WBK18

Dynamic Signal Conditioning Module

Description…… 1

Software Setup …… 7

Current Source with Transducer Fault Detection…… 2
Input Coupling …… 2
Programmable Gain Amplifier (PGA) …… 2
Low-Pass Anti-Aliasing Filter …… 3
Overrange Detection …… 3
Simultaneous Sample and Hold …… 3
TEDS Support …… 4
Excitation Source …… 4
LEDs …… 4

Hardware Setup …… 5
Configuration…… 5
Power…… 5
Assembly…… 6
Input Connections ……6

General ……7
Maximizing Alias Protection ……9Using the 2-Pole Filter and Bypass……11
Module Configuration …… 13

Using Accelerometers …… 18
Overview …… 18
Accelerometer Specification
Parameters …… 18
Electrical Grounding…… 20
Cable Driving…… 20

Fuse Replacement …… 22
Specifications …… 24

Description
The WBK18 is a dynamic analog signal input module for the WaveBook data acquisition system. The
WBK18 provides a complete system to interface to piezoelectric transducers that include accelerometers,
microphones, force/pressure transducers, and others.

WBK18, Front and Rear Panel Views
Each WBK18 channel features:
•
•
•
•
•
•
•
•

a 4 mA current source for transducer biasing
hardware detection of a transducer fault
AC (0.1 Hz or 10 Hz) or DC couplinga programmable gain amplifier (range selection)
hardware overrange detection
an anti-aliasing low-pass filtera simultaneous sample-and-hold (SSH) amplifier
support for optional TEDS (Transducer Electronic Data Sheet), if purchased

All of these parameters are independently controlled in software on a per channel basis except
for overrange detection level, which is set on a per module basis.

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WBK18, pg. 1

The WBK18 module includes a built-in programmable voltage excitation source. This source can be used
to stimulate dynamic systems for transfer function measurements, and also serves as a test signal for the
input channels.

WBK18 Block Diagram

Current Source with Transducer Fault Detection
The WBK18 module provides constant current of 4mA to bias ICP transducers. The bias current is sourced throughthe center conductor of the input channel BNC connector and returns to the WBK18 by the outer conductor. The
current source features an operating compliance of 24V and is short-circuit and overvoltage protected. Operatingcompliance refers to the highest voltage that can be applied without change of the current source value. In theabsence of a transducer, the current source will output an open circuit voltage of 30V. For applications that do not
require bias, the current source can be disconnected from the input via software control on a per channel basis.
When the current source is enabled, the input voltage is continuously monitored with level detection circuitry.
Recognition of a voltage greater than 25V (transducer open) or less than 1V (transducer short) triggers a transducer
fault condition for the affected channel. This error is communicated to the user via a front panel LED and is alsoavailable through a software status request at the end of an acquisition. When recognized, an error is latched until
the commencement of a new acquisition. Consequently, even intermittent faults are detected and communicated.
Detection of a fault does not, however, alter the acquisition process or its data.

Input Coupling
Each WBK18 channel offers the selection of three coupling modes: 0.1 Hz, 10 Hz, or DC. The 0.1 Hz path is a 1pole high-pass filter with a –3dB point at 0.1 Hz. The 10 Hz path is a 2-pole high-pass filter with a –3dB point at
10 Hz. The DC path provides a direct signal connection.

Programmable Gain Amplifier (PGA)The WBK18 provides programmable gains of 1, 2, 5, 10, 20, 50, 100, and 200. These correspond to bipolar input
ranges of 5V, 2.5V, 1V, 500mV, 250mV, 100mV, 50mV, and 25mV. Additionally, there is a 25V DC-coupled only
range that is suitable for proximity sensor measurements. Range selection is programmable on a per channel basis.

WBK18, pg. 2926896

WBK18, Dynamic Signal Input ModuleLow-Pass Anti-Aliasing Filter
Each channel features a programmable low-pass filter to provide alias protection and to allow for the removal ofundesired frequencies from the measured response. This filter is configurable within 3 modes: 8-pole, 2-pole, andBypass. The 8-pole Butterworth switched capacitor filter offers the greatest alias protection and is most commonlyused in vibration measurements. Its –3dB cutoff frequency is settable from 10 Hz to 50 kHz in a 1-2-5 progression.
Application information regarding the proper setting of this filter is provided in Maximizing Alias Protection.
2-pole mode utilizes two RC filters in series. Its –3dB cutoff frequency is settable as well from 10 Hz to 50 kHz in
a 1-2-5 progression. It provides tighter amplitude and offset accuracy than 8-pole mode at the expense of reduced
alias protection (due to its more gradual roll-off). It is most commonly used in proximity sensor measurements,
where the DC component of the input signal is critical. Additionally, the filter can be bypassed altogether, resulting
in a signal bandwidth of up to 200 kHz.
When the LPF (Low Pass Filter) is in the Bypass mode, the bandwidth of the system depends on the coupling mode
selected. For the 0.1 Hz and 10 Hz selections, the bandwidth is approximately 190 kHz. For the DC selection, thebandwidth is approximately 130 kHz. For the 25 V range, the bandwidth is approximately 120 kHz.
Reference Note:
Application information regarding the 2-pole and Bypass settings of the filter is provided in the section
entitled, Using the 2-Pole Filter and Bypass (page 11).

Overrange Detection
Each WBK18 channel is equipped with overrange detection circuitry. Use of this feature insures that all datacollected during an acquisition did not exceed a user-specified level, set as a percentage of range. In its mostcommon use, with the level set to 100%, the user is notified if the input signal exceeded the input full-scale range,even momentarily. This protection is critical, for overrange signals result in clipped data that significantly corrupts
FFT analysis. This error is communicated to the user via a front panel LED and is also available through a software
status request at the end of an acquisition. When recognized, an error is latched until the commencement of a newacquisition. Consequently, even intermittent faults are detected and communicated. However, an overrange event
does not stop the acquisition process or change the data, providing the user with full control over the disposition ofdata.
An extension of the overrange capability could involve its integration into a process monitor application, whereby
the fault condition is used to monitor the stability of a previously characterized dynamic signal. The overrange levelis programmable from 1 to 100% of range on a per WBK18 basis. Overrange detection can be enabled or disabled
on a per channel basis.

Simultaneous Sample and HoldAll WBK18 channels are sampled simultaneously, after which the WaveBook measures each output until allchannels are digitized. The time-skew between sampling on all channels is 100ns, regardless of the number of
WBK18s connected to the WaveBook. This maximizes channel-to-channel phase matching.
When using WaveBook with an SSH channel enabled, the per-channel sample rates are reduced.
The rate reduction is the same as that which would occur if another channel were added. The
per-channel rate (with SSH enabled) is:1 MHz / (n+1), where n is the number of active channels.

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WBK18, pg. 3

TEDS Support
TEDS, Transducer Electronic Data Sheet, is a purchased option. The TEDS feature enables a WBK18 module toaccess the calibration information that is stored within TEDS-compatible sensors. The WBK18 can read calibration
information from sensors and automatically scale the readings from each sensor, using the acquired calibration
information. TEDS support is a software option that can easily be added after the initial purchase of the WBK18.
Reference Note:
Information regarding TEDS in relation to the WaveView software application begins on page 8.

Excitation Source
The WBK18’s AC excitation source is a sine wave-based voltage source that is programmable in frequency from
1 Hz to 5 kHz and in discrete amplitudes from 100 mVp-p to 10 Vp-p. Continuous sine, sweep sine, and custom
sine modes are available. It can be used as a test source for the input channels or as excitation for other systemelements, such as the amplifier for a shaker table. All of its parameters are software controlled, and its output isconveniently provided on a front panel BNC connection. Detailed information on the excitation source and its
operation can be found in the Software Setup section.
Do not confuse excitation source with the Source Level column in WaveView’s main window, as source level refers
to transducer bias current (see Source Level, page 8) and not to the excitation source.

LEDs
The right-hand side of the WBK18 front panel includes 19 indicator LEDs. There are eight Transducer Fault LEDs
(1 for each channel), eight Overrange LEDs (1 for each channel), an Active LED, Ready LED and a Power LED.
The indicators have the following meanings.

Transducer Fault(1 LED per Channel)

Overrange(1 LED per Channel)

When lit, a Transducer Fault LED indicates that the transducer for the associated channel has
either an open circuit or a short circuit. In addition to LED indication, transducer fault
information is available through a software status request at the end of an acquisition.
Transducer fault errors are latched until the commencement of a new acquisition.
Consequently, even intermittent faults are detected and communicated. Detection of atransducer fault does not stop an acquisition or alter data. For related information refer toCurrent Source with Transducer Fault Detection on page 2.
When lit, an Overrange LED indicates that the associated channel’s input signal has exceeded
the input full-scale range, which was programmed for that specific WBK18 module. Even a
momentary exceeding of the range will cause the LED to light. This indication is critical, foroverrange signals result in clipped data that significantly corrupts FFT analysis. In addition
to LED indication, the overrange condition is available through a software status request at
the end of an acquisition. Overrange errors are latched until the commencement of a newacquisition. Consequently, even intermittent faults are detected and communicated.
Overrange events do not stop an acquisition or alter data. For related information refer toOverrange Detection on page 3.

ActiveLights when data is being converted.

Ready

Lights when the WBK18 has established communication via its Expansion Control In
connector.

PowerLights when power to the unit is turned on and present.

WBK18, pg. 4926896

WBK18, Dynamic Signal Input Module

Hardware Setup
Configuration
The WBK18 requires no physical hardware settings. All WBK18 configurations are controlled by software.
Reference Note:
Setup information pertaining to power, expansion control, and expansion signal connections iscontained in the chapter System Setup and Power Options, in the WaveBook User’s Manual.
It is possible to connect a WaveBook to the host computer’s parallel port with either a 2-foot(CA-35-2) or 6-foot (CA-35-6) communication cable. To minimize the amount of noise that is
introduced to the WBK18, use of the 2-foot (CA-35-2) cable with the WaveBook is
recommended.

Power
The WBK18 module can be powered by an AC power adapter or directly from any 10 to 30 VDC source, such as a
12 V car battery. For portable or field applications, the WBK18 and the WaveBook can be powered by the
DBK30A rechargeable battery module.
Reference Note:
For details regarding power, refer to the chapter, System Setup and Power Options, in the
WaveBook User’s Manual.
As described in this referenced chapter, it is possible to power the WBK18 from the POWER OUT
DIN5 connector on the WaveBook and to power other WBK expansion modules from the POWER
OUT DIN5 connector on the WBK18. The following notes apply to those types of power connections.

Tables for determining amp load are provided in the WaveBook User’s Manual chapter entitled
System Setup and Power Options. The following factors are very important.

• Calculate system amp load prior to creating a system daisy-chain. Although WaveBook
device connectors and CA-115 power cables have 5 amp limits, TR-40Us are limited to
2.2 amps. If necessary use auxiliary or high-current power supplies.

• If using an AC power adapter for the system power, use separate adapters for the
WaveBook and the WBK18.

• The WBK18 has a 5 amp current limit. TR-40U power supplies are limited to 2.2 amps.
Power consumption calculations must be done to ensure that a particular daisy-chain
scheme does not exceed either of these current limits.

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WBK18, pg. 5

To ensure that the software recognizes all system components, when powering up an Ethernet
connected WaveBook system, it is important that the WaveBook/516E (or WBK25) is powered
last, and that the most remote system components are powered first. Other power-up sequences
will result in software’s failure to recognize all components.*• First, power-on the WBK expansion modules.
• Second, power-on WaveBooks or WBK modules that are connected to the expansion
ports of the WaveBook/516E or WBK25.

• Finally, power-on the WaveBook/516E and/or WBK25 devices.
*An exception to this power-up scheme is to power-on the entire system at once.

Assembly
The WBK18 has the same footprint as the WaveBook and other modules, allowing for convenient mounting. A
fastener panel allows multiple units to be stacked vertically. Screw-on handles are available for portableapplications. For more assembly information, see chapter 3 of the WaveBook User’s Manual (p/n 489-0901).

Input Connections
All input connections are made into the front panel BNCs, in which the BNC center conductor is the signal HI and
the BNC shell is the signal LO. The BNC shell is common among all eight input channels and is not isolated fromearth ground. Consequently, the shell is not meant to be driven with respect to earth ground. An additional
consideration exists regarding the setup of the input transducer. If the transducer case is effectively earth groundedthrough its connection to a device under test, there exists the possibility for added measurement noise due to theground loop that is created. This issue is minimized by electrically isolating the transducer from the device.

CAUTION
The BNC shell is not to be driven with respect to earth ground. Attempting to do so could resultin equipment damage.

Additional measurement noise may be present when using earth grounded transducers.
For best results, electrically isolate the input transducers from earth ground.

WBK18, pg. 6926896

WBK18, Dynamic Signal Input Module

Software Setup
GeneralDepending on your application, you will need to set several software parameters. Proper settings willallow WaveView to organize data to meet your requirements. Some items of importance to the WBK18 are
the low-pass and high-pass filter options that can be selected from the WaveView Configuration main
window and the excitation source and overrange detection parameters that can be chosen from theModule Configuration window. The Module Configuration window can be accessed from the View pulldown menu or by use of the first toolbar button (located just below the File pull-down menu).
Reference Note:
For detailed WaveView information, refer to the WaveView Document Module.

WaveView Configuration Window
In the WaveView Configuration main window (see figure) the following columns are applicable to the WBK18.
LPF Mode – Click on a cell in the LPF Mode column to make the cell active, and then change its setting. Options
for WBK18’s LPF Mode are:(a) 8-Pole: selects the 8-pole low-pass filter(b) 2-Pole: selects the 2-pole low-pass filter(c) Bypass – bypasses the low-pass filter
LPF Cutoff - Click on a cell in the LPF Cutoff column to make the cell active, and then change its setting. Options
for LPF Cutoff (in Hz) are: 10, 20, 50, 100, 200, 500, 1000, 2000, 5000, 10000, 20000, and 50000. Note that whenthe LPF Mode is “Bypass,” this parameter is fixed at 200000 Hz.
Reference Note:
Application information regarding the proper setting of LPF Mode and LPF Cutoff is provided in thesections entitled Maximizing Alias Protection (page 9) and Using the 2-Pole Filter and Bypass (page 11).
HPF Cutoff - This is used to select input coupling. Click on a cell in the HPF Cutoff column to make the cell
active, and then change its setting. Options for HPF Cutoff are:(a) 0.1 Hz: selects the 0.1 Hz, 1-pole high-pass filter(b) 10 Hz: selects the 10 Hz, 2-pole high-pass filter(c) DC: selects DC coupling
Note that when the Range is “±25V,” the HPF Cutoff is fixed at DC.
Range - This is used to select the input range. Click on a cell in the Range column to make the cell active, andthen change its setting. Options for Range are: ±25V, ±5V, ±2.5V, ±1V, ±500mV, ±250mV, ±100mV, ±50mV,
and ±25mV. Note that when the Range is “±25V,” the HPF Cutoff is fixed at DC.

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WBK18, pg. 7

Source Level – Source Level refers to the transducer bias current and is not to be confused with theexcitation source that is discussed on pages 4 and 14. The current Source Level column of WaveView’s
main window is used to turn the transducer bias current on at a current value of 4 mA,or to turn the transducer bias current off. Click on a cell in the Source Level column to make the cell
active, and then change its setting to 4 mA or to off, according to the application. If a channel isconnected to a transducer that requires a current source, set the source level to 4 mA; otherwise set thesource level to off.

TEDS (Transducer Electronic Data Sheet)
TEDS is a purchased option that enables WBK18 modules to access calibration information from TEDS-compatible
sensors. The WBK18 automatically scales the readings and sets the range according to the information stored on thesensor. This is done independently for each TEDS associated channel, providing that “Yes” appears in the TEDS
Data cell (right-hand column, following figure).

WaveView Configuration Window
If no WBK18 channels are connected to a TEDS sensor, the entire TEDS
Data column, including the heading, will be grayed-out. When a channel
does have a TEDS sensor it will have an associated cell. You can click on
the cell to access the “Use TEDS Data” pull-down list, which offers 3
choices: No, Yes, and Show.
• “No” instructs WaveView not to use TEDS. When TEDS is not used

the associated channel will use the default range and units of volts(V).
•“Yes” instructs WaveView to use TEDS. The channel’s ranges will
be automatically scaled according to the TEDS sensor’s calibration
data and the units will appear as “g.”• “Show” accesses an Accelerometer TEDS Information box for the

associated channel. An example is provided to the right. The
channel, in this case channel 9, is identified in the title bar. When theinformation box is closed the TEDS Data cell will indicate its
previous status of Yes or No.

Accelerometer TEDS Information Box

If you add, remove, or relocate a TEDS sensor at the WBK18 channel inputs, the TEDS information,and WaveView’s range and units will not reflect the change until either (a) the WaveBook is
reselected as a device, or (b) WaveView is closed and then reopened.
WBK18, pg. 8926896

WBK18, Dynamic Signal Input Module

Maximizing Alias Protection
What is Aliasing?
Aliasing is a phenomenon of sampled data systems wherein a high frequency signal is misrepresented as a
low frequency signal when the A/D converter sampling rate being used is too slow. This misrepresentation
can result in severe data corruption and incorrect FFT results. Aliasing is a well-documented dataacquisition effect, and interested users are encouraged to research detailed information that is available online from companies such as Analog Devices and Texas Instruments. This text aims to not supplant thoseresources, but to provide most users with sufficient knowledge to avoid most alias problems throughproper filter and sampling rate configuration.
For a given sampling rate, FS, input signals of frequency up to FS/2 will be processed correctly. However,
input signals above FS/2 are subject to aliasing. For example, a sampling rate of 100 kHz can process
signals up to 50 kHz without aliasing. An input signal of 90 kHz, however, will be aliased. Specifically, it
will appear in the sampled data as a signal of frequency FS-FIN, which in this case is 100 kHz-90 kHz = 10
kHz.
Aliasing, and its prevention, should be a consideration in all sampled data systems. This is especially
important in mechanical vibration measurements, because most mechanical systems exhibit a resonanceapart from their fundamental frequency. That is, there may be signal energy present that has the potential
to be aliased that is unknown to the user. And the worst part of aliasing is that its effects areindistinguishable from real input signals. That is, in the given example, it is not apparent to the userwhether the 10 kHz energy is real or an alias.
Aliasing Protection using the WBK18
The WBK18 provides alias rejection via its 8-pole filter. This filter has anextremely steep roll-off characteristic, very closely achieving an ideal “brickwall” response. It consequently passes frequencies of interest without
significant attenuation, but significantly attenuates frequencies just above. Its
attenuation is so high that most alias frequency energy is reduced to a level
below the noise floor of the measurement system. However, it must be
configured correctly to achieve these results. In general, the cutoff frequency(FC) of the filter should be set as close to, but above, the highest input
frequency of interest. This will maximize the alias rejection it provides.
The 8-pole filter provides excellent filter response. However, no filter isperfect, meaning that some signal attenuation occurs for frequencies justbelow FC and maximum attenuation is not exhibited for frequencies justabove FC.
For reference, the typical response of the 8-pole filter is provided in the table
at the right and the graphs that follow.

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FIN/FC
<0.1
0.1
0.2
0.3

Gain (dB)
-0.15
-0.15
-0.18
-0.22

0.4
0.5
0.6
0.7
0.8
0.9
1.0
1.25
1.5
1.75
2.0
2.5
2.8
3.0
3.3
3.5
4.0

-0.27
-0.33
-0.39
-0.47
-0.68
-1.4
-3.6
-16
-28
-39
-48
-63
-70
-75
-80
-86
-95

WBK18, pg. 9

Gain of 8-pole Filter Mode
0

0.5

1

1.5

2

2.5

3

3.5

4

0

Gain (dB)

-20
-40
-60
-80
-100
FIN/FC

Gain of 8-pole Filter Mode
0

0.2

0.4

0.6

0.8

1

0

Gain (dB)

-2
-4
-6
-8
-10
-12
-14
FIN/FCFrequency Region
FIN/FC, Zoom-In to Filter Cutoff

As described above, aliasing results from the relationship between input frequency and sampling
frequency. Configuring the filter correctly serves to attenuate undesired frequencies. However, thought
must also be given to the sampling rate of the A/D converter. In general, for alias considerations, thesampling rate should be set as high as possible, given the number of active channels being used. Recall
that the maximum sampling rate is 1 MHz/(n +1) where n is the number of active channels. Because thesampling rate determines the frequency at which aliasing occurs, it determines the input signal bandwidth,
for a given level of alias rejection. This relationship is shown in the following example.
Example# of channels: 4
Alias rejection: -70dB min
The sampling rate (FS) is chosen to be the maximum of 1 MHz/(4 +1) = 200 kHz. The alias frequency is
FS/2, or 100 kHz. Referring to the attenuation table, to achieve a minimum of –70dB of alias rejection,
there must be at least a 2.8 ratio between FIN and FC. For the FIN value of 100 kHz, this translates into amaximum value of FC of 100 kHz / 2.8 = 35.7 kHz. The largest available FC value that satisfies thiscondition is 20 kHz. The input signal bandwidth for this case is then 20 kHz.

WBK18, pg. 10926896

WBK18, Dynamic Signal Input Module

1.2

Using the 2-pole Filter and Bypass
2-pole Filter Mode
For applications where the signal of interest is entirely AC in nature, the low-pass filter mode of 8-pole isthe best choice. Vibration signals coupled through an ICP accelerometer are an example of this. However,for applications where the DC component of the input signal is also of importance, 2-pole mode may
provide better results. Proximity sensor measurements are an example of this. This is because the 8-poleswitched capacitor filter, while providing excellent attenuation characteristics, does not process DC signals
with a high level of accuracy. For accelerometer applications this is not a limitation, as there is no
information in the DC component of the input signal. The 2-pole filter, in contrast, is formed by two 1pole RC filters in series. This filter provides excellent passband accuracy, at the expense of a more gradualroll-off characteristic, as detailed below.

Gain of 2-pole Filter Mode
0

10

20

30

40

50

60

70

80

90

100

3.5

4

4.5

5

0
-10
Gain (dB)

-20
-30
-40
-50
-60
-70
-80
FIN/FC

Gain of 2-pole Filter Mode
0

0.5

1

1.5

2

2.5

3

0

Gain (dB)

-5
-10
-15
-20
-25

FIN/FC, Zoom-In to Filter Cutoff Frequency Region

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WBK18, pg. 11

Bypass Mode
Bypass mode also provides excellent passband accuracy and provides minimal signal attenuation up tovery high frequencies for those applications that need to measure signals of frequency exceeding 20 kHz.
For reference, the typical roll-off characteristic of Bypass mode is the following:

Gain of Bypass Mode

Gain (dB)

0

25

50

75

100

125

150

175

200

225

250

35

40

45

50

0
-0.5
-1
-1.5
-2
-2.5
-3
-3.5
-4
-4.5
FIN (kHz)Gain of Bypass Mode
0

5

10

15

20

25

30

0

Gain (dB)

-0.05
-0.1
-0.15
-0.2
-0.25
-0.3

FIN (kHz), Zoom-In to Filter Cutoff Frequency Region

WBK18, pg. 12926896

WBK18, Dynamic Signal Input Module

DC Accuracy
As previously mentioned, the 2-pole and Bypass filter modes are most commonly used in applications
where DC signal information is important. The AC response of each of these modes is described above.
The DC accuracy, excluding noise, for both modes is:
Accuracy at 0° to 50°C (32° to 122°F)
Range± % of Reading
TypicalMaximum

Offset

±25V

0.5

1

±15mV

±5V

0.15

0.3

±3mV

±2.5V

0.15

0.3

±2mV

±1V

0.15

0.3

±1mV

±500mV0.15

0.3±900µV±250mV0.15

0.3±800µV±100mV0.15

0.3±800µV

±50mV

0.15

0.3

±800µV

±25mV

0.2

0.4

±800µV

These numbers are valid for 1 year after calibration and over the entire operating temperature rangeof the unit.

Module Configuration
Overrange Detection
The configuration of overrange detection is done through the
Module Configuration window. The Module Configuration
window can be accessed from the View pull-down menu or byuse of the first toolbar button (located just below the File pulldown menu). In this window, the user enables/disables
overrange detection on a per channel basis. A checkmark next tothe channel number indicates that overrange detection is enabled
for that channel. The overrange detection level is also set in thisscreen. It is set as a percentage of range that applies to allchannels of the WBK18 unit being configured. After channel
enable and level selections are made, the “Apply” button must be
clicked to accept the changes.

Module Configuration Window
When configuring overrange detection, after channel enable and level selections are made, the<Apply> button must be clicked to accept the changes.

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WBK18, pg. 13

Excitation Source
In order to configure the excitation source, click on the Configure Sine Wave Output button in the Module
Configuration window. This brings up a secondary window in which the excitation source is configured. Do notconfuse excitation source with the Source Level column in WaveView’s main window.
Continuous Mode
Continuous mode refers to a continuously running sine
wave of the selected amplitude and frequency. To
configure, select a frequency and amplitude, and then click“Start.” The selected output will begin and continue
running until the <Stop> button is clicked or WaveView isterminated.
Note: You can save output sine wave configuration files
and open pre-saved files as discussed in the upcoming
section, How to Save or Open Output Sine Wave
Configuration Files, page 17.

Continuous Tab Selected
Sweep Mode
Sweep mode refers to a constant amplitude sine wave thatis being swept in frequency from a selected start frequency
to a selected stop frequency over a selected sweep time
duration. The frequency sweep characteristic can bechosen to be linear or logarithmic, and is distributed among
1280 discrete steps. The transitions between steps arecontinuous in phase and in amplitude.
To configure, make selections for the available parameters,
and then click the <Start> button. Once a sweep iscompleted, the waveform returns to its start frequency andis swept again and again until stopped by the user or
WaveView is terminated.
Note: You can save output sine wave configuration files
and open pre-saved files as discussed in the upcoming
section, How to Save or Open Output Sine Wave
Configuration Files, page 17.
Sweep Tab Selected

WBK18, pg. 14926896

WBK18, Dynamic Signal Input Module

Sweep Mode (continued)

Example of a Linear Sweep Waveform

Example of a Log Sweep Waveform

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WBK18, pg. 15

Custom ModeIn this mode, the user can create customized waveforms built out of specified sine wave-based
components. For example, a waveform could be 1V, 1 kHz for 2 seconds, followed by 5V, 100 Hz for 5
seconds, and then 2V, 500 Hz for 1 second. Up to 1280 distinct points can be entered, providing thecapability to create a virtually unlimited waveform set. Within this mode, there is also an amplitudeselection of 0 mV. This corresponds to an active zero voltage and is used to create off time in a voltage
waveform. Programming of this mode is done by creating/editing a list of output amplitude/frequency
points. After the desired list is entered, the waveform output is begun by clicking “Start.” Once thewaveform sequence completes, it returns to the first entry in the list and cycles through again and again
until stopped by the user.
Note: You can save output sine wave configuration files and open pre-saved files as discussed in thefollowing section, How to Save or Open Output Sine Wave Configuration Files.

Setting Up Custom Waveforms from the Custom Tab

Example of Waveforms Created in the Custom Mode

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WBK18, Dynamic Signal Input Module

How to Save or Open Output Sine Wave Configuration Files
Within all modes, there is the ability to save and recall waveform configurations, which is very beneficial
for complex custom configurations. Within WaveView, this feature is accessed through File in the
WBK18 Output Sine Wave Configuration Window.
To Save a Configuration
1.

Click on “File” in the upper left corner of the screen.

2.

Click on the option labeled “Save Waveform Configuration As…”

3.

Name the file. Note that it will have a .dds extension.

4.

Save the file to the desired drive.

To Open a Configuration
1.

Click on “File” in the upper left corner of the screen.

2.

Click on the option labeled “Open Waveform Configuration…”

3.

Open the desired file.

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Using Accelerometers
Overview
A low-impedance piezoelectric accelerometer consists of a piezoelectric crystal and an electronic amplifier.
When stretched or compressed, the two crystal surfaces develop a charge variation that is related to theamount of stress, shock, or vibration on the crystal. The amplifier outputs a corresponding signal andtransforms the sensor’s high impedance to a lower output impedance of a few hundred ohms. Note that, in
addition to acceleration, these sensors can also measure pressure and force.
The circuit requires only two wires (coax or twisted pair) to transmit both power and signal. At low
impedance, the system is insensitive to external or “triboelectric” cable noise. Cable length does not affectsensitivity.
The following figure shows a simple sensor-WBK18 connection. The voltage developed across R isapplied to the gate of the MOSFET. The MOSFET is powered from a constant current source of
4 mA and 30 volts.

The MOSFET circuit will bias at approximately 12 V in the quiet state. As the system is excited, voltage isdeveloped across the crystal and applied to the gate of the MOSFET. This voltage will cause linear
variation in the impedance of the MOSFET and a proportional change in bias voltage. This voltage change
will be coupled to the WBK18 input amplifier through the capacitor C. The value of R and the internal
capacitance of the piezoelectric crystal control the low frequency corner. Units weighing only a few grams
can provide high-level outputs up to 1 V/g with response to frequencies below 1 Hz.

Accelerometer Specification Parameters
Noise in Accelerometers
The noise floor or resolution specifies the lowest discernible amplitude (minimum “g”) that can bemeasured. There are two main sources of noise as follows:• Noise from the crystal and microcircuit inside the accelerometer. Some types of crystals, such as
quartz, are inherently noisier than others. A good noise floor is 10 to 20 µV.
• Noise from electrical activity on the mounting surface. Since the signal from the accelerometer is a
voltage, 60 Hz or other voltages (ground loop, etc) can interfere with the signal. The best protection
is to electrically isolate the accelerometer.

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Sensitivity
The sensitivity of an accelerometer is defined as its output voltage per unit input of motion. The unitof motion used is “g.” One “g” is equal to the gravitational acceleration at the Earth’s surface, which is
32.2 ft/(sec)(sec) or 981 cm/(sec)(sec). The output is usually specified in millivolts per “g” (mV/g).
Sensitivity is usually specified under defined conditions such as frequency, testing levels, and temperature.
An example: 100 mV/g at a frequency of 100 Hz, level +1 g, at 72°F. Note that, although a sensor may
have a “typical” sensitivity of 100 mV/g, its actual sensitivity could range from 95 to 105 mV/g (whenchecked under stated conditions). Manufacturers usually provide sensor calibration values.
Transverse Sensitivity - An accelerometer is designed to have one major axis of sensitivity, usuallyperpendicular to the base and co-linear with its major cylindrical axis. The output caused by the motion
perpendicular to the sensing axis is called transverse sensitivity. This value varies with angle andfrequency and typically is less than 5% of the basic sensitivity.
Base-Strain Sensitivity - An accelerometer’s base-strain sensitivity is the output caused by a deformationof the base, due to bending in the mounting structure. In measurements on large structures with low
natural frequencies, significant bending may occur. Units with low base-strain sensitivity should beselected. Inserting a washer (smaller in diameter than the accelerometer base) under the base reduces
contact surface area; and can substantially reduce the effects of base-strain. Note that this technique lowers
the usable upper frequency range.
Acoustic Sensitivity - High-level acoustic noise can induce outputs unrelated to vibration input. In
general, the effect diminishes as the accelerometer mass increases. Use of a light, foam-rubber boot may
reduce this effect.
Frequency Response
An accelerometer’s frequency response is the ratio of the sensitivity measured at frequency (f) to the basic
sensitivity measured at 100 Hz. This response is usually obtained at a constant acceleration level, typically
1 g or 10 g. Convention defines the usable range of an accelerometer as the frequency band in which thesensitivity remains within 5% of the basic sensitivity. Measurements can be made outside these limits if
corrections are applied. Care should be taken at higher frequencies because mounting conditions greatly
affect the frequency range (see Mounting Effects, in upcoming text).
Dynamic Range
The dynamic measurement range is the ratio of the maximum signal (for a given distortion level) to theminimum detectable signal (for a given signal-to-noise ratio). The dynamic range is determined by several
factors such as sensitivity, bias voltage level, power supply voltage, and noise floor.
Bias Level
Under normal operation, a bias voltage appears from the output signal lead to ground. There are two basic
MOSFET configurations commonly used. One exhibits a 7-8 V bias and the second a 9-12 V bias.
Operation of the two circuits is identical except for the available signal swing.
Thermal Shock - Temperature Transients
Piezoelectric accelerometers exhibit a transient output that is a function of a temperature’s “rate-ofchange.” This “thermal shock” is usually expressed in g/°C and is related to:• Non-uniform mechanical stresses set up in the accelerometer structure.
• A pyroelectric effect in piezoelectric materials—an electrical charge is produced by thetemperature gradient across the crystal.
This quasi-static effect produces a low-frequency voltage input to the MOSFET amplifier. This voltage isusually well below the low-frequency corner, but the effect can reduce the peak clipping level and cause
loss of data. This effect does not affect the accelerometer’s basic sensitivity or the data unless the thermal
shift in the operation bias level results in clipping. Where drastic thermal shifts are expected, use 12 V bias
models. The effect’s severity is related to the mass of the accelerometer. In 100 mV/g industrial units, theeffect is usually negligible. Using rubber thermal boots can reduce the effect significantly.

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Overload Recovery
Recovery time from clipping due to over-ranging is typically less than 1 ms. Recoveries from quasi-static
overloads that generate high DC bias shifts are controlled by the accelerometer input RC time constant thatis fixed during manufacture.
Connector
This parameter specifies the connector type and size (4-48, 6-40, 10-32 coaxial etc) and the location on thesensor, that is, top or side (usually on the hex base). Where there is no connector on the sensor, an integral
cable is specified with the length and the connector, that is, integral 6-ft to 10-32.

Electrical Grounding
Case-Grounded Design
In case-grounded designs, the common lead on the internal impedance matching electronics is tied to theaccelerometer case. The accelerometer base/stud assembly forms the signal common and electricallyconnects to the shell of the output connector. Case-grounded accelerometers are connected electrically to
any conductive surface on which they are mounted. When these units are used, take care to avoid errors
due to ground noise.
Isolated-Base Design
To prevent ground noise error many accelerometers have base-isolated design. The outer case/base of theaccelerometer is isolated electrically off ground by means of an isolation stud insert. The proprietary
material used to form the isolation provides strength and stiffness to preserve high-frequency performance.

Cable Driving
Operation over long cables is a concern with all types of sensors. Concerns involve cost, frequency
response, noise, ground loops, and distortion caused by insufficient current available to drive the cablecapacitance.
The cost of long cables can be reduced by coupling a short (1 m) adapter cable from the accelerometer to along low-cost cable like RG-58U or RG-62U with BNC connectors. Since cable failure tends to occur at
the accelerometer connection where the vibration is the greatest, only the short adapter cable would needreplacement.
Capacitive loading in long cables acts like a low-pass, second-order filter and can attenuate or amplify
high-frequency signals depending on the output impedance of the accelerometer electronics. Generally thisis not a problem with low-frequency vibration (10 Hz to 2000 Hz). For measurements above 2000 Hz andcables longer than 100 ft, the possibility of high-frequency amplification or attenuation should beconsidered.
The maximum frequency that can be transmitted over a given length of cable is a function of both the cablecapacitance and the ratio of the maximum peak signal voltage to the current available from the constantcurrent source:f =WBK18, pg. 20

K
 V 

2πC
 Icc − Ib 

Drive Current

Cable Length(mA)@30 pF/ft (Ft)

Frequency Response to 5% ofMaximum Output Signal Amplitude
±1V

±5V

4

10

550 kHz110 kHz

4100

55 kHz

11 kHz41000

5.5 kHz

1.1 kHz

Where:
f = Maximum frequency in Hz
9
K = 3.45 ×10 . K is the scale factor to convert Farads to picoFarads and Amperes to milliAmperes anda factor to allow cable capacitance to charge to 95% of the final charge.
C = Cable capacitance in picoFarads
V = Maximum peak measured voltage from sensor in volts
Icc = Constant current from current source in mA
Ib = Current required to bias the internal electronics, typically 1 mA
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Fuse Replacement – for WBK18

CAUTION
Turn OFF the power to, and UNPLUG the WBK18 module and all connected equipment.
Remove all signal I/O lines from the unit. Electric shock or damage to equipment can result
even under low-voltage conditions.
Take ESD precautions, to include using a grounded wrist strap.
Use care to avoid touching board surfaces and onboard components. Ensure boards do notcome into contact with foreign elements such as oils, water, and industrial particulate.
You should only replace a fuse if your device shows no sign of damage. If your device appears
damaged such as evidenced by a “smoked” component, contact the factory as soon as possible.
If the replacement fuse blows, contact the factory as this indicates a problem may
exist with your WBK18 module.

Each WBK18 has one user-replaceable fuse designated as F900.
F900 Input Power Fuse. 4.0 A, MINI ATO.
This 4-amp fuse is located near the rear panel’s 5DIN POWER IN connector.
If this fuse has blown the WBK18 module will not power up.
Factory Part Number: FU-8-4
Littelfuse Part Number: 297-004, Littelfuse Body Color Code: Pink
You will need the following:••••

Phillips Screwdriver
3AG Fuse Puller, or needle-nose pliers*
Grounding wrist strap and associated anti-static pad
Replacement fuse F900

* Needle-nose pliers can be used to pull MINI ATO fuses; but should not be used to insert fuses.

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WBK18, pg. 21

1.

If you have not already done so, turn OFF the power to, and UNPLUG the WBK18 module andall connected equipment. Remove all signal I/O lines from the unit.

2.

Using a Phillips screwdriver, remove the four Cover Plate Screws from the left and right sidesof the unit. The following figure points out the screw locations.

3.

Remove the Cover Plate [not shown].

Cover Plate
Screw Locations

Cover Plate
Screw Locations

F900
F900 Fuse Location in a WBK18 Module4.

Locate the F900 fuse. It is located near the rear panel edge, close to the DIN5 POWER IN connector.

5.

While wearing a grounded wrist strap, remove and replace the bad fuse. Ensure that the new fuse is fully
seated.

6.

Replace the Cover Plate and secure it to the chassis with the 4 screws that were removed in step 2.

7.

Return the WBK18 module to normal service. Should any problems be noted, consult the factory.

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WBK18, Dynamic Signal Input Module

Specifications – WBK18

Specifications are subject to change without notice.

GeneralSystem Connectors: BNC connector, mates with expansion signal input on the WaveBook; female DB15
connector, mates with expansion control signal on the WaveBook.
Input Power Range: 10 to 30 VDC
Input Power Fuse F900: 4A MINI ATO, user replaceable; refer to page 21 for details.
Power Consumption@ 12V: 1.6A
@ 15V: 1.3A
@ 24V: 0.8A
Environment
Operating: 0° to 50°C; 0 to 95% RH, non-condensing
Storage: 0° to 70°C
Vibration: MIL STD 810E, category 1
Dimensions: 280 mm W x 216 mm D x 42 mm H (11” x 8.5” x 1.65”)
Weight: 1.3 kg (2.9 lbs)

Analog Inputs
Channels: 8
Signal Connection: 1 BNC per channel
Input Impedance: 200k Ohm (single-ended)
Input Coupling: AC, DC (software programmable per channel)
High-Pass Filter: 0.1 Hz or 10 Hz (software programmable per channel)
Input Ranges: ±25V (DC coupled only), ±5V, ±2.5V, ±1V, ±500mV, ±250mV, ±100mV, ±50mV, ±25mV(software programmable per channel)
Overrange Detection: Programmable from 1% to 100% of range
Overrange Indication: Front panel LED per channel, software status

Low-Pass Filter (software programmable per channel)
Type: 8-pole Butterworth with simultaneous sample-and-hold (SSH)
Cutoff Frequency (Fc): 10 Hz to 50 kHz in 1-2-5 progression
Alias Rejection: 75dB min
Channel-to-Channel Phase Matching*: 1° typ, 2° max
Unit-to-Unit Phase Matching*:

1° typ, 2° max

SSH latency: 100ns max
Amplitude Accuracy**:±0.5dB (Fin ≤ Fc/2)

Total Harmonic Distortion: -70dB typ
ICP Bias Source: 4mA, 24V compliance (on/off software programmable per channel)
ICP Fault Detection Thresholds: <1V (short), >25V (open)
ICP Fault Indication: Front panel LED per channel, software status* Conditions for Low-Pass Filter Phase-Matching
8-pole LPF mode, 0.1 Hz or DC HPF mode
1 Hz ≤ Fin ≤ Fc/2
200 Hz ≤ Fc ≤ 20 kHz
All WBK18 units connected to same WaveBook** Condition for Amplitude Accuracy
For Fin < 20 kHz

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Excitation Source
Channels: 1
Signal Connection: BNC
Frequency Range: 1 Hz to 5 kHz
Frequency Resolution: 0.01 Hz
Amplitude Settings (p-p): 10V, 5V, 2V, 1V, 500mV, 200mV, 100mV, 0mV
Waveform Modes: Continuous sine, Sweep sine, Custom sine
Output Impedance: 50 Ohm
Accuracy: ±0.1dB

DC Accuracy, Excluding Noise
Applies to 2-Pole and Bypass Filter Modes
Accuracy at 0° to 50°C (32° to 122°F)
Range± % of Reading
TypicalMaximum

Offset

±25V

0.5

1

±15mV

±5V

0.15

0.3

±3mV

±2.5V

0.15

0.3

±2mV

±1V

0.15

0.3

±1mV

±500mV

0.15

0.3

±1mV

±250mV

0.15

0.3

±1mV

±100mV

0.15

0.4

±1mV

±50mV

0.15

0.4

±1mV

±25mV

0.2

0.4

±1mV

These numbers are valid for 1 year after calibration and over theentire operating temperature range of the unit.

Specifications are continued on following page.

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Typical Performance Characteristics
WBK18 Frequency Spectrums (typical)
Each spectrum was taken from a WaveBook/516A that was sampling at 20kSamples/sec,
4096-point FFT, B-H Window.
3 Vpp, 1000Hz Sine wave input; ±5V range, 10Hz High pass filter, 10 kHz 8-pole Low pass filter.

8 Vpp, 1000Hz Sine wave input; ±5V range, 10Hz High pass filter, 10 kHz 2-pole Low pass filter.

8 Vpp, 1000Hz Sine wave input; ±5V range, 10Hz High pass filter, 200 kHz Low pass filter(Bypass mode).

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WBK18, pg. 26

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