Introduction
Diffraction Grating Spectrophotometer features the sphere size of Φ 48mm, enhancing light capture and accurate reflectance. It offers multiple detector options, ensuring for the selection of the ideal detector based on sample types. The instrument supports various color spaces for accurate color measurements across different materials. Our diffraction grating spectrophotometer has polygon colorimetric tolerance for adjusting temperature variations.
This analytical equipment is designed to meet the rigorous requirements of modern laboratory operations, ensuring high precision, reliability, and ease of use for various experimental applications.Applications
Diffraction Grating Spectrophotometer is an analytical instrument that uses a grating to split light into wavelengths for accurate analysis. It is widely used in the pharma and laboratories, ensuring precise color in tablets and packaging for quality control.
Specifications
| Optical Geometry | 45/0(45°Ring Shaped Illumination, Vertical Viewing) |
| Sphere Size | Φ48 mm |
| Sensor | 256 Image Element Double Arrays Image Sensor |
| Wavelength Range | 400 to 700 nm |
| Wavelength Pitch | 10nm |
| Half Bandwidth | 10nm |
| Reflectance Range | 0 to 200% |
| Measurement Aperature | Φ 20 mm |
| Color Spaces | , , Yxy, LCh, , Hunter , Bxy |
| Color Difference Formula | ΔE × ab ΔE × uv, ΔE × 94, ΔE × cmc (2:1), ΔE ×cmc (1:1), ΔE × 00, ΔE (Hunter) |
| Other Indices | WI ( E313, / , , Hunter) YI ( D1925, 313) MI (Metamerism Index) |
| Observer Angle | 2°/ 10° |
| Illuminants | D 65, A, C, D50, D55, D75, F1, F2 (), F3, F4, F5, F6, F7 (), F8, F9, F10 (), F11(TL84) F12 (TL83/ U30) |
| Measurement Time | 1.5 second |
| Repeatability | Spectral Reflectance: / Standard Deviation: 0.1% (400 to 700 nm) Chromaticity Value: Standard Deviation ΔE × ab 0.04 |
| Inter – Instrument Agreement | ΔE × ab 0.2 |
| Data Storage | Standard: 1000 Sample: 30000 |
| Measurement Mode | 2 to 99 times |
| Battery Performance | 5000 Measurement within 8 hrs |
| Working Environment | Temperature: 0 to 40°C Humidity: 0 to 85% (No Condensation) Altitude: Less than 2000 m |
| Storage Environment | Temperature: 20 to 50°C Humidity: 0 to 85% (No Condensation) |
| Power Consumption | DC 24V, 3A |
| Dimensions (L× W× H) | 184 × 77 × 105 mm |
| Weight | 600g |
Features
PC Software Integration
Reflective Film Evaluation
Standard White Calibration
Multiple Colorimetric Indices
Minimizing Stray Light
FAQs
1. What is the impact of polarization on Diffraction Grating Spectrophotometer?
It supplies premium Diffraction Grating Spectrophotometer. gratings are designed for specific polarization states, and if the light is not polarized correctly, the grating’s diffraction efficiency can drop, leading to weaker signals. The grating may diffract polarized light more efficiently in one direction compared to another. Polarization effects are more significant when using high-resolution gratings, as small changes in polarization can lead to noticeable shifts in spectral peaks. Polarizers or polarization-maintaining optical components can control the light's polarization state, ensuring more accurate measurements. Proper calibration for polarization ensures consistency across different setups and measurements.
2. What is the role of thermal effects in the performance of a Diffraction Grating Spectrophotometer?
Diffraction Grating Spectrophotometer have advanced features. Temperature has a critical role in performance. As temperature increases, materials within the optical system—such as the grating or mirrors—expand or contract, leading to shifts in the diffraction angles. Thermal effects also influence the detector’s sensitivity, causing fluctuations in the recorded signal. Advanced systems often include thermal compensation mechanisms, such as temperature-controlled stages or cooling systems, to mitigate these effects. Without proper thermal control, spectral data may drift, reducing the reliability of measurements over time. Regular calibration checks are essential to ensure that thermal influences do not compromise the accuracy of spectral readings.
3. What are the challenges associated with using Diffraction Grating Spectrophotometer for high-energy or intense light sources?
It manufactures advanced Diffraction Grating Spectrophotometers. Excessive light intensity may lead to nonlinear diffraction responses, resulting in distorted spectral data. This is especially problematic when working with narrow spectral lines, as intense light can induce higher-order diffraction or scattering effects, complicating analysis. Specialized gratings with high power tolerance are designed to handle intense light without damage. Filters or attenuators are often used to reduce the light intensity entering the system, protecting the grating from damage. Long-term exposure to high-energy sources can also degrade grating performance, requiring regular maintenance and recalibration. Ensuring proper management of light intensity is crucial to preserve grating efficiency and maintain accurate spectral measurements.
4. How does the signal-to-noise ratio () vary with wavelength in Diffraction Grating Spectrophotometer?
Diffraction Grating Spectrophotometer supports advanced features. Additionally, detectors often have reduced sensitivity at extreme ends of the UV and IR spectrum, further lowering the . In the visible range, where the detector is most sensitive, the is typically better. Grating efficiency plays a key role in ensuring a strong signal, but at higher diffraction orders, the signal tends to weaken, leading to a reduced . External factors like thermal noise, electrical interference, and stray light can also degrade . Signal processing techniques, such as signal averaging or digital filtering, can improve the . Calibration of the spectrophotometer for stray light and noise sources is essential for obtaining reliable and reproducible data.
5. What are the effects of aberrations in a Diffraction Grating Spectrophotometer?
It supplies different models of Diffraction Grating Spectrophotometers. Optical aberrations such as spherical, chromatic, and coma distort light paths, leading to blurred spectral peaks and reduced resolution. These distortions affect the diffraction efficiency and the clarity of the final spectrum, especially at higher diffraction orders where precision is critical. High-quality optical components such as aspheric lenses and minimizing geometrical imperfections can reduce the impact of aberrations. Proper alignment techniques are vital to ensure accurate spectral measurements, especially in high-resolution setups. Regular checks and calibration can correct for minor aberrations that accumulate over time. For certain applications, advanced correction algorithms in the system software can also compensate for these optical imperfections.
6. Can a Diffraction Grating Spectrophotometer be used for both transmission and reflection measurements?
Yes, Diffraction Grating Spectrophotometers can be used for both transmission and reflection measurements. In transmission mode, light passes through the sample and grating, with the diffracted light being analyzed. In reflection mode, the light is reflected off the grating surface, and the diffracted light is measured. The grating's design and angle of incidence determine how the light interacts, making it versatile for different setups. Different optical components, like beamsplitters, may be used depending on the measurement type. Calibration ensures that both modes provide accurate spectral data. Spectrophotometers are often designed to switch between modes for various applications.
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