Photodiode Light Sensor -- Light Sensors
Category: SOLAR
Model: Solar Energy
Avaibility: AVAILABLE
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Photodiode Light Sensor -- Light Sensors
Category: SOLAR
Model: Solar Energy
Avaibility: AVAILABLE
Call For Price
Three types of sealed photodiode sensors are now available:
• A photosynthetically active radiation PAR sensor (the QS2)
• A solar energy flux sensor (the ES2)
• A range of three UV sensors (the UV3pA, UV3pB, & UV3pAB)
These sensors replace the previous Delta-T models offered.
• mV outputs pre-set to identical standard values for each sensor type
• Self-cleaning, stay-dry diffuser with water drainage slots
• Good cosine response with infinity error correction ring
• Quality photodiodes – high stability with low temperature coefficient
• Hard-anodised aluminium body
• Lower purchase and recalibration cost
The UV sensors are fitted with a transimpedance amplifier operating from a single rail power supply. All sensors can be provided with an optional aluminium mounting plate (type SRLF1) which includes a bubble level, and levelling adjusters.Alternatively a levelling plate is available for standard Delta-T weather station masts (takes 2 ES2 or QS2 or 1 E/QS2 and 1 UV3p)
|
Type |
ES2 |
QS2 |
UV3pA |
UV3pB |
UV3pAB |
|
Spectral region |
Solar Energy |
PAR |
UV “A” |
UV “B” |
UV “AB” |
|
Spectral response |
400–1050 nm |
400–700 nm |
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|
Peak wavelength |
|
373 ±2nm |
313 ±2nm |
360 ±5nm |
|
|
Bandwidth |
|
31 ±2nm |
26 ±2nm |
72 ±5nm |
|
|
Relative spectral response |
Standard graph for all sensors |
Individual spectral response for each sensor |
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Ouput sensitivity |
10 mV per kW m-2 of total solar radiation |
10 mV per mmol m-2 s-1 |
1 mV per W m-2 |
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Accuracy (error) at 20°C traceable to NPL & BSI stds |
±3%* |
±5% |
±7.5% |
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Measuring range |
0-2 kW.m-2 |
0-3 mmol m-2 s |
0-150 W m-2 |
0-150 W m-2 |
0-200 W m-2 |
|
Cosine corrected |
within ±5% up to 70o incidence |
within ±5% up to 70o incidence |
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Voltage supply |
n/a |
7-15 V dc (<12mA> |
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Size (mm) |
48 high x 30 dia |
48 high x 50 dia (base) |
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* Calibrated under a spectro-radiometrically controlled Lambertian Source. |
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