SYA-27 (AK2800) Testing System for Visible Light Transmittance and Solar Heat Gain Coefficient of Architectural Glass
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Description
Product Introduction
The architectural glass visible‑light transmittance and solar heat gain coefficient testing system (JP‑AK3600) employs advanced optical and electronic technologies, complies with numerous international and national standards, and features ultra‑low stray light and high‑precision temperature control. Its stable, reliable performance, precise measurement capabilities, and user‑friendly operation give it broad application prospects in the field of architectural glass testing. The system supports multiple data‑format outputs and incorporates robust quality‑control functions, enabling it to meet the diverse needs of various users.
Reference standard:
ISO 9050 “Glass in building — Determination of visible light transmittance, direct solar transmittance, total solar transmittance, ultraviolet transmittance, and related window glass parameters”;
ISO 9050 “Glass in building — Determination of light transmittance, direct solar transmittance, total solar transmittance, ultraviolet transmittance, and related gloss coefficients”;
JGJ/T 151, “Technical Code for Thermal Calculation of Building Doors, Windows, and Curtain Walls.”
Key features:
1. Robust instrument performance: An exceptionally high‑quality optical system, an advanced electronics platform, and a state‑of‑the‑art mechanical design ensure ultra‑low stray light of 0.010%T, high‑precision PID temperature control, and 24‑bit voltage digital sampling.
2. Stable and reliable quality: The dual-beam dynamic feedback proportional‑recording photometric system ensures baseline stability, while key components such as the deuterium lamp and photomultiplier tube are all imported, guaranteeing the instrument’s stability, reliability, and long service life.
3. Precise Measurement: Utilizing a high-quality imported holographic grating, stray light in the instrument is further reduced, ensuring more accurate analytical results.
4. Easy and Efficient Human–Machine Interaction: The JP‑AFL25 series of intelligent architectural glass, designed for the Windows environment, features Chinese-language software that allows users to set parameters such as visible light transmittance, solar shading coefficient, and hemispherical emissivity. It offers a wide range of instrument control and operational functions, is simple to use, highly flexible, and efficiently meets users’ analytical needs.
5. Excellent scalability: The reflective optical integrating sphere can be equipped with optional specialized accessories, including a dedicated reflectance device for measuring the solar shading coefficient of architectural glass, significantly broadening the instrument’s range of applications.
6. Simple and convenient equipment maintenance: The unique plug-in tungsten and deuterium lamps eliminate the need for optical alignment during lamp replacement, making instrument setup and maintenance even more…
Simple and convenient: a vacuum pressure tester is used to inspect hydraulic fluids.
7. Logging Function: Automatically records user actions; log files are stored in a more reliable database format; administrators can manage the logs.
Perform categorized browsing and other processing.
8. It employs an integrated optical and hemispherical-emission testing system, offering high cost-effectiveness and ease of use.
9. Quality Control Function: Measurement data can be monitored according to user-defined settings; the system will display a warning message for data that falls outside the control limits.
Pause, apply color coding, or automatically remeasure.
10. Report Output Function: Enables data sharing with other systems; allows saving measurement results in Microsoft Word, Microsoft Excel, and text file formats; supports customizable report formatting; and provides a preview of the printed report before output.
Technical Specifications:
| Photometric Project | Indicator |
| Detection method | Optical measurement method |
| Optical wavelength range | 190–2800 nm |
| Wavelength accuracy | ±0.3 nm (automatic calibration upon startup) |
| Wavelength repeatability | ≤0.1 nm |
| Automatic spectral bandwidth | 1, 2, 5, 10, 50 nm |
| Stray light | < 0.01% (220 nm, Nal; 340 nm, NaNO2) |
| Light Source Conversion | Automatic switching (can be set arbitrarily within the 380 nm to 1000 nm and up to 2800 nm wavelength ranges) |
| Optical Test Accessories | Mirror Test Apparatus |
| Luminosity range | -4.0 to 4.0 A |
| Photometric accuracy | ±0.002 A (0–0.5 A) |
| ±0.004 A (0.5–1 A) | |
| Photometric repeatability | ±0.3%T (0–100%T) |
| 0.001 A (0–0.5 A) | |
| 0.002A (0.5–1A) | |
| Photometric baseline flatness | ±0.001 A (190–1000 nm) |
| ±0.005 A (1000–2800 nm) | |
| Photometric baseline drift | 0.0004 A/h (500 nm, 0 A, after warm-up) |
| Noise | ±0.0004A |
| Test metrics | Ultraviolet transmittance and reflectance; |
| Visible light transmittance and reflectance; | |
| Direct transmittance and direct reflectance of solar radiation; | |
| Direct solar absorptance and total solar transmittance; | |
| Solar heat gain coefficient, shading coefficient; | |
| Solar irradiance ratio, total solar infrared thermal energy irradiance ratio; |
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