Ocean Optics S2000 - Manual (Page 51)

6. The numbers of importance are indicated in the above figure. You will need to record the Intercept as well as
the First, Second, and Third Coefficients. Also, look at the value for R squared. It should be very close to 1. If
it is not, you have probably assigned one of your wavelengths incorrectly.
7. Select Spectrometer | Configure from the menu and choose the Wavelength Calibration page to update
the wavelength coefficients within OOIBase32.
8. Repeat this process for each channel in your setup.
Spectral Output
Mercury emission lines are <600 nm. Argon emission lines are >600 nm, and are shown here on the right on an
exaggerated amplitude scale. Below is a list of the most prominent mercury and argon peaks.
Specifications
Light Sources: HG-1
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Mercury Lines
253.65
296.73
302.15
313.16
334.15
365.01
404.66
407.78
435.84
546.08
576.96
579.07
Argon Lines
696.54
706.72
710.75
727.29
738.40
750.39
763.51
772.40
794.82
800.62
811.53
826.45
842.46
852.14
866.79
912.30
922.45
Output: low-pressure gas discharge lines of Mercury and Argon
Spectral range: 253-922 nm
Dimensions: 11.4 cm x 6.98 cm x 2.54 cm (LWH), 4.5" x 6.98" x 1.0" (LWH)
Power requirements: 12 VDC wall transformer (comes with unit) or 9 VDC battery
Internal voltage: 600 volts at 30 kHz
Bulb life: ~3,500 hours
Amplitude stabilization: ~1 minute
Aperture: 3 mm
Connector: SMA 905