Campbell Scientific TGA200A TGA Series Trace Gas Analzyers - Page 147

Appendix D. Optimizing Detector Parameters, D.1 Detector Gain and Offset, D.2 Detector Preamp Gain

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Appendix D. Optimizing Detector Parameters Set the detector parameters after the laser parameters are adjusted. D.1 Detector Gain and Offset The detector signals are processed in the TGA electronics, which include an amplifier with programmable gain and offset in the input module, and a second programmable-gain amplifier in the analog module. The detector gains and offsets are normally controlled automatically by the TGA software. To enable this automatic control, click the Auto gain/offset box on the Settings > Detectors > Preamp window. To set the offsets and gains manually, adjust one of the values to disable the automatic function. The detector gains and offsets should usually be controlled automatically. However there are two exceptions. First, automatic control should be disabled while performing some of the setup steps, such as optical alignment. Second, the automatic gain algorithm will not increase the sample gain beyond gain 7. Therefore, if the detector signals are extremely weak, it may be necessary to set the detector gains and offsets manually. D.2 Detector Preamp Gain The detector electronics have a fixed gain in the first preamplifier stage. Early TGAs used a gain of 200, but this was changed to 45 for TGA200s and TGA200As. This reduced gain allows the detector signals to be larger without saturating the input range. This is an advantage for higher-power lasers, and for LN2-cooled detectors used for longer wavelengths. Some early input modules have been modified to use a gain of 45 in the preamp. These instruments are identified by a label on the printed circuit board: Gain 45. Input modules upgraded for use with TE-cooled lasers have a gain of 45. These modules have a blue label on the top that designates them for use with TE-cooled lasers (see Appendix H.3.1, Basic Upgrade). The preamp gain (either 45 or 200) must be entered in the parameters at the Settings > Detectors > Preamp window. If it is unclear which gain is the correct one for a specific input module, or if an input module upgrade is desired, contact Campbell Scientific. D.3 Detector Temperature Most TGAs are equipped with TE-cooled detectors, but some are equipped with LN2-cooled detectors to work with longer-wavelength lasers. LN2-cooled detectors have no temperature measurement or control. They are designed to operate near LN2's boiling point, 77 K. TE-cooled detectors include a thermistor to measure the detector's temperature. The TGA measures this temperature and adjusts the TE-cooled current to cool the detector to the setpoint. Generally, a lower detector temperature will increase the detector signal and decrease the concentration noise. However, some lasers emit enough power to saturate the detectors if they are cooled to D-1

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Appendix D. Optimizing Detector
Parameters
Set the detector parameters after the laser parameters are adjusted.
D.1 Detector Gain and Offset
The detector signals are processed in the TGA electronics, which include an
amplifier with programmable gain and offset in the input module, and a second
programmable-gain amplifier in the analog module.
The detector gains and
offsets are normally controlled automatically by the TGA software.
To enable
this automatic control, click the
Auto gain/offset
box on the
Settings >
Detectors > Preamp
window.
To set the offsets and gains manually, adjust
one of the values to disable the automatic function.
The detector gains and offsets should usually be controlled automatically.
However there are two exceptions.
First, automatic control should be disabled
while performing some of the setup steps, such as optical alignment.
Second,
the automatic gain algorithm will not increase the sample gain beyond gain 7.
Therefore, if the detector signals are extremely weak, it may be necessary to set
the detector gains and offsets manually.
D.2 Detector Preamp Gain
The detector electronics have a fixed gain in the first preamplifier stage. Early
TGAs used a gain of 200, but this was changed to 45 for TGA200s and
TGA200As. This reduced gain allows the detector signals to be larger without
saturating the input range. This is an advantage for higher-power lasers, and
for LN
2
-cooled detectors used for longer wavelengths. Some early input
modules have been modified to use a gain of 45 in the preamp. These
instruments are identified by a label on the printed circuit board:
Gain 45
.
Input modules upgraded for use with TE-cooled lasers have a gain of 45.
These modules have a blue label on the top that designates them for use with
TE-cooled lasers (see Appendix H.3.1,
Basic Upgrade
).
The preamp gain (either 45 or 200) must be entered in the parameters at the
Settings > Detectors > Preamp
window. If it is unclear which gain is the
correct one for a specific input module, or if an input module upgrade is
desired, contact Campbell Scientific.
D.3 Detector Temperature
Most TGAs are equipped with TE-cooled detectors, but some are equipped
with LN
2
-cooled detectors to work with longer-wavelength lasers. LN
2
-cooled
detectors have no temperature measurement or control. They are designed to
operate near LN
2
’s boiling point, 77 K.
TE-cooled detectors include a thermistor to measure the detector’s temperature.
The TGA measures this temperature and adjusts the TE-cooled current to cool
the detector to the setpoint. Generally, a lower detector temperature will
increase the detector signal and decrease the concentration noise. However,
some lasers emit enough power to saturate the detectors if they are cooled to
D-1