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This product is no longer available and has been replaced by: SP230SS. Some accessories, replacement parts, or services may still be available.
SP230 Heated Pyranometer
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Overview

The SP230 and SP230SS pyranometers, manufactured by Apogee measure total sun and sky solar radiation. They include a 0.18 W internal heater and an elevated base that allow it to provide solar radiation measurements during the most severe weather. Its small heater draws just 15 mA of current, allowing it to be powered by a small solar panel and battery─even on days with a short duration of daylight and at high latitudes (far away from the equator).

Note: In the image, the SP230 is shown mounted to a #18356 Levelling Base and a CM225 Solar Sensor Mounting Stand.

Note: The SP230SS replaced the SP230 in August 2018. It has a stainless-steel connection, a removable cable, different wire colours, and a serial number of 9898 or above.

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Benefits and Features

  • Designed to prevent snow, frost, and dew accumulation
  • Heater uses 1/80th of the power that other heated pyranometers use, making it ideal for remote battery-powered applications
  • Measurement waveband of 360 to 1120 nm
  • Compatible with most Campbell Scientific data loggers
  • Dome-shaped head prevents water from accumulating on the sensor head

Technical Description

The SP230-L uses a silicon photovoltaic detector mounted in a cosine-corrected head to provide solar radiation measurements. It is calibrated against a Kipp & Zonen CM21 thermopile pyranometer to accurately measure sun plus sky radiation for the spectral range of 360 to 1120 nm. The SP230-L outputs a millivolt signal that Campbell Scientific data loggers can measure.

Note: Sensors calibrated to the 360 to 1120 nm spectral range should not be used under vegetation or artificial lights.

Images

The SP230-L mounted to a 18356 Leveling Base and a CM225 Solar Sensor Mounting Stand (sold separately)
The SP230-L mounted to a 18356 Leveling Base and a CM225 Solar Sensor Mounting Stand (sold separately)
The SP230-L mounted to a 18356 Leveling Base and a CM225 Solar Sensor Mounting Stand (sold separately)

Specifications

Light Spectrum Waveband 360 to 1120 nm (wavelengths where response is 10% of maximum)
Measurement Range 0 to 1750 W/m2 (full sunlight ≈1000 W/m2)
Heater 780 Ω, 15.4 mA current drain, 185 mW power at 12 Vdc
Absolute Accuracy ±5% for daily total radiation
Sensitivity (0.2 mV/W/m2)
Calibration Factor 5 W/m2/mV
Cosine Response ±5% at 75° zenith angle; ±1% at 45° zenith angle
Temperature Response -0.04 ±0.04% per °C
Long-Term Stability < 2% per year
Operating Temperature Range -40° to +70°C
Relative Humidity Range 0 to 100%
Diameter 3.15 cm (1.24 in.)
Height 12.75 cm (5.02 in.)
Weight 142.0 g (5.01 oz) with 2 m (6.56 ft) cable

Compatibility

Mounting

Accurate measurements require the sensor to be levelled using a #18356 levelling fixture. This levelling fixture incorporates a bubble level and three adjusting screws. The #18356 mounts to a crossarm using the CM225 mounting stand. The SP230 should be mounted away from all obstructions and reflective surfaces that might adversely affect the measurement.

Resources and Links


FAQs for

Number of FAQs related to SP230: 1

  1. 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.

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