AD AD598

a
FEATURES
Single Chip Solution, Contains Internal Oscillator and
Voltage Reference
No Adjustments Required
Insensitive to Transducer Null Voltage
Insensitive to Primary to Secondary Phase Shifts
DC Output Proportional to Position
20 Hz to 20 kHz Frequency Range
Single or Dual Supply Operation
Unipolar or Bipolar Output
Will Operate a Remote LVDT at Up to 300 Feet
Position Output Can Drive Up to 1000 Feet of Cable
Will Also Interface to an RVDT
Outstanding Performance
Linearity: 0.05% of FS max
Output Voltage: 611 V min
Gain Drift: 50 ppm/8C of FS max
Offset Drift: 50 ppm/8C of FS max
PRODUCT DESCRIPTION
The AD598 is a complete, monolithic Linear Variable Differential Transformer (LVDT) signal conditioning subsystem. It is
used in conjunction with LVDTs to convert transducer mechanical position to a unipolar or bipolar dc voltage with a high
degree of accuracy and repeatability. All circuit functions are
included on the chip. With the addition of a few external passive
components to set frequency and gain, the AD598 converts the
raw LVDT secondary output to a scaled dc signal. The device
can also be used with RVDT transducers.
LVDT Signal
Conditioner
AD598
FUNCTIONAL BLOCK DIAGRAM
EXCITATION (CARRIER)
3
2
VA
11
OSC
AMP
AD598
17
LVDT
10
A–B
A+B
FILTER
AMP
16
VOUT
VB
PRODUCT HIGHLIGHTS
1. The AD598 offers a monolithic solution to LVDT and
RVDT signal conditioning problems; few extra passive components are required to complete the conversion from mechanical position to dc voltage and no adjustments are
required.
2. The AD598 can be used with many different types of
LVDTs because the circuit accommodates a wide range of
input and output voltages and frequencies; the AD598 can
drive an LVDT primary with up to 24 V rms and accept secondary input levels as low as 100 mV rms.
The AD598 contains a low distortion sine wave oscillator to
drive the LVDT primary. The LVDT secondary output consists
of two sine waves that drive the AD598 directly. The AD598
operates upon the two signals, dividing their difference by their
sum, producing a scaled unipolar or bipolar dc output.
3. The 20 Hz to 20 kHz LVDT excitation frequency is determined by a single external capacitor. The AD598 input signal need not be synchronous with the LVDT primary drive.
This means that an external primary excitation, such as the
400 Hz power mains in aircraft, can be used.
The AD598 uses a unique ratiometric architecture (patent pending) to eliminate several of the disadvantages associated with
traditional approaches to LVDT interfacing. The benefits of this
new circuit are: no adjustments are necessary, transformer null
voltage and primary to secondary phase shift does not affect system accuracy, temperature stability is improved, and transducer
interchangeability is improved.
4. The AD598 uses a ratiometric decoding scheme such that
primary to secondary phase shifts and transducer null voltage
have absolutely no effect on overall circuit performance.
The AD598 is available in two performance grades:
Grade
Temperature Range Package
AD598JR 0°C to +70°C
AD598AD –40°C to +85°C
20-Pin Small Outline (SOIC)
20-Pin Ceramic DIP
It is also available processed to MIL-STD-883B, for the military
range of –55°C to +125°C.
5. Multiple LVDTs can be driven by a single AD598, either in
series or parallel as long as power dissipation limits are not
exceeded. The excitation output is thermally protected.
6. The AD598 may be used in telemetry applications or in hostile environments where the interface electronics may be remote from the LVDT. The AD598 can drive an LVDT at
the end of 300 feet of cable, since the circuit is not affected
by phase shifts or absolute signal magnitudes. The position
output can drive as much as 1000 feet of cable.
7. The AD598 may be used as a loop integrator in the design of
simple electromechanical servo loops.
REV. A
Information furnished by Analog Devices is believed to be accurate and
reliable. However, no responsibility is assumed by Analog Devices for its
use, nor for any infringements of patents or other rights of third parties
which may result from its use. No license is granted by implication or
otherwise under any patent or patent rights of Analog Devices.
One Technology Way, P.O. Box 9106, Norwood, MA 02062-9106, U.S.A.
Tel: 617/329-4700
Fax: 617/326-8703
AD598–SPECIFICATIONS
(typical @ +258C and 615 V dc, C1 = 0.015 mF, R2 = 80 kV, RL = 2 kV,
unless otherwise noted. See Figure 7.)
Parameter
Min
AD598J
Typ
TRANSFER FUNCTION1
VOUT =
OVERALL ERROR2
TMIN to TMAX
0.6
SIGNAL OUTPUT CHARACTERISTICS
Output Voltage Range (TMIN to TMAX)
Output Current (TMIN to TMAX)
Short Circuit Current
Nonlinearity3 (TMIN to TMAX)
Gain Error4
Gain Drift
Offset5
Offset Drift
Excitation Voltage Rejection6
Power Supply Rejection (± 12 V to ± 18 V)
PSRR Gain (TMIN to TMAX)
PSRR Offset (TMIN to TMAX)
Common-Mode Rejection (± 3 V)
CMRR Gain (TMIN to TMAX)
CMRR Offset (TMIN to TMAX)
Output Ripple7
EXCITATION OUTPUT CHARACTERISTICS (@ 2.5 kHz)
Excitation Voltage Range
Excitation Voltage
(R1 = Open)8
(R1 = 12.7 kΩ)8
(R1 = 487 Ω)8
Excitation Voltage TC9
Output Current
TMIN to TMAX
Short Circuit Current
DC Offset Voltage (Differential, R1 = 12.7 kΩ)
TMIN to TMAX
Frequency
Frequency TC, (R1 = 12.7 kΩ)
Total Harmonic Distortion
SIGNAL INPUT CHARACTERISTICS
Signal Voltage
Input Impedance
Input Bias Current (AIN and BIN)
Signal Reference Bias Current
Excitation Frequency
POWER SUPPLY REQUIREMENTS
Operating Range
Dual Supply Operation (± 10 V Output)
Single Supply Operation
0 to +10 V Output
0 to –10 V Output
Current (No Load at Signal and Excitation Outputs)
TMIN to TMAX
TEMPERATURE RANGE
JR (SOIC)
AD (DIP)
PACKAGE OPTION
SOIC (R-20)
Side Brazed DIP (D-20)
Max
Min
VA –VB
VA +VB
× 500 µA × R2
2.35
611
8
AD598A
Typ
Max
0.6
V
1.65
611
6
20
75
0.4
20
0.3
7
100
20
75
0.4
20
0.3
7
100
6500
61
6100
61
6200
Unit
6500
61
650
61
650
% of FS
V
mA
mA
ppm of FS
% of FS
ppm/°C of FS
% of FS
ppm/°C of FS
ppm/dB
300
100
100
15
400
200
100
15
ppm/V
ppm/V
100
100
25
6
4
200
200
25
6
4
ppm/V
ppm/V
mV rms
2.1
24
2.1
24
V rms
1.2
2.6
14
2.1
4.1
20
1.2
2.6
14
2.1
4.1
20
V rms
V rms
V rms
ppm/°C
mA rms
mA rms
mA
6100
20k
mV
Hz
ppm/°C
dB
3.5
V rms
kΩ
µA
µA
kHz
600
600
30
12
30
12
60
30
20
60
6100
20k
30
20
200
–50
0.1
200
–50
3.5
200
1
2
0
13
± 13
5
10
20
36
17.5
17.5
0.1
200
1
2
0
13
± 13
5
10
20
36
17.5
17.5
12
0
12
15
16
15
18
V
V
mA
mA
+85
°C
°C
+70
–40
V
V
AD598JR
AD598AD
–2–
REV. A
AD598
NOTES
1
VA and VB represent the Mean Average Deviation (MAD) of the detected sine waves. Note that for this Transfer Function to linearly represent positive displacement,
the sum of V A and VB of the LVDT must remain constant with stroke length. See “Theory of Operation.” Also see Figures 7 and 12 for R2.
2
From TMIN, to TMAX, the overall error due to the AD598 alone is determined by combining gain error, gain drift and offset drift. For example the worst case overall
error for the AD598AD from TMIN to TMAX is calculated as follows: overall error = gain error at +25°C (± 1% full scale) + gain drift from –40°C to +25°C (50 ppm/°C
of FS × +65°C) + offset drift from –40°C to +25°C (50 ppm/°C of FS × +65°C) = ± 1.65% of full scale. Note that 1000 ppm of full scale equals 0.1% of full scale.
Full scale is defined as the voltage difference between the maximum positive and maximum negative output.
3
Nonlinearity of the AD598 only, in units of ppm of full scale. Nonlinearity is defined as the maximum measured deviation of the AD598 output voltage from a
straight line. The straight line is determined by connecting the maximum produced full-scale negative voltage with the maximum produced full-scale positive voltage.
4
See Transfer Function.
5
This offset refers to the (V A–VB)/(VA+VB) input spanning a full-scale range of ± 1. [For (VA–VB)/(VA+VB) to equal +1, V B must equal zero volts; and correspondingly
for (VA–VB)/(VA+VB) to equal –1, VA must equal zero volts. Note that offset errors do not allow accurate use of zero magnitude inputs, practical inputs are limited to
100 mV rms.] The ± 1 span is a convenient reference point to define offset referred to input. For example, with this input span a value of R2 = 20 k Ω would give
VOUT span a value of ± 10 volts. Caution, most LVDTs will typically exercise less of the ((V A–VB))/((VA+VB)) input span and thus require a larger value of R2 to
produce the ± 10 V output span. In this case the offset is correspondingly magnified when referred to the output voltage. For example, a Schaevitz E100 LVDT
requires 80.2 kΩ for R2 to produce a ± 10.69 V output and (V A–VB)/(VA+VB) equals 0.27. This ratio may be determined from the graph shown in Figure 18,
(VA–VB)/(VA+VB) = (1.71 V rms – 0.99 V rms)/(1.71 V rms + 0.99 V rms). The maximum offset value referred to the ± 10.69 V output may be determined by
multiplying the maximum value shown in the data sheet (± 1% of FS by 1/0.27 which equals ± 3.7% maximum. Similarly, to determine the maximum values of offset
drift, offset CMRR and offset PSRR when referred to the ± 10.69 V output, these data sheet values should also be multiplied by (1/0.27). For this example for the
AD598AD the maximum values of offset drift, PSRR offset and CMRR offset would be: 185 ppm/ °C of FS; 741 ppm/V and 741 ppm/V respectively when referred
to the ± 10.69 V output.
6
For example, if the excitation to the primary changes by 1 dB, the gain of the system will change by typically 100 ppm.
7
Output ripple is a function of the AD598 bandwidth determined by C2, C3 and C4. See Figures 16 and 17.
8
R1 is shown in Figures 7 and 12.
9
Excitation voltage drift is not an important specification because of the ratiometric operation of the AD598.
Specifications subject to change without notice.
Specifications shown in boldface are tested on all production units at final electrical test. Results from those tested are used to calculate outgoing quality levels. All
min and max specifications are guaranteed, although only those shown in boldface are tested on all production units.
ORDERING GUIDE
THERMAL CHARACTERISTICS
SOIC Package
Side Brazed Package
θJC
θJA
22°C/W
25°C/W
80°C/W
85°C/W
Model
Temperature
Range
Package
Description
Package
Option
AD598JR
AD598AD
0°C to +70°C
–40°C to +85C
SOIC
Ceramic DIP
R-20
D-20
ABSOLUTE MAXIMUM RATINGS
Total Supply Voltage +VS to –VS . . . . . . . . . . . . . . . . . +36 V
Storage Temperature Range
R Package . . . . . . . . . . . . . . . . . . . . . . . . . –65°C to +150°C
D Package . . . . . . . . . . . . . . . . . . . . . . . . . –65°C to +150°C
Operating Temperature Range
AD598JR . . . . . . . . . . . . . . . . . . . . . . . . . . . . 0°C to +70°C
AD598AD . . . . . . . . . . . . . . . . . . . . . . . . . . –40°C to +85°C
Lead Temperature Range (Soldering 60 sec) . . . . . . . . +300°C
Power Dissipation Up to +65°C . . . . . . . . . . . . . . . . . . . 1.2 W
Derates Above +65°C . . . . . . . . . . . . . . . . . . . . . . . 12 mW/°C
–VS
EXC 1 2
19 OFFSET 1
EXC 2 3
18 OFFSET 2
17 SIGNAL REFERENCE
LEVEL 1 4
LEVEL 2 5
FREQ 1 6
FREQ 2
7
–3–
AD598
TOP VIEW
(Not to Scale)
16 SIGNAL OUTPUT
15 FEEDBACK
14 OUTPUT FILTER
B1 FILTER 8
13 A1 FILTER
B2 FILTER 9
12 A2 FILTER
VB 10
REV. A
20 +VS
1
11 VA
AD598–Typical Characteristics (at +258C and V = 615 V, unless otherwise noted)
S
120
40
OFFSET PSRR 12–15V
80
OFFSET PSRR 15–18V
TYPICAL GAIN DRIFT – ppm/°C
GAIN AND OFFSET PSRR – ppm/Volt
0
–40
GAIN PSRR 12–15V
–80
–120
GAIN PSRR 15–18V
–160
–200
40
20
0
–20
–40
–240
–60
–60
–20
0
20
60
100
–80
–60
140
–20
0
20
60
100
140
TEMPERATURE – °C
TEMPERATURE – °C
Figure 1. Gain and Offset PSRR vs. Temperature
Figure 2. Typical Gain Drift vs. Temperature
5
20
OFFSET CMRR ± 3V
TYPICAL OFFSET DRIFT – ppm/°C
GAIN AND OFFSET CMRR – ppm/Volt
0
–5
–10
–15
–20
GAIN CMRR ± 3V
–25
10
0
–10
–30
–35
–60
–20
0
20
60
100
–20
–60
140
TEMPERATURE – °C
2
10
AMP
AD598
A–B
A+B
FILTER
140
The oscillator comprises a multivibrator which produces a
triwave output. The triwave drives a sine shaper, which produces a low distortion sine wave whose frequency is determined
by a single capacitor. Output frequency can range from 20 Hz to
20 kHz and amplitude from 2 V rms to 24 V rms. Total harmonic distortion is typically –50 dB.
VA
LVDT
100
The AD598 energizes the LVDT primary, senses the LVDT
secondary output voltages and produces a dc output voltage
proportional to core position. The AD598 consists of a sine
wave oscillator and power amplifier to drive the primary, a decoder which determines the ratio of the difference between the
LVDT secondary voltages divided by their sum, a filter and an
output amplifier.
EXCITATION (CARRIER)
17
60
an external sine wave reference source, two secondary windings
connected in series, and the moveable core to couple flux between the primary and secondary windings.
A block diagram of the AD598 along with an LVDT (Linear
Variable Differential Transformer) connected to its input is
shown in Figure 5. The LVDT is an electromechanical transducer whose input is the mechanical displacement of a core and
whose output is a pair of ac voltages proportional to core position. The transducer consists of a primary winding energized by
OSC
20
Figure 4. Typical Offset Drift vs. Temperature
THEORY OF OPERATION
11
0
TEMPERATURE – °C
Figure 3. Gain and Offset CMRR vs. Temperature
3
–20
AMP
16
VOUT
The output from the LVDT secondaries consists of a pair of
sine waves whose amplitude difference, (VA–VB), is proportional
to core position. Previous LVDT conditioners synchronously
detect this amplitude difference and convert its absolute value to
VB
Figure 5. AD598 Functional Block Diagram
–4–
REV. A
AD598
a voltage proportional to position. This technique uses the primary excitation voltage as a phase reference to determine the
polarity of the output voltage. There are a number of problems
associated with this technique such as (1) producing a constant
amplitude, constant frequency excitation signal, (2) compensating
for LVDT primary to secondary phase shifts, and (3) compensating for these shifts as a function of temperature and frequency.
As shown in Figure 6, the input to the integrator is [(A+B)d]B.
Since the integrator input is forced to 0, the duty cycle d =
B/(A+B).
The output comparator which produces d = B/(A+B) also controls an output amplifier driven by a reference current. Duty
cycle signals d and (1–d) perform separate modulations on the
reference current as shown in Figure 6, which are summed. The
summed current, which is the output current, is IREF × (1–2d).
The AD598 eliminates all of these problems. The AD598 does
not require a constant amplitude because it works on the ratio of
the difference and sum of the LVDT output signals. A constant
frequency signal is not necessary because the inputs are rectified
and only the sine wave carrier magnitude is processed. There is
no sensitivity to phase shift between the primary excitation and
the LVDT outputs because synchronous detection is not employed. The ratiometric principle upon which the AD598 operates requires that the sum of the LVDT secondary voltages
remains constant with LVDT stroke length. Although LVDT
manufacturers generally do not specify the relationship between
VA+VB and stroke length, it is recognized that some LVDTs do
not meet this requirement. In these cases a nonlinearity will
result. However, the majority of available LVDTs do in fact
meet these requirements.
Since d = B/(A+B), by substitution the output current equals
IREF × (A–B)/(A+B). This output current is then filtered and
converted to a voltage since it is forced to flow through the scaling resistor R2 such that:
V OUT = I REF × ( A – B ) / (A + B ) × R2
CONNECTING THE AD598
The AD598 can easily be connected for dual or single supply
operation as shown in Figures 7 and 12. The following general
design procedures demonstrate how external component values
are selected and can be used for any LVDT which meets AD598
input/output criteria.
Parameters which are set with external passive components include: excitation frequency and amplitude, AD598 system
bandwidth, and the scale factor (V/inch). Additionally, there are
optional features, offset null adjustment, filtering, and signal integration which can be used by adding external components.
The AD598 utilizes a special decoder circuit. Referring to the
block diagram and Figure 6 below, an implicit analog computing loop is employed. After rectification, the A and B signals are
multiplied by complementary duty cycle signals, d and (I–d)
respectively. The difference of these processed signals is integrated and sampled by a comparator. It is the output of this
comparator that defines the original duty cycle, d, which is fed
back to the multipliers.
V TO I
INPUT
A
FILT
BINARY SIGNAL
d - DUTY CYCLE
d
COMP
0<d<1
±1
∑
V TO I
INTEG
(A+B) d–B
INPUT
B
FILT
COMP
1–d
d●
±1
1–d
IREF
IREF
BANDGAP
REFERENCE
d
∑
●
B
A+B
VOLTS
OUTPUT
A–B
A+B
FILT
∑
INTEG
V TO I
RTO
OFFSET
VOUT = RSCALE x I REF x A–B
A+B
Figure 6. Block Diagram of Decoder
REV. A
COMP
–5–
AD598
The AD598 signal input, VSEC, should be in the range of
1 V rms to 3.5 V rms for maximum AD598 linearity and
minimum noise susceptibility. Select VSEC = 3 V rms. Therefore, LVDT excitation voltage VEXC should be:
DESIGN PROCEDURE
DUAL SUPPLY OPERATION
Figure 7 shows the connection method with dual ±15 volt power
supplies and a Schaevitz E100 LVDT. This design procedure
can be used to select component values for other LVDTs as
well. The procedure is outlined in Steps 1 through 10 as follows:
VEXC = VSEC × VTR = 3 × 1.75 = 5.25 V rms
Check the power supply voltages by verifying that the peak
values of VA and VB are at least 2.5 volts less than the voltages at +VS and –VS.
1. Determine the mechanical bandwidth required for LVDT
position measurement subsystem, fSUBSYSTEM. For this
example, assume fSUBSYSTEM = 250 Hz.
6. Referring to Figure 7, for VS = ± 15 V, select the value of the
amplitude determining component R1 as shown by the curve
in Figure 8.
2. Select minimum LVDT excitation frequency, approximately
10 × fSUBSYSTEM. Therefore, let excitation frequency = 2.5 kHz.
3. Select a suitable LVDT that will operate with an excitation
frequency of 2.5 kHz. The Schaevitz E100, for instance, will
operate over a range of 50 Hz to 10 kHz and is an eligible
candidate for this example.
7. Select excitation frequency determining component C1.
C1 = 35 µF Hz/fEXCITATION
30
4. Determine the sum of LVDT secondary voltages VA and VB.
Energize the LVDT at its typical drive level VPRI as shown in
the manufacturer’s data sheet (3 V rms for the E100). Set the
core displacement to its center position where VA = VB. Measure these values and compute their sum VA+VB. For the
E100, VA+VB = 2.70 V rms. This calculation will be used
later in determining AD598 output voltage.
VEXC – Vrms
20
5. Determine optimum LVDT excitation voltage, VEXC. With
the LVDT energized at its typical drive level VPRI, set the
core displacement to its mechanical full-scale position and
measure the output VSEC of whichever secondary produces
the largest signal. Compute LVDT voltage transformation
ratio, VTR.
Vrms
10
VTR = VPRI/VSEC
0
0.01
For the E100, VSEC = 1.71 V rms for VPRI = 3 V rms.
VTR = 1.75.
0.1
10
1
100
1000
R1 – kΩ
Figure 8. Excitation Voltage VEXC vs. R1
+15V
6.8µF
6.8µF
0.1µF
0.1µF
+VS 20
1 –VS
–15V
R4
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
SIGNAL
REFERENCE
R3
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
RL
R1
R2
6 FREQ 1
FEEDBACK 15
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
C1
C4
C3
C2
VB
VOUT
10 VB
AD598
VA 11
NOTE
FOR C1, C2, C3 AND C4 MYLAR
CAPACITORS ARE
RECOMMENDED. CERAMIC
CAPACITORS MAY BE
SUBSTITUTED. FOR R2, R3 AND
R4 USE STANDARD 1%
RESISTORS.
VA
SCHAEVITZ E100
LVDT
Figure 7. Interconnection Diagram for Dual Supply Operation
–6–
REV. A
AD598
8. C2, C3 and C4 are a function of the desired bandwidth of
the AD598 position measurement subsystem. They should
be nominally equal values.
For no offset adjustment R3 and R4 should be open circuit.
To design a circuit producing a 0 V to +10 V output for a
displacement of ± 0.1 inch, set VOUT to +10 V, d = 0.2 inch
and solve Equation (1) for R2.
C2 = C3 = C4 = 10–4 Farad Hz/fSUBSYSTEM (Hz)
R2 = 37.6 kΩ
If the desired system bandwidth is 250 Hz, then
C2 = C3 = C4 = 10 Farad Hz/250 Hz = 0.4 µF
–4
This will produce a response shown in Figure 10.
See Figures 13, 14 and 15 for more information about
AD598 bandwidth and phase characterization.
VOUT (VOLTS)
+5
9. In order to Compute R2, which sets the AD598 gain or fullscale output range, several pieces of information are needed:
+0.1 d (INCHES)
– 0.1
a. LVDT sensitivity, S
–5
b. Full-scale core displacement, d
Figure 10. VOUT (± 5 V Full Scale)
vs. Core Displacement (± 0.1 Inch)
c. Ratio of manufacturer recommended primary drive level,
VPRI to (VA + VB) computed in Step 4.
LVDT sensitivity is listed in the LVDT manufacturer’s catalog and has units of millivolts output per volts input per inch
displacement. The E100 has a sensitivity of 2.4 mV/V/mil.
In the event that LVDT sensitivity is not given by the manufacturer, it can be computed. See section on Determining
LVDT Sensitivity.
In Equation (2) set VOS = 5 V and solve for R3 and R4.
Since a positive offset is desired, let R4 be open circuit.
For a full-scale displacement of d inches, voltage out of the
AD598 is computed as
Figure 11 shows the desired response.
VOUT
Rearranging Equation (2) and solving for R3
R3 =
1.2 × R2
– 5 kΩ = 4.02 kΩ
VOS
VOUT (VOLTS)
 VPRI 
=S×
× 500 µA × R2 × d.
 (VA +VB ) 
+10
– 0.1
VOUT is measured with respect to the signal reference,
Pin 17 shown in Figure 7.
+5
+0.1 d (INCHES)
Solving for R2,
R2 =
VOUT × (VA +VB )
S ×VPRI × 500 µA × d
Figure 11. VOUT (0 V–10 V Full Scale)
vs. Displacement (± 0.1 Inch)
(1)
Note that VPRI is the same signal level used in Step 4 to
determine (VA + VB).
DESIGN PROCEDURE
SINGLE SUPPLY OPERATION
For VOUT = 20 V full-scale range (± 10 V) and d = 0.2 inch
full-scale displacement (± 0.1 inch),
Figure 12 shows the single supply connection method.
R2 =
For single supply operation, repeat Steps 1 through 10 of the
design procedure for dual supply operation, then complete the
additional Steps 11 through 14 below. R5, R6 and C5 are additional component values to be determined. VOUT is measured
with respect to SIGNAL REFERENCE.
20V × 2.70V
= 75. 3 kΩ
2.4 × 3 × 500 µA × 0.2
VOUT as a function of displacement for the above example is
shown in Figure 9.
11. Compute a maximum value of R5 and R6 based upon the
relationship
VOUT (VOLTS)
R5 + R6 ≤ VPS/100 µA
+10
12. The voltage drop across R5 must be greater than
+0.1 d (INCHES)
– 0.1
1.2V

2 + 10 kΩ* 
 R4 + 5 kΩ
–10
Figure 9. VOUT (± 10 V Full Scale)
vs. Core Displacement (± 0.1 Inch)


1.2 V
V
2 +10 kΩ* 
+ 250 µA + OUT 
4 × R2 
 R4 + 5 kΩ
R5 ≥
Ohms
100 µA
*These values have ± 20% tolerance.
(2)
Based upon the constraints of R5 + R6 (Step 11) and R5
(Step 12), select an interim value of R6.
*These values have a ± 20% tolerance.
REV. A
VOUT 
 Volts
4 × R2 
Therefore
10. Selections of R3 and R4 permit a positive or negative output
voltage offset adjustment.
1
1


VOS = 1.2V × R2 × 
–

 R3 + 5 kΩ* R4 + 5 kΩ* 
+ 250 µA +
–7–
AD598
equal in value. Note also a shunt capacitor across R2 shown as a
parameter (see Figure 7). The value of R2 used was 81 kΩ with
a Schaevitz E100 LVDT.
13. Load current through RL returns to the junction of R5 and
R6, and flows back to VPS. Under maximum load conditions, make sure the voltage drop across R5 is met as
defined in Step 12.
As a final check on the power supply voltages, verify that the
peak values of VA and VB are at least 2.5 volts less than the
voltages at +VS and –VS.
14. C5 is a bypass capacitor in the range of 0.1 µF to 1 µF.
+ 30V
R5
Vps
6.8µF
0.1µF
C5
R6
+VS 20
1 –VS
R4
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
SIGNAL
REFERENCE
R3
RL
R1
C1
15nF
6 FREQ 1
FEEDBACK 15
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
VOUT
C4
C3
C2
VB
R2
33k
10 VB
AD598
VA 11
VA
SCHAEVITZ E100
LVDT
Figure 13. Gain and Phase Characteristics vs. Frequency
(0 kHz–10 kHz)
Figure 12. Interconnection Diagram for Single
Supply Operation
Gain Phase Characteristics
To use an LVDT in a closed loop mechanical servo application,
it is necessary to know the dynamic characteristics of the transducer and interface elements. The transducer itself is very quick
to respond once the core is moved. The dynamics arise primarily from the interface electronics. Figures 13, 14 and 15 show
the frequency response of the AD598 LVDT Signal Conditioner. Note that Figures 14 and 15 are basically the same; the
difference is frequency range covered. Figure 14 shows a wider
range of mechanical input frequencies at the expense of accuracy. Figure 15 shows a more limited frequency range with enhanced accuracy. The figures are transfer functions with the
input to be considered as a sinusoidally varying mechanical position and the output as the voltage from the AD598; the units of
the transfer function are volts per inch. The value of C2, C3 and
C4, from Figure 7, are all equal and designated as a parameter
in the figures. The response is approximately that of two real
poles. However, there is appreciable excess phase at higher frequencies. An additional pole of filtering can be introduced with
a shunt capacitor across R2, (see Figure 7); this will also increase phase lag.
When selecting values of C2, C3 and C4 to set the bandwidth of
the system, a trade-off is involved. There is ripple on the “dc”
position output voltage, and the magnitude is determined by the
filter capacitors. Generally, smaller capacitors will give higher
system bandwidth and larger ripple. Figures 16 and 17 show the
magnitude of ripple as a function of C2, C3 and C4, again all
Figure 14. Gain and Phase Characteristics vs. Frequency
(0 kHz–50 kHz)
–8–
REV. A
AD598
1000
RIPPLE – mV rms
100
10
10kHz , C SHUNT = 0nF
1
10kHz , C SHUNT = 1nF
10kHz , C SHUNT = 10nF
0.1
0.001
0.01
0.1
1
10
C2, C3, C4; C2 = C3 = C4 – µF
Figure 17. Output Voltage Ripple vs. Filter Capacitance
Determining LVDT Sensitivity
LVDT sensitivity can be determined by measuring the LVDT
secondary voltages as a function of primary drive and core position, and performing a simple computation.
Energize the LVDT at its recommended primary drive level,
VPRI (3 V rms for the E100). Set the core to midpoint where
VA = VB. Set the core displacement to its mechanical full-scale
position and measure secondary voltages VA and VB.
Figure 15. Gain and Phase Characteristics vs. Frequency
(0 kHz–10 kHz)
Sensitivity =
1000
VA (at Full Scale ) – VB (at Full Scale )
VPRI × d
From Figure 18,
Sensitivity =
RIPPLE – mV rms
100
1.71 – 0.99
= 2.4 mV/V/mil
3 × 100 mils
VSEC WHEN VPRI = 3V rms
VA
1.71V rms
10
2.5kHz, C SHUNT = 0nF
0.99V rms
VB
1
2.5kHz, C SHUNT = 1nF
d = –100 mils
2.5kHz, C SHUNT =10nF
0.1
0.01
0.1
1
d=0
d = +100 mils
Figure 18. LVDT Secondary Voltage vs. Core Displacement
10
C2, C3, C4; C2 = C3 = C4 – µF
Thermal Shutdown and Loading Considerations
The AD598 is protected by a thermal overload circuit. If the die
temperature reaches 165°C, the sine wave excitation amplitude
gradually reduces, thereby lowering the internal power dissipation and temperature.
Figure 16. Output Voltage Ripple vs. Filter Capacitance
Due to the ratiometric operation of the decoder circuit, only
small errors result from the reduction of the excitation amplitude. Under these conditions the signal-processing section of
the AD598 continues to meet its output specifications.
The thermal load depends upon the voltage and current delivered to the load as well as the power supply potentials. An
LVDT Primary will present an inductive load to the sine wave
excitation. The phase angle between the excitation voltage and
current must also be considered, further complicating thermal
calculations.
REV. A
–9–
AD598–Applications
The value of R3 or R4 can be calculated using one of two separate methods. First, a potentiometer may be connected between
Pins 18 and 19 of the AD598, with the wiper connected to
–VSUPPLY. This gives a small offset of either polarity; and the
value can be calculated using Step 10 of the design procedures.
For a large offset in one direction, replace either R3 or R4 with
a potentiometer with its wiper connected to –VSUPPLY.
PROVING RING-WEIGH SCALE
Figure 20 shows an elastic member (steel proving ring) combined with an LVDT to provide a means of measuring very
small loads. Figure 19 shows the electrical circuit details.
The advantage of using a Proving Ring in combination with an
LVDT is that no friction is involved between the core and the
coils of the LVDT. This means that weights can be measured
without confusion from frictional forces. This is especially important for very low full-scale weight applications.
The resolution of this weigh-scale was checked by placing a 100
gram weight on the scale and observing the AD598 output signal deflection on an oscilloscope. The deflection was 4.8 mV.
+15V
6.8µF
6.8µF
The smallest signal deflection which could be measured on the
oscilloscope was 450 µV which corresponds to a 10 gram
weight. This 450 µV signal corresponds to an LVDT displacement of 1.32 microinches which is equivalent to one tenth of the
wave length of blue light.
0.1µF
0.1µF
+VS 20
1 –VS
–15V
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
RL
SIG OUT 16
5 LEV 2
1µF
C1
0.015µF
C2
0.1µF
VB
6 FREQ 1
VOUT
FEEDBACK 15
634k
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
10 VB
The Proving Ring used in this circuit has a temperature coefficient of 250 ppm/°C due to Young’s Modulus of steel. By putting a resistor with a temperature coefficient in place of R2 it is
possible to temperature compensate the weigh-scale. Since the
steel of the Proving Ring gets softer at higher temperatures, the
deflection for a given force is larger, so a resistor with a negative
temperature coefficient is required.
SIGNAL
REFERENCE
AD598
10k
C4
0.33µF
C3
0.1µF
VA 11
SYNCHRONOUS OPERATION OF MULTIPLE LVDTS
In many applications, such as multiple gaging measurement, a
large number of LVDTs are used in close physical proximity. If
these LVDTs are operated at similar carrier frequencies, stray
magnetic coupling could cause beat notes to be generated. The
resulting beat notes would interfere with the accuracy of measurements made under these conditions. To avoid this situation
all the LVDTs are operated synchronously.
VA
SCHAEVITZ HR050
LVDT
Figure 19. Proving Ring-Weigh Scale Circuit
FORCE/LOAD
PROVING
RING
CORE
LVDT
Figure 20. Proving Ring-Weigh Scale Cross Section
Although it is recognized that this type of measurement system
may best be applied to weigh very small weights, this circuit was
designed to give a full-scale output of 10 V for a 500 lb weight,
using a Morehouse Instruments model 5BT Proving Ring. The
LVDT is a Schaevitz type HR050 (± 50 mil full scale). Although
this LVDT provides ± 50 mil full scale, the value of R2 was calculated for d = ± 30 mil and VOUT equal to 10 V as in Step 9 of
the design procedures.
The 1 µF capacitor provides extra filtering, which reduces noise
induced by mechanical vibrations. The other circuit values were
calculated in the usual manner using the design procedures.
The circuit shown in Figure 21 has one master oscillator and
any number of slaves. The master AD598 oscillator has its frequency and amplitude programmed in the usual manner via R1
and C2 using Steps 6 and 7 in the design procedures. The slave
AD598s all have Pins 6 and 7 connected together to disable
their internal oscillators. Pins 4 and 5 of each slave are connected to Pins 2 and 3 of the master via 15 kΩ resistors, thus
setting the amplitudes of the slaves equal to the amplitude of the
master. If a different amplitude is required the 15 kΩ resistor
values should be changed. Note that the amplitude scales linearly with the resistor value. The 15 kΩ value was selected because it matches the nominal value of resistors internal to the
circuit. Tolerances of 20% between the slave amplitudes arise
due to differing internal resistors values, but this does not affect
the operation of the circuit.
Note that each LVDT primary is driven from its own power amplifier and thus the thermal load is shared between the AD598s.
There is virtually no limit on the number of slaves in this circuit,
since each slave presents a 30 kΩ load to the master AD598
power amplifier. For a very large number of slaves (say 100 or
more) one may need to consider the maximum output current
drawn from the master AD598 power amplifier.
This weigh-scale can be designed to measure tare weight simply
by putting in an offset voltage by selecting either R3 or R4 (as
shown in Figures 7 and 12). Tare weight is the weight of a container that is deducted from the gross weight to obtain the net
weight.
–10–
REV. A
AD598
MASTER
–V
–V
15k
+V
15k
+VS 20
1 –VS
SLAVE 1
SLAVE 2
+V
+VS 20
1 –VS
OFFSET 1 19
2 EXC 1
OFFSET 1 19
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
3 EXC 2
OFFSET 2 18
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
82.5kΩ
82.5kΩ
6 FREQ 1
FEEDBACK 15
6 FREQ 1
FEEDBACK 15
6 FREQ 1
FEEDBACK 15
7 FREQ 2
OUT FILT 14
7 FREQ 2
OUT FILT 14
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
8 B1 FILT
A1 FILT 13
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
0.33µF
0.1µF
0.1µF
A2 FILT 12
9 B2 FILT
0.1µF
15k
2 EXC 1
82.5kΩ
0.015µF
–V
15k
+V
+VS 20
1 –VS
10 VB
0.1µF
9 B2 FILT
VA 11
AD598
10 VB
LVDT
SCHAEVITZ E 100
MECHANICAL POSITION INPUT
0.33µF
0.1µF
A2 FILT 12
AD598
VA 11
0.33µF
0.1µF
10 VB
LVDT
SCHAEVITZ E 100
MECHANICAL POSITION INPUT
AD598
VA 11
LVDT
SCHAEVITZ E 100
MECHANICAL POSITION INPUT
Figure 21. Multiple LVDTs—Synchronous Operation
such circuits. The analog input signal to the AD652 is converted
to digital frequency output pulses which can be counted by
simple digital means.
HIGH RESOLUTION POSITION-TO-FREQUENCY
CIRCUIT
In the circuit shown in Figure 22, the AD598 is combined with
an AD652 voltage-to-frequency (V/F) converter to produce an
effective, simple data converter which can make high resolution
measurements.
This circuit transfers the signal from the LVDT to the V/F converter in the form of a current, thus eliminating the errors normally caused by the offset voltage of the V/F converter. The V/F
converter offset voltage is normally the largest source of error in
–Vs
This circuit is particularly useful if there is a large degree of
mechanical vibration (hum) on the position to be measured.
The hum may be completely rejected by counting the digital frequency pulses over a gate time (fixed period) equal to a multiple
of the hum period. For the effects of the hum to be completely
rejected, the hum must be a periodic signal.
+Vs
GND
0.1µF
0.1µF
1 +VS
+VS 20
1 –VS
0.015µF
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
6 FREQ 1
0.33µF
OUT FILT 14
8 B1 FILT
A1 FILT 13
0.1µF
9 B2 FILT
0.1µF
10 VB
COMP REF 16
COMP“+” 15
2
TRIM
3
TRIM
4
OP AMP OUT
ANALOG GND 13
5
OP AMP “–”
DIGITAL GND 12
6
OP AMP “+”
FREQ OUT 11
COMP“–” 14
0.02µF
FEEDBACK 15
7 FREQ 2
AD652
SYNCHRONOUS
VOLTAGE TO
FREQUENCY
CONVERTER
7 10 VOLT INPUT
VA 11
+VS
CLOCK INPUT 10
A2 FILT 12
AD598
2.5k
500KHZ
8
–VS
COS
9
+VS
LVDT
SCHAEVITZ E 100
MECHANICAL POSITION INPUT
Figure 22. High Resolution Position-to-Frequency Converter
REV. A
–11–
CK
FREQ
OUT
AD598
The V/F converter is currently set up for unipolar operation.
The AD652 data sheet explains how to set up for bipolar operation. Note that when the LVDT core is centered, the output frequency is zero. When the LVDT core is positioned off center,
and to one side, the frequency increases to a full-scale value.
To introduce bipolar operation to this circuit, an offset must be
introduced at the LVDT as shown in Step 10 of the design
procedures.
LOW COST SET-POINT CONTROLLER
A low cost set-point controller can be implemented with the circuit shown in Figure 23. Such a circuit could possibly be used
in automobile fuel control systems. The potentiometer, P1, is
attached to the gas pedal, and the LVDT is attached to the butterfly valve of the fuel injection system or carburetor. The position of the butterfly valve is electronically controlled by the
position of the gas pedal, without mechanical linkage.
This circuit is a simple two IC closed loop servo-controller. It is
simple because the LVDT circuit is functioning as the loop integrator. By putting a capacitor in the feedback path (normally occupied by R2), the output signal from the AD598 corresponds
to the time integral of the position being measured by the
LVDT. The LVDT position signal is summed with the offset
signal introduced by the potentiometer, P1. Since this sum is integrated, it must be forced to zero. Thus the LVDT position is
forced to follow the value of the input potentiometer, P1. The
output signal from the AD598 drives the LM675 power amplifier, which in turn drives the solenoid.
This circuit has dual advantages of being both low cost and high
accuracy. The high accuracy results from avoiding the offset errors normally associated with converting the LVDT signal to a
voltage and then subsequently integrating that voltage.
MECHANICAL FOLLOWER SERVO-LOOP
Figure 24 shows how two Schaevitz E100 LVDTs may be combined with two AD598s in a mechanical follower servo-loop
configuration. One of the LVDTs provides the mechanical input
position signal, while the other LVDT mimics the motion.
signal is summed with the signal from the output position
LVDT; this summed signal is integrated such that the output
position is now equal to the input position. This circuit is an
efficient means of implementing a mechanical servo-loop since
only three ICs are required.
This circuit is similar to the previous circuit (Figure 23) with
one exception: the previous circuit uses a potentiometer instead
of an LVDT to provide the input position signal. Replacing the
potentiometer with an LVDT offers two advantages. First, the
increased reliability and robustness of the LVDT can be exploited in applications where the position input sensor is located
in a hostile environment. Second, the mechanical motions of the
input and output LVDTs are guaranteed to be identical to
within the matching of their individual scale factors. These
particular advantages make this circuit ideal for application as a
hydraulic actuator controller.
DIFFERENTIAL GAGING
LVDTs are commonly used in gaging systems. Two LVDTs
can be used to measure the thickness or taper of an object. To
measure thickness, the LVDTs are placed on either side of the
object to be measured. The LVDTs are positioned such that
there is a known maximum distance between them in the fully
retracted position.
This circuit is both simple and inexpensive. It has the advantage
that two LVDTs may be driven from one AD598, but the disadvantage is that the scale factor of each LVDT may not match
exactly. This causes the workpiece thickness measurement to
vary depending upon its absolute position in the differential
gage head.
This circuit was designed to produce a ± 10 V signal output
swing, composed of the sum of the two independent ± 5 V
swings from each LVDT. The output voltage swing is set with
an 80.9 kΩ resistor. The output voltage VOUT for this circuit is
given by:
 (V –V B ) (VC –VD ) 
× 500 µA × R2.
VOUT =  A
+
 (VA +V B ) (VC +VD ) 
The signal from the input position circuit is fed to the output as
a current so that voltage offset errors are avoided. This current
MASS ON SPRING
620 N/m
33 GRAMS
100Ω
0.1µF
INPUT PI
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
150k
+V
10k
+VS 20
1 –VS
INPUT
MECHANICAL
POSITION
OUTPUT
POSITION
SCHAEVITZ E 100
LVDT
+V
1000pF
0.33µF
0.068µF
0.1µF
LM675
50kΩ
49.9k
4.99k
GUARDIAN SOLENOID
12 VDC 2–INT–12D
62 CONE
30k
0.015µF
0.1µF
6 FREQ 1
FEEDBACK 15
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
10 VB
AD598
VA 11
0.33µF
+V
1µF
+ 25V
20k
47µF
33µF
0.1µF
0.01µF
IN4740A
10V
47µF
GND
POWER SUPPLY
Figure 23. Low Cost Set-Point Controller
–12–
REV. A
AD598
MASS ON SPRING
620 N/m
33 GRAMS
0.1µF
100Ω
1000pF
0.33µF
+V
150k
+V
10k
+VS 20
1 –VS
OUTPUT
MECHANICAL
POSITION
SCHAEVITZ E 100
LVDT
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
0.068µF
0.1µF
LM675
49.9k
4.99k
GUARDIAN SOLENOID
12 VDC 2-INT-12D
62 CONE
SIG OUT 16
5 LEV 2
30k
0.015µF
0.1µF
6 FREQ 1
FEEDBACK 15
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
10 VB
AD598
0.33µF
1µF
0.1µF
0.01µF
VA 11
+V
+ 25V
20k
0.1µF
47µF
33µF
+V
47µF
+VS 20
1 –VS
INPUT
MECHANICAL
POSITION
SCHAEVITZ E 100
LVDT
0.015µF
0.1µF
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
6 FREQ 1
FEEDBACK 15
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
10 VB
AD598
GND
IN4740A
10V
POWER SUPPLY
4.99k
0.33µF
0.1µF
VA 11
Figure 24. Mechanical Follower Servo-Loop
–V
0.1µF
0.1µF
+VS 20
1 –VS
A
B
LVDT 1
0.015µF
+V
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
R2
6 FREQ 1
FEEDBACK 15
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
80.9kΩ
0.33µF
SCHAEVITZ E 100
0.1µF
0.1µF
C
10 VB
AD598
VA 11
D
LVDT 2
VOUT = (V A–VB)+(V C–VD) • 500µA • R2
(V A+VB)+(V C+VD)
SCHAEVITZ E 100
Figure 25. Differential Gaging
REV. A
–13–
VOUT ± 10V
FULL SCALE
AD598
PRECISION DIFFERENTIAL GAGING
The circuit shown in Figure 26 is functionally similar to the differential gaging circuit shown in Figure 25. In contrast to Figure
25, it provides a means of independently adjusting the scale factor of each LVDT so that both scale factors may be matched.
R1 and R2 are chosen to be 80.9 kΩ resistors to give a ± 10 V
full-scale output signal for a single Schaevitz E100 LVDT. R3 is
chosen to be 40.2 kΩ to give a ± 10 V output signal when the
two E100 LVDT output signals are summed. The output voltage for this circuit is given by:
The two LVDTs are driven in a master-slave arrangement
where the output signal from the slave LVDT is summed with
the output signal from the master LVDT. The scale factor of the
slave LVDT only is adjusted with R1 and R2. The summed
scale factor of the master LVDT and the slave LVDT is adjusted with R3.
 (V –V B ) (VC –VD ) R2 
× 500 µA × R3.
VOUT =  A
+
×
 (VA +V B ) (VC +VD ) R1 
–V
0.1µF
0.1µF
+VS 20
1 –VS
0.015µF
+V
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
R3
6 FREQ 1
FEEDBACK 15
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
40.2kΩ
VOUT ± 10V
FULL SCALE
0.33µF
15kΩ
0.1µF
A
15kΩ
0.1µF
10 VB
AD598
VA 11
B
MASTER LVDT
–V
SCHAEVITZ E 100
0.1µF
0.1µF
R1
80.9kΩ
+V
C
+VS 20
1 –VS
D
SLAVE
LVDT
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
6 FREQ 1
FEEDBACK 15
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
R2
80.9kΩ
0.33µF
0.1µF
0.1µF
10 VB
VOUT =
AD598
VA 11
VA–VB + VC–VD R2
VA+VB
VC+VD • R1
• 500µA • R3
Figure 26. Precision Differential Gaging
–14–
REV. A
AD598
trial and error. The 300 Ω resistors in this circuit optimize the
nonlinearity of the transfer function to within several tenths of
1%. This circuit uses a Sangamo AGH1 half-bridge transducer.
The 1 µF capacitor blocks the dc offset of the excitation output
signal. The 4 nF capacitor sets the transducer excitation frequency to 10 kHz as recommended by the manufacturer.
OPERATION WITH A HALF-BRIDGE TRANSDUCER
Although the AD598 is not intended for use with a half-bridge
type transducer, it may be made to function with degraded
performance.
A half-bridge type transducer is a popular transducer. It works
in a similar manner to the LVDT in that two coils are wound
around a moveable core and the inductance of each coil is a
function of core position.
ALTERNATE HALF-BRIDGE TRANSDUCER CIRCUIT
This circuit suffers from similar accuracy problems to those
mentioned in the previous circuit description. In this circuit the
VA input signal to the AD598 really and truly is a linear function
of core position, and the input signal VB, is one half of the excitation voltage level. However, a nonlinearity is introduced by
the A–B/A+B transfer function.
In the circuit shown in Figure 27 the VA and VB input voltages
are developed as two resistive-inductor dividers. If the inductors
are equal (i.e., the core is centered), the VA and VB input voltages to the AD598 are equal and the output voltage VOUT is
zero. When the core is positioned off center, the inductors are
unequal and an output voltage VOUT is developed.
The 500 Ω resistors in this circuit are chosen to minimize errors
caused by dc bias currents from the VA and VB inputs. Note that
in the previous circuit these bias currents see very low resistance
paths to ground through the coils.
The linearity of this circuit is dependent upon the value of the
resistors in the resistive-inductor dividers. The optimum value
may be transducer dependent and therefore must be selected by
–V
1µF
1µF
300Ω
300Ω
0.1µF
0.1µF
+V
+VS 20
1 –VS
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
5kΩ
82.5kΩ
SANGAMO
AGHI
HALF-BRIDGE
6 FREQ 1
FEEDBACK 15
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
4nF
VOUT ± 10V
FULL SCALE
0.33µF
0.1µF
0.1µF
MECHANICAL
POSITION
INPUT
10 VB
AD598
VA 11
Figure 27. Half-Bridge Operation
–V
0.1µF
0.1µF
+VS 20
1 –VS
1µF
+V
2 EXC 1
OFFSET 1 19
3 EXC 2
OFFSET 2 18
4 LEV 1
SIG REF 17
5 LEV 2
SIG OUT 16
1.87kΩ
SANGAMO
AGHI
HALF-BRIDGE
143kΩ
500Ω
500Ω
FEEDBACK 15
7 FREQ 2
OUT FILT 14
8 B1 FILT
A1 FILT 13
9 B2 FILT
A2 FILT 12
0.33µF
0.1µF
0.1µF
MECHANICAL
POSITION
INPUT
6 FREQ 1
4nF
10 VB
AD598
VA 11
Figure 28. Alternate Half-Bridge Circuit
REV. A
–15–
VOUT ± 10V
FULL SCALE
AD598
OUTLINE DIMENSIONS
Dimensions shown in inches and (mm).
C1330–10–10/89
20-Pin Sized Brazed Ceramic DIP
PRINTED IN U.S.A.
20-Lead Wide Body Plastic SOIC (R) Package
–16–
REV. A