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 | 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 **HF-8999-532-AUTO 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
u Low 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
u Spectral-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.