Optical Spectrometer
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This page explains how CCD Detector Array is classified within Computer, Electronic and Optical Product Manufacturing. Technical values and manufacturer relationships are research references; confirm the current specification and supplier evidence for each order.
A photosensitive electronic component that converts light signals into electrical signals for detection and measurement in optical spectrometers.
Technical details and manufacturing context for CCD Detector Array
| Parameter | Typical range | Notes & selection driver |
|---|---|---|
| Pixel Array Size | 2048–3648 pixels | Determines spectral resolution and coverage |
| Pixel Size | 14–24 μm | Affects sensitivity and dynamic range |
| Spectral Response Range | 200–1100 nm | Covers UV to NIR |
| Quantum Efficiency | 40–90 % | Peak QE at 600 nm typical |
| Dark Current | 0.5–10 e-/pixel/s | At 25°C; lower is better for low-light |
| Readout Noise | 10–50 e- rms | Affects signal-to-noise ratio |
| Dynamic Range | 1000–10000 :1 | Ratio of full well to noise |
| Full Well Capacity | 100–500 ke- | Determines maximum signal |
| ADC Resolution | 16–24 bit | Higher bits for finer intensity resolution |
| Maximum Data Rate | 1–10 MHz | Limits frame rate |
| Operating Temperature | -40–85 °C | Storage temperature may differ |
| Cooling Method | TEC or air | TEC reduces dark current |
| Package Type | PGA or CLCC | Affects mounting and thermal management |
| Weight | 5–50 g | Depends on package and cooling |
Ranges are indicative industry figures for RFQ preparation, not a supplier commitment. Confirm every value and standard with the legal manufacturer before ordering.
This component is essential for the following industrial systems and equipment:
| pressure: | Atmospheric (sealed package, not pressure-rated) |
| other spec: | Max illumination: 100 mW/cm², Dark current: <0.1 nA/cm² at 25°C |
| temperature: | -40°C to +85°C |
Indicative industry ranges for design and RFQ preparation. Confirm the exact figures and applicable standard with the manufacturer before specifying.
Quoted from the published standard.
Manufacturer profiles associated with CCD Detector Array.
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A practical evidence checklist for RFQ preparation and supplier evaluation.
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The typical spectral response range is 200–1100 nm, covering ultraviolet to near-infrared. However, the exact range depends on the specific model and coating, so verify with the manufacturer.
Cooling reduces dark current, which is the thermal generation of electrons in the absence of light. Lower dark current improves signal-to-noise ratio, especially for low-light applications. The cooling method can be TEC (thermoelectric cooling) or air cooling, depending on the model.
Pixel array size (e.g., 2048–3648 pixels) determines the spectral resolution and coverage of the spectrometer. A larger array can capture more wavelengths simultaneously, but the exact impact depends on the optical design.
The operating temperature range is typically -40 to 85°C, but storage temperature may differ. For reliable operation, ensure the environment stays within the specified range and consider cooling if needed for low-light measurements.
Editorial classification, named public sources where available, and source-reviewed manufacturer records.
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