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Thermonicolet Omnic Software User's Guide 6.1 (PDF) - Charles E ...

Thermonicolet Omnic Software User's Guide 6.1 (PDF) - Charles E ...

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As an example, for a standard DTGS detector operating at a mirror velocity of<br />

0.633 cm/s and an optical cutoff at 7900 wavenumbers, the electronic filter should<br />

be set to 10 kHz (see the equation below).<br />

10 kHz = 2 * (0.633 cm/s) * 7900/cm<br />

Note<br />

The available settings depend on your application. The 10 kHz setting used in this<br />

example may not be available. ▲<br />

For near-IR measurements, OMNIC automatically sets the sample spacing to<br />

every laser crossing. Thus, the free spectral range is opened up to 15,800<br />

wavenumbers, and the low pass filter can also be opened up to a higher value<br />

(20,000 Hz in the case of our example). For visible spectroscopy, a sample<br />

spacing of one-half the HeNe frequency is also available.<br />

Finally, there are some research applications where a sample spacing of 4 is<br />

desirable. In such cases, pay close attention to the effects of folding on the infrared<br />

spectrum. For these sample spacing values, you must use both optical and<br />

electronic filtering to prevent folding of spectral features and noise into the desired<br />

spectrum. For more information, please see the excellent text by Peter R. Griffiths<br />

and James A. de Haseth entitled Fourier Transform Infrared Spectrometry, New<br />

York, John Wiley and Sons, 1986.<br />

If you want the cutoff to be set automatically based on the velocity of the moving<br />

mirror, turn on Set Filters Based On Velocity. The Low Pass Filter drop-down list<br />

box is unavailable when the check box is on.<br />

Note<br />

If you use the SST software to perform an AM step scan, PM step scan, PEM,<br />

TRS or SMM experiment, the settings of Low Pass Filter, High Pass Filter and Set<br />

Filters Based On Velocity are ignored. ▲<br />

Specifying the<br />

cutoff frequency<br />

of the high pass filter<br />

High Pass Filter determines the frequency below which the effects of low-frequency<br />

noise are removed from collected data. Sources of this noise include room<br />

vibrations, fans, etc. This noise is normally a concern only when you are using a<br />

very low mirror velocity, such as for a slow-scan photoacoustic measurement, or<br />

when you are collecting far-IR spectra.<br />

You should normally set this parameter to a value equal to 1 divided by the<br />

frequency of the noise.<br />

Note<br />

Note<br />

If you want the cutoff to be set automatically based on the velocity of the moving<br />

mirror, turn on Set Filters Based On Velocity. The High Pass Filter drop-down list<br />

box is unavailable when the check box is on. ▲<br />

If you use the SST software to perform an AM step scan, PM step scan, PEM,<br />

TRS or SMM experiment, the settings of Low Pass Filter, High Pass Filter and Set<br />

Filters Based On Velocity are ignored. ▲<br />

Collecting<br />

single-sided<br />

interferograms<br />

Turn on Single-Sided Interferogram if you want to collect single-sided, rather than<br />

double-sided, interferograms. This speeds up data collection and is useful when<br />

you are performing GC/IR, kinetics or other series experiments in which a large<br />

number of scans are collected during a given amount of time.<br />

Note<br />

The signal-to-noise ratio will be lower when you collect data with this option<br />

turned on. ▲<br />

140 Thermo Nicolet

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