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Daily Instrument Tuning
Delta Plus Advantage
Although our instrument configuration does change over time, we currently
(April 2007) have three peripherals connected to the Delta Plus: an EA, and a
TOC analyzer, both connected via a Conflo interface, and a Gasbench with the
multiprep heating block. Gas flow must go from the peripheral that will be used to the mass
spectrometer during the tuning. It also needs to be in its operational mode: ie.
the EA or TOC analyzer should be in "work" mode.
MAT 253
The MAT 253 has three peripherals: a TC/EA, with associated Conflo interface,
a GC-C/TC with associated interface, and a dual inlet. If
we are doing dual inlet analyses, then the SGE valves for the continuous flow
inlets should be closed. If we are doing continuous flow measurements then only the SGE valve for the appropriate peripheral should be open.
We record the ion source pressure with each peripheral connected and that number
has remained constant over years.
The overall tuning process includes:
1) background checks for leaks or high moisture
2) peak centering the reference gas
3) autofocusing the instrument
4) stability checks
5) linearity checks (including the H3 factor measurement
for hydrogen)
1) Background checks:
Before any analyses it is necessary to check the
background levels of H2O, N2, O2, and Ar. We start with the instrument in the CO2 gas
configuration. Then do a mass jump with the center cup to the appropriate mass
(say, m/z 18 for H2O). We then do a peak center at this mass
and record the beam intensity on the center cup. We repeat this process for
m/z 28 (N2), 32 (O2), and 40 (Ar). Note that high N2
and O2 are indicative of a leak with atmosphere somewhere in the
system, additionally, a high water background will result in a higher m/z
32 background. High water can indicate moisture collecting somewhere or failing water
traps. In particular, if the instrument has been vented to atmosphere then a
high water background can be expected for a couple of days. Although the
atmosphere is about 1% argon, monitoring this gas is not as sensitive to leaks as N2 and O2. In a
well operating system, argon is mainly present as an impurity in the UHP helium.
For us, the argon background is an indication of the quality of our helium. It
happens that occasionally the argon background is 50 to 100 times higher than
usual with a new helium tank. In this case we return the helium tank to the
supplier and ask for another one. High argon
tells us that the quality of helium in the tank is not reliable and it also
makes it difficult for us to troubleshoot leaks in the system. There will be
more information on this in the "troubleshooting" section, but briefly:
if we suspect leaks then we set the center cup to monitor m/z 40 in
instrument control and spray the fittings with argon. If there is a big enough
leak then we'll see the m/z 40 beam rise. If there is a lot of argon in
our background then it becomes more difficult to see leaks when troubleshooting.
2) Peak centering the reference gas
After we have documented the background levels, then we
set the center cup to m/z 45 and insert the CO2 reference into the open
split. A new peak
center is done and the value of the high voltage is recorded.
3) Autofocusing the instrument
There are special precautions that need to be taken for
hydrogen analysis. These are not addressed here, instead check the "Hydrogen"
section.
With the reference gas on, we then choose the autofocus
option and let Isodat do the work. We had done some initial studies to see how
the beam intensity and isotope ratio varies with the tuning parameters. This
should be done for any new gas on any instrument in order to characterize its
behavior. After the autofocus is
done the new parameters are saved with the "add to gas configuration" option.
4) Stability checks
The instrument stability (and precision) are checked by
running a series of reference gas pulses and seeing what the precision of the
measurement is. The manual refers to this as the "zero enrichment" test. We generally define the second reference gas peak as the
standard in the method file and set its isotope ratios to zero. We then check
the standard deviation of a series of 10 reference gas pulses. For a reason that
we really don't understand, the first run usually comes out worse than the
others, so we perform this check two to three times in sequence. For
d13C, d18O
(from CO2), and d15N we
generally get standard deviations that are below 0.05‰. It is important that the
standard deviation here be low as it represents the best precision that can be
obtained with the instrument. If poor
precision occurs here then it is necessary to figure out why the precision has
died before proceeding with any sample analyses.
5) Linearity checks
Another issue with mass spectrometers is linearity.
Linearity refers to the reproducibility of a result with different amounts of
sample or signal. One way to test this is by performing a series of 10
reference gas pulses, but manually increasing the reference gas
pressure at the end of each pulse. The result is a series of reference gas peaks
stepping up in intensity. The spec for the both of our mass spectrometers is
that the isotope ratio should not change by more than 0.06‰/V. Ie. if one
reference gas peak is 1 volt higher in intensity than another one, then its
measured isotope ratio should not be more than 0.06‰ different from the first
peak. The way this is monitored is by looking at the slope of the regression curve
for the series of gas pulses. For any continuous flow device, the best way to
perform a linearity check is by varying the amount of a real standard that is
analyzed and observing the effect of the sample size on the measured isotope
ratio. This most closely
reflects the real run conditions, and also allows you to make an appropriate
linearity correction to the data.
d13C, d18O
and d15N: All of the above
checks are performed for each reference gas that will be used.
d2H: All of the
above checks are performed for hydrogen. However, the H3+
factor must be determined for hydrogen. This is effectively a linearity
correction as well.
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Page last updated: April 16, 2007
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