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Ocean Optics Flame-S
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5: How the Flame Spectrometer Works
225-00000-000-11-201604 41
Grating
Number
Intended Use
Groove Density
Spectral Range
Blaze Wavelength
Best Efficiency
(>30%)
12
UV-VIS
2400
50-120 nm
Holographic VIS
260-780 nm
14
NIR
600
625 nm
1000 nm
650-1100 nm
31
UV-NIR
500
200-1025 nm
250 nm
200-450 nm
Grating efficiency curves are available to view by using our online range and resolution
calculator at www.oceanoptics.com/product-category/modular-
spectrometers/.
Gratings Showing Light Diffracted into its Constituent Wavelengths
6. Focusing Mirror (specify standard or SAG+): This mirror focuses first-order spectra
on the detector plane. Both the collimating and focusing mirrors are made in-house to
guarantee the highest reflectance and the lowest stray light possible. You can opt to
install a standard or SAG+ mirror. As with the collimating mirror, the mirror type needs
to be specified when ordering.
7. Detector Collection Lens (optional): This cylindrical lens is fixed to the detector to
focus the light from the tall slit onto the shorter detector elements. It increases light-
collection efficiency and reduces stray light. It also is useful in a configuration with a
large-diameter fiber and slit for low light-level applications such as fluorescence.
Preconfigured Flame spectrometers with a collector lens are available look for ES at
the end of the name.
8. Detector: There are two choices of detector available for the flame. We offer a 2048-
element FLAME-S (Sony ILX511B) or a 3648 element FLAME-T (Toshiba
TCD1304AP) linear CCD array. These both have an effective range of 190-1100 nm. The
optics split the light into its component wavelengths which fall across the different

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