Triple Spectrometer, Raman Commander
Work closer to the Raligh scatter with the Raman Commander. Use the f/4.8 aperture to collect more precious photons. The all reflective optical system works fine in the UV. The double subtractive 350mm focal length pre- monochromator is efficient. There are many available gratings capable of getting you to within 20cm-1. The spectrometer stage can be f/4.7 670-mm when you need the most light or specify f/9.4 1330-mm. The latter provides wonderful symetrical line profiles and resolution of 0.3cm-1.
The Raman Commander is a research tool everyone can use. Reflective optics with optimized coatings provide good efficiency in the ultraviolet (UV.)
Optical Design | Czerny Turner design Monochromator / Spectrometer |
Focal Length | 350 mm |
Aperture Ratio | f/4.8 (NA 0.1) |
Wavelength Range | refer to grating of interest for range |
Wavelength Accuracy | ±0.2 nm |
Wavelength Reproducibility | ± 0.05 nm (with 1200 G/mm grating) |
Grating Size | 68 x 68 mm (single grating holder, optional dual-grating turret) |
Slits | Micrometer adjustable width 0.01 to 4 mm, height settings from 2 to 20 mm |
Slit Locations | Axial and lateral, with optional port selection mirrors |
Focal Plane | 25-mm, multiply dispersion by the width of your detector for range |
Grating Groove Density (g/mm) | 3600 | 2400 | 1800 | 1200 | 600 | 300 | 150 | 75 | 50 |
Spectral Resolution at 312.6nm (nm, FWHM) | 0.02 | 0.025 | 0.035 | 0.05 | 0.1 | 0.2 | 0.4 | 0.8 | 1.2 |
Reciprocal Linear Dispersion (nm/mm) | 0.7 | 1 | 1.5 | 2 | 4 | 8 | 16 | 32 | 48 |
Wavelength Range from 185nm to | 430 | 650 | 865 | 1.3 um | 2.6 um | 5.2 um | 10.4 um | 20.8 um | 31.2 um |
First Order Littrow Blaze (nm) | 240 | 240 | 180 | 200 | 250 | 280 | 300 | 2 um | 600 |
holo | 300 | 250 | 300 | 300 | 300 | 500 | 3 um | 12 um | |
holo | 400 | 400 | 500 | 500 | 800 | 8 um | 14 um | ||
holo | 500 | 750 | 750 | 1.25 um | 10 um | ||||
750 | 1 um | 1 um | 2.5 um | 12 um | |||||
1 um | 1.8 um | 3 um | 4 um | ||||||
holo | holo | 4 um | 6 um | ||||||
8 um | |||||||||