- Extremely low stray light allows the multi-element detector to simultaneously acquire both Stokes and Anti-Stokes components at the distance up to 20 cm-1 from the excitation line (1200 l/mm gratings) without using any Notch or Edge-filters.
- The compact long-focus instrument (f=833mm) with the unique high aperture (F# 1:5.5)
enables solving tasks, that demand high spectral resolution, yet
occupies little space in your laboratory and, furthermore, is mobile.
- The M833i in the Imaging mode provides absolute
astigmatism compensation and high spatial resolution along the exit
slit, meanwhile preserving the ideal line quality.
- Three pairs of gratings (number of lines per mm
and blaze wavelength are tailored to the Customer's requirements) are
supplied in a standard set and ensure the widest range of applications.
- Two input and two output ports can be completed
with the full set of accessories manufactured by SOLAR LS: standard and
crossed entrance slits, order separating filter wheels, aperture
matching units and optical fibers, CCD detectors and adapters for them.
- Full computer control: slits, diffraction
grating turrets and filter wheels, input/output port switching is
controlled by the intelligent and easy-to-use software.
- The SolarLS.LAB software provides automated
control over the M833 and its detectors. It allows stitching spectra
obtained by several diffraction grating scans in order to get a
panoramic spectrum. Many possibilities of spectra processing and
analysis are provided as well.
- At your request, DLL and/or VI program modules are supplied for controlling the instrument via the customised software or LabVIEW.
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Features
- Extremely low stray light allows the multi-element detector to simultaneously acquire both Stokes and Anti-Stokes components at the distance up to 20 cm-1 from the excitation line (1200 l/mm gratings) without using any Notch or Edge-filters.
- The compact long-focus instrument (f=833mm) with the unique high aperture (F# 1:5.5)
enables solving tasks, that demand high spectral resolution, yet
occupies little space in your laboratory and, furthermore, is mobile.
- The M833i in the Imaging mode provides absolute
astigmatism compensation and high spatial resolution along the exit
slit, meanwhile preserving the ideal line quality.
- Three pairs of gratings (number of lines per mm
and blaze wavelength are tailored to the Customer's requirements) are
supplied in a standard set and ensure the widest range of applications.
- Two input and two output ports can be completed
with the full set of accessories manufactured by SOLAR LS: standard and
crossed entrance slits, order separating filter wheels, aperture
matching units and optical fibers, CCD detectors and adapters for them.
- Full computer control: slits, diffraction
grating turrets and filter wheels, input/output port switching is
controlled by the intelligent and easy-to-use software.
- The SolarLS.LAB software provides automated
control over the M833 and its detectors. It allows stitching spectra
obtained by several diffraction grating scans in order to get a
panoramic spectrum. Many possibilities of spectra processing and
analysis are provided as well.
- At your request, DLL and/or VI program modules are supplied for controlling the instrument via the customised software or LabVIEW.
Applications:
- Raman Spectroscopy
- Emission and Fluorescence Spectroscopy
- Analytical Tasks Demanding High Resolution in the Range from UV to IR
- Multi-Channel Spectroscopy
Instrument Configuration
The M833 comprises either one or two input and output ports. Input
port may hold either a standard entrance slit, or a crossed entrance
slit (optionally). All the spectral slits are automated; their width is
adjusted by the instrument software. The slit design also contains a
microscrew, which provides the possibility to manually adjust the
opening width of the slit knives.
The standard M833 version comprises three pairs of diffraction
gratings mounted on two turrets. Since the M833 implements separate
control for scanning and grating changing, each diffraction grating,
when scanning the spectrum, rotates around an axis passing through its
center. This allows to bring your real optical system close to the
initial optical design and to provide its highest optical quality.
The standard optics comprises spherical and flat mirrors with Al+MgF2
coating optimized for high UV efficiency. Optionally the M833 may
contain optics with Al+SiO2 or gold coating for high efficiency in the
infrared spectral range.
The M833 output ports may hold either two exit slits, or one exit slit and detector, or two detectors concurrently.
Direct (axial) and lateral (radial) output ports operate alternately.
Switching between the output ports is effected by the software with the
use of the swinging mirror, which in its operating position directs
light to the lateral (radial) output port. The instrument is also
available with one output (axial) port. If the radial output port is not
used, it is plugged.
The M833 exit slit has 4 mounting holes M2.5 that allow you fixing
your own detector to the slit housing, if necessary. Location of
mounting holes is shown in the figure below.
Note: To avoid a breakdown of the slit mechanism it is prohibited to fix any units weighing more than 1 kg to the slit housing!
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