The SI-111, manufactured by Apogee, is a precision infrared radiometer that determines the surface temperature of an object without physical contact. It measures both the subject's surface temperature and the sensor-body temperature. A Campbell Scientific datalogger uses these measurements to calculate the correct temperature of the subject.Read More
The SI-111 consists of a thermopile, which measures surface temperature, and a thermistor, which measures sensor body temperature. The two temperature sensors are housed in a rugged aluminum body that contains a germanium window.
Both the thermopile and the thermistor output a millivolt signal that most of our dataloggers can measure. The datalogger uses the Stefan-Boltzman equation to correct for the effect of sensor body temperature on the target temperature. The corrected readings yield an absolute accuracy of ±0.2°C from -10° to 65°C.
Field of View (FOV)
The SI-111 has a 22 degree half angle field of view (FOV). The FOV is reported as the half-angle of the apex of the cone formed by the target (cone base) and the detector (cone apex). The target is a circle from which 98% of the radiation viewed by the detector is being emitted; see image.
Note: Prior to November 2008, the SI-111 was named the IRR-P.
|Input Power||2.5 V excitation (for thermistor)|
|Response Time||< 1 s (to changes in target temperature)|
|Target Temperature Output Signal||60 μV per °C difference from sensor body|
|Body Temperature Output Signal||0 to 2500 mV|
|Wavelength Range||8 to 14 μm (corresponds to atmospheric window)|
|Field of View (FOV)||22° half angle|
|Operating Temperature Range||-55° to +80°C|
|Operating Relative Humidity Range||0 to 100% RH|
|Cable Description||4.5 m (14.76 ft) twisted, shielded 4-conductor wire with Santoprene casing, ending in pigtails|
|Diameter||2.3 cm (0.9 in.)|
|Length||6 cm (2.4 in.)|
|Weight||190 g (6.7 oz)|
The SI-111 is often mounted to a CM202, CM204, or CM206 crossarm, a tripod or tower mast, or a user-supplied pole via a CM220 Right Angle Mount or CM230 Adjustable Inclination Mount. The SI-111 should be mounted perpendicular to the target surface. Therefore, the CM230 mount is recommended when the target surface is on an incline. The SI-111 may also be mounted directly to a user-supplied camera tripod.
|CR200(X) Series||CR800/CR850||CR1000||CR3000||CR9000X||CR6 Series||CR300 Series|
Number of FAQs related to SI-111: 8
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The window in the Apogee infrared sensor is inset and protected, but it can become partially blocked in three ways:
Clean the inner threads and sensor window using a cotton swab dipped in the appropriate solvent. For additional cleaning information, see the Maintenance section of the instruction manual.
As a general recommendation, recalibration should be done every two years.
There are two accuracy specifications listed for the SI-111:
Using a radiation shield with the sensor helps keep the sensor body temperature in close approximation to the ambient air temperature. Ultimately, the need to protect the sensor from short-wave radiation is dependent on what is being measured and under what conditions. For example, Campbell Scientific recommends using a radiation shield for canopy measurements.
The SI-111 has been successfully calibrated with a maximum cable length of 100 m without a loss in accuracy. Ideally, the sensor is calibrated with the overall cable length already configured. Our tests have shown, however, that adding a few meters of cable in the field has a negligible effect on the calibration, provided the measurement device has significantly high input impedance, such as with the CR1000.
The SI-111 can be used to measure a wide variety of surfaces, including water and snow. When measuring objects with low emissivity, however, it is particularly important to apply corrections to the measurement.
The information included on a calibration sheet differs with each sensor. For some sensors, the sheet contains coefficients necessary to program a datalogger. For other sensors, the calibration sheet is a pass/fail report.
Because of the loss of IR radiation, nearly all thermopile instruments typically have a negative offset. This offset is most easily visible at night-time, when a small negative value is read instead of zero. This same offset is present during the daytime, but it is not as visible because of the large solar signal.
Another common issue involves leveling an instrument. Leveling a thermopile instrument can cause errors in the direct beam component because the cosine response is not correct. These errors are more notable when the sun is close to the horizon because the angle is so shallow.
This depends on the information contained in the calibration sheet: