframe
±15Vdc, and two sections monitor the
±18Vdc from the I/O Card voltage regulators. If the +15Vdc or +18Vdc drop below
+10Vdc, an error condition is detected
and the transfer relays de-energize. If the
15Vdc or 18Vdc go less negative than
12Vdc, an error condition is detected and
the transfer relays de-energize.
A switch located on the front edge of the I/O
Card allows manual I/O bypassing.
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ISS
The Remote I/O Bypass function allows an
external signal to place the ISS in the I/O
Bypass condition. The actual signal that
controls the I/O Bypass function is derived
from remote control input circuitry located
on the Mode Select Card. Pin 20 of the
ribbon cable bus carries the signal between
the two cards. The switch on the I/O Card
selects whether the Remote I/O Bypass
function is active.
Working in conjunction with the I/O Bypass
circuitry on the I/O Card is the I/O status
relay on the Crossfade Card. A contact on
the I/O status relay controls the Transfer
Relay Assembly. The I/O status relay is
controlled by the I/O Card via pin 19 of the
ribbon cable bus.
Line Input Stage: The purpose of the line
input stage is to take a balanced audio
input signal, reduce the level by a fixed
amount, and convert it to unbalanced. For
best operating performance, the internal
operating level of the ISS was selected to
be 6dBu. This level combines a good
signal to noise figure with ample peak
signal headroom for circuits operating with
±15Vdc power sources. Since television
broadcast facilities run different average
operating levels, the line input stage has
three switch selectable input levels: 0, +4,
or +8dBu. This translates to attenuating the
input signal by 6, 10, or 14dB.
Two sections of operational amplifier and a
3-position switch serve as the gain reduction section. The input signal is capacitor
coupled to the op amps. Two 100pf capacitors in conjunction with the input resistors
provide a high frequency roll-off to limit the
chance of a radio frequency interference
problem. An op amp connected in a differential mode unbalances the signal. The
output of the unbalancing op amp is capacitor coupled to the ribbon cable bus for
use by other ISS cards. Resistor locations
are available on the I/O Card for the installation of input load resistors. In most cases
this is not required, or desirable, and the
card is manufactured with no load resistors
installed.
Line Output Stage: The purpose of the line
output stage is to take an unbalanced
signal with a nominal level of 6dBu, add
gain, and convert it to a balanced, differential type. This 6dBu signal is the final
output of the other ISS cards. The amount
of gain in this circuit is set by a 3-position
switch. The audio output stage uses a
modern, sophisticated electronically balanced circuit to eliminate the need for an
audio transformer.
Signal enters the line output stage using an
op amp configured as a summing junction.
In this way, signals from more than one ISS
card can be combined. The summed signal
then connects to another op amp that
boosts the level by 6, 10, or 14dB. This level
increase has been switch selected to give a
nominal output level of 0, +4, or +8dBu.
After being boosted in level, the signal
connects to two op amps, one as an inverting buffer and the other as one side of a
balanced line driver circuit. The inverted
signal connects to the other side of the
balanced line driver circuit. Each side of the
line driver uses an op amp to feed a set of
current boost transistors. To preserve the
low frequency response, no output capacitors are used. This is one tough circuitit is
capable of driving high signal levels into
150 ohms! The balanced line driver circuit
utilizes cross feedback to insure stability
even when driving unbalanced loads. This
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means that if one side of the line output is
grounded, the circuit is not harmed and the
other side of the line output still functions
correctly. A trim potentiometer, in series
with the non-inverting input of one of the
output op amps, is used to balance the
positive and negative output signal excursions. This ensures that, as an example, a
1.00V positive excursion AC signal on the
+ line output connection will be matched
by a 1.00V negative excursion AC signal on
the line output connection.
Transfer Relay Assembly
The Transfer Relay Assembly provides the
capability to connect the audio inputs to the
audio outputs in the event of a system
malfunction or an operator initiated command. The simple circuitry consists of three
relays and a transistor control circuit. In
the normal operating mode, the transistor
is forward biased, and the relays are held
energized. One relay routes the left channel
line input signal to the ISS mainframe. The
ISS left channel line output is routed to the
output connector. The right channel is
handled the same way via another relay.
A third relay provides the I/O Bypass Enabled Status Relay Contact, accessible to
the user via the 25-pin plug. An LED and
current limiting resistor is in parallel with
the relay coils as a status indicator. The
relays can release for two reasons: loss of
24Vdc power coming from the mainframe,
or closing of the I/O Bypass status relay
contact that comes from the mainframe.
When the relays de-energize, the left audio
input is connected directly to the left audio
output. The left channel input and output
signals to/from the mainframe are disconnected. The same action occurs for the
right channel. In the I/O Bypass mode, the
aforementioned relay contact shorts, providing the I/O Bypass status relay contact.
The LED is now not lit, showing that the
Transfer Relay Panel is in the transfer
mode.
Stereo Simulator Cards
The input signal enters the Type I and
Type II cards via pin 9 of the ribbon cable
bus. One section of an op amp U7 acts
as an inverting buffer. The signal then
goes through a simple Resistor/Capacitor
pre-emphasis network that precedes U4a,
which acts as a compressor in a compandor circuit. U5 is an integrated circuit
compandor. The compressor attack time is
speeded by a charge pump, which reduces
transient distortion that is often associated
with compandors.
The signal now proceeds in different directions in the Type I and Type II cards. In the
Type I Card the companded signal connects to the anti-aliasing low-pass filter
discussed in the next paragraph. In the
Type II Card the signal proceeds to a band
reject filter. The band reject filter is made up
of four sections of op amp U9. The 3dB
points are at 400 and 2200Hz, with an 11dB
dip at 1100Hz. This filter is set to attenuate
signals in the voice band, while leaving low
and high frequency audio signals unaffected. This filter is the reason why the Type
II Card can add simulation only in the nonvoice region of the audio spectrum. The
filtered signal leaves the band-reject filter
and proceeds to the low-pass filter section.
Low-Pass Filter: Three sections of op amp
U7 form a 6-pole, 20kHz Butterworth lowpass filter. This reduces the possibility of
audio frequencies aliasing with the clock
frequency produced by U3.
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The audio is delayed by bucket brigade
delay (BBD) integrated circuit U2. The
length of the delay is directly proportional
to the frequency of the clock signals sent
to U2 by U3. U3 produces three signals for
BBD U2: Clock 1, Clock 2, and a voltage
reference. Clock 1 and 2 are identical
square wave signals 180 degrees apart in
phase. The frequency of Clock 1 and 2 is
set by the resistor/capacitor combination
C17 and R19/R20. A reference voltage is
produced by U3 (for use by the BBD) and
is not adjustable.
The clock is set for 119.5kHz for the Type I
Simulator Card and 64kHz for the Type II
Simulator Card.
The time delayed audio enters a 5-pole,
20kHz low-pass Butterworth filter created
using three sections of operational amplifier
U1. This filter removes clock frequency from
the output signal.
The signal was previously compressed in
anticipation of being delayed. It is now
expanded to recreate the initial dynamic
range. The expander portion of compandor
U5 restores the dynamic range. Again a
charge pump is used, this time in the
compandor rectifier.
The signal now enters a proprietary randomizing circuit, labeled N1. Frankly, the
great sound of the ISSs simulated stereo
is a result of this network. It modifies the
delayed signal so as to ensure that the
peaks and dips in the soon to be created
combs do not fall on objectionable harmonics, preserving the natural sound of the
audio.
The final outputs of the Stereo Simulator
cards are created by two sections of operational amplifier U6.
For the Type I Card: The left channel output
is created by summing the output of N1
with the direct input signal. The right channel output is created by connecting the
direct input signal to the inverting input and
connecting the output of N1 to the noninverting input.
For the Type II Card: The left channel output
is created by inverting the signal from N1.
The right channel output is created by
simply buffering the signal from N1.
The left and right channel outputs of the
Type I Card are actually a complete simulated stereo signal. The left and right channel outputs of the Type II Card are actually
just an inverted and non-inverted stereo
information signal. Summing op amps on
the Crossfade Card combine the Type I and
Type II signals to form the full ISS simulated
stereo signal. If you were to remove the
Type II Card, the ISS would still produce a
usable, but much less full stereo sound.
The Type II Card adds the extended low
and high frequency simulation. Removing
the Type I Card, while leaving the Type II
Card in place, would result in a left and right
channel signal with no simulated stereo on
it at all. Summing the left and right signals
would leave the ISS with no signal, i.e., they
completely cancel out. The Type II Card
outputs left and right stereo information to
be added to the simulated stereo produced
by the Type I.
The mono compatibility of the ISSs simulated stereo can be easily understood by a
careful study of how the stereo is actually
made in op amp U6. The output of network
N1 is really our stereo information. To
create the left channel of our simulated
stereo we simply add some of our stereo
information to the incoming mono signal; to
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create the right channel we subtract the
same amount. The amount we add and
subtract is directly related to how much
stereo effect we desire. Trim pot R43, Stereo Depth, controls how much of N1s
output is combined with the incoming
mono. Our resulting stereo signal for the
left channel is the sum of the input signal
(mono) and our stereo information; the right
channel is the difference between the input
signal and our stereo information. When
listening in MTS stereo, you hear a good
stereo feel. When listening in MTS mono,
the left and right signals are summed
(added together), giving you just the original signal. Our stereo information simply
cancels out! Remember, what we added
to the left channel, we subtracted from the
right channel. Add left and right together
and our stereo information drops out. This
process holds true when we have two
simulator cards. The Type I Card adds and
subtracts full bandwidth stereo information.
The Type II Card adds and subtracts bandpassed stereo information. Add left and
right together and the stereo information
from both cards cancels out. Perfect mono
compatibility!
Mode Select Card
The Mode Select Card features a simple set
of logic circuitry that efficiently controls ISS
system operation. The Mode Select Card
directs and creates logic signals that are
sent to the Crossfade Card, which in turn
creates the signals you hear on the air and
observe with your remote controls.
Dual 4 input/1 output analog switch U8
serves to route logic signals to the simulate
from left and the simulate from right inputs
on the Crossfade Card.
The Mode select switch chooses one of
three operating modes. In the manual
mode, the Crossfade speed is held in the
SLOW position, and the X1/Y1 signals on
U8 are routed to the Crossfade Card. The
Manual front panel switch is then used to
control the Crossfade Card. This mode is
primarily intended for testing or special
applications.
In the AUTO mode, the FAST/SLOW speed
line is no longer held logic low, and the
X0/Y0 signals on U8 are routed to the
Crossfade Card. Signals originating from
the Recognition Card (if present in the
system) are processed and then sent to
X0/Y0. Three signals come from the Recognition Card: R=L, L Only and R Only.
Logic SignalR=LL OnlyR Only
Logic HighX0X0Y0
Logic LowY0Y0X0
FAST/SLOWLow for High forHigh for
LogicSlowFastFast
In the AUTO + REMOTE mode, the signal
going to the Crossfade Card depends on
the state of the B input to U8. When B is
logic low, remote control has not been
enabled and operation is the same as in the
AUTO mode. When B is logic high, remote
control has been enabled. The signals
present on X2/Y2 are sent to the Crossfade
Card. When simulate from left is requested
via remote control, X2 is high and Y2 is low.
When simulate from right is requested via
remote control, X2 is low and Y2 is high.
When no simulation is requested, X2 and
Y2 are low.
Four identical circuits buffer the remote
control inputs. Optocoupler integrated
circuits provide complete isolation between
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the source of the remote control signals
and the ISS circuitry. A resistor in series
with the optocoupler photodiode provides
current limiting to protect the remote control
signal source and the photodiode. A diode
is connected anode to cathode/cathode to
anode across the photodiode to prevent a
polarity reversal on the remote control
signal from damaging the optocoupler.
The optocoupler output signals are buffered
using inverting Schmidt trigger logic buffers. The output of the buffer is now truly a
clean logic signal. This logic signal directly follows the remote control input. A
feature of the ISS is that continuous or
pulse remote control signals can be interfaced. To accommodate this, a four pole
switch selects whether the ISS will respond
to continuous or pulse signals. In the continuous mode, the output of the Schmidt
inverting buffer is sent directly to the next
section of circuitry. In the pulse mode, the
output of a D flip-flop, whose input is from
the Schmidt inverting buffer, is connected to
the next section of circuitry. The four signals
from the remote control inputs go to different paths.
arrangement is used to provide power-up
reset and a circuit active signal using a
Schmidt trigger inverting buffer. When in
the AUTO + REMOTE mode, the remote
enable signal connects to three places:
selector pin B of U8, the ribbon cable bus
as the IMMEDIATE signal, and to a buffer
acting as an LED driver. When the remote
enable signal is high, U8 selector pin B
goes high, selecting the signals on pins X2
and Y2 to go to the outputs. This lets the
Remote Sim L and Remote Sim R control
the Crossfade Card. The remote enable
command is buffered and sent to the
Crossfade Card as the IMMEDIATE command. (This triggers the Remote Control
Enabled relay and changes the crossfade
speed to immediate.) The remote enable
signal also causes the Remote Enabled
LED to light on the front edge of the Mode
Select Card.
The Remote Sim L and Remote Sim R
signals have a set of NAND gates (U11)
associated with them to insure that only
one can be selected at a time.
Crossfade Card
The Remote I/O Bypass signal drives the
base of NPN transistor Q1. Q1 is connected
The Crossfade Card contains two major
sections: audio control and logic control.
to the ribbon cable bus in an open collector
configuration. The I/O Card uses this signal
to control its I/O Bypass control circuit.
Notice that the reset pin of the Remote I/O
Bypass flip-flop is connected to one section
of the inverting Schmidt trigger acting as a
power-up reset circuit. This power-up reset
circuit insures that upon power-up the flipflop starts in the desired state.
Audio Control: The audio inputs to the
Crossfade Card are selected via the three
position INPUT switch. These three input
sources are connected to the Crossfade
Card via the ribbon cable bus. The switch
chooses the input source: signals from the
I/O Card, the Polarity Correction Card, or
the optional Tone Detection Card. The
switch selected audio inputs connect to
The signal from Remote Control Enable is
active only when the mode select switch is
two points in the circuit: analog switch U9
and voltage controlled amplifier (VCA)
in the AUTO + REMOTE position. A tricky
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integrated circuits U8 and U3. Analog
switch U9 selects which input, left or right,
gets sent to the simulator cards.
The left and right audio output signals from
the Type I and Type II simulator cards come
into the Crossfade Card via two sections of
op amp U5, which serve as inverting summing junctions to combine the signals from
the two simulator cards. The outputs of the
summing amplifiers each connect to two
points in the circuit: summing with the line
input signal going into the VCA, and summing with the output of the VCA going into
another op amp section of U5.
The crossfade action occurs by the cancellation process that is directly proportional to
the output level of the VCA. The VCA output
level is determined by a 0 to 800mV control
voltage whose source will be discussed
later. A control voltage of 800mV gives
maximum attenuation; 0mV gives unity gain
(0 attenuation). When 0mV is fed to a VCA,
the summed signal from the simulator cards
is cancelled out; when 800mV is fed to the
VCA the line input signal is canceled out.
The null adjusts, trim pots R6 and R25, are
set at the factory to provide the best attenuation at the extreme end of the crossfade.
An incorrectly set null adjustment would
give cross talk between the inputs and the
outputs of the stereo simulator cards.
Logic Control: The logic and crossfade
control voltage circuitry is quite straight
forward. Four logic input signals, entering
via the ribbon cable bus, give the functional
commands to the Crossfade Card. These
signals request simulate from the left channel, simulate from the right channel,
crossfade at FAST, and crossfade at
IMMEDIATE.
The heart of the circuitry is a simple
resistor/capacitor circuit created by C7 and
R7, and 5V and 10V reference voltages
created by R31, R32 and R38. We add to
this three op amps acting as comparators
(sections of U7 and U11) which allow the
RC circuit to swing between 5V and 10V.
The 5V to 10V swing is controlled in direction (up or down) and speed. Two sections
of NAND gate U1 provide a logic high when
simulate from left or simulate from right is
requested. This logic high (15V) moves the
voltage on the RC circuit from 5V to 10V.
Since the capacitance is fixed, the speed at
which the RC circuit goes from 5V to 10V is
dependent on the resistance in the RC
circuit. The FAST/SLOW and IMMEDIATE
speed logic signals determine if additional
resistance is placed in parallel with R7,
decreasing the time constant and speeding
up the crossfade. The additional resistance
is placed in or out of the RC circuit using
two sections of analog switch U2. When
simulate from left or simulate from right is
not requested, the RC circuit moves back to
5V; the speed is again determined by the
status of the speed logic signals.
The 5V to 10V ramp signal is sent to two
places in the circuitry. A section of op amp
U11 provides a linear conversion, taking the
5V to 10V swing and changing it to a 0V to
800mV swing. This voltage swing provides
the VCAs with the crossfade voltage. The
circuit is designed so as to lock within a
few mV of 0V so as to keep the VCA precisely at unity gain. Another section of op
amp U11 converts the 5V to 10V swing to a
0V to 15V swing. This swing is used to light
the crossfade status lights. Note that two
sections of analog switch U2 control the
simulate from left and simulate from right
LEDs.
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Two sections of op amp U7 act as comparators to create an indication of when the
reference ramp signal is at 5V or 10V.
These signals are used for two functions:
maintain feed to the simulator cards and
enable the simulating from right and simulating from left relays.
There are four relays contained on the
Crossfade Card. Three of the relays are not
integral to the operation of the ISS but are
used to provide status indication to the
associated broadcast system. The fourth
provides the Transfer Relay Assembly with
the I/O Bypass status. Four normally open
(not shorted) relay contacts provide the
following indications: simulating from left,
simulating from right, ISS operating via the
remote control input (remote operation
enabled), and I/O Bypass request. Notice
that Remote Enable relay energizes whenever the IMMEDIATE crossfade speed is
selected. This is because the only time the
immediate speed is active is when the ISS
is remotely controlled.
Recognition Card
The Recognition Card contains four major
sections: Band-Pass Filters, Peak Detection,
L=R Recognition, and Left Only/Right Only
Recognition.
Band-Pass Filters: Left and right channel
audio signals enter the Recognition Card
via the three position INPUT switch. This
switch selects the input source. In the A
position the signals come from the output
of the I/O Card. In the B position the signals
come from the output of the Polarity Correction Card. In the C position signals come
from the output of the optional Tone Detection Card. The input signals then enter lowpass Butterworth filters consisting of three
op amp sections. The signals then go
through high-pass Butterworth filters that
use two op amp sections. The resultant
signals have a 3dB band-pass of 100 to
1kHz. For accurate left versus right performance, all resistors and capacitors have
1% tolerance. The band-pass filters have
a unity gain design so that the input and
output levels should be roughly identical
within the pass band; 500Hz should enter
and leave at the same level. The signals
are filtered so that accurate recognition is
possible. If the high frequencies are not
removed, the normal phase shifts due to
tape head azimuth errors or short differential time delays will interfere with actual left
versus right differences. If the low frequencies are not removed, the large amounts of
energy at the low frequencies will create
false recognition results. The band-passed
output signals then go to the three other
sections.
Peak Detector: The band-passed left and
right signals are summed using one op
amp section. This op amp, along with one
other, creates a half-wave rectifier circuit
that produces a DC signal that is representative of the summed amplitude of the left
and right signals. A comparator serves to
gate the DC signal so as to speed up the
rectification. This speeded up signal is a
peak DC picture of the band-passed left
and right signals. This peak DC is used by
the remaining two sections.
L=R Recognition: This circuit determines
if signals present on the left and right channels at the same time are mono, i.e., identical. A comparator is used to compare the
band-passed left channel signal with a
resistor divider scaled version of the peak
reference signal. The output of this comparator is 0 volts when the left channel
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meets this criteria; 15 volts when it does
not. This results in a series of short pulses
representative of the phase activity of the
signal. Another comparator is used for the
band-passed right channel. These two
output signals are sent to an exclusive-OR
(XOR) gate which produces a logic high
only when the input signals are phase
coherent. If the pulses sent to the inputs of
the XOR gate are not in phase, the XOR
gate output will stay at logic low. Input
pulses that are coherent will result in a logic
high output pulse. These XOR gate output
pulses charge a resistor-capacitor low pass
filter. The output of this filter represents the
amount of phase coherency. This output is
fed to a comparator whose trigger has been
calibrated so that when sufficient phase
coherency is detected a L=R logic high is
generated. A feedback path is used to hold
the state of the final comparator during
periods of time when the peak detector
amplitude is not sufficient for accurate
recognition. During actual broadcast operation this hold would come into effect when
an audio track fades out at the end of a
commercial, etc. The result is a logic high
when the two channels are determined to
be phase coherent. This logic high, called
L=R, is sent via one section of DIP switch,
and the ribbon cable bus, to the Mode
Select Card. The DIP switch allows disabling of the L=R recognition feature.
Left Only/Right Only Recognition: The bandpassed left and right signals each come
into this section via a section of op amp
set for a gain of about 30dB. These op
amps create what is effectively a signal
present output. Very little input amplitude
will cause the output of the op amps to go
to 15 volts. Our friend the peak detector
now comes into play again. Two identical
circuits determine a left only or right only
condition. We will discuss the right only
circuit. A comparator is used to compare
the left channel signal present level with
the amplitude of the peak detector. The
output of this comparator goes logic low
when the amplitude of the peak detector is
greater than the amplitude of left channel
signal present. This logic low, in effect,
says that the left channel is not contributing
much to the peak detector amplitude. This
signal is further refined with another comparator section using a DC level as its
reference. A logic low on the output of this
comparator can be considered as a right
only indication. Two other comparators
produce a left only indication. These two
signals are fed to a flip-flop whose outputs
create the Left Only and Right Only outputs.
Besides going to two sections of DIP
switch, these outputs are fed back to the
signal present points, creating a holding
level. This holding level keeps the circuit
stable when audio is not present at a sufficient level to produce an accurate detection
result. The outputs of the DIP switches are
sent to the Mode Select Card via the ribbon
cable bus.
Polarity Correction Card
The Polarity Correction Card contains five
major sections: Audio Input/Output, BandPass Filters, Peak Detection, Polarity Detection, and Mode Select and Remote Control.
Audio Input/Output: Left and right channel
audio signals enter the Polarity Correction
Card via the ribbon cable bus from the
outputs of the I/O Card. The left channel
signal connects to the input of the left channel band-pass filter, as well as directly out
again via another pin in the ribbon cable
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bus. The right channel signal connects to
three points. The first is to a comparator
that produces a string of pulses that correspond to the signals zero crossings. The
purpose of this will be discussed later. The
second point is to the input of an op amp
configured as an inverting unity gain amplifier. The output of this op amp feeds an
analog switch. The third point is to another
analog switch. The outputs of the two analog switches connect together and feed the
input of the right channel band-pass filter,
as well as back out on another pin on the
ribbon cable bus. The gate of one analog
switch connects to the Q output of a flipflop; the other to Q invert. The right channel
output polarity depends on the state of this
flip-flop. In one state the right channel input
connects directly to the output; in the other
state the right channel output is derived
from the inverting op amp. In this simple
way the left and right channels can be put
in the same relative polarity.
Band-Pass Filters: The left and right signals
enter the filter section via separate low-pass
Butterworth filters consisting of three op
amp sections. The signals then go through
separate high-pass Butterworth filters that
use two op amp sections. The resultant
signals have a 3dB band-pass of 100Hz to
1kHz. For accurate left versus right tracking,
all filter related resistors and capacitors
have 1% tolerance. The band-pass filters
have a unity gain design so that the input
and output levels should be roughly identical within the pass band; a 500Hz signal
should enter and leave at the same level.
The signals are filtered so that an accurate
determination of relative phase can be
made. If the high frequencies were not
removed, the normal phase shifts, due
to tape head azimuth errors or short
differential time delays, would interfere with
relevant left versus right differences. If the
low frequencies were not removed, the
large amounts of energy at the low frequencies could create false results. The bandpassed left and right signals go on to
the Peak Detector and Polarity Detection
sections.
Peak Detector: The band-passed left and
right signals are summed using one op
amp section. This op amp, along with one
other, create a half-wave rectifier circuit that
forms a DC signal that is representative of
the summed amplitude of the left and right
signals. A comparator serves to gate the
DC signal so as to speed up the rectification. This speeded up signal is a peak DC
picture of the band-passed left and right
signals.
Polarity Detection: The band-passed left
and right signals are fed differentially to the
inputs of an op amp. The resultant output is
the difference between the left and right
signals. This difference signal, along with
the peak signal, is fed into a comparator.
This comparator acts as a polarity normal,
polarity flipped detector. If the left and right
signals have roughly the same polarity, the
peak signal will be greater than the difference signal. If the opposite is true, the
polarity of the left and right signals are, at
least at any one instant, opposite. The
output of this comparator feeds an RC lowpass filter, and then on to another comparator. This comparator uses a fixed voltage
reference, along with hysteresis, to insure
that a true polarity reversal is occurring, and
not one that is very brief due to normal,
phase complex stereo signals. The output
of this comparator is effectively a logic
signal that changes state when a polarity
Issue 3, June 1990ISS User Guide
Page 34Studio Technologies, Inc.
ISS
reversal is detected. This logic signal clocks
a flip-flop, whose output is configured to
change state on a clock transition. The flipflop output feeds the D input of another flipflop. This second flip-flop outputs the final
polarity correction signals that control the
polarity correction audio circuitry. The
output of the second flip-flop has two constraints placed on it. The first requirement
is that the D signal is sent to the output only
during a zero crossing of the right channel
audio signal. As previously discussed, the
right channel audio is sent to a comparator
that produces an invert clock signal. This
invert clock signal is a string of pulses that
correspond to the zero crossings of the
right channel audio. The second requirement is that the flip-flop is enabled, or
more accurately, has not been disabled
by the front panel switch or remote control
request.
To review: The Polarity Detection circuit
simply looks to see if the left and right
signals are in the same relative polarity;
there is no absolute reference. The circuit
performs the same action when going
between what, to a broadcaster, is two
different events. The first event is the transition from polarity correct to polarity reversed audio. The circuitry detects this
condition and flips the right channels
polarity. The circuitry now detects the left
and right signals as polarity correct. The
second event is the broadcast audio source
going from polarity incorrect back to polarity correct. The circuitry again sees a problem and flips the right channel again. The
right channel audio now passes through
the analog switches without a polarity flip.
Mode Select and Remote Control: A switch
controls the operating mode of the Polarity
Correction Card. One remote control input,
and two relay outputs give remote control
access to several Polarity Correction
Card functions. Two LEDs provide status
indication.
The Remote Disable input allows operation
of the card to be disabled. An optocoupler
integrated circuit provides isolation between
the source of the remote control signal and
the ISS circuitry. A resistor in series with the
optocoupler photodiode provides current
limiting to protect the remote control signal
source and the photodiode. A diode is
connected anode to cathode/cathode to
anode across the photodiode to prevent
a polarity reversal on the remote control
signal from damaging the optocoupler. The
optocoupler output signal is buffered using
an inverting Schmidt trigger gate. The
output of the buffer is now truly a clean
logic signal. This logic signal directly follows the remote control input. A switch
selects whether the Remote Disable input
will respond to a continuous or pulse signal.
In the continuous mode, the output of the
Schmidt inverting buffer is sent directly to
the next section of circuitry. In the pulse
mode, the output of a D flip-flop, whose
input is from the Schmidt inverting buffer,
is connected to the next section of circuitry.
A single pole, three position switch controls
three sections of analog switch which set
the mode of the card. In the DISABLE
position the flip-flop that controls the right
channel audio analog switches is disabled.
In the OPERATE position the flip-flop is
active but a Remote Disable request is
ignored. In the OPERATE + REMOTE
position the flip-flop is active, and a Remote
Disable request will disable the flip-flop.
Two relay contacts provide status indication
to the outside world. The Remote Disable
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 35
contact closes (shorts) when the card is in
the OPERATE + REMOTE mode and a
remote disable command is received. The
Correcting contact closes (shorts) whenever the card has flipped the polarity of the
right channel. Status LEDs, located on the
front of the card, mimic the operation of the
relays.
ISS
Issue 3, June 1990ISS User Guide
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Appendices
Appendix A
Specifications
Mounting
Three spaces in a standard 19-inch (48.3cm) rack
AC Mains Requirements
100 to 125Vac (nominal 115Vac), or 200 to 250Vac
(nominal 230Vac), switch selectable 50/60Hz, 100
watts maximum
Fuse
0.75A, 3AG for 115V operation 0.375A for 230V
operation Slow-Blow Type
Audio Connections
Line Inputs: 3-pin XL-Type, Female
Line Outputs: 3-pin XL-Type, Male Pin 2 Audio High
Remote Control/Status Relay Connections
25-pin D-type, Male
Input/Output Format
Discrete left and right
Input Level
0, +4, or +8dBu, switch selectable
Remote Control Inputs
Optically coupled, current limited logic level, switch
selectable for continuous or pulse type. +30Vdc
maximum, 4mA minimum, 20mA maximum
Audio Switching
Electronic Crossfade: VCA based circuit Hard
Bypass via Relay Contacts
Relay Contacts
Isolated, sealed, bifurcated type For noise control
limit current to DC only, maximum 50mA
Recognition Card
Contains circuitry to detect left only as mono, right
only as mono, and mono signal on left and right as
mono. Each condition can be defeated by a switch.
Polarity Correction Card
Contains circuitry to detect and correct 180 degree
phase reversal on input signals. Correction occurs
at signal zero crossing.
Dimensions (Overall)
19.00 inches wide (48.3cm)
5.25 inches high (13.3cm)
13.75 inches deep (34.9cm)
Weight
22.5 pounds
Specifications subject to change without notice.
Input Impedance
20k ohms (with no input load resistor installed),
electronically balanced
Output Level
0, +4, or +8dBu, switch selectable
Output Impedance
60 ohms, electronically balanced
Output Level at Clipping (0dBu = 0.7746V)
+22dBu into 150 ohms, Balanced +28dBu into 600
ohms, Balanced Output level current limited for
safety
Frequency Response
(Simulator VCA Bypassed) ±0.1dB, 20Hz to 20kHz
Signal to Noise Ratio (Simulator In Circuit)
76dB
Distortion (THD) (20Hz to 20kHz)
Simulator VCA Bypassed: less than 0.06% Simulator In Circuit: less than 0.40%
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 37
ISS
Appendix B
ISS Alignment Notes
Stereo Simulator Card Alignment
A number of trim potentiometers are factory
adjusted on the Type I and Type II Simulator Cards. These pots do not require adjustment unless parts have been changed due
to repair of the Simulator Card. Changing
the setting of any pot without going through
the entire procedure can cause incorrect
operation of the Simulator Card and ISS
System.
Type I and Type II Cards
Stereo Simulator Cards are built as Type I
or Type II. The same raw printed circuit
board is used for each version. The Type II
Card contains a band dip filter; the Type I
does not have the parts for the filter installed. Several minor differences between
the two cards are also present but do not
effect alignment.
Materials Required for Alignment
Procedure for Type I Card
1)Place the Type I Simulator Card onto
the Extender Card System. Refer to the
ISS Technical Manual for Extender Card
installation details.
2)Turn the ISS mains power on.
6)Set the signal generator frequency to
1kHz, with output level to OFF so that
no signal is getting sent to the ISS left
line input. The signal generator signal
must be a sine wave.
Checking the Power Supply Voltages
With the DC voltmeter common lead connected to COM test point: check +15 test
point for +15 ±1Vdc, 15 test point for
15 ±1Vdc.
Checking for the Correct Rough Setting
of the Compander
1)Again insure that no audio is coming
into the ISS.
2)With DC voltmeter common lead connected to COM test point: check TP5
for 1.35 ±0.3Vdc. If not within this
range, set R69 to give 1.35Vdc at TP5.
3)With DC voltmeter common lead connected to COM test point: check TP7
for 1.35 ±0.3Vdc. If not within this
range, set R56 to give 1.35Vdc at TP7.
Setting the Analog Delay Clock
Frequency
1)Connect common lead of frequency
counter to COM test point. Check TP2
for 119.5kHz ±0.5kHz. If not within this
range, set R20 to give a value in this
range.
3)Set the ISS to: I/O Normal, mode to
MAN, SIM LEFT.
4)Set R4 and R43 to 50% clockwise; R18
to 75% clockwise.
5)Connect the signal generator output to
the ISS left channel line input, located
Adjusting the Incoming Audio Test
Signal
1)Connect the AC voltmeter common
lead to the COM test point.
2)Adjust audio generator output level to
give 10dBu reading at TP3.
on the back of the ISS.
Issue 3, June 1990ISS User Guide
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ISS
Adjusting the Compressor
1)Move AC voltmeter lead to test point
TP4. Note the reading that you observe.
It should be 10 ±2.5dBu.
2)Reduce generator output level by 20dB.
Note: This means drop the level by
20dB.
3)Observe level at TP4. It should have
dropped 15 ±0.3dB. If not, adjust R69
to get this condition.
4)Raise generator level 20dB. Observe
level at TP4.
5)Reduce generator output level 20dB.
Observe level at TP4. It should drop 15
±0.3dB. If not, again adjust R69 to get
this condition.
Adjusting the Analog Delay for Minimum
Distortion
1)Set generator frequency to 5kHz; adjust
level to give 10dBu when measured at
TP3.
2)Connect distortion analyzer to measure
at TP1.
3)Adjust R18 to give minimum distortion
(THD + Noise). The acceptable minimum distortion is 0.35% or lower. The
usual minimum is 0.25% to 0.10%.
Adjusting the Expander
1)Set generator frequency to 1kHz; adjust
level to give 10dBu when measured at
TP3.
4)Raise generator level 20dB. Observe
level at TP1.
5)Drop generator level 20dB. Observe
level at TP1. It should drop 20 ±0.3dB.
If not, again adjust R56 to get this
condition.
Adjusting the Transient Response of the
Expander
1)Adjust generator level to give 0dBu
when measured at TP3. Set the generator to tone burst mode: two cycles
open, 64 cycles closed. In this way, two
cycles of audio pass to the ISS, then
64 cycles of no audio, etc.
2)Observe TP1 on the oscilloscope.
Adjust R4 to give the flattest base band
signal. The signal should not over or
under shoot.
3)This completes the entire procedure.
Procedure for Type II Card
1)Temporarily remove op amp U9. Use
jumper clip to connect TP4 to the top
of resistor R63. Refer to schematic to
see that you have removed the band
dip filter from the circuit. This makes
alignment much easier.
2)Place the Type II Simulator Card onto
the Extender Card Assembly. Refer to
the Technical Notes section of the ISS
Technical Manual for Extender Card
installation details.
3)Turn the ISS mains power on.
2)Measure level at TP1.
3)Drop generator level 20dB. Level at TP1
should drop 20 ±0.3dB. Adjust R56 to
get this condition.
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 39
4)Set the ISS to: I/O Normal, mode to
MAN, SIM LEFT.
5)Set R4 and R43 to 50% clockwise; R18
to 75% clockwise.
ISS
6)Connect the signal generator output to
the ISS left channel line input, located
on the back of the ISS.
7)Set the signal generator frequency to
1kHz, with output level to OFF so that
no signal is getting sent to the ISS left
line input. The signal generator signal
must be a sine wave.
Checking the Power Supply Voltages
With the DC voltmeter common lead connected to COM test point: check +15 test
point for +15 ±1Vdc, 15 test point for
15 ±1Vdc.
Checking for the Correct Rough Setting
of the Compander
1)Again insure that no audio is coming
into the ISS.
2)With DC voltmeter common lead connected to COM test point: check TP5
for 1.35 ±0.3Vdc. If not within this
range, set R69 to give 1.35Vdc at TP5.
3)With DC voltmeter common lead connected to COM test point: check TP7
for 1.35 ±0.3Vdc. If not within this
range, set R56 to give 1.35Vdc at TP7.
Setting the Analog Delay Clock
Frequency
1)Connect common lead of frequency
counter to COM test point. Check TP2
for 64kHz ±0.5kHz. If not within this
range, set R20 to give a value in this
range.
Adjusting the Incoming Audio Test
Signal
1)Connect the AC voltmeter common
lead to the COM test point.
2)Adjust audio generator output level to
give 10dBu reading at TP3.
Adjusting the Compressor
1)Move AC voltmeter lead to test point
TP4. Note the reading that you observe.
It should be 10 ±2.5dBu.
2)Reduce generator output level 20dB.
3)Observe level at TP4. It should have
dropped 15 ±0.3dB. If not, adjust R69
to get this condition.
4)Raise generator level 20dB. Observe
level at TP4.
5)Reduce generator output level 20dB.
Observe level at TP4. It should drop 15
±0.3dB. If not, again adjust R69 to get
this condition.
Adjusting the Analog Delay for Minimum
Distortion
1)Adjust generator frequency to 5kHz.
Set level to give 10dBu when measured at TP3.
2)Connect distortion analyzer to measure
at TP1.
3)Adjust R18 to give minimum distortion
(THD + Noise). The acceptable minimum distortion is 0.35% or lower. The
usual minimum is 0.25% to 0.10%.
Adjusting the Expander
1)Adjust generator frequency to 1kHz.
Set level to give 10dBu at TP3.
2)Measure level at TP1.
3)Drop generator level 20dB. Level at TP1
should drop 20 ±0.3dB. Adjust R56 to
get this condition.
Issue 3, June 1990ISS User Guide
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4)Raise generator level 20dB. Observe
level at TP1.
5)Reduce generator output level 20dB.
Observe level at TP1. It should drop 20
±0.3dB. If not, again adjust R56 to get
this condition.
Adjusting the Transient Response of the
Expander
1)Adjust generator frequency to 1kHz.
Adjust level to give 0dBu when measured at TP3. Set the generator to tone
burst mode: two cycles open, 64 cycles
closed. In this way, two cycles of audio
pass to the ISS, then 64 cycles of no
audio, etc.
2)Observe TP1 on the oscilloscope.
Adjust R4 to give the flattest base band
signal. The signal should not over or
under shoot.
The Band Dip Filter Returns
the AC balance. One pot is set for each of
the two channels.
Materials Required for Alignment
ISS Extender Card System (two cards
and two cables)
Low Distortion Audio Signal (Sine Wave)
Generator
Audio Voltmeter with high input
impedance (AC VTVM), quantity of 2
DC Voltmeter, high input impedance type
Test Probes for above
Procedure
1)Place the I/O Card onto the Extender
Card System. Refer to the ISS Technical Manual for Extender Card installation details.
2)Turn the ISS mains power on.
3)Set the ISS to: I/O Normal, mode to
MAN, BYPASS.
1)Turn mains power to OFF.
2)Remove the Type II Card from the
extender.
3)Remove the test clip linking the two test
points.
4)Reinsert integrated circuit U9.
5)This ends the procedure.
Aligning the I/O Card
The I/O Card provides a balanced output. A
positive excursion on the audio high lead
should be matched in negative amplitude
on the audio low lead. How closely these
excursions match in amplitude is called AC
balance. These excursions are referenced
to signal ground. The I/O Card contains two
potentiometers. These are set to provide
4)If your facility uses resistive loading of
audio outputs, load the ISS left and
right line outputs with your standard
load, e.g., 150 ohms, 600 ohms, etc.
5)Connect the signal generator output to
the ISS left channel line input, located
on the back of the ISS.
6)Set the signal generator output to 1kHz,
with level set to your nominal operating
level, e.g., +4dBu
Checking the Power Supply Voltages
With the DC voltmeter common lead connected to COM test point: check +18 test
point for +18 ±1Vdc, 18 test point for 18
±1Vdc.
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 41
ISS
Setting the Left Channel AC Balance
1)Connect one of the AC voltmeters
between COM and the left channel
audio high connection, test point B+
on Extender Card 2. Connect the other
AC voltmeter between COM and left
channel audio low connection, test
point B on Extender Card 2.
2)Set pot R29 to give equal amplitude
on the two meters. You should be able
to adjust the balance within about 10
millivolts.
Setting the Right Channel Balance
1)Move the signal generator output to
the ISS right channel line input.
2)Connect one of the AC voltmeters
between COM and the right channel
audio high connection, test point D+
on Extender Card 2. Connect the other
AC voltmeter between COM and right
channel audio low connection, test
point D on Extender Card 2.
3)Set pot R28 to give equal amplitude
on the two meters. You should be able
to adjust the balance within about 10
millivolts.
4)This ends the procedure.
Aligning the Crossfade Card
The Crossfade Card contains two potentiometers. These are set to provide the
maximum attenuation of the input signals
from the Type I and Type II Simulator Cards
when the ISS is in the bypass mode. One
pot is set for each of the two channels.
Materials Required for Alignment
ISS Extender Card System (two cards
and two cables)
Low Distortion Audio Signal (Sine Wave)
Generator
Audio Voltmeter with high impedance
input (AC VTVM)
DC Voltmeter, high input impedance type
Test Probes for above
10k ohm, ¼W Resistor
Jumper wire with test clips at each end,
6-inch maximum length
Procedure
1)Place the Crossfade Card onto the
Extender Card System. Refer to the ISS
Technical Manual for Extender Card
installation details.
2)Turn the ISS mains power on.
3)Set the ISS to: I/O Normal, mode to
MAN, BYPASS.
4)Set the signal generator output frequency to 1kHz, level 6dBu.
Checking the Power Supply Voltages
With the DC voltmeter common lead connected to COM test point: check +15 test
point for +15 ±1Vdc, +24 test point for
+24 ±1Vdc, and, 15 test point for 15
±1Vdc.
Checking the Ramp Voltage
With the DC voltmeter common lead connected to COM test point: check RAMP test
point for 0Vdc ±0.050Vdc. This insures you
are in the bypass mode.
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Setting the Left Channel for Maximum
Attenuation
1)Connect the common lead of the AC
voltmeter to the COM test point. Connect the other lead to LEFT OUTPUT
test point.
2)Connect the common lead of the audio
generator to the COM test point. Connect the high lead to one end of the 10k
resistor. Use the jumper wire to connect
the other end of the resistor to the
junction of U5 pin 2, C22, and R16. You
can get at this point by connecting to
the bottom of R16. The 10k resistor is
acting as a summing resistor to feed a
signal into the inverting input of an op
amp.
3)Adjust 10-turn trim pot R25 to give a
minimum reading on the AC VTVM. You
are nulling the left channel crossfade
circuit. A normal level when nulled for
minimum would be 45 to 60dBu.
There is no exact correct value.
3)Adjust R6 to give a minimum reading
on the AC VTVM. You are nulling the
right channel crossfade circuit. A normal level when nulled for minimum
would be 45 to 60dBu. Again, there
is no exact correct value.
4) This ends the procedure.
Setting the Right Channel for Maximum
Attenuation
1)Connect the common lead of the AC
voltmeter to the COM test point. Connect the other lead to RIGHT OUTPUT
test point.
2)Connect the common lead of the audio
generator to the COM test point. Connect the high lead to one end of the 10k
resistor. Use the jumper wire to connect
the other end of the resistor to the
junction of U5 pin 13, C9, and R18. You
can get at this point by connecting to
the bottom of R18.
ISS User GuideIssue 3, June 1990
Studio Technologies, Inc.Page 43
ISS
Figure 1ISS Connection Diagram
Audio Signals
Pin NumberISS Function
1Chassis Ground
2Audio High
3Audio Low
Remote Control Input Signals
P1 Pin NumberISS Function
1+Remote Polarity Correction Function Disable
2
3+Remote Control Enable
4
5+Remote Simulate from Left
6
7+Remote Simulate from Right
8
9+Remote I/O Bypass
10
Note: Use current limited DC signal, 4mA minimum, 20mA maximum.
Status Relay Outputs
P1 Pin NumberISS Function
14Polarity Correction Taking Place
15
16Polarity Correction Function Disabled
17
18ISS Remote Control Enabled
19
20ISS Simulating from Left
21
22ISS Simulating from Right
23
24ISS I/O Bypass Enabled
25
Note: These are normally open relay contacts that close when the described
functions are active.
Issue 3, June 1990ISS User Guide
Page 44Studio Technologies, Inc.
ISS
Figure 2ISS Ribbon Cable Bus
Note: This figure is for reference purposes only. It does not
affect installation or operation.
Bus NumberDescription
1Left Audio from I/O (ISS Left Audio Input)
2Right Audio from I/O (ISS Right Audio Input)
3Left Audio from Polarity Correction Card
4Right Audio from Polarity Correction Card
5Left Audio from Tone Detection Card (Optional)
6Right Audio from Tone Detection Card (Optional)
7Left Audio to I/O (ISS Left Audio Output)
8Right Audio to I/O (ISS Right Audio Output)
9Audio Send to Simulators from Crossfade Card
10Left Audio from Simulators
11Right Audio from Simulators
12Logic, high if Recognition Card detects L=R
13Logic, high if Recognition Card detects L only
14Logic, high if Recognition Card detects R only
15Logic, high if Simulate from Left requested
16Logic, high if Simulate from Right requested
17Logic, high if Fast Crossfade Speed requested
18Logic, high if Immediate Crossfade Speed requested
19Logic, high if Remote Enable requested
20Modified Logic, low if I/O Bypass requested