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AvaRaman Operating manual AvaSoft Raman 7.3 November 2008

AvaRaman Operating manual AvaSoft Raman 7.3 November 2008

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The spline interpolation can be<br />

useful for applications in which<br />

the output of line sources, like<br />

laser diodes is displayed, or for<br />

other applications, which<br />

require a high resolution. Note<br />

that for the AvaSpec-2048 with<br />

2048 pixels, the effect of<br />

spline interpolation is not<br />

visible if the data is shown at<br />

full scale. The monitor<br />

resolution is much less than<br />

2048 pixels. The effect of<br />

spline interpolation can only<br />

be visualized if the number of<br />

detector pixels that are<br />

displayed is smaller than the<br />

number of monitor pixels at<br />

the x-axis.<br />

Smoothing<br />

To get a smoother spectrum without losing information it is important to set in the software the<br />

right smoothing parameter. The optimal smoothing parameter in a standard <strong>Ava<strong>Raman</strong></strong> system with<br />

50 micron slit is 1, in which case the data at each pixel will be averaged with one neighbor pixel at<br />

the left and one at the right. This can be done without losing resolution, because the 50 micron<br />

beam will cover at least 3 detector pixels (the distance between the pixels at the CCD detector is<br />

14 micron). The <strong>Ava<strong>Raman</strong></strong>-TEC includes a 25 micron slit in which case the smoothing should be set<br />

to zero.<br />

If resolution is not an important issue, a higher smoothing parameter can be set to decrease noise<br />

against the price of less resolution.<br />

2.3.2.4 Setup Menu: Correct for Dynamic Dark<br />

The pixels of the CCD detector (AvaSpec-2048) are thermally sensitive, which causes a small dark<br />

current, even without light exposure. To get an approximation of this dark current, the signal of the<br />

first 14 optical black pixels of the CCD-detector can be taken and subtracted from the raw scope<br />

data. This will happen if the correct for dynamic dark option is enabled. As these 14 pixels have the<br />

same thermal behaviour as the active pixels, the correction is dynamic.<br />

If this menu option is preceded by a checkmark, the scope data is corrected with the dynamic dark<br />

algorithm. It is recommended to leave this setting checked, which is the default state.<br />

32 AvaRAMAN <strong>manual</strong>.doc Nov-08<br />

Avantes www.avantes.com info@avantes.com

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