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Multi-detector line-scan hyperspectral camera | SIMTRUM Photonics Store

Multi-detector line-scan hyperspectral camera
SIMTRUM's HY-1X series adopts self-developed slit-prisms-rasters-prism hyperspectral imaging technology, using push-sweep imaging, fully reflects the technical advantages of volume holographic grating, with high spectral resolution, high efficiency, good spectral linearity, small spectral line bending, simple use, small size, light weight and many other advantages, the main performance indicators have been achieved Leading level of similar international products. It features multiple spectral bands and different sizes of spectroscopic modules and detector types to choose from, with the band range covering 400-2500nm.
 
Features
  • Band covering 400-2500 nm
  • By adopting the prism-grating spectral separation method, more accurate and higher-resolution spectral data can be obtained
  • Self-developed module can be adapted to a variety of detectors, with multi-band, multi-size, multi-detector types to choose from
  • Full target surface high imaging quality optical design, with point sequence spot diameters less than 0.5 pixels
  • Standard C-Mount type lens interface, and the focal length can be changed according to the user's requirements

 

Application
  • Analysis of agricultural pests and diseases
  • Environmental monitoring
  • Industrial sorting

VIS-NIR Wide-Spectrum Hyperspectral Camera(VNIR-NIR)
Parameter LA-HY01-1710-01 LA-HY01-1710-05
Spectrophotometric mode Linear - Transmission grating spectral separation
Spectral channel VNIR NIR VNIR SWIR
Grating type Transmission grating
Spectral range 400-1000nm 900-1700nm 400-1000nm 1000-2500nm
Merge spectral range 400-1700nm 400-2500nm
Number of spectral channels 300 512 300 ≥400
Merge the number of spectral channels ≥700 ≥640
Spectral resolution better than 2.8nm better than 6nm better than 2.8nm better than 10nm
F number F/2.6 F/2.0 F/2.6 F/2.0
Detector CMOS InGaAs(TE Cooled) CMOS HgCdTe(Stirling Refrigeration)
Detector interface USB3.0 GigE USB3.0 USB3.0/GigE
Detector target surface size 11.3mm x 7.1mm 9.6mm x 7.68mm 11.3mm x 7.1mm 9.6mm x 7.68mm
Original pixel size of the detector 5.86 µm x 5.86 µm 15µm x15 µm 5.86µm x 5.86 µm 15µm x15 µm
Effective pixel bit depth 12bits 14bit 12bits 14bits
Effective slit length 11.3mm 9.6mm 11.3mm 9.6mm
Slit width 25μm 25μm 25μm 25μm
Number of spatial channels 1920 640 1920 640
Merge the number of spatial channels 640 640
Field of View (FOV) 21°@f=25mm 21°@f=25mm 21°@f=25mm 21°@f=25mm
Merge Field of View (FOV) 21°@f=25mm 21°@f=25mm
Instantaneous Field of View (IFOV) 1mrad@f=25mm 1mrad@f=25mm 1mrad@f=25mm 1mrad@f=25mm
Merge Instantaneous Field of View (IFOV) 1mrad@f=25mm 1mrad@f=25mm
Max frame rate 128fps 175fps 128fps 100fps
Power supply for the detector 12V DC ,4.3W 12V DC ,16W(TEC ON) 12V DC ,4.3W 24V DC ,30W
Merge power Max 20-25w Max 35w

Technical Guide

If you need our technical team for guidance on product selection or customization, please help to provide below technical information, it helps to speed up the process.

Items Detail Remark
Application? Agriculture/Mining/Food safety/Industrial sorting/Environmental monitoring  
What is the required spectral range? UV/VIS/NIR/MIR/LWIR  
What spectral resolution is required? eg:2nm  
What spatial resolution is required?    
What is the size of the field of view? eg:18°  
What is the motion state of the object being measured? Motion/static?  
What is the required frame rate? Moving objects require a high frame rate; otherwise, there will be ghosting when shooting  
What is the required data interface? USB /GigE port  
Is a lighting source needed?  

 

The core of hyperspectral imaging is to obtain the reflection information of the target object at different wavelengths. Under low-light conditions, an external light source is required for illumination. Meanwhile, external light source illumination can provide more uniform and stable light, avoiding the dark differences and spectral distortion of the image caused by uneven illumination. The lighting source can be selected as: halogen lamp /LED light source

Is a reflectance board needed?  

 

The function of a reflectance board is to provide a calibration reference for hyperspectral data, ensuring the accuracy and traceability of spectral reflectance data.Since there are usually certain differences in reflectance measured by different devices and at different times, after calibration with a reflectance board, the spectral data of the same target collected by different cameras/times can be directly compared. That is: The function of the reflectance board is to enable the quantification of hyperspectral data.

 

 

 

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Compare Model Drawings & Specs Availability Reference Price
(USD)
LA-HY01-1710-01
Spectral range: VNIR:400-1000nm;NIR:900-1700nm; Merge spectral range:400-1700nm; Number of spectral channels: VNIR: 300;NIR: 512; Merge the number of spectral channels:≥700; Spectral resolution: VNIR: better than2.8nm;NIR: better than 6nm; Slit width:25μm; Number of spatial channels: VNIR: 1920;NIR: 640; Merge the number of spatial channels:640; Frame rate: VNIR: 128fps;NIR: 175fps
4-6周 $41362.00
LA-HY01-1710-05
Spectral range: VNIR:400-1000nm;NIR:1000-2500nm; Merge spectral range:400-2500nm; Number of spectral channels: VNIR: 300;NIR: ≥400; Merge the number of spectral channels:≥640; Spectral resolution: VNIR: better than2.8nm;NIR: better than 10nm; Slit width:25μm; Number of spatial channels: VNIR: 1920;NIR: 640; Merge the number of spatial channels:640; Frame rate: VNIR: 128fps;NIR: 100fps
4-6周 $213307.00

LA-HY01-1710-05 - Parameter

LA-HY01-1710-01 - Parameter

LA-HY01-1710-05 - Download

LA-HY01-1710-01 - Download

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Compare Model Drawings & Specs Availability Reference Price
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