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UV-VIS-IR Triple Spectral Fusion Camera | SIMTRUM Photonics Store

UV-VIS-IR Triple Spectral Fusion Camera
SIMTRUM'S UV-VIS-IR Triple Spectral Fusion Camera adopts solar-blind UV module, visible detect module and infrared temperature measurement module at the same time, which can not only detect the weak UV light emited by voltage-related electrical defects, but also detect the infrared ray emitted by current-related electrical defects. The product has the characteristics of high integration, strong performance stability and many fault determination methods.

Our UV-VIS-IR Triple Spectral Fusion Camera, with a friendly man-machine operating interface and smaller size, can conduct location for the corona, indicate the problem position, measuring the temperature at the fault point ,and assess the condition and seriousness of the problem; additionally, it also can assist inspectors all day in checking the transmission line andequipment of electrical power, factories, railways.

Features

  • High sensitivity
  • Solar-blind wavelength range of 240-280nm
  • Triple spectral fusion
  • Efficient digital processing
  • Function customization

Applications

  • Corona detection
  • Temperature measurement
  • Forest fire prevention
  • Navigation of channel and port
Triple light fusion
UV and VIS Fusion

Product Specifications
UV - Optical Properties
Spectrum Band of Detecting 240nm~280nm
Minimum UV Sensitivity 5pc/10m
Focus Distance 3m~∞
IR - Optical Properties
Resolution 640×480
Measuring Range -20°C~400°C
Temperature Measurement Accuracy ±2°C
Visible - Optical Properties
Focus Distance 3m~∞
Minimum Visible Light 0.1lux
Focus Auto - focusing
UV/Visible Overlay Accuracy ≤1mrad
 
 

Other Specifications

Function
Display mode, Photon Counting UV image, IR image, Visible image, Fusion image
Storage One area/Four areas
Video Record/Replay TF@32G
Photograph/Playback Format mp4
Display
Type LCD
Spotlight 450cd/m²
Resolution 640×480
Size 5inch
Physical Characteristics and Power System
Operating Temperature -20℃~+55℃
Power Consumption DC 14.8V 18.7W
Working Hours >2h
Measurement(length×width×height) 229mm×207mm×103mm
Weight 2.6kg
 

Sales Guide

Items Detail Unit Remark
What are the application scenarios?      
Fine detection of power equipment     Recommended long focal length (> 50mm) narrow field of view Angle
Substation global inspection     Recommended medium focal length (25-50mm)
Security fire source check     Recommended short focus (< 25mm)
Scientific chemical reaction     Ultra-long focal length
Do you need an optional laser ranging function?      
Do you need online monitoring?      
Do you need to image visible light?      
Do you need to extend the detection channel tovisible and near-infrared wavelengths?      
Do you need an airborne UV camera?      

 

Q&A

Q: How does the solar-blind UV camera work?

A: The working principle of solar blind UV cameras is based on their sensitivity to specific UV bands and their ability to suppress environmental interference.

  • The ultraviolet (UV) in solar radiation is divided into UVC (200-280nm), UVB (280-315nm), and UVA (315-400nm). UVC is almost completely absorbed by the ozone layer, resulting in extremely weak UVC radiation naturally occurring on the surface, forming a "sunblind zone." Solar-blind cameras only detect the UVC band of 200-280nm, reducing the interference of visible light.

 

  •  Imaging principle: The UVC light emitted by the target is focused into the camera through the lens, and the interfered light in the solar-blind band is filtered through the filter light, the detector converts the UVC photon into an electronic signal (analog signal), the ADC converts the analog signal into a digital signal, and the image is generated after noise reduction and contrast reduction by the algorithm.

 

 

Q: What are the core components of a solar-blind camera?

A: The core components of the solar-blind UV camera include: UV sensitive detector, efficient filter system, signal processing unit. Using UVC-sensitive semiconductor materials whose band gap width exactly matches the photon energy of the UVC, photons can be converted into electrical signals. The built-in narrow-band filter allows only 200-280nm UVC to pass through, completely blocking visible, UVA/UVB and infrared light. Low noise amplifiers are used to enhance weak signals.

 

 

Q: Advantages of solar-blind UV cameras?

A:

• High signal to noise ratio. It can significantly improve the ability of target signal recognition.

• Ability to work day and night. It can suppress sunlight interference during the day, and no additional light source is required at night.

• Non-contact detection. Suitable for remote detection in high-risk environment.

 

 

Q: What is the difference between UV solar-blind camera and ordinary camera?

A: Solar-blind cameras rely primarily on UVC source radiation and do not require ambient light to work. The image contrast is high, but the penetration of UVC is weak, resulting in less detail in the image.

Normal cameras rely on reflecting visible light for imaging and require ambient light. Rich in color and clear in detail, but easily limited by strong or low light conditions.


Products Description
Scientific CMOS Camera spectral range:200-1100 nm;QE:up to 95%;Frame rate:up to 100.
Scientific CCD Camera spectral range:VUV EUV X-ray(5 eV-20 KeV),UV-NIR(160-1100 nm),in-vacuum camera
Microscope Camera CCD camrea:380-650 nm;CMOS camera:200-1100 nm;USB 3.0 interface;Black and white, pseudo color.
Industrial Machine Vision Camera Line Scan/Area Array Camera;single line scan/multi-line scan;resolution:up to 16K;Frame Grabber
Solar Build UV Camera Solar blindness in the 240-280nm band;can be fused with UV and IR bands;airborne UV solar blind camera
Infrared Pyrometer /Camera Infrared Pyrometers(-40~3000℃);Infrared Linear Array Camera(0.8~14um);Infrared Matrix Array Camera(-30~3000℃)
SW/MW/LW Infrared Camera SWIR:400-1700 nm;MWIR:3.7-4.8 um/7.7-9.4 μm;LWIR:7.7-9.4μm/8-14μm;

 

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IM-BY01-UV-TS01
UV - Optical Properties Spectrum Band of Detecting:240nm~280nm;Minimum UV Sensitivity:5pc/10m;Focus Distance:3m~∞;IR - Optical Properties Resolution:640×480;Measuring Range:-20°C~400°C;Visible - Optical Properties Minimum Visible Light:0.1lux;UV/Visible Overlay Accuracy:≤1mrad
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