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NOTE: WAVELENGTH POSITION ACCURACY AT HIGH WAVELENGTHS (632.8NM) IS
ACHIEVED WHEN CALIBRATING THE SYSTEM USING THE GADJUST FUNCTION IN MONO
CONTROL SOFTWARE. THIS WILL REQUIRE USE OF A CCD DETECTOR.
Calibrating the SCT-320 using Software
This procedure requires the use of a CCD detector, Lighfield or WinSpec software, and a mercury lamp
installed on the entrance slit of the SCT-320. The CCD should be running for this procedure.
16)
Make sure that MONO CONTROL SOFTWARE is running before starting Lightfield or WinSpec. This is
important because MONO CONTROL SOFTWARE must have control of the SCT-320 for this alignment
procedure. Lightfield or WinSpec will be controlling the CCD.
17)
Set the entrance slit width to 10 microns
18)
Set CCD region of interest to the center row (1 pixel binning)
19)
Scan the SCT-320 to 0.0nm using MONO CONTROL SOFTWARE
20)
Run the CCD in continuous or focus mode
21)
Verify that the zero order (0.0nm) line is located at the center of the CCD (for example, pixel 670 for a Pixis
CCD)
22)
If the position of the zero order line needs to be adjusted to the center of the CCD, adjust the grating rotation
screw. Refer to Figure 4 for location of the Grating Rotation Screw.
23)
When zero order has been set, scan the SCT-320 to 546.074nm
24)
Note the location of the 546.074nm mercury line. If it is located at pixel 670, then it does not require further
calibration. If the 547.074nm mercury line is NOT located at pixel 670, continue to the GADJUST section below.
GADJUST Procedure
25)
Monochromator Control Software Main Menu. Select the
OPERATION
button.