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Ultraviolet Camera for Drone| SIMTRUM Photonics Store

Ultraviolet Camera for Drone

SIMTRUM'S Ultraviolet Camera for Drone mainly adopts ultraviolet detection technology, solar-blind ultraviolet filter technologyoptical technology and fusion algorithm technology,can eliminate the disturbance of background, anddetect weak signals generated from the corona under full sunlight by using the signal of the solar-blind ultraviolet spectrum band ( 240-280nm) .Through the fusion between UV and the visible spectrum, it can realize UV/visible double spectrum imaging ,and conduct accurate location for the corona vividly.

This product is applicable to the patrol inspection of overhead transmission lines, and can dock with UAV. At the same time, it provides customers with a free secondary development package, which is very convenient for integrated development. It can be customized according to different requirementsand has the advantages of high sensitivity, strong anti-interference ability, low power consumption and strong scalability.

 

Features

  • High sensitivity
  • Solar-blind wavelength range of 240-280nm
  • Adjustable gain
  • Compact structure
  • Efficient digital processing
  • High overlay accuracy
  • Function customization

Applications

  • Corona detection
  • Forest fire prevention
  • Navigation of channel and port

 

 

 

 
 
 
Product Specifications
UV - Optical Properties
Spectrum Band of Detecting 240nm~280nm
Minimum UV Sensitivity 5pc/10m
Focus Distance 3m~ꝏ
Visible - Optical Properties
Focus Distance 3m~ꝏ
Minimun Visible Light 0.5lux
Focus Auto - focusing
UV/Visible Overlay Accuracy ≤1mrad

 

Other Specifications

In - Out
Image Resolution 1280H×720V
Field of view 12.4°×7°
Function UV, Visible and Fusion
Physical Characteristics
Measurement (length×width×height) 180mm×104mm×60mm
Weight <930g
Connectors POWER、RJ45、RS232、HDMI
Power Consumption DC 12V <8.5W
Power Dissipation <8.5W
Operating Temperature -20℃~+55℃
Development Environment
Network Data Protocol ONVIF, RTSP

SIMTRUM'S Lightweight UV Camera for Drone (Support 2nd Development) adopts ultraviolet detection technology, solar-blind ultraviolet filter technology, and fusion algorithm technology. By utlizing the day blind ultraviolet band (240-280nm) signal, it can elimi-nate background interference in full sunlight and detect weak signals generated by corona. Through the fusion of ultraviolet and visible spectra, dual spectral imaging of ultravioletivisible light can be achievedand the position of corona can be accurately and intuitively located. This product is suitable for inspectionof overhead transmission lines and can dock with DJl drones, making it very convenient for integrated development. lt can be customized according to different needs, with advantages such as high sensitivity, small size, low power consumption, and light weight.

Features

  • High sensitivity
  • Solar-blind wavelength range of 240-280nm
  • Adjustable Gain
  • Compact structure
  • Efficient digital processing
  • Function customization
  • Adapt to X-port

Applications

  • Corona detection
  • Forest fre prevention
  • Navigation of channel and port

 

 

 

 

 
Product Specifications
 
UV Channel Characteristics
Spectral Detection Range 240nm~280nm
Minimum Discharge Sensitivity 5pC@10m
Focus Distance 3m~ꝏ
UV Channel Resolution 1280×1024
Visible Light Channel Characteristics
Focus Distance 3m~ꝏ
Minimum Visible Light Illumination 0.5lux
FOCUS Autofocus
Stacking Accuracy ≤1mrad
Visible Light Amplification Factor 10x optical × 12 times digital

 

 

Other Specifications

Function
Storage TF@64G
Photon Counting Single region / Sub region
Function UV mode, Visible mode, Fusion mode
Physical Property
Size (length×wide×High) 99.7mm×85.3mm×54mm
Weight <450g
Interface Docking with DJI X - port
Ppower Supply DC 12V
Consumption <7.2W
Operation Temperature -20℃~+55℃
Network Protocol
Network Data Protocol Supports ONVIF and RTSP protocols
Development Platform Provide Windows/Linux secondary development package

 


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-UAV-01
UV - Optical Properties Spectrum Band of Detecting:240nm~280nm;Minimum UV Sensitivity:5pc/10m;Focus Distance:3m~∞; Visible - Optical Properties Minimun Visible Light:0.5lux;UV/Visible Overlay Accuracy:≤1mrad;Image Resolution:1280×720
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UV Channel Characteristics Spectral Detection Range:240nm~280nm; Minimum Discharge Sensitivity:5pC@10m; Focus Distance:3m~∞; UV Channel Resolution:1280×1024; Visible Light Channel Characteristics Minimum Visible Light Illumination:0.5lux; Stacking Accuracy:≤1mrad; Visible Light Amplification Factor:10x optical × 12 times digital
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