Long Range Monitoring IR Cooled Camera Module Core 1280x1024 12μm
Product Overview
GAVIN GC1212MA high resolution thermal camera module integrates large array 1280x1024/12μm cooled MWIR detector. Various image processing algorithms are embedded to output clear infrared images in total darkness or bad weather conditions. It can detect and recognize risks and threats at long distance while presenting more target details at short distance.
With large array 1280x1024 resolution, it can realize wider field of view and provide more image details. The reduced 12µm pixel size offers better spatial resolution and matches shorter optical lens focus to achieve the same range mission. Ideal for systems integrators designing custom applications.
Main Features
- Megapixel Resolution, Exceptional Image Quality
- Powered by 1280×1024/12μm mid-wave cooled infrared detector for sharp, detailed thermal imaging
- Integrates advanced image processing algorithms including DRC, 2D/3D noise reduction, and edge enhancement (EE) for superior clarity
- High Reliability, Superior Sensitivity
- Mid-wave cooled thermal imaging technology ensures excellent adaptability and consistency
- Outstanding thermal sensitivity with NETD as low as 18mK
- Easy Integration, Flexible Configuration
- Supports CameraLink interface with RAW/YUV image data output
- Multiple continuous zoom optical configurations available for different needs
Product Specifications
| Model |
GAVIN GC1212MA |
| Resolution |
1280×1024 |
| Pixel Size |
12μm |
| Cryocooler |
RS058 |
| Spectral Response |
3.7μm±0.2μm～4.8μm±0.2μm |
| IR Detector NETD(23℃) |
18mK(F2/F4) |
| Frame Rate |
50Hz |
| Dimming Mode |
Linear/Histogram/Mixed |
| Digital Zoom |
1× to 8× continuous digital zoom |
| Image Direction |
Horizontally/Vertically/Diagonally Flip |
| Image Algorithm |
DRC, 2D/3D Image Noise Reduction, EE |
| Standard External Interface |
J30JZ 25-pin HDMI Dedicated Output Interface |
| Analog Video |
PAL/NTSC |
| Digital Video |
Standard: DVP
Option: Cameralink/USB3.0/GigE/SDI/HDMI/MIPI/Single-mode Optical Fiber/Multi-mode Optical Fiber |
| External Sync |
Standard: LV-TTL
Option: RS422/LVDS |
| Communication |
Standard: USB2.0/LV-TTL
Option: RS422/CAN/USB3.0/GigE |
| Power Supply |
24V±4V |
| Steady Power Consumption(23℃) |
≤11W |
| Cooling Time(23℃) |
≤8min |
| Size(mm) |
149×58.5×80 |
| Weight(g) |
≤680 |
| Operating Temperature |
-40℃~+71℃ |
| Vibration |
Vibration: High-speed transport intensity; Impact: Half Sine Wave, 40g/11ms, 3 Axis, 6 Direction, 3 Times/Direction |
| Lens Options |
Fixed focus: 19mm/F2
Continuous zoom: 60~360mm/F4, 37.5~750mm/F4, 100~1000mm/F4 |
Industrial Applications
The GAVIN GC1212MA thermal infrared camera module is widely used in many areas such as NDT, Environmental Monitoring, Long-Range Surveillance, Scientific Research, and more.
IR Detection Solutions
- High sensitivity and excellent performance
- World-leading technology in infrared industry
- Various infrared detectors available - both uncooled and cooled IR detectors in different formats and pixel sizes
- Volume production to ensure fast delivery - three production lines with annual production capability up to millions of detectors
Frequently Asked Questions
Advantages of Optical Gas Imaging
- Time-saving & Efficient: Support large-scale real-time detection, rapid leak location, no need for interrupting production
- Long Range Detection: Away from dangerous and complex areas, non-contact non-destructive testing, without additional radiation source
- Easy to Analyze: Intuitive imaging, instant storage, convenient analysis
- Multi-function Inspection: Variety of gases can be detected, with excellent remote temperature measurement function
Working Principle of Optical Gas Imaging
Optical gas imaging is a type of infrared technology that enables visualization of invisible industrial gases. After absorbing infrared radiation at specific wavelengths, infrared radiation differences occur between the gas and the background. The gas leak detection infrared detector with built-in narrowband filter only receives the infrared band near the gas infrared absorption peak, and can convert the gas into visible infrared images through the radiation difference between the gas and the background.
