specifications
part number | spectral region | form | total range | simultaneous range | resolution* | resolution |
with grating rotation | at a fixed grating position | pm | 1/cm | |||
hf-8888-uv | uv | c | 200 - 400nm | fixed 60nm range | <30pm | 0.9/cm |
hf-8888-uvlibs | uv (gated) | c | 200 - 400nm | fixed 60nm range | <30pm | 0.9/cm |
hf-9332 | vis | c | 450 - 700nm | fixed 250nm range | <25pm | 0.9/cm |
hf-9353 | nir | c | 750 -1050nm | fixed 300nm range | <40pm | 0.5/cm |
hf-8989-1 | vis | a | 425 - 500 nm | 17 nm | 1.7 pm | 0.08/cm |
hf-8989-2 | vis | a | 500 - 600 nm | 16 nm | 1.6 pm | 0.05/cm |
hf-8989-2e | vis | a | 525 - 640 nm | 16 nm | 1.6 pm | 0.05/cm |
hf-8989-3 | vis | a | 600 - 700 nm | 16 nm | 1.6 pm | 0.04/cm |
hf-8995-1 | nir | a | 700 - 800 nm | 20 nm | 2.0 pm | 0.03/cm |
hf-8991-3 | nir | a | 800-950 nm | 25 nm | 2.0 pm | 0.02/cm |
hf-8995-2 | nir | a | 950 - 1100 nm | 25 nm | 2.5 pm | 0.02/cm |
hf-8995-3-plasma | nir | d | 775-900nm | 9 nm | 0.9 pm | 0.01/cm |
hf-8999-pk-lll-** | vis | d | 1.0 pm | 0.04/cm | ||
*-uhr | 2x resolution upgrade to any model. | |||||
notes
u form factors (enclosure dimensions, does not include camera or input port)
ø a dimensions; 250 x 600 x 150mm, weight; 20kg
ø b dimensions; 200 x 200 x 90mm, weight; 2kg
ø c dimensions; 160 x 200 x 100mm, weight; 1.5kg
ø d dimensions; 700 x 150 x 400mm, weight; 28kg
ø e dimensions; 700 x 150 x 250mm, weight 28kg
ø f dimensions; 400 x 500 x 150mm, weight 24kg
u *range and resolution are measured at the middle of the wavelength range
u accuracy: < 200pm for fixed grating units, <20pm for all others following calibration, an external calibration source is required
u dynamic range: 100:1 to 500:1 in a single shot measurement, up to 50db with exposure bracketing
u simultaneous range / resolution: >10,000 at 532nm
u acquisition speed: >10hz typical
u ** is specifically designed for brillouin scattering and includes a multi-pass etalon for 532nm elastic scattering suppression.
options
u mmf input with a 10um slit, smf input with no slit is standard
ulow resolution mode, covers the total range with 0.2nm resolution
u camera options;
ø cmos for laser characterization, passive element characterization, brillouin, raman and solar spectroscopy
ø ccd for low light applications (non -scanning of brillouin biological samples)
ø scientific cmos for low light applications requiring fast acquisition
ø iccd for applications requiring gating (libs)
ø uv c-mos with good quantum efficiency down to 260nm
features
u fast, no moving parts (single shot laser spectrum analysis)
u sub picometer resolution
u fiber optic input
u quick data acquisition and export
u simple usb interface
u labview drivers
benefits
u fast
u compact
u can resolve hyper fine spectra below 1 picometer
u ultra-reliable
u lightmachinery's legendary customer support
application
light sources characterization
u lasers of all types
u single shot pulsed laser spectrum
u super luminescent diodes
u gas discharge lamps, etc
spectroscopy
u plasma spectroscopy
u high-precision gas spectroscopy
u brillouin or raman spectroscopy
u femtosecond comb fingerprinting spectroscopy
uspectral-domain optical coherence tomography, etc
u solar spectroscopy
u astronomical spectroscopy
u ultra low frequency raman
u undergraduate physics and chemistry laboratories
ø zeeman splitting
ø hyperfine magnetic structure of elements
ø hydrogen structure
ø doppler shift of fraunhofer lines due to sun rotation
passive components characterization
u notch filters
u etalons
u fiber bragg gratings, etc
how does it work?
light enters the hyperfine spectrometer though a fiber. a vipa etalon, manufactured using lightmachinery's proprietary fluid jet polishing technology, is used to produce very high dispersion in the vertical axis with sub picometer resolution. this is followed by a conventional grating to disperse overlapping orders in the horizontal direction and produce a 2d spectrum of the input light. lightmachinery software unwraps the spectrum to produce an ultra high resolution wavelength spectrum of the input light. a secondary camera provides a wide wavelength range, lower resolution view of the spectrum.

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