DX6106 Optical Units for Gas Analyzers

RMT Ltd
RMT Ltd
Joint Stock Company
Optical Unit
DX6106 Series
User Guide
2002
Rev. 1.10
DX6106
RMT Ltd
Edition April 2002
Copyright
All right reserved. Reproduction in any manner, in whole or in part
is straightly prohibited without written permission of RMT Ltd
The information contained in this document is subject to change
without notice.
Limited Warranty
RMT Ltd warrants that DX6106 Optical Unit, if properly used and
installed, will be free from defects in material and workmanship
and will substantially conform to RMT’s publicly available
specification for a period of one (1) year after date of DX6106
Optical Unit was purchased.
If the DX6106 Optical Unit which is the subject of this Limited
Warranty fails during the warranty period for the reasons covered
by this Limited Warranty, RMT, at this option, will :
REPAIR the DX6106 Optical Unit; OR
REPLACE the DX6106 Optical Unit with another DX6106 Optical
Unit.
Trademark Acknowledgments
All trademarks are the property of their respective owners.
RMT Ltd. 53 Leninskij prosp. Moscow 119991 Russia
phone: 095-132-6817 fax: 095-132-5870
e-mail: [email protected] http://www.rmtltd.ru
REV. 1.10/2002
RMT Ltd
DX6106
Contents
1. Introduction
2. Theory of Operation
Principles of Operation
Design Features
Operation Overview
3. Construction of Optical Unit
Gas Sampling Cell
Optocomponent
6102 Optocomponent Mating Module
Preamplifier
Thermoelectric Cooler
Thermistor
Light Emitters
EEPROM
EEPROM Data Format
4. Installation Tips
5. Calibration
Preparation
Zero Adjustments
Re-Calibration
6. Maintenance
Optics Cleaning
7. Standard Kit
8. Specifications
9. Ordering Guide
Contents
1-1
2-1
2-4
2-5
3-1
3-2
3-5
3-7
3-10
3-13
3-19
3-24
3-27
3-30
4-1
5-1
5-1
5-3
5-4
6-1
7-1
8-1
9-1
C-1
DX6106
C-2
RMT Ltd
REV. 1.10/2002
RMT Ltd
DX6106
1. Introduction
The company RMT Ltd introduces new DX6106 series
of Optical Units for gas measurement systems.
The principle of operation is based on selective
absorption of IR radiation by gas molecules.
The differential double frequency optical scheme
provides high accuracy in wide ranges of humidity and
temperature due to the internal thermostabilization.
New type of middle infrared combined optocomponent
with built-in thermoelectric cooling is used.
There are several models suitable for the following
gases : CO2, CH4, CnHm, water vapor.
Advantages
Ÿ
Ÿ
Ÿ
Ÿ
Ÿ
high selectivity and stability
wide range of measured concentrations
fast response
no direct contact of sensitive element with
measured gas
the long service life
Features
Ÿ
Ÿ
Ÿ
no moving parts
minimum dimensions and light weight
low power consumption
Introduction
1-1
DX6106
1-2
RMT Ltd
REV. 1.10/2002
RMT Ltd
DX6106
2. Theory of Operation
Principles of Operation
The NDIR (Non-Dispersive Infra-Red Spectroscopy)
measurement method is implemented in the DX6106
Optical Unit.
The device provides gases concentration measurement based on the classical double channel optical
scheme (Fig. 2.1). One of the beams (measuring
channel) has the wavelength which is tuned to the
optical absorption line of the measured gas. The other
beam (reference channel) has the wavelength which is
out of the adsorption band of the measured gas.
Intensity
Intensity
Intensities of two light beams that passed through the
measured gas sampling cell are compared.
l1 l2
Wavelength
Photoresistor
Gas Flow
Light Emitters
l1 l2
Wavelength
Fig. 2.1. The principle of gas concentration
Theory of Operation
2-1
RMT Ltd
DX6106
According to the Beer-Bouguer-Lambert law, light
absorption in a gas volume is proportional to the
absorbing gas concentration:
where
I = I0 × e
-a L X
I0 – intensity of light before pass through the gas
I
volume;
– intensities of light after pass through the gas
volume;
Relative response
a – absorption coefficient of the gas at the chosen
light wavelength;
L – optical pass length;
X – gas concentration.
At a fixed L and
1.0
known
Photodetector
absorption a it is
possible to find
gas concen0.5
Reference
Measuring
tration using
channel
channel
measured
intensity of light
(measuring
0
channel) that
2.0
3.0
4.0
Wavelength, µm
passed from
Light Emitter to
Fig. 2.2. Spectral bands of light
emitters for methane analyzer
Photodetector.
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REV. 1.10/2002
RMT Ltd
Emission band
1.0
Reference
channel
Measuring
channel
0.5
0
2.0
Relative absorption
Reference channel is
used for indirect
measuring of the
initial intensity of
light, and allows to
eliminate actual
measurements
conditions (total
transparency of gas
volume, optics
imperfection and so
on).
DX6106
3.0
4.0
3.0
4.0
1.0
Methane
0.5
0
2.0
Wavelength, µm
In Fig. 2.2 the
Fig. 2.3. Spectral bands of light
emitters and methane
example of spectral
bands of light
emitters for methane
analyzer is shown.
The detailed description of the optocomponent is given
in Chapter 3.
In Fig. 2.3 the spectral bands of light emitters of the
optopair are given in comparison with methane
absorption spectra.
Theory of Operation
2-3
DX6106
RMT Ltd
Design Features
The DX6106 Optical Unit is specially designed for a fast
response, high sensitivity, low noise and low power
consumption.
A number of design features contribute to the
performance :
Ÿ The infrared sources are special narrow-band
pulsed Light Emitters which operate in
microsecond range. The light sources have long
life (more then 10,000 hours).
Ÿ Radiation from Light Emitters passes through the
gas sampling cell, reflects from the mirror and is
focused onto the wide-band Photodetector.
Ÿ Both Light Emitters and Photodetector chips are
integrated into a single housing and placed onto
a miniature TE cooler for thermostabilization.
Ÿ Heat, dissipated from warm side of the TE cooler,
leads to few degrees of overheating of gas
sampling cell above ambient. This factor plays a
role of vapor anti-condensation at operation in
wet conditions.
Ÿ For signal processing the calibrating data of
Optical Unit is used. The data is stored in Optical
Unit’s EEPROM.
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REV. 1.10/2002
RMT Ltd
DX6106
Operation Overview
The subsequent description assumes User has already
developed, manufactured and connected to the Optical
Unit some electronic device for Optical Unit
management. (See recommendations in Chapter 3).
The order of measurements with DX6106 device is as
follows:
1. Firstly, individual calibration of device is required
with using of standard gas mixtures.
The Detector output signal is non-linear with respect
to measuring gas concentration. In spite of theoretical
formula the intensity of light which passed through gas
sampling cell, is the integral of various optical rays
from Light Emitter. Also sensitivity of Detector and
performance of Light Emitter are very sensitive to its
operating temperatures.
Detector’s output signals (both measuring Um and
reference Ur channels) must be measured to calculate
the following D ratio as a function of known concentration X of standard mixtures.
Zero ratio D0 = f(X=0) at zero gas concentration should
be used for polynomial extrapolation of calibration
results as:
U
D= m
Ur
Theory of Operation
2-5
RMT Ltd
DX6106
Y=
D0
D
X = A0 + A1 × Y + A2 × Y 2 + A3 × Y 3 + A4 × Y 4
Calculated coefficients A0 … A4 of polynomial
expression and zero ratio D0 may be stored into device
internal on-board EEPROM memory.
The first calibration is made by Manufacturer.
The factory standard calibration uses not less than 5
standard gas mixtures.
Several calibrations as above described are made at
different ambient temperatures (in a specified
operating range) and at corresponding optimal
operating temperatures of integrated detector-emitter
pair.
Up to 15 such calibrations are possible to store for
further application.
Format of calibration data stored in the EEPROM
memory chip after manufacturer calibration is
described below in Chapter 3.
2. During routine operation the detector’s output
signals should be measured to calculate D ratio. Using
known “zero” ratio D0 value Y is calculated.
Finally, using known polynomial coefficients A0 … A4
gas concentration X may be calculated with high
accuracy.
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REV. 1.10/2002
RMT Ltd
DX6106
3. To preserve high accuracy of the device it is
necessary to do “zero” adjustments periodically as
recommended in Chapter 5.
4. Periodicity of device recalibration is 1 year. It could
be done at the factory of Manufacturer, or by a User.
Theory of Operation
2-7
DX6106
2-8
RMT Ltd
REV. 1.10/2002
RMT Ltd
DX6106
3. Construction of Optical Unit
The DX6106 Optical
Unit (Fig. 3.1 and 3.2)
consists of an isolated
gas sampling cell (the
spherical mirror and
the flat mirror with a
hole are placed at the
end sides) and a new
generation integrated
optopair with 6102 electronic module.
The 6102 Optocomponent Mating Module is connected
to optopair’s leads and is fixed with two screws on a
bottom cover of the
gas sampling cell.
Fig. 3.2. DX6106 Optical Unit with
optopair detached
Construction of Optical Unit
3-1
RMT Ltd
DX6106
Gas Sampling Cell
The body of gas
sampling cell is made of
anodized aluminum alloy
(Fig. 3.3). It has two gas
inlets with 5.0 mm
internal diameter.
The gas sampling cell
can be easily
Fig. 3.3. DX6106.C40 gas
sampling cell
disassembled for service
of internal optics (mirrors
and optopair). For this purpose both the top and bottom
covers can be removed and the optical components
extracted out.
The gas sampling cell design is shown in Fig. 3.4.
Bottom
cover
Rubber
gasket
Integrated
Spherical
optopair mirror
Flat mirror
with a hole
Top
cover
Rubber
Housing gasket
Fig. 3.4. Gas sampling cell design
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DX6106
The optical scheme of gas cell is represented in Fig. 3.5.
Flat Mirror
with a hole
Gas
Integrated
optopair
Outlet brunch pipe
Spherical
Mirror
Inlet
brunch
pipe
The main parameters of gas sampling cell are in Table
3.1
Table 3.1. Main parameters of gas
Parameter
Value
No. of passes
4
Total path length, mm
80
Internal volume, ml
Construction of Optical Unit
10.4
3-3
RMT Ltd
DX6106
The outline dimensions of DX6106.C40 gas sampling
cell are shown in Fig. 3.6.
42
27
27
36.5
40
Fig. 3.6 DX6106.C40 gas sampling cell outline dimensions
(in millimeters)
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REV. 1.10/2002
RMT Ltd
DX6106
Optocomponent
The new generation OPRI optopair
consists of three optoelements integrated
into one case : two narrow-band light
emitters (of about 0.1 µm emission band)
and one wide-band photodetector.
The optopair consists of two special solid
state light emitters (light sources) and one
sensitive element (photodetector).
The peak emission wavelength of one light emitter is near
the absorption band of measured gas (measuring channel).
The peak wavelength of the other one is out of the
absorption band of gas (reference channel).
The photodetector has approximately equal sensitivity to
signals of both emitters.
All the elements of the optopair are mounted onto the
cooling surface of a single stage thermoelectric module of
1MT04-059-16 type with an
Reference
internal thermosensor (Fig.
channel
emitter
3.7).
Measuring
channel
emitter
Photodetector
Fig. 3.7. OPRI elements
arrangement
Construction of Optical Unit
A number of steps have been
taken to decrease the
optoelements mutual
influence.
The pins layout of the
optopair is shown in Fig. 3.8.
3-5
RMT Ltd
DX6106
As an example, the parameters
of optoelements for methane
(CH4) measurements are
12
11 10
t°
1
R
2
introduced in the table bellow:
M
4
8
7
+
3
9
5
6
Fig. 3.8. OPxxx optopair
pins layout (top view)
Element
Peak wavelength
[ µm ]
Bandwidth
[ µm ]
Measuring channel emitter
Reference channel emitter
Photodetector
3.23
2.98
3.3
0.1
0.1
2.5
The above table is illustrated with Fig. 3.9.
1.0
Relative response
Photodetector
0.5
Reference
channel
Measuring
channel
0
2.0
3.0
Wavelength, µm
4.0
Fig. 3.9. Emission bands of light emitters for
methane analyzer
3-6
REV. 1.10/2002
RMT Ltd
DX6106
6102 Optocomponent Mating Module
The 6102 Optocomponent
Mating Module (Fig. 3.10)
provides:
Ÿ preamplification of
photodetector’s signals,
Ÿ light emitters driving,
Fig. 3.10. 6102
Optocomponent
Mating Module
Ÿ power supply of
photodetector and
thermistors with precise voltage.
The connectors and optopair location at the 6102
Module’s board is shown in Fig. 3.11.
The outline dimensions of 6101 Module are given in
Fig. 3.12.
47
System
System
interface
interface
Optopair connector X2 connector X1
26
Pin 1
Pin 1
Fig. 3.12. 6102 Module outline
Fig. 3.11. Location of the
dimensions (in millimeters)
connectors and optopair at
the 6102 Modules board.
Construction of Optical Unit
3-7
RMT Ltd
DX6106
X2 8
SCL
SDA
X2 2
TEC
X2 6
+ELED
X1 5
OUTS
X1 7
OUTT
3
4
6
8
GNDA
GNDA
GNDA
GNDA
Filter
X1 2
+5VIN
Filter
X1 1
–5VIN
X2 4
GATEM
X2 5
GATER
X2 3
SOURCE
X2 1
GND
X2 7
t°
+
EEPROM
X1
X1
X1
X1
Legend
t°
– TE cooler
– Light Emitter
– MOSFET switch
– thermistor
– Photodetector
– amplifier
Fig. 3.13. Functional Diagram of 6102 Optocomponent
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REV. 1.10/2002
RMT Ltd
DX6106
The functional diagram of the 6102 module is drawn in Fig.
3.13.
System interface connectors’ pins assignment is given in
Tables 3.2 and 3.3.
Table 3.2. DX6106 system interface connector X1 pins
function description
Pin
Mnemonic
1
2
3
4
5
6
7
8
–5VIN
+5VIN
GNDA
GNDA
OUTS
GNDA
OUTT
GNDA
Description
– 5V supply input
+ 5V supply input
Ground reference point for analog circuitry and
Ground reference point for analog circuitry and
Photodetector output
Ground reference point for analog circuitry and
Thermistor output
Ground reference point for analog circuitry and
Table 3.3. DX6106 system interface connector X2 pins
function description
Pin
1
2
3
4
5
6
7
8
Mnemonic
GND
TEC
SOURCE
GATEM
GATER
+ELED
SCL
SDA
Description
Ground reference point for power circuitry
Cooler power supply input
Current sense resistor output
Measuring channel LED enable
Reference channel LED enable
LEDs power supply
I2C interface. Synchronization line
I2C interface. Data line
Construction of Optical Unit
3-9
RMT Ltd
DX6106
Preamplifier
The preamplifier’s circuit diagram is presented in Fig.
3.14.
+5V
X1 1
+5VIN
–5VIN
X1 5
OUTS
3
4
6
8
GNDA
GNDA
GNDA
GNDA
X1 2
X1
X1
X1
X1
Fig. 3.14. Simplified diagram of preamplifier of
the 6102 module
The preamplifier alternatively processes the signals of
measuring and reference channels.
The preamplifier output signal should be conditioned
and then digitized by A/D converter (ADC) with not
worse than 12 bit resolution.
Recommended outside schematic is placed in Fig.
3.15.
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REV. 1.10/2002
RMT Ltd
DX6106
+5V
X1 1
+5V
–5V
X1 5
Attenuator
X1 2
X1
X1
X1
X1
ADC
Microcontroller
DX6106 Optical Unit
3
4
6
8
Fig. 3.15. Output signal processing
Within the gas concentration varying scale, the output
signal of measuring channel changes by order of value.
To preserve accuracy at large measuring gas
concentrations it is necessary to use an external
amplifier with a variable gain. It is to coordinate the
amplified signal with an ADC range.
Alternatively, an attenuator may be used. The attenuator
can be based on a digital potentiometer chip or D/A
converter.
It is unnecessary if LEDs pumping current control
scheme is implemented.
Construction of Optical Unit
3-11
RMT Ltd
DX6106
The preamplifier typical output signal waveform is
showm in Fig. 3.16.
MTB = 20 HS
CH1 = .5V
Fig. 3.16. Typical output signal
waveform
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DX6106
Thermoelectric Cooler
The TEC circuit diagram is
presented in Fig. 3.17.
X2 2
TEC
X2 1
GND
Driving by TE cooler requires
particular attention.
First of all, the operation of TE
cooler directly affects
performance parameters of
Optical Unit and gas sensor
based on it.
Fig. 3.17. Schematics
of TE cooler in
Second, the TE cooler is the
component which consume
the largest part of power (Fig. 3.18).
The output signal of Photodetector depends very much
on its temperature (Fig. 3.19).
This ratio is approximately 100%/20 °C. It is equivalent
to the temperature drift 1%/0.2 °C. It means that if the
thermo-stabilization should be with the accuracy of
0.1°C, then the accuracy of measurements will be 0.5%.
The accuracy of thermo-stabilization must be not less
than required for gas sensing.
Operating temperature of TE cooler must be selected
optimal (from Fig. 3.18 and Fig. 3.19): too low
temperature stabilization leads to higher power
Construction of Optical Unit
3-13
RMT Ltd
DX6106
Power, W
2.0
1.5
1.0
0.5
0
–20
–15
–10
–5
0
5
10
Temperature, °C
Fig. 3.18. TEC power consumption vs operating
temperature
Output, V
1.4
1.2
0.8
Um
0.6
1.0
0.8
0.6
0.4
0.4
Ur
Um/Ur
Um/Ur Ratio
1.6
0.2
0.2
0
–15
–10
–5
0
5
0
10
Temperature, °C
Fig. 3.19. Typical preamplifier output vs operating
temperature
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REV. 1.10/2002
RMT Ltd
DX6106
consumption; at higher temperature the output signals
(and signal/noise ratio) are lower.
The Optical Unit housing has been designed for
additional heat dissipation from warm side of working
TE coolers. The maximal heat dissipation is 2 W. At
Ta-Top > 40 °C it is necessary to use additional heat
dissipation - a bigger heat sink (optional available) or
a fan.
A developer of thermo-stabilization algorithm has to
take into account that time constant of TE cooler is
approximately 2 s.
An example of recommended scheme of thermostabilization is presented in Fig. 3.20.
DX6106 Optical Unit
X2 2
+VCC
+
+
X2 1
Construction of Optical Unit
PWM
Microcontroller
GND
3-15
DX6106
RMT Ltd
If step-down DC/DC converter is used, the VCC
voltage should be not less than 7V to provide the
appropriate range of TEC control voltage.
The maximum converter’s output current is determined
by TECs characteristics behavior. (See Fig. 3.21).
Fig. 3.21. Maximal temperature
difference vs operating current
for 1MT04-059-16.
(At zero heat load)
As one can see in this diagram, there is some peak
current value, the efficiency of TE cooler falls down
after that.
It is obvious, that the exceeding of this parameter is not
meaningful. So 0.5 amp can be considered as an upper
bound of a DC/DC converter load.
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DX6106
TE Cooler Specifications
TAMB = +20°C
Parameter
Units
Min
Typ
Max
Comments
Electrical Parameters
Operating T
°C
Operating Voltage V
Operating Current A
Resistance
Ohm
–40
6.8
0.5
11.1 11.7 12.3
1 kHz @ +20°C
Dynamical Parameters
Time Constant
s
Construction of Optical Unit
2
3-17
DX6106
3-18
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REV. 1.10/2002
RMT Ltd
DX6106
Thermistor
UREF
RT
Filter
X1 2
+5VIN
X1 7
OUTT
3
4
6
8
GNDA
GNDA
GNDA
GNDA
t°
For a TE cooler temperature controlling NTC
thermistor is mounted onto
the cold side of a TE
cooler. This thermistor is
applied in a scheme with
serial loading resistor RL
and a reference UREF (Fig.
3.22).
RL
C
X1
X1
X1
X1
Fig. 3.22. Thermistor
connection in the 6102
Component list
Designation
Value
RT
2.2 kW ±5%
RL
3.83 kW ±0.1%
C
0.1 mF, ceramic
The typical dependence of thermistor resistance on
temperature is presented in Fig. 3.20. The dark area
around the curve marks technological deviation
determined by resistance and Beta Constant straggling
from rated values.
Construction of Optical Unit
3-19
RMT Ltd
DX6106
30
Resistance, kOhm
25
20
15
10
5
0
–40
–20
0
20
Temperature, °C
40
60
80
Fig. 3.23. Calibration of thermistor vs measured temperature
The curve in Fig 3.23 is plotted on the basis of the
fundamental equation
R = R0 e
(
1
1
b T -T
0
)
(3.1)
where
b
R0
3-20
- Beta Constant,
- resistance at standard temperature T0.
REV. 1.10/2002
RMT Ltd
DX6106
The output signal from thermistor scheme depends on
its resistance as :
æ
ö
U TR = U REF çç R L ÷÷
è R L + RT ø
(3.2)
One can see that the temperature measurement accuracy depends directly on UREF. So the voltage +5VIN on
the pin X1/2 must be stable.
With the help of equations (3.1) and (3.2) we obtain the
plot in Fig. 3.24.
5
Output, V
4
3
2
1
0
–40
–20
0
20
40
60
80
Temperature, °C
Fig. 3.24. Thermistor circuit output vs measured temperature
Construction of Optical Unit
3-21
DX6106
RMT Ltd
It is obvious that the scheme responds to temperature
in a nonlinear manner. At the same time over a limited
temperature range it is possible to consider the
scheme response as linear.
It is also obvious that the solution of this problem
should be based on the usage of a microcontroller. A
look-up table for temperature measurements
linearization must be formed in the external memory.
The table may be located in the Optical Unit’s EEPROM
or in another memory chip. The base points of this
table must correspond to the set of operating
temperatures of the Optical Unit (See Chapter
“Calibration”).
In a vicinity of each point the response of the scheme
should be linearized. The total number of points must
be equal to the number of calibration tables (the
number of operating temperatures ranges).
The recommended external circuit schematic is
presented in Fig. 3.25. Not worse than 12-bit resolution
A/D converters (ADCs) are recommended.
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DX6106
DX6106 Optical Unit
RT
+5V
X1 2
t°
Filter
ADC
X1 7
RL
C
X1
X1
X1
X1
3
4
6
8
Fig. 3.25. Typical thermistor usage
Thermistors Specifications
TAMB = +20°C; VCC = 5±5% V
Parameter
Units
Resistivity
Beta-Constant
kOhm
K·10-3
Construction of Optical Unit
Min
Typ
Max
2.09 2.2 2.31
2.9 3.1 3.5
Comments
@20°C
3-23
RMT Ltd
DX6106
Light Emitters
+
RE
C
RS
RG RG
X2 6
+ELED
X2 4
GATEM
X2 5
GATER
X2 3
SOURCE
X2 1
GND
Fig 3.26. LED drive switches
Electronic
scheme for Light
Emitters driving
is shown in Fig.
3.26.
The MOSFET
transistors are
used as a switch
keys which are
driven by TTL
logic levels.
The resistors RG
in a gate circuits fix closed state of transistors at the
absence of activity from external electronic scheme.
The sense resistor RS (0.22 Ohm) produces the feedback signal for current stabilization circuit.
The typical volt-ampere plot of the Light Emitter is
presented in Fig. 3.27. Dark area means technological
deviations of Light Emitter performance.
The capacitor C together with other external
capacitors, serves for accumulation of pulse energy for
Light Emitter.
Recommended circuit for driving by the Light Emitter is
presented in Fig. 3.28.
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DX6106
T = +25°C
5
4
ILED, A
Power Supply 5 V
(+4…+6 V are
available) through
resistor R charges the
capacitor C in time
duration between
pulses. Total capacity
(the capacitor C and
available external ones)
must be enough for
pulse current stability.
3
Safe Area
2
1
0
2
4
6
ULED, V
Fig. 3.27. Typical volt-ampere
Component list
Designation
Value
RE
4.7 W ±5%
RS
0.22 W ±5%
C
2 ´ 220 mF 6.3V
Construction of Optical Unit
3-25
RMT Ltd
DX6106
DX6106 Optical Unit
X2 6
DAC
X2 4
DAC
X2 5
RS
RG RG
Microcontroller
+
RE
C
X2 3
X2 1
Fig. 3.28. Typical LED control circuit
It is advisable in the real design to use some number of
analog multiplexors to distribute, for example, the
signal of singe DAC into two OPs or output signal of
one OP into two MOSFET gates. It will enable to spare
some equipment.
The current limiting and stabilizing circuit must be
implemented essentially into LED driving circuit. It is
because of the following reasons:
Ÿ The only current limiting factor is the RS = 0.22
Ohms sense resistor. (The MOSFET RON
resistance is negligible in comparison with RS).It
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DX6106
is easy to plot the load line (the curve in Fig.3.X)
and to see that the forward current through the
LED can run up to 5 amperes if +ELED voltage is
chosen as 6V.
Ÿ There is some difference of a photodetector’s
response to measuring and reference channel
LEDs emittance. To decrease the dynamic range
losses, the emitting powers of both LEDs should
be balanced.
Construction of Optical Unit
3-27
RMT Ltd
DX6106
EEPROM
EEPROM
SCL
X2 8 SDA
X2 7
The standard Electrically
Erasable PROM (EEPROM)
24LC64 chip with two wire serial
Fig. 3.21. I 2C interface connection
I2C interface is placed on Optical
Unit's PCB. It is used for storage
of the Optical Unit identification
code, calibration data and some additional data for
operation of the unit. Additional data are used for
operation of the Optical Units with manufacturer's
controller DX6101. In no power state the data retention
time is more than 200 years.
DX6106 Optical Unit
+5V
EEPROM
X2 7
X2 8
X1
X1
X1
X1
1 kW
1 kW
X1 2
SCL
SDA Microcontroller
3
4
6
8
Fig. 3.22. On-board Memory
typical connection
The recommended schematic for EEPROM connection
is presented in Fig. 3.22. Pay attention to the 1 kOhm
resistors that must pull-up the lines of I2C interface.
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RMT Ltd
DX6106
The detailed description of 24LC64 transfer protocol is
possible to obtain, for example, from Data sheet
retrieved from Microchip Corporation Web site
(http://www.microchip.com).
Besides the similar memory devices, are manufactured
by other corporations. For example Atmel, Fairchild, ST
Microelectronics, etc.
EEPROM Specification
Parameter
Value
Volume, bit
16 K (2K´8)
Number of re-writing cycles, not less than
10×106
Write speed, ms
5
Construction of Optical Unit
3-29
DX6106
RMT Ltd
EEPROM Data Format
Various operating parameters can be stored in onboard EEPROM circuit:
Ÿ calibration data,
Ÿ synchronization parameters,
Ÿ measuring mode presets,
Ÿ TE cooling algorithm presets,
Ÿ Optical Unit identification.
See recommended EEPROM data structure in Table
3.4.
The formats of the First Calibration Data Block is given
in Table 3.5.
Formats of other reserved (if applied) Calibration Data
Blocks are the same as the first one.
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DX6106
*)
Item
Table 3.4. EEPROM Data Format
Address
(hex)
1
0000
Calibration data block (first calibration
2
0018
Calibration data block
3
0030
Calibration data block
4
0048
Calibration data block
5
0060
Calibration data block
6
0078
Block of synchronization
7
0082
Block of parameters of measuring
8
008C
Parameters of thermostabilization of
9
008C
Parameters of thermostabilization of Light
10
008C
Optical Unit Identifier
Content
used only with DX6101 Controller
Item
Table 3.5. Format of the First Calibration Data Block
Address
(hex)
1
0000
TE coolers Operating Temperature
2
0002
Ambient Temperature of Calibration
3
0004
“Zero” Value
4
0008
5
Content
Name Format
Tc
Tenv
int16
float
Polynomial Coefficient A0
d0
A0
0014
Polynomial Coefficient A1
A1
float
6
0020
Polynomial Coefficient A2
A2
float
7
0024
Polynomial Coefficient A3
A3
float
8
0028
Polynomial Coefficient A4
A4
float
9
002C
Polynomial Coefficient A5
A5
float
10
0030
Polynomial Coefficient A6
A6
float
Construction of Optical Unit
int16
float
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DX6106
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RMT Ltd
DX6106
4. Installation Tips
There are two external power sources required for
Optical Unit supply.
An external +5V and -5V DC power sources with
±2.5% output tolerance are required for Optical Unit
supply. The operating current must be not less than 7.5
mA.
The power supplies are to be connected to pins X1/1
and X1/2.
They are necessary for supply of:
Ÿ preamplifier of Photodetector,
Ÿ thermistors and sensitive elements of Photodetector,
Ÿ EEPROM.
The power supply for customer external electronics
depends on scheme concepts. But one must take into
account that the total current consumption of Light
Emitters and TE Cooler of DX6106 Optical Unit is not
more than 300 mA at 0…-5°C operating temperature of
TE coolers.
For proper Optical Unit operation the ground line
should be separated into three wires and joined in the
one, close to power supply common terminal.
Shielding ground should be in contact with the Optical
Unit housing.
The recommended connection is shown in Fig. 4.1.
Installation Tips
4-1
RMT Ltd
DX6106
DX6106 Optical Unit
+5V / –5V
Converter
X1 1
+5V
+6¼9.5 V
Linear
Regulator
X1 2
X1 5
X1 7
Control &
Measuring
Circuits
Power
supply
0
X2 2
X2 6
X2 4
X2 5
X2 3
X1
X1
X1
X1
3
4
6
8
X2 1
LED &
TE Coolers
Drivers
Signal Ground
Power Ground
Shielding Ground
Fig. 4.1. DX6106 power supplies connection
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RMT Ltd
DX6106
5. Calibration
Preparation
First of all User should prepare the set of calibration
gases.
The number of calibration gases should be at least two
more than the desirable polynomial order (See Chapter
2). In turn the order of a polynomial determines
accuracy of approximation, and hence the measurement accuracy.
The following close to optimum set of calibration gases
can be recommended (in percentages to upper
concentration of measurement range):
Extended Kit
Calibration
Standard Kit
0
0
1
1
5
5
10
10
15
–
30
–
50
50
65
–
100
100
5-1
DX6106
RMT Ltd
Any other sets of standard samples User can apply
according to own reasons. But be sure that the samples
are within specified measurement range and the
customer standard gases provide accurate calibration.
As a “zero” gas one can use any standard pure gas.
Argon (Ar) or Nitrogen (N2) are quite suitable.
As other concentrations, the mixture of measured gas
with the “zero” gas is usually used.
Prepare some portions of plastic tubes for gas bottles
connection with Optical Unit’s gas inlets.
In further actions be guided by Chapter 3.
5-2
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RMT Ltd
DX6106
Zero Adjustments
To ensure the high accuracy, simple adjustment can be
made during operation to adjust “zero” ratio D0.
The procedure requires to flow up any "zero" gas
through the gas sampling cell.
The new D0 coefficient should be stored into EEPROM
in place of old value after the completing adjustment
procedure (See Chapter 2).
Calibration
5-3
DX6106
RMT Ltd
Re-Calibration
In standard option, the DX6106 Optical Unit is delivered
with one calibration data. The calibration is made at
optimal operating temperature.
User can make re-calibration at any time. It is possible
to do this at other operating temperatures, with larger
set of reference gases (larger order polynomial) and to
replace stored data by the new one.
According to customer demands the re-calibration
could be done by Manufacturer on request.
On-board memory can contain itself additionally 13
data blocks for more calibrations. Totally up to 14
different calibrations could be done.
The polynomial coefficients Aj depend on the design
of the Optical Unit’s optical scheme. It is not necessary
to make re-calibration often.
It is recommended to perform re-calibration annually.
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RMT Ltd
DX6106
6. Maintenance
Optics Cleaning
If the output signal of either channels (or both) became
appreciably less than usually, the Optical Unit’s optics
is most likely to require cleaning.
Cleaning of optics is executed with the help of suede
and the special optic cleaning fluid.
For optics cleaning the DX6106 Optical Unit must be
disassembled.
Remove screws from each end face of the Optical Unit.
Remove the covers (Fig. 6.1).
Bottom
cover
Optocomponent
Spherical
mirror
Housing
Top
cover
Rubber
gasket
Fig. 6.1. DX6106 Optical Unit disassembling illustration
Maintenance
6-1
RMT Ltd
DX6106
The Optical Unit after disassembling is shown in Fig.
6.2.
Fig. 6.2. DX6106 Optical Unit with the
The spherical mirror is glued to the top cover.
Do not try to rip it off.
Clean now
Ÿ the window of the optopair,
Ÿ spherical mirror,
Ÿ internal mirror (with a hole) from both sides.
Wait some minutes and assemble the Optical Unit in
the reverse order.
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REV. 1.10/2002
RMT Ltd
DX6106
7. Standard Kit
Item
#
Code
Quan.
1
Optical Unit
DX6106
1
2
Interconnection cable
DX6100-C-25
1
3
Interconnection cable
DX6100-C-26
1
4
Connector’s housing
ZHR-8
1
5
Connector’s housing
SHR-08V-S-B
1
6
Connector’s shrouded header
B8B-ZR
1
7
Connector’s shrouded header
BM08B-SRSS-TB
1
8
DX6106 User Manual
1
9
DX6100 software CD
1
Standard Kit
7-1
DX6106
7-2
RMT Ltd
REV. 1.10/2002
RMT Ltd
DX6106
8. Specifications
Common
Type
Detector
NDIR multipass scheme
Lead selenide with TE cooler
Measured gases
Carbon Dioxide
Hydrocarbons
CO2
CmHn
Operation conditions
Moisture protection
Temperature range
Relative humidity
IP65
-10° to 50°C
5 to 100%
Mechanical
Dimensions 4)
Weight
Specifications
42 ´ 27 ´ 27 mm
60 g (max)
8-1
RMT Ltd
DX6106
Carbon Dioxide (CO2) Sensor*)
Concentration range
1)
0...1000 ppm 0...5 % vol 0...20 % vol
Noise level 2, 3)
< 3 ppm
< 0.15 %
< 0.15 %
Accuracy 3)
10 ppm
0,5 %
0,5 %
Zero drift 3)
0.02 %
Hydrocarbons (CmHn) Sensor*)
Concentration range
1)
0...1000 ppm
Noise level 2, 3)
< 2 ppm
< 0.1 %
Accuracy 3)
10 ppm
0,5 %
Zero drift 3)
*)
If to use with DX6101 controller.
1)
Optional ranges up to 100% vol. are available.
2)
At Averaging Time Constant =0.2 s.
3)
If value in %, then it means relative units DX/X
4)
Without gas inlet pipes and 6102 module.
8-2
0...5 % vol
0.02 %
REV. 1.10/2002
RMT Ltd
DX6106
9. Ordering Guide
XXXXXX . XX . XXX . X
Gas Sampling Option
A - Aspiration
D - Diffusion
Concentration Range
The largest concentration value, in ppm,
includes 2 significant digits
followed by the number of zeros to follow
Gas Code
Code Gas
01 CO2
02 CnHm
03 CH4
04 CO
05 H2O
Part Number
Example:
DX6106.01.504.A
[DX6106] DX6106 Series,
[01]
CO2 Gas Option,
[504]
[A]
Ordering Guide
0...5.0×104 ppm (0...5%) concentration range,
aspiration type gas cell,
9-1
DX6106
9-2
RMT Ltd
REV. 1.10/2002
RMT Ltd
DX6106
RMT Ltd. Leninskij prosp. 53, Moscow 119991 Russia
phone: 095-132-6817 fax: 095-135-0565
e-mail: [email protected] http://www.rmtltd.ru
Specifications