DAQ-STC2 S Series Simultaneous Sampling Multifunction Input/Output Devices
NI 6124/6154 User Manual
August 2008
372613A-01
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ni.com/certification, search by model number or product line,
Changing Data Transfer Methods between DMA and IRQ............................ 10-2
Chapter 11
Triggering
Triggering with a Digital Source...................................................................................11-1
Triggering with an Analog Source ................................................................................ 11-2
Analog Input Channel ..................................................................................... 11-3
Analog Trigger Actions .................................................................................. 11-3
Analog Trigger Types.................................................................................................... 11-3
Analog Trigger Accuracy .............................................................................................. 11-6
Appendix A
Device-Specific Information
Appendix B
Technical Support and Professional Services
Glossary
Index
NI 6124/6154 User Manualxni.com
About This Manual
The NI 6124/6154 User Manual contains information about using the
National Instruments S Series NI 6124 and NI 6154 data acquisition (DAQ)
devices with NI-DAQmx 8.8 and later.
Conventions
The following conventions appear in this manual:
<>Angle brackets that contain numbers separated by an ellipsis represent
a range of values associated with a bit or signal name—for example,
AO <3. .0>.
»The » symbol leads you through nested menu items and dialog box options
to a final action. The sequence File»Page Setup»Options directs you to
pull down the File menu, select the Page Setup item, and select Options
from the last dialog box.
This icon denotes a note, which alerts you to important information.
This icon denotes a caution, which advises you of precautions to take to
avoid injury, data loss, or a system crash.When this symbol is marked on a
product, refer to the Read Me First: Safety and Radio-Frequency Interference document for information about precautions to take.
boldBold text denotes items that you must select or click in the software, such
as menu items and dialog box options. Bold text also denotes parameter
names.
italicItalic text denotes variables, emphasis, a cross-reference, or an introduction
to a key concept. Italic text also denotes text that is a placeholder for a word
or value that you must supply.
monospaceText in this font denotes text or characters that you should enter from the
keyboard, sections of code, programming examples, and syntax examples.
This font is also used for the proper names of disk drives, paths, directories,
programs, subprograms, subroutines, device names, functions, operations,
variables, filenames, and extensions.
PlatformText in this font denotes a specific platform and indicates that the text
Each application software package and driver includes information about
writing applications for taking measurements and controlling measurement
devices. The following references to documents assume you have
NI-DAQmx 8.8 or later, and where applicable, version 7.1 or later of the
NI application software.
NI-DAQmx for Windows
The DAQ Getting Started Guide describes how to install your NI-DAQmx
for Windows software, how to install your NI-DAQmx-supported DAQ
device, and how to confirm that your device is operating properly. Select
Start»All Programs»National Instruments»NI-DAQ»DAQ Getting
Started Guide.
The NI-DAQ Readme lists which devices are supported by this version of
NI-DAQmx. Select Start»All Programs»National Instruments»NI-DAQ»NI-DAQ Readme.
The NI-DAQmx Help contains general information about measurement
concepts, key NI-DAQmx concepts, and common applications that are
applicable to all programming environments. Select Start»All Programs»National Instruments»NI-DAQ»NI-DAQmx Help.
LabVIEW
If you are a new user, use the Getting Started with LabVIEW manual to
familiarize yourself with the LabVIEW graphical programming
environment and the basic LabVIEW features you use to build data
acquisition and instrument control applications. Open the Getting Started
with LabVIEW manual by selecting Start»All Programs»National
Instruments»LabVIEW»LabVIEW Manuals or by navigating to the
labview\manuals directory and opening LV_Getting_Started.pdf.
Use the LabVIEW Help, available by selecting Help»Search the
LabVIEW Help in LabVIEW, to access information about LabVIEW
programming concepts, step-by-step instructions for using LabVIEW, and
reference information about LabVIEW VIs, functions, palettes, menus, and
tools. Refer to the following locations on the Contents tab of the LabVIEW Help for information about NI-DAQmx:
•Getting Started with LabVIEW»Getting Started with DAQ—
Includes overview information and a tutorial to learn how to take an
NI-DAQmx measurement in LabVIEW using the DAQ Assistant.
NI 6124/6154 User Manualxiini.com
•VI and Function Reference»Measurement I/O VIs and
•Taking Measurements—Contains the conceptual and how-to
LabWindows/CVI
The Data Acquisition book of the LabWindows/CVI Help contains
measurement concepts for NI-DAQmx. This book also contains Taking an NI-DAQmx Measurement in LabWindows/CVI, which includes
step-by-step instructions about creating a measurement task using the DAQ
Assistant. In LabWindows
Using LabWindows/CVI»Data Acquisition.
The NI-DAQmx Library book of the LabWindows/CVI Help contains
API overviews and function reference for NI-DAQmx. Select Library Reference»NI-DAQmx Library in the LabWindows/CVI Help.
Measurement Studio
If you program your NI-DAQmx-supported device in Measurement Studio
using Visual C++, Visual C#, or Visual Basic .NET, you can interactively
create channels and tasks by launching the DAQ Assistant from MAX or
from within Visual Studio .NET. You can generate the configuration code
based on your task or channel in Measurement Studio. Refer to the DAQ Assistant Help for additional information about generating code. You also
can create channels and tasks, and write your own applications in your
ADE using the NI-DAQmx API.
About This Manual
Functions—Describes the LabVIEW NI-DAQmx VIs and properties.
information you need to acquire and analyze measurement data in
LabVIEW, including common measurements, measurement
fundamentals, NI-DAQmx key concepts, and device considerations.
™
/CVI™, select Help»Contents, then select
For help with NI-DAQmx methods and properties, refer to the NI-DAQmx
.NET Class Library or the NI-DAQmx Visual C++ Class Library included
in the NI Measurement Studio Help. For general help with programming in
Measurement Studio, refer to the NI Measurement Studio Help, which is
fully integrated with the Microsoft Visual Studio .NET help. To view
this help file in Visual Studio. NET, select Measurement Studio»NI Measurement Studio Help.
To create an application in Visual C++, Visual C#, or Visual Basic .NET,
follow these general steps:
1.In Visual Studio .NET, select File»New»Project to launch the New
Project dialog box.
2.Find the Measurement Studio folder for the language you want to
create a program in.
3.Choose a project type. You add DAQ tasks as a part of this step.
ANSI C without NI Application Software
The NI-DAQmx Help contains API overviews and general information
about measurement concepts. Select Start»All Programs»National Instruments»NI-DAQ»NI-DAQmx Help.
The NI-DAQmx C Reference Help describes the NI-DAQmx Library
functions, which you can use with National Instruments data acquisition
devices to develop instrumentation, acquisition, and control applications.
Select Start»All Programs»National Instruments»NI-DAQ»NI-DAQmx C Reference Help.
.NET Languages without NI Application Software
With the Microsoft .NET Framework version 1.1 or later, you can use
NI-DAQmx to create applications using Visual C# and Visual Basic .NET
without Measurement Studio. You need Microsoft Visual Studio
.NET 2003 or Microsoft Visual Studio 2005 for the API documentation to
be installed.
The installed documentation contains the NI-DAQmx API overview,
measurement tasks and concepts, and function reference. This help is fully
integrated into the Visual Studio .NET documentation. To view the
NI-DAQmx .NET documentation, go to Start»Programs»National
Instruments»NI-DAQ»NI-DAQmx .NET Reference Help. Expand
NI Measurement Studio Help»NI Measurement Studio .NET Class
Library»Reference to view the function reference. Expand
NI Measurement Studio Help»NI Measurement Studio .NET Class
Library»Using the Measurement Studio .NET Class Libraries to view
conceptual topics for using NI-DAQmx with Visual C# and Visual Basic
.NET.
To get to the same help topics from within Visual Studio, go to Help»Contents. Select Measurement Studio from the Filtered By drop-down
list and follow the previous instructions.
NI 6124/6154 User Manualxivni.com
Device Documentation and Specifications
The NI 6124 Specifications and NI 6154 Specifications documents contain
all specifications for the NI 6124 and NI 6154 S Series devices respectively.
Documentation for supported devices and accessories, including PDF
and help files describing device terminals, specifications, features, and
operation are on the NI-DAQmx CD that includes Device Documentation.
Insert the CD, open the Device Documentation directory, and double-click
the Device Documents shortcut for your language to find, view, and print
device documents.
Training Courses
If you need more help getting started developing an application with
NI products, NI offers training courses. To enroll in a course or obtain a
detailed course outline, refer to
Technical Support on the Web
For additional support, refer to ni.com/support or zone.ni.com.
Note You can download these documents at ni.com/manuals.
About This Manual
ni.com/training.
DAQ specifications and some DAQ manuals are available as PDFs. You
must have Adobe Acrobat Reader with Search and Accessibility 5.0.5 or
later installed to view the PDFs. Refer to the Adobe Systems Incorporated
Web site at
National Instruments Product Manuals Library at
updated documentation resources.
www.adobe.com to download Acrobat Reader. Refer to the
ni.com/manuals for
Getting Started
The NI 6124 and NI 6154 are simultaneous sampling multifunction I/O
devices (S Series) that use the DAQ-STC2 ASIC.
The NI 6124 S Series is a non-isolated device featuring PXI Express
connectivity, four simultaneously sampling 16-bit analog inputs,
two 16-bit voltage analog outputs, 24 lines of bidirectional DIO,
and two general-purpose 32-bit counter/timers.
The NI 6154 S Series is an isolated PCI device featuring four isolated
differential 16-bit analog inputs, four isolated 16-bit analog outputs,
six DI lines, four DO lines, and two general-purpose 32-bit counter/timers.
If you have not already installed your device, refer to the DAQ Getting Started Guide. For specifications arranged by S Series device family, refer
to the specifications document for your device on
Before installing your DAQ device, you must install the software you plan
to use with the device.
1
ni.com/manuals.
Installing NI-DAQmx
The DAQ Getting Started Guide, which you can download at ni.com/
manuals, offers NI-DAQmx users step-by-step instructions for installing
software and hardware, configuring channels and tasks, and getting started
developing an application.
Installing Other Software
If you are using other software, refer to the installation instructions that
accompany your software.
The DAQ Getting Started Guide contains non-software-specific
information about how to install PCI and PXI Express devices, as well as
accessories and cables.
Device Self-Calibration
NI recommends that you self-calibrate your S Series device after
installation and whenever the ambient temperature changes.
Self-calibration should be performed after the device has warmed up for the
recommended time period. Refer to the device specifications to find your
device warm-up time. This function measures the onboard reference
voltage of the device and adjusts the self-calibration constants to account
for any errors caused by short-term fluctuations in the environment.
Disconnect all external signals when you self-calibrate a device.
You can initiate self-calibration using Measurement & Automation
Explorer (MAX), by completing the following steps.
1.Launch MAX.
2.Select My System»Devices and Interfaces»NI-DAQmx Devices»your device.
3.Initiate self-calibration using one of the following methods:
•Click Self-Calibrate in the upper right corner of MAX.
•Right-click the name of the device in the MAX configuration tree
and select Self-Calibrate from the drop-down menu.
Note You can also programmatically self-calibrate your device with NI-DAQmx,
as described in Device Calibration in the NI-DAQmx Help or the LabVIEW Help in
version 8.0 or later.
NI 6124/6154 User Manual1-2ni.com
Device Pinouts
Refer to Appendix A, Device-Specific Information, for NI 6124 and
NI 6154 device pinouts.
Device Specifications
Refer to the specifications for your device, the NI 6124 Specifications or
the NI 6154 Specifications, available on the NI-DAQ Device Document
Browser or
NI 6124 and NI 6154 devices.
Chapter 1Getting Started
ni.com/manuals, for more detailed information about the
Figure 2-1 shows a typical DAQ system setup, which includes transducers,
signal conditioning, cables that connect the various devices to the
accessories, the S Series device, and the programming software. Refer to
Appendix A, Device-Specific Information, for a list of devices and their
compatible accessories.
3
2
2
4
+
V
–
1
1 Sensors and Transducers
2 Signal Conditioning
3 Cable Assembly
DAQ hardware digitizes signals, performs D/A conversions to generate
analog output signals, and measures and controls digital I/O signals. The
following sections contain more information about specific components of
the DAQ hardware.
Figure 2-2 shows the components of the non-isolated S Series (NI 6124)
device.
Analog Input
Analog Output
Digital I/O
I/O Connector
Counters
PFI
Digital
Routing
RTSI
Figure 2-2. General NI 6124 Block Diagram
Bus
Interface
Bus
NI 6124/6154 User Manual2-2ni.com
Analog Input
Analog Output
Counters
I/O Connector
PFI/Static DI
Chapter 2DAQ System Overview
(NI 6154 Only) S Series isolated hardware also includes bank and
channel-to-channel isolation. Isolated DAQ hardware allows for increased
protection against hazardous voltages, rejection of common-mode
voltages, and reduction of ground loops and their associated noise.
Figure 2-3 shows the components of the isolated S Series (NI 6154) device.
A
Isolation
Barrier
AI GND
AO GND
P0.GND
A
A
Digital
Isolators
P0
Digital
Routing
RTSI
Bus
Interface
Bus
PFI/Static DO
P1.GND
P1
Figure 2-3. General NI 6154 Block Diagram
DAQ-STC2
The DAQ-STC2 implements a high-performance digital engine for
S Series data acquisition hardware. Some key features of this engine
include the following:
•Flexible AI and AO sample and convert timing
•Many triggering modes
•Independent AI, AO, DI, and DO FIFOs
•Generation and routing of RTSI signals for multi-device
synchronization
•Generation and routing of internal and external timing signals
•Two flexible 32-bit counter/timer modules with hardware gating
•Digital waveform acquisition and generation
•Static DIO signals
•True 5 V high current drive DO
•PLL for clock synchronization
•PCI/PXI interface
•Independent scatter-gather DMA controllers for all acquisition and
generation functions
Calibration Circuitry
Calibration is the process of making adjustments to a measurement device
to reduce errors associated with measurements. Without calibration, the
measurement results of your device will drift over time and temperature.
Calibration adjusts for these changes to improve measurement accuracy
and ensure that your product meets its required specifications.
DAQ devices have high precision analog circuits that must be adjusted to
obtain optimum accuracy in your measurements. Calibration determines
what adjustments these analog circuits should make to the device
measurements. During calibration, the value of a known, high precision
measurement source is compared to the value your device acquires or
generates. The adjustment values needed to minimize the difference
between the known and measured values are stored in the EEPROM of the
device as calibration constants. Before performing a measurement, these
constants are read out of the EEPROM and are used to adjust the calibration
hardware on the device. NI-DAQmx determines when this is necessary and
does it automatically. If you are not using NI-DAQmx, you must load these
values yourself.
You can calibrate S Series devices in two ways—through internal
(or self-calibration) or through external calibration.
Internal or Self-Calibration
Self-calibration is a process to adjust the device relative to a highly accurate
and stable internal reference on the device. Self-calibration is similar to the
autocalibration or autozero found on some instruments. You should
perform a self-calibration whenever environmental conditions, such as
ambient temperature, change significantly. To perform self-calibration, use
the self-calibrate function or VI that is included with your driver software.
Self-calibration requires no external connections.
NI 6124/6154 User Manual2-4ni.com
External Calibration
External calibration is a process to adjust the device relative to a traceable,
high precision calibration standard. The accuracy specifications of your
device change depending on how long it has been since your last external
calibration. National Instruments recommends that you calibrate your
device at least as often as the intervals listed in the accuracy specifications.
For a detailed calibration procedure for NI 6154 S Series devices, refer to
the Isolated M/S Series Calibration Procedure, which you can find at
ni.com/calibration and selecting Manual Calibration Procedures.
Signal Conditioning
Many sensors and transducers require signal conditioning before a
computer-based measurement system can effectively and accurately
acquire the signal. The front-end signal conditioning system can include
functions such as signal amplification, attenuation, filtering, electrical
isolation, simultaneous sampling, and multiplexing. In addition, many
transducers require excitation currents or voltages, bridge completion,
linearization, or high amplification for proper and accurate operation.
Therefore, most computer-based measurement systems include some form
of signal conditioning in addition to plug-in data acquisition DAQ devices.
Chapter 2DAQ System Overview
Sensors and Transducers
Sensors can generate electrical signals to measure physical phenomena,
such as temperature, force, sound, or light. Some commonly used sensors
are strain gages, thermocouples, thermistors, angular encoders, linear
encoders, and resistance temperature detectors (RTDs).
To measure signals from these various transducers, you must convert them
into a form that a DAQ device can accept. For example, the output voltage
of most thermocouples is very small and susceptible to noise. Therefore,
you may need to amplify or filter the thermocouple output before digitizing
it. The manipulation of signals to prepare them for digitizing is called
signal conditioning.
For more information about sensors, refer to the following documents.
•For general information about sensors, visit
•If you are using LabVIEW, refer to the LabVIEW Help by selecting
Help»Search the LabVIEW Help in LabVIEW and then navigate to
the Taking Measurements book on the Contents tab.
•If you are using other application software, refer to Common Sensors
in the NI-DAQmx Help or the LabVIEW Help in version 8.0 or later.
Programming Devices in Software
National Instruments measurement devices are packaged with NI-DAQmx
driver software, an extensive library of functions and VIs you can call from
your application software, such as LabVIEW or LabWindows/CVI, to
program all the features of your NI measurement devices. NI-DAQmx
driver software has an application programming interface (API), which is
a library of VIs, functions, classes, attributes, and properties for creating
applications for your device.
NI-DAQ includes two NI-DAQ drivers—Traditional NI-DAQ (Legacy) and
NI-DAQmx. DAQ-STC2-based S Series devices use the NI-DAQmx driver.
Each driver has its own API, hardware configuration, and software
configuration. Refer to the DAQ Getting Started Guide for more
information about the two drivers.
NI-DAQmx includes a collection of programming examples to help you get
started developing an application. You can modify example code and save
it in an application. You can use examples to develop a new application or
add example code to an existing application.
To locate LabVIEW and LabWindows/CVI examples, open the National
Instruments Example Finder. In LabVIEW and LabWindows/CVI, select
Help»Find Examples.
Measurement Studio, Visual Basic, and ANSI C examples are in the
following directories:
•NI-DAQmx examples for Measurement Studio-supported languages
are in the following directories:
–MeasurementStudio\VCNET\Examples\NIDaq
–MeasurementStudio\DotNET\Examples\NIDaq
•NI-DAQmx examples for ANSI C are in the NI-DAQ\Examples\
DAQmx ANSI C Dev
For additional examples, refer to
NI 6124/6154 User Manual2-6ni.com
directory
zone.ni.com.
3
I/O Connector
This chapter contains information about the S Series I/O connector. Refer
to one of the following sections, depending on your device:
•NI 6124 I/O Connector Signal Descriptions
•NI 6154 I/O Connector Signal Descriptions
Refer to Appendix A, Device-Specific Information, for the I/O connector
pinout for your device.
NI 6124 I/O Connector Signal Descriptions
(NI 6124 Only) Table 3-1 describes the signals found on the NI 6124 I/O
connector. For more information about these signals, refer to the NI 6124
Specifications.
P0.<0..7>D GNDInput or OutputDigital I/O Channels 0 through 7—You can
individually configure each signal as an input or output.
P0.6 and P0.7 can also control the up/down signal of
Counters 0 and 1, respectively.
PFI <0..7>/P1.<0..7>
PFI <8..15>/P2.<0..7>
+5 VD GNDOutput+5 Power Source—These pins provide +5 V power. For
D GNDInput or OutputProgrammable Function Interface or Digital I/O
Channels 0 through 7 and Channels 8 through
15—Each of these terminals can be individually
configured as a PFI terminal or a digital I/O terminal.
As an input, each PFI terminal can be used to supply an
external source for AI, AO, DI, and DO timing signals or
counter/timer inputs.
As a PFI output, you can route many different internal AI,
AO, DI, or DO timing signals to each PFI terminal. You
also can route the counter/timer outputs to each PFI
terminal.
As a Port 1 or Port 2 digital I/O signal, you can
individually configure each signal as an input or output.
more information, refer to the +5 V Power Source
section.
NI 6154 I/O Connector Signal Descriptions
(NI 6154 Only) Table 3-2 describes the signals found on the NI 6154 I/O
connector. For more information about these signals, refer to the NI 6154
Specifications.
Table 3-2. NI 6154 I/O Connector Signal Descriptions
PFI <0..5>/P0.<0..5>D GNDInputProgrammable Function Interface or Static Digital
Input Channels 0 to 5—Each of these terminals can be
individually configured as a PFI terminal or a digital input
terminal.
As an input, each PFI terminal can be used to supply an
external source for AI or AO timing signals or
counter/timer inputs.
Note: PFI <0..5>/P0.<0..5> are isolated from earth
ground and chassis ground.
PFI <6..9>/P1.<0..3>D GNDOutputProgrammable Function Interface or Static Digital
Output Channels 6 to 9—Each of these terminals can be
individually configured as a PFI terminal or a digital
output terminal.
As a PFI output, you can route many different internal AI
or AO timing signals to each PFI terminal. You also can
route the counter/timer outputs to each PFI terminal.
Note: PFI <6..9>/P1.<0..3> are isolated from earth
ground and chassis ground.
D GND——Digital Ground—D GND supplies the reference
for input PFI <0..5>/P0.<0..5> and output PFI <6..9>/
P1.<0..3>.
Note: D GND is isolated from earth ground and chassis
ground.
NC——No Connect—Do not connect signals to these terminals.
+5 V Power Source
(NI 6124 Only) The +5 V pins on the I/O connector supply +5 V power. You
can use these pins, referenced to D GND, to power external circuitry.
Power rating (most devices): +4.65 to +5.25 VDC at 1 A.
To find your device’s power rating, refer to the specifications document for
your device.
Caution Never connect these +5 V power pins to analog or digital ground or to any other
voltage source on the S Series device or any other device. Doing so can damage the device
and the computer. NI is not liable for damage resulting from such a connection.
On S Series devices, each channel uses its own instrumentation amplifier,
FIFO, multiplexer (mux), and A/D converter (ADC) to achieve
simultaneous data acquisition. The main blocks featured in the S Series
analog input circuitry are as follows:
•Mux—By default, the mux is set to route AI signals to the analog front
end. When you calibrate your device, the state of the mux switches.
You can manually switch the state of the mux to measure AI GND.
•Instrumentation Amplifier—The instrumentation amplifier can
amplify or attenuate an AI signal to ensure that you get the maximum
resolution of the ADC. Some S Series devices provide programmable
instrumentation amplifiers that allow you to select the input range.
•Analog Trigger—
circuitry of S Series devices, refer to the Analog Input Triggering
section.
•Filter—The filter on these S Series devices minimizes high frequency
noise and some attenuating signals by 3 dB at 2 MHz.
•ADC—The analog-to-digital converter (ADC) digitizes the AI signal
by converting the analog voltage into a digital number.
•AI Timing Signals—For information about the analog input timing
signals available on S Series devices, refer to the Analog Input Timing
Signals section.
•Isolation Barrier and Digital Isolators—
isolators across the isolation barrier provide a ground break between
the isolated analog front end and the chassis ground. For more
information about isolation and digital isolators, refer to the NI 6154
Isolation and Digital Isolators section of Appendix A, Device-Specific
Information.
•AI FIFO—A large first-in-first-out (FIFO) buffer, located inside the
FPGA, holds data during A/D conversions to ensure that no data is lost.
S Series devices can handle multiple A/D conversion operations with
DMA, interrupts, or programmed I/O.
(NI 6124 Only) For information about the trigger
(NI 6154 Only) The digital
Analog Input Terminal Configuration
S Series devices support only differential (DIFF) input mode. The channels
on S Series devices are true differential inputs, meaning both positive and
negative inputs can carry signals of interest. For more information about
DIFF input, refer to the Connecting Analog Input Signals section, which
contains diagrams showing the signal paths for DIFF input mode.
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Caution Exceeding the differential and common-mode input ranges distorts the input
signals. Exceeding the maximum input voltage rating can damage the device and the
computer. NI is not liable for any damage resulting from such signal connections. The
maximum input voltage ratings can be found in the specifications document for each
S Series device.
Input Polarity and Range
Input range refers to the set of input voltages that an analog input channel
can digitize with the specified accuracy. On some S Series devices, you can
individually program the input range of each AI channel.
The input range affects the resolution of the S Series device for an
AI channel. Resolution refers to the magnitude of one ADC code. For
example, a 16-bit ADC converts analog inputs into one of 65,536 (=2
codes, meaning one of 65,536 possible digital values. These values are
spread fairly evenly across the input range. So, for an input range of –5 V
to 5 V, the code width of a 16-bit ADC is:
5 V5 V–()–
--------------------------------153 μV=
16
2
Chapter 4Analog Input
16
)
S Series devices support bipolar input ranges. A bipolar input range means
that the input voltage range is between –V
and V
ref
.
ref
The instrumentation amplifier applies a different gain setting to the
AI signal depending on the input range. Gain refers to the factor by which
the instrumentation amplifier multiplies (amplifies) the input signal before
sending it to the ADC.
On S Series devices with programmable input ranges, choose an input
range that matches the expected input range of your signal. A large input
range can accommodate a large signal variation, but reduces the voltage
resolution. Choosing a smaller input range improves the voltage resolution,
but may result in the input signal going out of range. For more information
about programming these settings, refer to the NI-DAQmx Help or the
LabVIEW Help in version 8.0 or later.
On most S Series devices, the PGIA operates normally by amplifying
signals of interest while rejecting common-mode signals under the
following three conditions:
•The common-mode voltage (V
AI <0..x> GND from AI <0..x> –, must be less than ±10 V. This V
is a constant for all range selections.
•The signal voltage (V
from AI <0..x> –, must be less than or equal to the range selection of
the given channel. If V
clips and information are lost.
•The total working voltage of the positive input, which is equivalent to
(V
+ Vs), or subtracting AI <0..x> GND from AI <0..x> +, must be
cm
less than ±11 V.
If any of these conditions are exceeded, the input voltage is clamped until
the fault condition is removed.
Note All inputs are protected at up to ±35 V.
), which is equivalent to subtracting
cm
cm
), which is equivalent to subtracting AI <0..x>+
s
is greater than the range selected, the signal
s
(NI 6154 Only) The isolation features of the NI 6154 improve the working
voltage range in your applications. Refer to the NI 6154 Specifications for
more information.
AI Data Acquisition Methods
When performing analog input measurements, there are several different
data acquisition methods available. You can either perform software-timed
or hardware-timed acquisitions:
•Software-Timed Acquisitions—With a software-timed acquisition,
software controls the rate of the acquisition. Software sends a separate
command to the hardware to initiate each ADC conversion. In
NI-DAQmx, software-timed acquisitions are referred to as having On
Demand timing. Software-timed acquisitions are also referred to as
immediate or static acquisitions and are typically used for reading a
single point of data.
•Hardware-Timed Acquisitions—With hardware-timed acquisitions,
a digital hardware signal controls the rate of the acquisition. This
signal can be generated internally on your device or provided
externally.
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Chapter 4Analog Input
Hardware-timed acquisitions have several advantages over
software-timed acquisitions:
–The time between samples can be much shorter.
–The timing between samples can be deterministic.
–Hardware-timed acquisitions can use hardware triggering. For
more information, refer to Chapter 11, Triggering.
Hardware-timed operations can be buffered or non-buffered. A buffer
is a temporary storage in the computer memory where acquired
samples are stored.
–Buffered—In a buffered acquisition, data is moved from the DAQ
device’s onboard FIFO memory to a PC buffer using DMA or
interrupts before it is transferred to ADE memory. Buffered
acquisitions typically allow for much faster transfer rates than
non-buffered acquisitions because data is moved in large blocks,
rather than one point at a time. For more information about DMA
and interrupts, refer to the Data Transfer Methods section of
Chapter 10, Bus Interface.
One property of buffered I/O operations is the sample mode. The
sample mode can be either finite or continuous.
Finite sample mode acquisition refers to the acquisitions of a
specific, predetermined number of data samples. After the
specified number of samples has been collected into the buffer, the
acquisition stops. If you use a reference trigger, you must use
finite sample mode. Refer to the AI Reference Trigger Signal
section for more information.
Continuous acquisition refers to the acquisition of an unspecified
number of samples. Instead of acquiring a set number of data
samples and stopping, a continuous acquisition continues until
you stop the operation. A continuous acquisition is also referred
to as double-buffered or circular-buffered acquisition.
If data cannot be transferred across the bus fast enough, the data
in the FIFO will be overwritten and an error will be generated.
With continuous operations, if the user program does not read data
out of the PC buffer fast enough to keep up with the data transfer,
the buffer could reach an overflow condition, causing an error to
be generated.
–Non-Buffered—In non-buffered acquisitions, data is read directly
from the FIFO on the device. Typically, hardware-timed
non-buffered operations are used to read single samples with
known time increments between them and small latency.
Analog input supports two different triggering actions: start and reference.
An analog or digital hardware trigger can initiate these actions. All S Series
devices support digital triggering, and some also support analog triggering.
To find your device’s triggering options, refer to the specifications
document for your device.
The AI Start Trigger Signal and AI Reference Trigger Signal sections
contain information about the analog input trigger signals.
Refer to Chapter 11, Triggering, for more information about triggers.
Connecting Analog Input Signals
Table 4-1 summarizes the recommended input configuration for different
types of signal sources for S Series devices.
Table 4-1. S Series Analog Input Signal Configuration
Floating Signal Sources
(Not Connected to Earth Ground)
Ground-Referenced Signal Sources
Examples:
• Ungrounded thermocouples
• Signal conditioning with isolated
Example:
• Plug-in instruments with
non-isolated outputs
outputs
Input
NI 6124
Non-Isolated
Differential
(DIFF)
• Battery devices
+
V
1
–
AI 0+
AI 0–
R
AI GND
+
–
+
V
1
–
AI 0+
AI 0–
+
–
AI GND
NI 6154
Isolated
Differential
AI+
+
A I–
–
(DIFF)
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Isolation
+
Barrier
–
AI+
+
AI–
–
Isolation
+
Barrier
–
Refer to the Analog Input Terminal Configuration section for descriptions
of the input modes.
Types of Signal Sources
When configuring the input channels and making signal connections,
first determine whether the signal sources are floating or ground-referenced:
•Floating Signal Sources—A floating signal source is not connected in
any way to the building ground system, and instead has an isolated
ground-reference point. Some examples of floating signal sources are
outputs of transformers, thermocouples, battery-powered devices,
optical isolators, and isolation amplifiers. An instrument or device that
has an isolated output is a floating signal source. You must connect the
ground reference of a floating signal to the AI ground of the device to
establish a local or onboard reference for the signal. Otherwise, the
measured input signal varies as the source floats outside the
common-mode input range.
•Ground-Referenced Signal Sources—A ground-referenced signal
source is connected in some way to the building system ground and is,
therefore, already connected to a common ground point with respect to
the device, assuming that the computer is plugged into the same power
system as the source. Non-isolated outputs of instruments and devices
that plug into the building power system fall into this category.
The difference in ground potential between two instruments connected
to the same building power system is typically between 1 mV and
100 mV, but the difference can be much higher if power distribution
circuits are improperly connected. If a grounded signal source is
incorrectly measured, this difference can appear as measurement error.
Follow the connection instructions for grounded signal sources to
eliminate this ground potential difference from the measured signal.
Isolated devices have isolated front ends that are isolated from
ground-reference signal sources and are not connected to building
system grounds. Isolated devices require the user to provide a
ground-reference terminal to which its input signals are referenced.
Chapter 4Analog Input
Differential Connections for Ground-Referenced Signal Sources
Figure 4-6 shows how to connect a ground-referenced signal source to a
channel on a non-isolated S Series device.
Figure 4-3. Differential Connection for Ground-Referenced Signals
on Non-Isolated Devices
Figure 4-4 shows how to connect a ground-referenced signal source to a
channel on an isolated S Series device.
Isolated SSeries Device
AI 0+
AI 0–
AI 0 ConnectionsShown
Instrumentation
+
–
Amplifier
V
+
Measured
m
Voltage
–
Isolation
Barrier
Digital
Isolators
Figure 4-4. Differential Connection for Ground-Referenced Signals
on Isolated Devices
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Chapter 4Analog Input
With these types of connections, the instrumentation amplifier rejects both
the common-mode noise in the signal and the ground potential difference
between the signal source and the device ground, shown as V
in these
cm
figures.
Common-Mode Signal Rejection Considerations
The instrumentation amplifier can reject any voltage caused by ground
potential differences between the signal source and the device. In addition,
the instrumentation amplifier can reject common-mode noise pickup in the
leads connecting the signal sources to the device. The instrumentation
amplifier can reject common-mode signals as long as V+
and V–in (input
in
signals) are both within the working voltage range of the device.
Differential Connections for Non-Referenced or Floating Signal Sources
Figure 4-5 shows how to connect a floating signal source to a channel on a
non-isolated S Series device.
Non-Isolated SSeries Device
AI 0+
Floating
Signal
Source
+
V
s
–
Current
Return
Paths
Bias
Resistor
I/O Connector
AI 0–
Bias
AI 0 GND
AI 0 ConnectionsShown
Instrumentation
+
–
Amplifier
+
V
m
–
Measured
Voltage
Figure 4-5. Differential Connection for Non-Referenced Signals on
Figure 4-5 shows a bias resistor connected between AI 0 – and the floating
signal source ground. This resistor provides a return path for the bias
current. A value of 10 kΩ to 100 kΩ is usually sufficient. If you do not use
the resistor and the source is truly floating, the source is not likely to remain
within the common-mode signal range of the instrumentation amplifier, so
the instrumentation amplifier saturates, causing erroneous readings. You
must reference the source to the respective channel ground.
Figure 4-6 shows how to connect a floating signal source to a channel on
an isolated S Series device.
Floating
Signal
Source
Isolated SSeries Device
AI 0+
+
V
s
–
AI 0–
AI 0 ConnectionsShown
Instrumentation
Amplifier
+
–
+
V
m
–
Measured
Voltage
Isolation
Barrier
Digital
Isolators
Figure 4-6. Differential Connection for Non-Referenced Signals on Isolated Devices
DC-Coupled
You can connect low source impedance and high source impedance
DC-coupled sources:
•Low Source Impedance—You must reference the source to AI GND.
The easiest way to make this reference is to connect the positive side
of the signal to the positive input of the instrumentation amplifier and
connect the negative side of the signal to AI GND as well as to the
negative input of the instrumentation amplifier, without using resistors.
This connection works well for DC-coupled sources with low source
impedance (less than 100 Ω).
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Chapter 4Analog Input
•High Source Impedance—For larger source impedances, this
connection leaves the DIFF signal path significantly off balance. Noise
that couples electrostatically onto the positive line does not couple
onto the negative line because it is connected to ground. Hence, this
noise appears as a DIFF-mode signal instead of a common-mode
signal, and the instrumentation amplifier does not reject it. In this case,
instead of directly connecting the negative line to AI GND, connect the
negative line to AI GND through a resistor that is about 100 times the
equivalent source impedance. The resistor puts the signal path nearly
in balance, so that about the same amount of noise couples onto both
connections, yielding better rejection of electrostatically coupled
noise. This configuration does not load down the source (other than the
very high input impedance of the instrumentation amplifier).
You can fully balance the signal path by connecting another resistor of
the same value between the positive input and AI GND. This fully
balanced configuration offers slightly better noise rejection but has the
disadvantage of loading the source down with the series combination
(sum) of the two resistors. If, for example, the source impedance is
2kΩ and each of the two resistors is 100 kΩ, the resistors load down
the source with 200 kΩ and produce a –1% gain error.
AC-Coupled
Both inputs of the instrumentation amplifier require a DC path to ground in
order for the instrumentation amplifier to work. If the source is AC-coupled
(capacitively coupled), the instrumentation amplifier needs a resistor
between the positive input and AI GND. If the source has low-impedance,
choose a resistor that is large enough not to significantly load the source but
small enough not to produce significant input offset voltage as a result of
input bias current (typically 100 kΩ to 1 MΩ). In this case, connect the
negative input directly to AI GND. If the source has high output
impedance, balance the signal path as previously described using the same
value resistor on both the positive and negative inputs; be aware that there
is some gain error from loading down the source.
Field Wiring Considerations
Environmental noise can seriously affect the measurement accuracy of the
S Series device if you do not take proper care when running signal wires
between signal sources and the device. The following recommendations
apply mainly to AI signal routing, although they also apply to signal
routing in general.
Minimize noise pickup and maximize measurement accuracy by taking the
following precautions.
•Use differential AI connections to reject common-mode noise.
•Use individually shielded, twisted-pair wires to connect AI signals to
the device. With this type of wire, the signals attached to the AI + and
AI – inputs are twisted together and then covered with a shield. You
then connect this shield only at one point to the signal source ground.
This kind of connection is required for signals traveling through areas
with large magnetic fields or high electromagnetic interference.
•Route signals to the device carefully. Keep cabling away from noise
sources. The most common noise source in a PCI DAQ system is the
video monitor. Separate the monitor from the analog signals as far as
possible.
•Separate the signal lines of the S Series device from high-current or
high-voltage lines. These lines can induce currents in or voltages on
the signal lines of the S Series device if they run in close parallel paths.
To reduce the magnetic coupling between lines, separate them by a
reasonable distance if they run in parallel, or run the lines at right
angles to each other.
•Do not run signal lines through conduits that also contain power lines.
•Protect signal lines from magnetic fields caused by electric motors,
welding equipment, breakers, or transformers by running them through
special metal conduits.
Refer to the NI Developer Zone document, Field Wiring and Noise Considerations for Analog Signals, for more information.
Minimizing Drift in Differential Mode
If the readings from the DAQ device are random and drift rapidly, you
should check the ground-reference connections. The signal can be
referenced to a level that is considered floating with reference to the device
ground reference. Even though you are in DIFF mode, you must still
reference the signal to the same ground level as the device reference. There
are various methods of achieving this reference while maintaining a high
common-mode rejection ratio (CMRR). These methods are outlined in the
Connecting Analog Input Signals section.
AI GND is an AI common signal that routes directly to the ground
connection point on the devices. You can use this signal if you need a
general analog ground connection point to the device.
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Analog Input Timing Signals
An acquisition with posttrigger data allows you to view data that is
acquired after a trigger event is received. A typical posttrigger DAQ
sequence is shown in Figure 4-7. The sample counter is loaded with the
specified number of posttrigger samples, in this example, five. The value
decrements with each pulse on AI Sample Clock (ai/SampleClock), until
the value reaches zero and all desired samples have been acquired.
AI Start Trigger
AI Sample Clock
Chapter 4Analog Input
An acquisition with pretrigger data allows you to view data that is acquired
before the trigger of interest, in addition to data acquired after the trigger.
Figure 4-8 shows a typical pretrigger DAQ sequence. The AI Start Trigger
signal (ai/StartTrigger) can be either a hardware or software signal. If
AI Start Trigger is set up to be a software start trigger, an output pulse
appears on the AI START TRIG line when the acquisition begins. When the
AI Start Trigger pulse occurs, the sample counter is loaded with the number
of pretrigger samples, in this example, four. The value decrements with
each pulse on AI Sample Clock, until the value reaches zero. The sample
counter is then loaded with the number of posttrigger samples, in this
example, three.
If an AI Reference Trigger (ai/ReferenceTrigger) pulse occurs before the
specified number of pretrigger samples are acquired, the trigger pulse is
ignored. Otherwise, when the AI Reference Trigger pulse occurs, the
sample counter value decrements until the specified number of posttrigger
samples have been acquired. For more information about start and
reference triggers, refer to the Analog Input Triggering section.
In order to provide all of the timing functionality described throughout this
section, the DAQ-STC2 provides an extremely powerful and flexible
timing engine. For more information about all of the clock routing and
timing options that the analog input timing engine provides, refer to the
NI-DAQmx Help or the LabVIEW Help in version 8.0 or later.
S Series devices feature the following analog input timing signals:
•AI Sample Clock Signal
•AI Sample Clock Timebase Signal
•AI Convert Clock Signal
•AI Convert Clock Timebase Signal
•AI Hold Complete Event Signal
•AI Start Trigger Signal
•AI Reference Trigger Signal
AI Sample Clock Signal
Use the AI Sample Clock (ai/SampleClock) signal to initiate a set of
measurements. Your S Series device samples the AI signals of every
channel in the task once for every AI Sample Clock.
You can specify an internal or external source for AI Sample Clock. You
also can specify whether the measurement sample begins on the rising edge
or falling edge of AI Sample Clock.
Using an Internal Source
One of the following internal signals can drive AI Sample Clock:
•Counter n Internal Output
•AI Sample Clock Timebase (divided down)
•A pulse initiated by host software
A programmable internal counter divides down the sample clock timebase.
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Chapter 4Analog Input
Several other internal signals can be routed to AI Sample Clock through
RTS I. Refer to Device Routing in MAX in the NI-DAQmx Help or the
LabVIEW Help in version 8.0 or later for more information.
Using an External Source
Use one of the following external signals as the source of AI Sample Clock:
•PFI <0..15>
•RTSI <0..7>
•PXI_STAR
•Analog Comparison Event (an analog trigger)
Routing AI Sample Clock Signal to an Output
Terminal
You can route AI Sample Clock out to any PFI <0..15> or RTSI <0..7>
terminal. This pulse is always active high.
You can specify the output to have one of two behaviors. With the pulse
behavior, your DAQ device briefly pulses the PFI terminal once for every
occurrence of AI Sample Clock.
With level behavior, your DAQ device drives the PFI terminal high during
the entire sample.
All PFI terminals are configured as inputs by default.
Other Timing Requirements
A counter on your device internally generates AI Sample Clock unless you
select some external source. AI Start Trigger starts this counter and either
software or hardware can stop it once a finite acquisition completes. When
using an internally generated AI Sample Clock, you also can specify a
configurable delay from AI Start Trigger to the first AI Sample Clock
pulse. By default, this delay is set to two ticks of the AI Sample Clock
Timebase signal.
Figure 4-9 shows the relationship of AI Sample Clock to AI Start Trigger.
AI Sample Clock Timebase
Figure 4-9. AI Sample Clock and AI Start Trigger
AI Sample Clock Timebase Signal
You can route any of the following signals to be the AI Sample Clock
Timebase (ai/SampleClockTimebase) signal:
•20 MHz Timebase
•100 kHz Timebase
•PXI_CLK10
•RTSI <0..7>
•PFI <0..15>
•PXI_STAR
•Analog Comparison Event (an analog trigger)
AI Start Trigger
AI Sample Clock
Delay
From
Start
Trigger
AI Sample Clock Timebase is not available as an output on the
I/O connector. AI Sample Clock Timebase is divided down to provide one
of the possible sources for AI Sample Clock. You can configure the polarity
selection for AI Sample Clock Timebase as either rising or falling edge.
AI Convert Clock Signal
Use the AI Convert Clock (ai/ConvertClock) signal to initiate a single A/D
conversion on every channel.
You can specify either an internal or external signal as the source of
AI Convert Clock. You also can specify whether the measurement sample
begins on the rising edge or falling edge of AI Convert Clock.
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Chapter 4Analog Input
Using an Internal Source
One of the following internal signals can drive AI Convert Clock:
•AI Convert Clock Timebase (divided down)
•Counter n Internal Output
A programmable internal counter divides down the AI Convert Clock
Timebase to generate AI Convert Clock. The counter is started by
AI Sample Clock and continues to count down to zero, produces an
AI Convert Clock, reloads itself, and repeats the process until the sample is
finished. It then reloads itself in preparation for the next AI Sample Clock
pulse.
Using an External Source
Use one of the following external signals as the source of AI Convert
Clock:
•PFI <0..15>
•RTSI <0..7>
•PXI_STAR
•Analog Comparison Event (an analog trigger)
Routing AI Convert Clock Signal to an Output
Terminal
You can route AI Convert Clock (as an active low signal) out to any
PFI <0..15> or RTSI <0..7> terminal.
All PFI terminals are configured as inputs by default.
AI Convert Clock Timebase Signal
The AI Convert Clock Timebase (ai/ConvertClockTimebase) signal is
divided down to provide on of the possible sources for AI Convert Clock.
Use one of the following signals as the source of AI Convert Clock
Timebase:
•AI Sample Clock Timebase
•20 MHz Timebase
AI Convert Clock Timebase is not available as an output on the I/O
connector.
The AI Hold Complete Event (ai/HoldCompleteEvent) signal
generates a pulse after each A/D conversion begins. You can route
ai/HoldCompleteEvent out to any PFI <0..15> or RTSI <0..7> terminal.
The polarity of ai/HoldCompleteEvent is software-selectable, but is
typically configured so that a low-to-high leading edge can clock external
AI multiplexers indicating when the input signal has been sampled and can
be removed.
AI Start Trigger Signal
Use the AI Start Trigger (ai/StartTrigger) signal to begin a measurement
acquisition. A measurement acquisition consists of one or more samples.
If you do not use triggers, begin a measurement with a software command.
Once the acquisition begins, configure the acquisition to stop:
•When a certain number of points are sampled (in finite mode)
•After a hardware reference trigger (in finite mode)
•With a software command (in continuous mode)
An acquisition that uses a start trigger (but not a reference trigger) is
sometimes referred to as a posttriggered acquisition.
Using a Digital Source
To use AI Start Trigger with a digital source, specify a source and an edge.
The source can be any of the following signals:
•PFI <0..15>
•RTSI <0..7>
•Counter n Internal Output
•PXI_STAR
The source also can be one of several other internal signals on your DAQ
device. Refer to Device Routing in MAX in the NI-DAQmx Help or the
LabVIEW Help in version 8.0 or later for more information.
You also can specify whether the measurement acquisition begins on the
rising edge or falling edge of AI Start Trigger.
NI 6124/6154 User Manual4-18ni.com
Using an Analog Source
When you use an analog trigger source, the acquisition begins on the
first rising edge of the Analog Comparison Event signal.
Routing AI Start Trigger to an Output Terminal
You can route AI Start Trigger out to any PFI <0..15> or RTSI <0..7>
terminal. The output is an active high pulse. All PFI terminals are
configured as inputs by default.
The device also uses AI Start Trigger to initiate pretriggered DAQ
operations. In most pretriggered applications, a software trigger generates
AI Start Trigger. Refer to the AI Reference Trigger Signal section for a
complete description of the use of AI Start Trigger and AI Reference
Trigger in a pretriggered DAQ operation.
AI Reference Trigger Signal
Use AI Reference Trigger (ai/ReferenceTrigger) signal to stop a
measurement acquisition. To use a reference trigger, specify a buffer of
finite size and a number of pretrigger samples (samples that occur before
the reference trigger). The number of posttrigger samples (samples that
occur after the reference trigger) desired is the buffer size minus the
number of pretrigger samples.
Chapter 4Analog Input
Once the acquisition begins, the DAQ device writes samples to the buffer.
After the DAQ device captures the specified number of pretrigger samples,
the DAQ device begins to look for the reference trigger condition. If the
reference trigger condition occurs before the DAQ device captures the
specified number of pretrigger samples, the DAQ device ignores the
condition.
If the buffer becomes full, the DAQ device continuously discards the oldest
samples in the buffer to make space for the next sample. This data can be
accessed (with some limitations) before the DAQ device discards it. Refer
to the KnowledgeBase document, Can a Pretriggered Acquisition be Continuous?, for more information. To access this KnowledgeBase, go to
When the reference trigger occurs, the DAQ device continues to write
samples to the buffer until the buffer contains the number of posttrigger
samples desired. Figure 4-10 shows the final buffer.
Reference Trigger
Pretrigger Samples
lete Buffer
Com
Figure 4-10. Reference Trigger Final Buffer
Using a Digital Source
To use AI Reference Trigger with a digital source, specify a source and an
edge. The source can be any of the following signals:
•PFI <0..15>
•RTSI <0..7>
•PXI_STAR
The source also can be one of several internal signals on your DAQ device.
Refer to Device Routing in MAX in the NI-DAQmx Help or the LabVIEW Help in version 8.0 or later for more information.
You also can specify whether the measurement acquisition stops on the
rising edge or falling edge of AI Reference Trigger.
Using an Analog Source
When you use an analog trigger source, the acquisition stops on the
first rising edge of the Analog Comparison Event signal.
Routing AI Reference Trigger Signal to an Output
Terminal
You can route AI Reference Trigger out to any PFI <0..15> or RTSI <0..7>
terminal.
All PFI terminals are configured as inputs by default.
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Chapter 4Analog Input
Getting Started with AI Applications in Software
You can use the S Series device in the following analog input applications:
•Simultaneous sampling
•Single-point analog input
•Finite analog input
•Continuous analog input
You can perform these applications through DMA, interrupt, or
programmed I/O data transfer mechanisms. Some of the applications also
use start and reference pause triggers.
Note For more information about programming analog input applications and triggers in
software, refer to the NI-DAQmx Help or the LabVIEW Help in version 8.0 or later.
The main blocks featured in the S Series analog output circuitry are as
follows:
•AO FIFO—The AO FIFO enables analog output waveform
generation. It is a first-in-first-out (FIFO) memory buffer between the
computer and the DACs that allows you to download all the points of
a waveform to your board without host computer interaction.
•AO Sample Clock—The DAC reads a sample from the FIFO with
every cycle of the AO Sample Clock signal and generates the AO
voltage. For more information, refer to the AO Sample Clock Signal
section.
•Isolation Barrier and Digital Isolators—
isolators across the isolation barrier provide a ground break between
the isolated analog front end and the chassis ground. For more
information about isolation and digital isolators, refer to the NI 6154
Isolation and Digital Isolators section of Appendix A, Device-Specific
Information.
•DAC—Digital-to-analog converters (DACs) convert digital codes to
analog voltages.
Minimizing Glitches on the Output Signal
(NI 6154 Only) The digital
When you use a DAC to generate a waveform, you may observe glitches
on the output signal. These glitches are normal; when a DAC switches from
one voltage to another, it produces glitches due to released charges. The
largest glitches occur when the most significant bit (MSB) of the DAC code
switches. You can build a lowpass deglitching filter to remove some of
these glitches, depending on the frequency and nature of the output signal.
Visit
ni.com/support for more information about minimizing glitches.
AO Data Generation Methods
When performing an analog output operation, there are several different
data generation methods available. You can either perform software-timed
or hardware-timed generations:
•Software-Timed Generations—With a software-timed generation,
software controls the rate at which data is generated. Software sends a
separate command to the hardware to initiate each DAC conversion. In
NI-DAQmx, software-timed generations are referred to as On Demand
timing. Software-timed generations are also referred to as immediate
or static operations. They are typically used for writing a single value
out, such as a constant DC voltage.
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Chapter 5Analog Output
•Hardware-Timed Generations—With a hardware-timed generation,
a digital hardware signal controls the rate of the generation. This signal
can be generated internally on your device or provided externally.
Hardware-timed generations have several advantages over
software-timed generations:
–The time between samples can be much shorter.
–The timing between samples can be deterministic.
–Hardware-timed generations can use hardware triggering. For
more information, refer to Chapter 11, Triggering.
Hardware-timed operations can be buffered or non-buffered. A buffer
is a temporary storage in computer memory for acquired or
to-be-generated samples.
–Buffered—In a buffered generation, data is moved from a PC
buffer to the DAQ device’s onboard FIFO using DMA or
interrupts before it is written to the DACs one sample at a time.
Buffered generations typically allow for much faster transfer rates
than non-buffered generations because data is moved in large
blocks, rather than one point at a time. For more information about
DMA and interrupts, refer to the Data Transfer Methods section
of Chapter 10, Bus Interface.
One property of buffered I/O operations is the sample mode. The
sample mode can be either finite or continuous.
Finite sample mode generation refers to the generation of a
specific, predetermined number of data samples. When the
specified number of samples has been written out, the generation
stops.
Continuous generation refers to the generation of an unspecified
number of samples. Instead of generating a set number of data
samples and stopping, a continuous generation continues until
you stop the operation. There are several different methods of
continuous generation that control what data is written. These
methods are regeneration, FIFO regeneration and
non-regeneration modes.
Regeneration is the repetition of the data that is already in the
buffer. Standard regeneration is when data from the PC buffer is
continually downloaded to the FIFO to be written out. New data
can be written to the PC buffer at any time without disrupting the
output.
With FIFO regeneration, the entire buffer is downloaded to the
FIFO and regenerated from there. After the data is downloaded,
new data cannot be written to the FIFO. To use FIFO regeneration,
the entire buffer must fit within the FIFO size. The advantage of
using FIFO regeneration is that it does not require communication
with the main host memory after the operation is started, thereby
preventing any problems that may occur due to excessive bus
traffic.
With non-regeneration, old data will not be repeated. New data
must be continually written to the buffer. If the program does not
write new data to the buffer at a fast enough rate to keep up with
the generation, the buffer will underflow and cause an error.
data is written directly to the FIFO on the device. Typically,
hardware-timed non-buffered operations are used to write single
samples with known time increments between them and good
latency.
Analog Output Triggering
Analog output supports two different triggering actions: start and pause. An
analog or digital hardware trigger can initiate these actions. All S Series
devices support digital triggering, and some also support analog triggering.
To find your device’s triggering options, refer to the specifications
document for your device.
The AO Start Trigger Signal and AO Pause Trigger Signal sections contain
information about the analog output trigger signals.
Refer to Chapter 11, Triggering, for more information about triggers.
Connecting Analog Output Signals
The AO signals are AO 0, AO 1, and AO GND. AO 0 is the voltage output
signal for AO channel 0. AO 1 is the voltage output signal for
AO channel 1. AO GND is the ground reference for the AO channels.
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Chapter 5Analog Output
Figure 5-3 shows how AO 0 and AO 1 are wired on a non-isolated S Series
device.
AO 0
+
Load
Load
VOUT 0
VOUT 1
–
–
+
AO GND
AO 1
Non-Isolated SSeries Device
Figure 5-3. Analog Output Connections for Non-Isolated S Series Devices
Channel 0
Channel 1
Analog Output Channels
Figure 5-4 shows how AO 0 is wired on an isolated S Series device.
Isolation
AO+
DAC
Lo
ad
VOUT
+
Analog Output Channel
–
AO–
Isolated SSeries Device
Figure 5-4. Analog Output Connections for Isolated S Series Devices
There is one AO Sample Clock that causes all AO channels to update
simultaneously. Figure 5-5 summarizes the timing and routing options
provided by the analog output timing engine.
RTSI 7
20 MHz
Timebase
Master
Timebase
Onboard
Clock
÷200
S Series devices feature the following waveform generation timing signals:
•AO Sample Clock Signal
•AO Sample Clock Timebase Signal
•AO Start Trigger Signal
•AO Pause Trigger Signal
AO Sample Clock Signal
You can use the AO Sample Clock (ao/SampleClock) signal to initiate
AO samples. Each sample updates the outputs of all of the DACs.
The source of the AO Sample Clock signal can be internal or external. You
can specify whether the DAC update begins on the rising edge or falling
edge of the AO Sample Clock signal.
Onboard
Clock
Divisor
Ctr1InternalOutput
PFI 0–9,
RTSI 0–6
÷
PFI 0–9,
RTSI 0–6
ao/SampleClock
Timebase
Figure 5-5. Analog Output Engine Routing Options
ao/SampleClock
Using an Internal Source
By default, AO Sample Clock is created internally by dividing down the
AO Sample Clock Timebase signal.
Several other internal signals can be routed to the sample clock. Refer to
Device Routing in MAX in the NI-DAQmx Help or the LabVIEW Help in
version 8.0 or later for more information.
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Chapter 5Analog Output
Using an External Source
You can use a signal connected to any PFI or RTSI <0..6> pin as the source
of AO Sample Clock. Figure 5-6 shows the timing requirements of the
AO Sample Clock source.
t
w
Rising-Edge
Polarity
Falling-Edge
Polarity
t
= 10 ns minimum
w
Figure 5-6. AO Sample Clock Timing Requirements
Routing AO Sample Clock Signal to an Output
Terminal
You can route ao/SampleClock (as an active low signal) out to any
PFI <0..15> or RTSI <0..7> terminal.
Other Timing Requirements
A counter on your device internally generates AO Sample Clock unless you
select some external source. The AO Start Trigger signal starts this counter.
It is stopped automatically by hardware after a finite acquisition completes
or manually through software. When using an internally generated
AO Sample Clock in NI-DAQmx, you can also specify a configurable
delay from the AO Start Trigger to the first AO Sample Clock pulse. By
default, this delay is two ticks of the AO Sample Clock Timebase signal.
Figure 5-7 shows the relationship of the AO Sample Clock signal to the
AO Start Trigger signal.
AO Sample Clock Timebase
AO Start Trigger
AO Sample Clock
Figure 5-7. AO Sample Clock and AO Start Trigger
AO Sample Clock Timebase Signal
You can select any PFI or RTSI pin as well as many other internal signals
as the AO Sample Clock Timebase (ao/SampleClockTimebase) signal.
This signal is not available as an output on the I/O connector. AO Sample
Clock Timebase is divided down to provide the Onboard Clock source for
the AO Sample Clock. You specify whether the samples begin on the rising
or falling edge of AO Sample Clock Timebase.
Delay
From
Start
Trigger
You might use the AO Sample Clock Timebase signal if you want to use an
external sample clock signal, but need to divide the signal down. If you
want to use an external sample clock signal, but do not need to divide the
signal, then you should use the AO Sample Clock signal rather than the
AO Sample Clock Timebase. If you do not specify an external sample clock
timebase, NI-DAQmx uses the Onboard Clock.
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Figure 5-8 shows the timing requirements for the AO Sample Clock
Timebase signal.
The maximum allowed frequency is 20 MHz, with a minimum pulse width
of 10 ns high or low. There is no minimum frequency.
Unless you select an external source, either the 20MHzTimebase or
100kHzTimebase generates the AO Sample Clock Timebase signal.
AO Start Trigger Signal
You can use the AO Start Trigger signal (ao/StartTrigger) to initiate a
waveform generation. If you do not use triggers, you begin a generation
with a software command.
Chapter 5Analog Output
t
p
t
t
w
w
tp = 50 ns minimum
t
= 23 ns minimum
w
Figure 5-8. AO Sample Clock Timebase Timing Requirements
Using a Digital Source
To use AO Start Trigger, specify a source and an edge. The source can be
an external signal connected to any PFI or RTSI <0..6> pin. The source can
also be one of several internal signals on your DAQ device. Refer to Device Routing in MAX in the NI-DAQmx Help or the LabVIEW Help in
version 8.0 or later for more information.
Figure 5-9 shows the timing requirements of the AO Start Trigger digital
source.
t
w
Rising-Edge
Polarity
Falling-Edge
Polarity
tw = 10 ns minimum
Figure 5-9. AO Start Trigger Timing Requirements
Using an Analog Source
When you use an analog trigger source, the waveform generation begins on
the first rising edge of the Analog Comparison Event signal. For more
information, refer to the Triggering with an Analog Source section of
Chapter 11, Triggering.
Routing AO Start Trigger Signal to an Output
Terminal
You can route ao/StartTrigger out to any PFI <0..15> or RTSI <0..7>
terminal.
The output is an active high pulse.
PFI terminals are configured as inputs by default.
AO Pause Trigger Signal
You can use the AO Pause Trigger signal (ao/PauseTrigger) to mask off
samples in a DAQ sequence. That is, when AO Pause Trigger is active,
no samples occur.
The AO Pause Trigger does not stop a sample that is in progress. The pause
does not take effect until the beginning of the next sample. This signal is
not available as an output.
NI 6124/6154 User Manual5-10ni.com
Chapter 5Analog Output
Using a Digital Source
To use ao/Pause Trigger, specify a source and a polarity. The source can be
an external signal connected to any PFI or RTSI <0..6> pin. The source can
also be one of several other internal signals on your DAQ device. Refer to
Device Routing in MAX in the NI-DAQmx Help or the LabVIEW Help in
version 8.0 or later for more information.
Also, specify whether the samples are paused when AO Pause Trigger is at
a logic high or low level.
Using an Analog Source
When you use an analog trigger source, the samples are paused when the
Analog Comparison Event signal is at a high level. For more information,
refer to the Triggering with an Analog Source section of Chapter 11,
Triggering.
Getting Started with AO Applications in Software
You can use the S Series device in the following analog output
applications:
•Single-point generation
•Finite generation
•Continuous generation
•Waveform generation
You can perform these generations through DMA, interrupt, or
programmed I/O data transfer mechanisms. Some of the applications also
use start triggers and pause triggers.
Note For more information about programming analog output applications and triggers in
software, refer to the NI-DAQmx Help or the LabVIEW Help in version 8.0 or later.
Refer to one of the following sections, depending on your device:
•Digital I/O for Non-Isolated Devices—NI 6124 devices have eight
lines of bidirectional DIO lines on Port 0, and 16 PFI signals that can
function as static DIO lines.
•Digital I/O for Isolated Devices—NI 6154 devices have six
bank-isolated digital inputs and four bank-isolated digital outputs.
Digital I/O for Non-Isolated Devices
(NI 6124 Only) NI 6124 devices contain eight lines of bidirectional DIO lines
on Port 0. In addition, The NI 6124 has 16 PFI lines that can function as
static DIO lines.
These S Series devices support the following DIO features on Port 0:
•Eight lines of DIO
•Direction and function of each terminal individually controllable
Figure 6-1 shows the circuitry of one DIO line. Each DIO line is similar.
The following sections provide information about the various parts of the
DIO circuit.
DO Waveform
Generation FIFO
Static DO
Buffer
DO.x Direction Control
I/O Protection
P0.x
Static DI
DI Waveform
Measurement
FIFO
DI Sample Clock
DI Change
Detection
Figure 6-1. Non-Isolated S Series Digital I/O Circuitry
The DIO terminals are named P0.<0..7> on the device I/O connector.
The voltage input and output levels and the current drive levels of the DIO
lines are listed in the specifications of your device.
Static DIO for Non-Isolated Devices
(NI 6124 Only) Each DIO line can be used as a static DI or DO line. You can
use static DIO lines to monitor or control digital signals. Each DIO can be
individually configured as a digital input (DI) or digital output (DO).
All samples of static DI lines and updates of DO lines are software-timed.
Weak Pull-Down
P0.6 and P0.7 on these devices also can control the up/down input of
general-purpose counters 0 and 1, respectively. However, it is
recommended that you use PFI signals to control the up/down input of the
counters. The up/down control signals, Counter 0 Up_Down and Counter 1
Up_Down, are input-only and do not affect the operation of the DIO lines.
NI 6124/6154 User Manual6-2ni.com
Digital Waveform Triggering for Non-Isolated Devices
(NI 6124 Only) NI 6124 devices do not have an independent DI or DO Start
Trigger for digital waveform acquisition or generation. To trigger a DI or
DO operation, first select a signal to be the source of DI Sample Clock or
DO Sample Clock. Then, generate a trigger that initiates pulses on the
source signal. The method for generating this trigger depends on which
signal is the source of DI Sample Clock or DO Sample Clock.
For example, consider the case where you are using AI Sample Clock as the
source of DI Sample Clock. To initiate pulses on AI Sample Clock (and
therefore on DI Sample Clock), you use AI Start Trigger to trigger the start
of an AI operation. The AI Start Trigger causes the non-isolated
DAQ-STC2 S Series device to begin generating AI Sample clock pulses,
which in turn generates DI Sample clock pulses, as shown in Figure 6-2.
Chapter 6Digital I/O
(AI Start Trigger)
PFI 1
AI Sample Clock
DI Sample Clock
AI Start Trigger initiates
AI Sample Clock and DI Sample Clock.
Figure 6-2. Digital Waveform Triggering
Similarly, if you are using AO Sample Clock as the source of DI Sample
Clock, then AO Start Trigger initiates both AO and DI operations.
If you are using a Counter output as the source of DI Sample Clock, the
counter’s start trigger, enables the counter which drives DI Sample Clock.
If you are using an external signal (such as PFI x) as the source for
DI Sample Clock or DO Sample Clock, you must trigger that external
signal.
Digital Waveform Acquisition for Non-Isolated Devices
(NI 6124 Only) You can acquire digital waveforms on the Port 0 DIO lines.
The DI waveform acquisition FIFO stores the digital samples. S Series
devices have a DMA controller dedicated to moving data from the
DI waveform acquisition FIFO to system memory. The DAQ device
samples the DIO lines on each rising or falling edge of a clock signal,
DI Sample Clock.
You can configure each DIO line to be an output, a static input, or a digital
waveform acquisition input.
DI Sample Clock Signal
(NI 6124 Only) Use the DI Sample Clock (di/SampleClock) signal to sample
the P0.<0..7> terminals and store the result in the DI waveform acquisition
FIFO. These S Series devices do not have the ability to divide down a
timebase to produce an internal DI Sample Clock for digital waveform
acquisition. Therefore, you must route an external signal or one of many
internal signals from another subsystem to be the DI Sample Clock. For
example, you can correlate digital and analog samples in time by sharing
your AI Sample Clock or AO Sample Clock as the source of your
DI Sample Clock. To sample a digital signal independent of an AI, AO,
or DO operation, you can configure a counter to generate the desired
DI Sample Clock or use an external signal as the source of the clock.
If the DAQ device receives a DI Sample Clock when the FIFO is full,
it reports an overflow error to the host software.
Using an Internal Source
To use DI Sample Clock with an internal source, specify the signal source
and the polarity of the signal. The source can be any of the following
signals:
•AI Sample Clock (ai/SampleClock)
•AI Convert Clock (ai/ConvertClock)
•AO Sample Clock (ao/SampleClock)
•Counter n Internal Output
•Frequency Output
•DI Change Detection Output
Several other internal signals can be routed to DI Sample Clock through
RTS I. Refer to Device Routing in MAX in the NI-DAQmx Help or the
LabVIEW Help in version 8.0 or later for more information.
Using an External Source
You can route any of the following signals as DI Sample Clock:
•PFI <0..15>
•RTSI <0..7>
NI 6124/6154 User Manual6-4ni.com
•PXI_STAR
•Analog Comparison Event (an analog trigger)
You can sample data on the rising or falling edge of DI Sample Clock.
Routing DI Sample Clock to an Output Terminal
You can route DI Sample Clock out to any PFI terminal. The PFI circuitry
inverts the polarity of DI Sample Clock before driving the PFI terminal.
Digital Waveform Generation for Non-Isolated Devices
(NI 6124 Only) You can generate digital waveforms on the Port 0 DIO lines.
The DO waveform generation FIFO stores the digital samples. These
S Series devices have a DMA controller dedicated to moving data from the
system memory to the DO waveform generation FIFO. The DAQ device
moves samples from the FIFO to the DIO terminals on each rising or falling
edge of a clock signal, DO Sample Clock. You can configure each DIO
signal to be an input, a static output, or a digital waveform generation
output.
The FIFO supports a retransmit mode. In the retransmit mode, after all the
samples in the FIFO have been clocked out, the FIFO begins outputting all
of the samples again in the same order. For example, if the FIFO contains
five samples, the pattern generated consists of sample #1, #2, #3, #4, #5,
#1, #2, #3, #4, #5, #1, and so on.
Chapter 6Digital I/O
DO Sample Clock Signal
(NI 6124 Only) Use the DO Sample Clock (do/SampleClock) signal to update
the DO terminals with the next sample from the DO waveform generation
FIFO. These S Series devices do not have the ability to divide down a
timebase to produce an internal DO Sample Clock for digital waveform
generation. Therefore, you must route an external signal or one of many
internal signals from another subsystem to be the DO Sample Clock. For
example, you can correlate digital and analog samples in time by sharing
your AI Sample Clock or AO Sample Clock as the source of your
DO Sample Clock. To generate digital data independent of an AI, AO,
or DI operation, you can configure a counter to generate the desired
DO Sample Clock or use an external signal as the source of the clock.
If the DAQ device receives a DO Sample Clock when the FIFO is empty,
the DAQ device reports an underflow error to the host software.
To use DO Sample Clock with an internal source, specify the signal source
and the polarity of the signal. The source can be any of the following
signals:
•AI Sample Clock (ai/SampleClock)
•AI Convert Clock (ai/ConvertClock)
•AO Sample Clock (ao/SampleClock)
•Counter n Internal Output
•Frequency Output
•DI Change Detection Output
Several other internal signals can be routed to DO Sample Clock through
RTS I. Refer to Device Routing in MAX in the NI-DAQmx Help or the
LabVIEW Help in version 8.0 or later for more information.
Using an External Source
You can route any of the following signals as DO Sample Clock:
•PFI <0..15>
•RTSI <0..7>
•PXI_STAR
•Analog Comparison Event (an analog trigger)
You can generate samples on the rising or falling edge of DO Sample
Clock.
You must ensure that the time between two active edges of DO Sample
Clock is not too short. If the time is too short, the DO waveform generation
FIFO is not able to read the next sample fast enough. The DAQ device
reports an overrun error to the host software.
Routing DO Sample Clock to an Output Terminal
You can route DO Sample Clock out to any PFI terminal. The PFI circuitry
inverts the polarity of DO Sample Clock before driving the PFI terminal.
NI 6124/6154 User Manual6-6ni.com
I/O Protection for Non-Isolated Devices
(NI 6124 Only) Each DIO and PFI signal is protected against overvoltage,
undervoltage, and overcurrent conditions as well as ESD events. However,
you should avoid these fault conditions by following these guidelines:
•If you configure a PFI or DIO line as an output, do not connect it to any
external signal source, ground, or power supply.
•If you configure a PFI or DIO line as an output, understand the current
requirements of the load connected to these signals. Do not exceed the
specified current output limits of the DAQ device. NI has several signal
conditioning solutions for digital applications requiring high current
drive.
•If you configure a PFI or DIO line as an input, do not drive the line with
voltages outside of its normal operating range. The PFI or DIO lines
have a smaller operating range than the AI signals.
•Treat the DAQ device as you would treat any static sensitive device.
Always properly ground yourself and the equipment when handling
the DAQ device or connecting to it.
Programmable Power-Up States for Non-Isolated Devices
(NI 6124 Only) At system startup and reset, the hardware sets all PFI and DIO
lines to high-impedance inputs by default. The DAQ device does not drive
the signal high or low. Each line has a weak pull-down resistor connected
to it, as described in the specifications document for your device.
Chapter 6Digital I/O
NI-DAQmx supports programmable power-up states for PFI and DIO lines.
Software can program any value at power up to the P0, P1, or P2 lines. The
PFI and DIO lines can be set as:
•A high-impedance input with a weak pull-down resistor (default)
•An output driving a 0
•An output driving a 1
Refer to the NI-DAQmx Help or the LabVIEW Help in version 8.0 or later
for more information about setting power-up states in NI-DAQmx or MAX.
Note When using your S Series device to control an SCXI chassis, DIO lines 0, 1, 2, and
4 are used as communication lines and must be left to power-up in the default
high-impedance state to avoid potential damage to these signals.
(NI 6124 Only) You can configure the DAQ device to detect changes in the
DIO signals. Figure 6-3 shows a block diagram of the DIO change
detection circuitry.
P0.0
P0.7
Synch
Synch
Enable
Enable
Change Detection Event
Enable
Enable
Figure 6-3. DI Change Detection
You can enable the DIO change detection circuitry to detect rising edges,
falling edges, or either edge individually on each DIO line. The DAQ
devices synchronize each DI signal to 80MHzTimebase, and then sends the
signal to the change detectors. The circuitry ORs the output of all enabled
change detectors from every DI signal. The result of this OR is the Change
Detection Event signal.
The Change Detection Event signal can do the following:
•Drive any RTSI <0..7>, PFI <0..15>, or PXI_STAR signal
•Drive the DO Sample Clock or DI Sample Clock
•Generate an interrupt
NI 6124/6154 User Manual6-8ni.com
The Change Detection Event signal also can be used to detect changes on
digital output events.
DI Change Detection Applications for Non-Isolated
Devices
(NI 6124 Only) The DIO change detection circuitry can interrupt a user
program when one of several DIO signals changes state.
You also can use the output of the DIO change detection circuitry to trigger
a DI or counter acquisition on the logical OR of several digital signals. To
trigger on a single digital signal, refer to the Triggering with a Digital
Source section of Chapter 11, Triggering. By routing the Change Detection
Event signal to a counter, you also can capture the relative time between
samples.
You also can use the Change Detection Event signal to trigger DO or
counter generations.
Connecting Digital I/O Signals on Non-Isolated Devices
(NI 6124 Only) The DIO signals, P0.<0..7>, PFI <0..7>/P1.<0..7>, and
PFI <8..15>/P2.<0..7> are referenced to D GND. You can individually
program each line as an input or output. Figure 6-4 shows
PFI <0..3>/P1.<0..3> configured for digital input and PFI <4..7>/P1.<4..7>
configured for digital output. Digital input applications include receiving
TTL signals and sensing external device states, such as the state of the
switch shown in the figure. Digital output applications include sending
TTL signals and driving external devices, such as the LED shown in the
figure.
Exceeding the maximum input voltage ratings, which are listed in the
specifications document for each non-isolated DAQ-STC2 S Series device, can damage the
DAQ device and the computer. NI is not liable for any damage resulting from such signal
connections.
Getting Started with DIO Applications in Software on Non-Isolated
Devices
(NI 6124 Only) You can use non-isolated S Series devices in the following
digital I/O applications:
•Static digital input
•Static digital output
•Digital waveform generation
•Digital waveform acquisition
•DI change detection
Note For more information about programming digital I/O applications and triggers in
software, refer to the NI-DAQmx Help or the LabVIEW Help in version 8.0 or later.
NI 6124/6154 User Manual6-10ni.com
Digital I/O for Isolated Devices
(NI 6154 Only) S Series isolated devices contain ten lines of unidirectional
DIO signals. The digital I/O port is comprised of six digital inputs and
four digital outputs, all bank-isolated. Each digital line has the functionality
of a PFI line. Input PFI lines can be used to input trigger signals to the
different function modules of the DAQ-STC2 ASIC. The PFI pins also can
be used as static digital inputs when not used to input triggers. Output PFI
lines can export internal signals generated in any internal function module,
as well as signals present in the RTSI bus. The PFI pins also can be used as
static digital outputs when not used as trigger lines.
The voltage input and output levels and the current drive levels of the DIO
lines are listed in the NI 6154 Specifications.
Figure 6-5 shows the circuitry of one bank-isolated DIO line.
PFI/
Static DI
PFI/
Static DO
Chapter 6Digital I/O
Isolation
Barrier
Digital
Isolators
I/O Connector
Figure 6-5. Isolated S Series Devices Digital I/O Block Diagram
Static DIO for Isolated Devices
(NI 6154 Only) Isolated devices have unidirectional digital lines that are
either static digital inputs (DI) or static digital outputs (DO). You can use
DI and DO lines to monitor or control digital signals. All samples of static
DI lines and updates of DO lines are software-timed. All DO lines are
controlled by the same output enable. When a digital output line is enabled,
all other digital output lines will also be enabled and driven to a default
value of 0.
You can select the up/down control input of general-purpose counters 0
and 1 from any of the six digital input lines.
(NI 6154 Only) Each DIO and PFI signal is protected against over-voltage,
under-voltage, and over-current conditions as well as ESD events.
However, you should avoid these fault conditions by following these
guidelines:
•Do not connect any DO line to any external signal source, ground
signal, or power supply.
•Understand the current requirements of the load connected to DO
signals. Do not exceed the specified current output limits of the DAQ
device. NI has several signal conditioning solutions for digital
applications requiring high-current drive.
•Do not drive any DI line with voltages outside of its normal operating
range. The PFI or DIO lines have a smaller operating range than the AI
signals.
•Treat the DAQ device as you would treat any static sensitive device.
Always properly ground yourself and the equipment when handling
the DAQ device or connecting to it.
Connecting Digital I/O Signals on Isolated Devices
(NI 6154 Only) The DIO signals, PFI <0..5>/P0.<0..5> and
PFI <6..9>/P1.<0..3>, are referenced to D GND. PFI <0..5>/P0.<0..5> are
inputs and PFI <6..9>/P1.<0..3> are outputs. Figure 6-6 shows digital
inputs PFI <0..5>/P0.<0..5> and digital outputs PFI <6..9>/P1.<0..3>.
Digital input applications include receiving TTL signals and sensing
external device states, such as the state of the switch shown in the figure.
Digital output applications include sending TTL signals and driving
external devices, such as the LED shown in Figure 6-6.
NI 6124/6154 User Manual6-12ni.com
+5 V
LED
Chapter 6Digital I/O
+5 V
Isolation
Barrier
PFI <6..9>/P1.<0..3>
Digital
Isolators
TTL Signal
PFI <0..5>/P0.<0..5>
Switch
D GND
I/O Connector
Isolated SSeries Device
Figure 6-6. Isolated S Series Device Digital I/O Signal Connections
Caution
Exceeding the maximum input voltage ratings, which are listed in the NI 6154
Specifications, can damage the DAQ device and the computer. NI is not liable for any
damage resulting from such signal connections.
Getting Started with DIO Applications in Software on Isolated Devices
(NI 6154 Only) You can use isolated S Series devices in the following digital
I/O applications:
•Static digital input
•Static digital output
Note For more information about programming digital I/O applications and triggers in
software, refer to the NI-DAQmx Help or the LabVIEW Help in version 8.0 or later.
S Series devices have two general-purpose 32-bit counter/timers and
one frequency generator, as shown in Figure 7-1. The general-purpose
counter/timers can be used for many measurement and pulse generation
applications.
The counters have seven input signals, although in most applications only
a few inputs are used.
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Counter Input Applications
Counting Edges
In edge counting applications, the counter counts edges on its Source after
the counter is armed. You can configure the counter to count rising or
falling edges on its Source input. You also can control the direction of
counting (up or down).
The counter values can be read on demand or with a sample clock.
Single Point (On-Demand) Edge Counting
With single point (on-demand) edge counting, the counter counts the
number of edges on the Source input after the counter is armed. On-demand
refers to the fact that software can read the counter contents at any time
without disturbing the counting process. Figure 7-2 shows an example of
single point edge counting.
Counter Armed
SOURCE
Counter Value1 0 5 4 3 2
Figure 7-2. Single Point (On-Demand) Edge Counting
You also can use a pause trigger to pause (or gate) the counter. When the
pause trigger is active, the counter ignores edges on its Source input. When
the pause trigger is inactive, the counter counts edges normally.
You can route the pause trigger to the Gate input of the counter. You can
configure the counter to pause counting when the pause trigger is high or
when it is low. Figure 7-3 shows an example of on-demand edge counting
with a pause trigger.
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Pause Trigger
(Pause When Low)
SOURCE
Chapter 7Counters
Counter Armed
Counter Value
1 0 0 5 4 3 2
Figure 7-3. Single Point (On-Demand) Edge Counting with Pause Trigger
Buffered (Sample Clock) Edge Counting
With buffered edge counting (edge counting using a sample clock), the
counter counts the number of edges on the Source input after the counter is
armed. The value of the counter is sampled on each active edge of a sample
clock. A DMA controller transfers the sampled values to host memory.
The count values returned are the cumulative counts since the counter
armed event. That is, the sample clock does not reset the counter.
You can route the counter sample clock to the Gate input of the counter. You
can configure the counter to sample on the rising or falling edge of the
sample clock.
Figure 7-4 shows an example of buffered edge counting. Notice that
counting begins when the counter is armed, which occurs before the first
active edge on Gate.
In edge counting applications, the counter can count up or down. You can
configure the counter to do the following:
•Always count up
•Always count down
•Count up when the Counter n B input is high; count down when it is
low
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Pulse-Width Measurement
In pulse-width measurements, the counter measures the width of a pulse on
its Gate input signal. You can configure the counter to measure the width
of high pulses or low pulses on the Gate signal.
You can route an internal or external periodic clock signal (with a known
period) to the Source input of the counter. The counter counts the number
of rising (or falling) edges on the Source signal while the pulse on the Gate
signal is active.
You can calculate the pulse width by multiplying the period of the Source
signal by the number of edges returned by the counter.
A pulse-width measurement will be accurate even if the counter is armed
while a pulse train is in progress. If a counter is armed while the pulse is in
the active state, it will wait for the next transition to the active state to begin
the measurement.
Single Pulse-Width Measurement
With single pulse-width measurement, the counter counts the number of
edges on the Source input while the Gate input remains active. When the
Gate input goes inactive, the counter stores the count in a hardware save
register and ignores other edges on the Gate and Source inputs. Software
then reads the stored count.
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Chapter 7Counters
Figure 7-5 shows an example of a single pulse-width measurement.
GATE
SOURCE
1 0
Counter Value
2
GATE
SOURCE
Counter Value
Buffer
HW Save Register
2
Figure 7-5. Single Pulse-Width Measurement
Buffered Pulse-Width Measurement
Buffered pulse-width measurement is similar to single pulse-width
measurement, but buffered pulse-width measurement takes measurements
over multiple pulses.
The counter counts the number of edges on the Source input while the Gate
input remains active. On each trailing edge of the Gate signal, the counter
stores the count in a hardware save register. A DMA controller transfers the
stored values to host memory.
Figure 7-6 shows an example of a buffered pulse-width measurement.
103
33
3
212
2
2
Figure 7-6. Buffered Pulse-Width Measurement
Note that if you are using an external signal as the Source, at least one
Source pulse should occur between each active edge of the Gate signal.
This condition ensures that correct values are returned by the counter. If this
condition is not met, consider using duplicate count prevention, described
in the Duplicate Count Prevention section.
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Period Measurement
In period measurements, the counter measures a period on its Gate input
signal after the counter is armed. You can configure the counter to measure
the period between two rising edges or two falling edges of the Gate input
signal.
You can route an internal or external periodic clock signal (with a known
period) to the Source input of the counter. The counter counts the number
of rising (or falling) edges occurring on the Source input between the
two active edges of the Gate signal.
You can calculate the period of the Gate input by multiplying the period of
the Source signal by the number of edges returned by the counter.
Single Period Measurement
With single period measurement, the counter counts the number of rising
(or falling) edges on the Source input occurring between two active edges
of the Gate input. On the second active edge of the Gate input, the counter
stores the count in a hardware save register and ignores other edges on the
Gate and Source inputs. Software then reads the stored count.
Figure 7-7 shows an example of a single period measurement.
GATE
SOURCE
1 0 3 5 4
Counter Value
HW Save Re
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ister
Figure 7-7. Single Period Measurement
2
5
GATE
SOURCE
Chapter 7Counters
Buffered Period Measurement
Buffered period measurement is similar to single period measurement, but
buffered period measurement measures multiple periods.
The counter counts the number of rising (or falling) edges on the Source
input between each pair of active edges on the Gate input. At the end of
each period on the Gate signal, the counter stores the count in a hardware
save register. A DMA controller transfers the stored values to host memory.
The counter begins when it is armed. The arm usually occurs in the middle
of a period of the Gate input. So the first value stored in the hardware save
register does not reflect a full period of the Gate input. In most applications,
this first point should be discarded.
Figure 7-8 shows an example of a buffered period measurement.
Counter Armed
Counter Value
Buffer
1 1 2 3
2
(Discard) (Discard) (Discard)
Figure 7-8. Buffered Period Measurement
32
2
3
3 1 1
2
3
2
3
3
2
Note that if you are using an external signal as the Source, at least one
Source pulse should occur between each active edge of the Gate signal.
This condition ensures that correct values are returned by the counter. If this
condition is not met, consider using duplicate count prevention, described
in the Duplicate Count Prevention section.
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Semi-Period Measurement
In semi-period measurements, the counter measures a semi-period on its
Gate input signal after the counter is armed. A semi-period is the time
between any two consecutive edges on the Gate input.
You can route an internal or external periodic clock signal (with a known
period) to the Source input of the counter. The counter counts the number
of rising (or falling) edges occurring on the Source input between
two edges of the Gate signal.
You can calculate the semi-period of the Gate input by multiplying the
period of the Source signal by the number of edges returned by the counter.
Single Semi-Period Measurement
Single semi-period measurement is equivalent to single pulse-width
measurement.
Buffered Semi-Period Measurement
In buffered semi-period measurement, on each edge of the Gate signal, the
counter stores the count in a hardware save register. A DMA controller
transfers the stored values to host memory.
The counter begins counting when it is armed. The arm usually occurs
between edges on the Gate input. So the first value stored in the hardware
save register does not reflect a full semi-period of the Gate input. In most
applications, this first point should be discarded.
Figure 7-9 shows an example of a buffered semi-period measurement.
ounter Armed
GATE
SOURCE
1 1
Counter Value
Buffer
2
2
1 3
1 2 1 0 2
2
3
3
2
2
1
2
2
3
3
1
1
2
Figure 7-9. Buffered Semi-Period Measurement
Note that if you are using an external signal as the Source, at least one
Source pulse should occur between each active edge of the Gate signal.
This condition ensures that correct values are returned by the counter. If this
condition is not met, consider using duplicate count prevention, described
in the Duplicate Count Prevention section.
NI 6124/6154 User Manual7-8ni.com
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Frequency Measurement
You can use the counters to measure frequency in several different ways.
You can choose one of the following methods depending on your
application:
•Method 1: Measure Low Frequency with One Counter—In this
method, you measure one period of your signal using a known
timebase. This method is good for low frequency signals.
You can route the signal to measure (F1) to the Gate of a counter. You
can route a known timebase (Ft) to the Source of the counter. The
known timebase can be 80MHzTimebase. For signals that might be
slower than 0.02 Hz, use a slower known timebase.
You can configure the counter to measure one period of the gate signal.
The frequency of F1 is the inverse of the period. Figure 7-10 illustrates
this method.
Chapter 7Counters
Interval Measured
F1
Ft
Gate
Source
Single Period
Measurement
F1
123…N
Ft
Period of F1 =
Frequency of F1 =
Figure 7-10. Method 1
…
N
Ft
Ft
N
•Method 1b: Measure Low Frequency with One Counter
(Averaged)—In this method, you measure several periods of your
signal using a known timebase. This method is good for low to medium
frequency signals.
You can route the signal to measure (F1) to the Gate of a counter. You
can route a known timebase (Ft) to the Source of the counter. The
known timebase can be 80MHzTimebase. For signals that might be
slower than 0.02 Hz, use a slower known timebase.
You can configure the counter to make K + 1 buffered period
measurements. Recall that the first period measurement in the buffer
should be discarded.
Average the remaining K period measurements to determine the
average period of F1. The frequency of F1 is the inverse of the average
period. Figure 7-11 illustrates this method.
ntervals Measured
T
T
1
2
… T
K
F1
Ft
Gate
Source
Buffered Period
Measurement
F1
2...N
1......N2 … 1......N
1
1
Ft
Average Period of F1 =
Frequency of F1 =
N
1
N
+ N2 + …N
1
K × Ft
+ N2 + …N
K
1
K
×
K
K
Ft
Figure 7-11. Method 1b
•Method 2: Measure High Frequency with Two Counters—In this
method, you measure one pulse of a known width using your signal
and derive the frequency of your signal from the result. This method is
good for high frequency signals.
In this method, you route a pulse of known duration (T) to the Gate of
a counter. You can generate the pulse using a second counter. You also
can generate the pulse externally and connect it to a PFI or RTSI
terminal. You only need to use one counter if you generate the pulse
externally.
Route the signal to measure (F1) to the Source of the counter.
Configure the counter for a single pulse-width measurement. If you
measure the width of pulse T to be N periods of F1, the frequency of
F1 is N/T.
NI 6124/6154 User Manual7-10ni.com
Chapter 7Counters
Figure 7-12 illustrates this method. Another option would be to
measure the width of a known period instead of a known pulse.
Width of Pulse (T)
Pulse
F1
Pulse
Gate
1 2 … N
Source
Pulse-Width
Measurement
F1
Width of
Pulse
Frequency of F1 =
T =
N
F1
Figure 7-12. Method 2
•Method 3: Measure Large Range of Frequencies Using
Two Counters—By using two counters, you can accurately measure
a signal that might be high or low frequency. This technique is called
reciprocal frequency measurement. In this method, you generate a long
pulse using the signal to measure. You then measure the long pulse
with a known timebase. The S Series device can measure this long
pulse more accurately than the faster input signal.
You can route the signal to measure to the Source input of Counter 0,
as shown in Figure 7-13. Assume this signal to measure has frequency
F1. Configure Counter 0 to generate a single pulse that is the width of
N periods of the source input signal.
Signal to
Measure (F1)
Signal of Known
Frequency (F2)
CTR_0_SOURCE
(Signal to Measure)
CTR_0_OUT
(CTR_1_GATE)
CTR
SOURCE
SOURCE OUT
COUNTER 0
SOURCE
COUNTER 1
GATE
0 1 2 3 … N
Interval
to Measure
OUT
Figure 7-13. Method 3
Then route the Counter 0 Internal Output signal to the Gate input of
Counter 1. You can route a signal of known frequency (F2) to the
Counter 1 Source input. F2 can be 80MHzTimebase. For signals that
might be slower than 0.02 Hz, use a slower known timebase. Configure
Counter 1 to perform a single pulse-width measurement. Suppose the
result is that the pulse width is J periods of the F2 clock.
From Counter 0, the length of the pulse is N/F1. From Counter 1, the
length of the same pulse is J/F2. Therefore, the frequency of F1 is
given by F1 = F2 * (N/J).
Choosing a Method for Measuring Frequency
The best method to measure frequency depends on several factors
including the expected frequency of the signal to measure, the desired
accuracy, how many counters are available, and how long the measurement
can take.
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Chapter 7Counters
•Method 1 uses only one counter. It is a good method for many
applications. However, the accuracy of the measurement decreases as
the frequency increases.
Consider a frequency measurement on a 50 kHz signal using an
80 MHz Timebase. This frequency corresponds to 1600 cycles of the
80 MHz Timebase. Your measurement may return 1600 ± 1 cycles
depending on the phase of the signal with respect to the timebase. As
your frequency becomes larger, this error of ±1 cycle becomes more
significant; Table 7-1 illustrates this point.
•Method 1b (measuring K periods of F1) improves the accuracy of the
measurement. A disadvantage of Method 1b is that you have to take
K + 1 measurements. These measurements take more time and
consume some of the available PCI or PXI bandwidth.
•Method 2 is accurate for high frequency signals. However, the
accuracy decreases as the frequency of the signal to measure
decreases. At very low frequencies, Method 2 may be too inaccurate
for your application. Another disadvantage of Method 2 is that it
requires two counters (if you cannot provide an external signal of
known width). An advantage of Method 2 is that the measurement
completes in a known amount of time.
•Method 3 measures high and low frequency signals accurately.
However, it requires two counters.
Table 7-2 summarizes some of the differences in methods of measuring
frequency.
Table 7-2. Frequency Measurement Method Comparison
Number of
Counters
Method
111PoorGood
1b1ManyFairGood
21 or 21GoodPoor
321GoodGood
Used
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Position Measurement
You can use the counters to perform position measurements with
quadrature encoders or two-pulse encoders. You can measure angular
position with X1, X2, and X4 angular encoders. Linear position can be
measured with two-pulse encoders. You can choose to do either a single
point (on-demand) position measurement or a buffered (sample clock)
position measurement. You must arm a counter to begin position
measurements.
Number of
Measurements
Returned
Measures High
Frequency
Signals
Accurately
Measures Low
Frequency
Signals
Accurately
Measurements Using Quadrature Encoders
The counters can perform measurements of quadrature encoders that use
X1, X2, or X4 encoding. A quadrature encoder can have up to three
channels—channels A, B, and Z.
•X1 Encoding—When channel A leads channel B in a quadrature
cycle, the counter increments. When channel B leads channel A in a
quadrature cycle, the counter decrements. The amount of increments
and decrements per cycle depends on the type of encoding—X1, X2,
or X4.
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Chapter 7Counters
Figure 7-14 shows a quadrature cycle and the resulting increments and
decrements for X1 encoding. When channel A leads channel B, the
increment occurs on the rising edge of channel A. When channel B
leads channel A, the decrement occurs on the falling edge of
channel A.
Ch A
Ch B
Ch A
Ch B
Counter Value
5
6
7
7
6
5
Figure 7-14. X1 Encoding
•X2 Encoding—The same behavior holds for X2 encoding except the
counter increments or decrements on each edge of channel A,
depending on which channel leads the other. Each cycle results in
two increments or decrements, as shown in Figure 7-15.
Ch A
Ch B
Counter Value
5 6 8
7
9
9
8
6
7
5
Figure 7-15. X2 Encoding
•X4 Encoding—Similarly, the counter increments or decrements on
each edge of channels A and B for X4 encoding. Whether the counter
increments or decrements depends on which channel leads the other.
Each cycle results in four increments or decrements, as shown in
Figure 7-16.
Counter Value5 6 8 9 10 10 11 11 12 12 13 13 7
5 6 8 7 9
Figure 7-16. X4 Encoding
Channel Z Behavior
Some quadrature encoders have a third channel, channel Z, which is also
referred to as the index channel. A high level on channel Z causes the
counter to be reloaded with a specified value in a specified phase of the
quadrature cycle. You can program this reload to occur in any one of the
four phases in a quadrature cycle.
Channel Z behavior—when it goes high and how long it stays
high—differs with quadrature encoder designs. You must refer to the
documentation for your quadrature encoder to obtain timing of channel Z
with respect to channels A and B. You must then ensure that channel Z is
high during at least a portion of the phase you specify for reload. For
instance, in Figure 7-17, channel Z is never high when channel A is high
and channel B is low. Thus, the reload must occur in some other phase.
In Figure 7-17, the reload phase is when both channel A and channel B are
low. The reload occurs when this phase is true and channel Z is high.
Incrementing and decrementing takes priority over reloading. Thus, when
the channel B goes low to enter the reload phase, the increment occurs first.
The reload occurs within one maximum timebase period after the reload
phase becomes true. After the reload occurs, the counter continues to count
as before. The figure illustrates channel Z reload with X4 decoding.
Ch A
Ch B
Ch Z
Max Timebase
Counter Value
5 6
Figure 7-17. Channel Z Reload with X4 Decoding
8 9 0 2 1 7 4 3
A = 0
B = 0
Z = 1
Measurements Using Two Pulse Encoders
The counter supports two pulse encoders that have two channels—channels
A and B.
The counter increments on each rising edge of channel A. The counter
decrements on each rising edge of channel B, as shown in Figure 7-18.
Ch A
Ch B
Counter Value2 3 5 4 3 4 4
Figure 7-18. Measurements Using Two Pulse Encoders
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Chapter 7Counters
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Buffered (Sample Clock) Position Measurement
With buffered position measurement (position measurement using a
sample clock), the counter increments based on the encoding used after the
counter is armed. The value of the counter is sampled on each active edge
of a sample clock. A DMA controller transfers the sampled values to host
memory. The count values returned are the cumulative counts since the
counter armed event; that is, the sample clock does not reset the counter.
You can route the counter sample clock to the Gate input of the counter.
You can configure the counter to sample on the rising or falling edge of the
sample clock.
Figure 7-19 shows an example of a buffered edge X1 position
measurement.
(Sample on Rising Edge)
Sample Clock
Ch A
Ch B
Buffer
Counter
Armed
1
Figure 7-19. Buffered Position Measurement
Two-Signal Edge-Separation Measurement
Two-signal edge-separation measurement is similar to pulse-width
measurement, except that there are two measurement signals—Aux and
Gate. An active edge on the Aux input starts the counting and an active
edge on the Gate input stops the counting. You must arm a counter to begin
a two edge separation measurement.
After the counter has been armed and an active edge occurs on the Aux
input, the counter counts the number of rising (or falling) edges on the
Source. The counter ignores additional edges on the Aux input.
4102 5Count
1
4
The counter stops counting upon receiving an active edge on the Gate input.
The counter stores the count in a hardware save register.
You can configure the rising or falling edge of the Aux input to be the active
edge. You can configure the rising or falling edge of the Gate input to be
the active edge.
Use this type of measurement to count events or measure the time that
occurs between edges on two signals. This type of measurement is
sometimes referred to as start/stop trigger measurement, second gate
measurement, or A-to-B measurement.
Single Two-Signal Edge-Separation Measurement
With single two-signal edge-separation measurement, the counter counts
the number of rising (or falling) edges on the Source input occurring
between an active edge of the Gate signal and an active edge of the Aux
signal. The counter then stores the count in a hardware save register and
ignores other edges on its inputs. Software then reads the stored count.
Figure 7-20 shows an example of a single two-signal edge-separation
measurement.
Counter
Armed
Measured Interval
AUX
GATE
SOURCE
Counter Value
HW Save Register
Figure 7-20. Single Two-Signal Edge-Separation Measurement
0 0 0 0 1 2 3 4 5 6 7 8 8 8
8
Buffered Two-Signal Edge-Separation Measurement
Buffered and single two-signal edge-separation measurements are similar,
but buffered measurement measures multiple intervals.
The counter counts the number of rising (or falling) edges on the Source
input occurring between an active edge of the Gate signal and an active
edge of the Aux signal. The counter then stores the count in a hardware save
register. On the next active edge of the Gate signal, the counter begins
another measurement. A DMA controller transfers the stored values to host
memory.
NI 6124/6154 User Manual7-18ni.com
Figure 7-21 shows an example of a buffered two-signal edge-separation
measurement.
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Counter Output Applications
Simple Pulse Generation
Chapter 7Counters
1 2 3 1 2 3 1 2 3
3 3
3
3
3
3
Single Pulse Generation
The counter can output a single pulse. The pulse appears on the Counter n
Internal Output signal of the counter.
You can specify a delay from when the counter is armed to the beginning
of the pulse. The delay is measured in terms of a number of active edges of
the Source input.
You can specify a pulse width. The pulse width is also measured in terms
of a number of active edges of the Source input. You also can specify the
active edge of the Source input (rising or falling).
Figure 7-22 shows a generation of a pulse with a pulse delay of four and a
pulse width of three (using the rising edge of Source).
Counter Armed
SOURCE
OUT
Figure 7-22. Single Pulse Generation
Single Pulse Generation with Start Trigger
The counter can output a single pulse in response to one pulse on a
hardware Start Trigger signal. The pulse appears on the Counter n Internal
Output signal of the counter.
You can route the Start Trigger signal to the Gate input of the counter. You
can specify a delay from the Start Trigger to the beginning of the pulse. You
also can specify the pulse width. The delay and pulse width are measured
in terms of a number of active edges of the Source input.
After the Start Trigger signal pulses once, the counter ignores the Gate
input.
Figure 7-23 shows a generation of a pulse with a pulse delay of four and a
pulse width of three (using the rising edge of Source).
GATE
(Start Trigger)
SOURCE
OUT
Figure 7-23. Single Pulse Generation with Start Trigger
Retriggerable Single Pulse Generation
The counter can output a single pulse in response to each pulse on a
hardware Start Trigger signal. The pulses appear on the Counter n Internal
Output signal of the counter.
NI 6124/6154 User Manual7-20ni.com
Chapter 7Counters
You can route the Start Trigger signal to the Gate input of the counter. You
can specify a delay from the Start Trigger to the beginning of each pulse.
You also can specify the pulse width. The delay and pulse width are
measured in terms of a number of active edges of the Source input.
The counter ignores the Gate input while a pulse generation is in progress.
After the pulse generation is finished, the counter waits for another Start
Trigger signal to begin another pulse generation.
Figure 7-24 shows a generation of two pulses with a pulse delay of five and
a pulse width of three (using the rising edge of Source).
GATE
(Start Trigger)
SOURCE
OUT
Figure 7-24. Retriggerable Single Pulse Generation
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Pulse Train Generation
Continuous Pulse Train Generation
This function generates a train of pulses with programmable frequency and
duty cycle. The pulses appear on the Counter n Internal Output signal of the
counter.
You can specify a delay from when the counter is armed to the beginning
of the pulse train. The delay is measured in terms of a number of active
edges of the Source input.
You specify the high and low pulse widths of the output signal. The pulse
widths are also measured in terms of a number of active edges of the Source
input. You also can specify the active edge of the Source input (rising or
falling).
The counter can begin the pulse train generation as soon as the counter is
armed, or in response to a hardware Start Trigger. You can route the Start
Trigger to the Gate input of the counter.
You also can use the Gate input of the counter as a Pause Trigger (if it is not
used as a Start Trigger). The counter pauses pulse generation when the
Pause Trigger is active.
Figure 7-25 shows a continuous pulse train generation (using the rising
edge of Source).
SOURCE
OUT
Counter Armed
Figure 7-25. Continuous Pulse Train Generation
Continuous pulse train generation is sometimes called frequency division.
If the high and low pulse widths of the output signal are M and N periods,
then the frequency of the Counter n Internal Output signal is equal to the
frequency of the Source input divided by M + N.
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Finite Pulse Train Generation
This function generates a train of pulses of predetermined duration. This
counter operation requires both counters. The first counter (for this
example, Counter 0) generates a pulse of desired width. The second
counter, Counter 1, generates the pulse train, which is gated by the pulse of
the first counter. The routing is done internally. Figure 7-26 shows an
example finite pulse train timing diagram.
Counter 0
(Paired Counter)
Counter 1
Generation
Complete
Figure 7-26. Finite Pulse Train Timing Diagram
NI 6124/6154 User Manual7-22ni.com
Frequency Generation
You can generate a frequency by using a counter in pulse train generation
mode or by using the frequency generator circuit.
Using the Frequency Generator
The frequency generator can output a square wave at many different
frequencies. The frequency generator is independent of the
two general-purpose 32-bit counter/timer modules on S Series devices.
Figure 7-27 shows a block diagram of the frequency generator.
20 MHz Timebase
100 kHz Timebase
÷ 2
Chapter 7Counters
Frequency
Output
Timebase
Frequency Generator
Divisor
(1–16)
Figure 7-27. Frequency Generator Block Diagram
FREQ OUT
The frequency generator generates the Frequency Output signal. The
Frequency Output signal is the Frequency Output Timebase divided by a
number you select from 1 to 16. The Frequency Output Timebase can be
either the 20 MHz Timebase divided by 2 or the 100 kHz Timebase.
The duty cycle of Frequency Output is 50% if the divider is either 1 or
an even number. For an odd divider, suppose the divider is set to D.
In this case, Frequency Output is low for (D + 1)/2 cycles and high for
(D – 1)/2 cycles of the Frequency Output Timebase.
Figure 7-28 shows the output waveform of the frequency generator when
the divider is set to 5.
Frequency Output can be routed out to any PFI <0..15> or RTSI <0..7>
terminal. All PFI terminals are set to high-impedance at startup. The FREQ
OUT signal also can be routed to DO Sample Clock and DI Sample Clock.
In software, program the frequency generator as you would program one of
the counters for pulse train generation.
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Frequency Division
The counters can generate a signal with a frequency that is a fraction of
an input signal. This function is equivalent to continuous pulse train
generation. Refer to the Continuous Pulse Train Generation section for
detailed information.
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Pulse Generation for ETS
In the equivalent time sampling (ETS) application, the counter produces a
pulse on the output a specified delay after an active edge on Gate. After
each active edge on Gate, the counter cumulatively increments the delay
between the Gate and the pulse on the output by a specified amount. Thus,
the delay between the Gate and the pulse produced successively increases.
The increase in the delay value can be between 0 and 255. For instance, if
you specify the increment to be 10, the delay between the active Gate edge
and the pulse on the output will increase by 10 every time a new pulse is
generated.
Suppose you program your counter to generate pulses with a delay of 100
and pulse width of 200 each time it receives a trigger. Furthermore, suppose
you specify the delay increment to be 10. On the first trigger, your pulse
delay will be 100, on the second it will be 110, on the third it will be 120;
the process will repeat in this manner until the counter is disarmed. The
counter ignores any Gate edge that is received while the pulse triggered by
the previous Gate edge is in progress.
NI 6124/6154 User Manual7-24ni.com
The waveform thus produced at the counter’s output can be used to provide
timing for undersampling applications where a digitizing system can
sample repetitive waveforms that are higher in frequency than the Nyquist
frequency of the system. Figure 7-29 shows an example of pulse generation
for ETS; the delay from the trigger to the pulse increases after each
subsequent Gate active edge.
GATE
OUT
For information about connecting counter signals, refer to the Default
Counter/Timer Pinouts section.
Counter Timing Signals
Chapter 7Counters
D1 D2 = D1 + ΔD D3 = D1 + 2ΔD
Figure 7-29. Pulse Generation for ETS
S Series devices feature the following counter timing signals:
•Counter n Source Signal
•Counter n Gate Signal
•Counter n Aux Signal
•Counter n A Signal
•Counter n B Signal
•Counter n Z Signal
•Counter n Up_Down Signal
•Counter n HW Arm Signal
•Counter n Internal Output Signal
•Counter n TC Signal
•Frequency Output Signal
In this section, n refers to either Counter 0 or 1. For example, Counter n
Source refers to two signals—Counter 0 Source (the source input to
Counter 0) and Counter 1 Source (the source input to Counter 1).
The selected edge of the Counter n Source signal increments and
decrements the counter value depending on the application the counter
is performing. Table 7-3 lists how this terminal is used in various
applications.
One Counter Time MeasurementsCounter Timebase
Two Counter Time MeasurementsInput Terminal
Non-Buffered Edge CountingInput Terminal
Routing a Signal to Counter n Source
Each counter has independent input selectors for the Counter n Source
signal. Any of the following signals can be routed to the Counter n Source
input:
•80MHz Timebase
•20MHz Timebase
•100 kHz Timebase
•RTSI<0..7>
•PFI <0..15>
•PXI_CLK10
•PXI_STAR
•Analog Comparison Event
Table 7-3. Counter Applications and Counter n Source
ApplicationPurpose of Source Terminal
Pulse GenerationCounter Timebase
Buffered Edge CountingInput Terminal
Two-Edge SeparationCounter Timebase
In addition, Counter 1 TC or Counter 1 Gate can be routed to
Counter 0 Source. Counter 0 TC or Counter 0 Gate can be routed to
Counter 1 Source.
Some of these options may not be available in some driver software.
NI 6124/6154 User Manual7-26ni.com
Routing Counter n Source to an Output Terminal
You can route Counter n Source out to any PFI <0..15> or RTSI <0..7>
terminal. All PFIs are set to high-impedance at startup.
Counter n Gate Signal
The Counter n Gate signal can perform many different operations
depending on the application including starting and stopping the counter,
and saving the counter contents.
Routing a Signal to Counter n Gate
Each counter has independent input selectors for the Counter n Gate signal.
Any of the following signals can be routed to the Counter n Gate input:
•RTSI<0..7>
•PFI <0..15>
•AI Reference Trigger (ai/ReferenceTrigger)
•AI Start Trigger (ai/StartTrigger)
•AI Sample Clock (ai/SampleClock)
•AI Convert Clock (ai/ConvertClock)
•AO Sample Clock (ao/SampleClock)
•DI Sample Clock (di/SampleClock)
•DO Sample Clock (do/SampleClock)
•PXI_STAR
•Change Detection Event
•Analog Comparison Event
Chapter 7Counters
In addition, Counter 1 Internal Output or Counter 1 Source can be routed to
Counter 0 Gate. Counter 0 Internal Output or Counter 0 Source can be
routed to Counter 1 Gate.
Some of these options may not be available in some driver software.
Routing Counter n Gate to an Output Terminal
You can route Counter n Gate out to any PFI <0..15> or RTSI <0..7>
terminal. All PFIs are set to high-impedance at startup.
The Counter n Aux signal indicates the first edge in a two-signal
edge-separation measurement.
Routing a Signal to Counter n Aux
Each counter has independent input selectors for the Counter n Aux signal.
Any of the following signals can be routed to the Counter n Aux input:
•RTSI<0..7>
•PFI <0..15>
•AI Reference Trigger (ai/ReferenceTrigger)
•AI Start Trigger (ai/StartTrigger)
•PXI_STAR
•Analog Comparison Event
In addition, Counter 1 Internal Output, Counter 1 Gate, Counter 1 Source,
or Counter 0 Gate can be routed to Counter 0 Aux. Counter 0 Internal
Output, Counter 0 Gate, Counter 0 Source, or Counter 1 Gate can be routed
to Counter 1 Aux.
Some of these options may not be available in some driver software.
Counter n A, Counter n B, and Counter n Z Signals
Counter n B can control the direction of counting in edge counting
applications. Use the A, B, and Z inputs to each counter when measuring
quadrature encoders or measuring two pulse encoders.
Routing Signals to A, B, and Z Counter Inputs
Each counter has independent input selectors for each of the A, B, and
Z inputs. Any of the following signals can be routed to each input:
•RTSI<0..7>
•PFI <0..15>
•PXI_STAR
•Analog Comparison Event
Routing Counter n Z Signal to an Output Terminal
You can route Counter n Z out to RTSI <0..7>.
NI 6124/6154 User Manual7-28ni.com
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