If you are considering using pyranometers in your measurement application, there are many things you should know about them and how they work. Having this information in hand will help ensure you select the type of pyranometer most suitable for the data you need for your application.
Note: Because of the focus of this article, I will not be covering how to measure the individual direct solar or diffuse solar radiation, or discussing the different types of radiation in depth.
Our sun outputs radiation over wavelengths from 0.15 to 4.0 µm, which is called the solar spectrum. The measurement of the sun’s radiation on the earth is referred to as global solar radiation. Sometimes called short-wave radiation, global solar radiation is both the direct and diffuse solar radiation received from the hemisphere above the plane of the pyranometer.
It is difficult to find an environmental process on the earth that isn’t driven directly or indirectly by the sun’s energy. Therefore, it is likely that global solar radiation affects the process you are researching.
Global solar radiation measurements are used in several applications for different purposes:
A pyranometer is a sensor that converts the global solar radiation it receives into an electrical signal that can be measured. Pyranometers measure a portion of the solar spectrum. As an example, the CMP21 Pyranometer measures wavelengths from 0.285 to 2.8 µm. A pyranometer does not respond to long-wave radiation. Instead, a pyrgeometer is used to measure long-wave radiation (4 to 100 µm).
Pyranometers must also account for the angle of the solar radiation, which is referred to as the cosine response. For example, 1000 W/m2 received perpendicular to the sensor (that is, 0° from zenith) is measured as 1000 W/m2. However, 1000 W/m2 received at an angle 60° from zenith is measured as 500 W/m2. Pyranometers that have diffusors instead of glass domes require precise diffusors to provide the correct cosine response.
A pyranometer with a diffusor
A pyranometer with a glass dome
There are several different types of solar radiation sensors, including pyranometers, net radiometers, and pyrheliometers.
A net radiometer measures incoming and outgoing short-wave radiation using two thermopile pyranometers, and it measures incoming and outgoing long-wave radiation using two pyrgeometers. These four measurements are frequently part of an energy budget. Energy budget assessments help us understand whether solar energy is being stored in the ground or lost from the ground, reflected, emitted back to space, or used to evaporate water.
A net radiometer
A pyrheliometer consists of a radiation-sensing element enclosed in a casing (collimation tube) that has a small aperture through which only the direct solar rays enter. Radiation bounced off a cloud or particle in the air does not make it through this small opening and collimation tube to the detector. To make measurements all day, a pyrheliometer needs to be pointed directly at the sun using a solar tracker.
The most common types of pyranometers used for measuring global solar radiation are thermopiles and silicon photocells (Tanner, B. “Automated weather stations," 73-98). These pyranometer types are discussed below, along with their advantages and disadvantages.
Tip: You will need to connect the pyranometer to a digital multimeter or datalogger programmed to measure the mV dc voltage.
There are also pyranometers on the market where short-wave radiation (W/m2) is returned in digital format. This will require either a computer or dataloggger to read the serial data string (along with the appropriate interface data cable and communications software).
Thermopile pyranometers use a series of thermoelectric junctions (multiple junctions of two dissimilar metals—thermocouple principle) to provide a signal of several µV/W/m2 proportional to the temperature difference between a black absorbing surface and a reference. The reference may be either a white reflective surface or the internal portion of the sensor base. The thermopile pyranometer’s black surface uniformly absorbs solar radiation across the solar spectrum.
The solar spectrum is the range of wavelengths of the light given off by the sun. Blue, white, yellow, and red stars each have different temperatures and therefore different solar spectrums.
Our yellow sun outputs radiation in wavelengths from 0.15 to 4.0 µm. The thermopile pyranometer accurately captures the sun’s global solar radiation because its special black absorptive surface uniformly responds to most of the solar spectrum’s energy. The sensing element is usually enclosed inside one or two specialty glass domes that uniformly pass the radiation to the sensing element.
The advantages of thermopile pyranometers relate to their broad usage and accuracy. A thermopile pyranometer’s black surface uniformly absorbs solar radiation across the short-wave solar spectrum from 0.285 to 2.800 µm (such as with the CMP6 Pyranometer). The uniform spectral response allows thermopile pyranometers to measure the following: reflected solar radiation, radiation within canopies or greenhouses, and albedo (reflected:incident) when two are deployed as an up-facing/down-facing pair.
Although thermopile pyranometers can be the most accurate type of solar short-wave radiation sensors, they are typically significantly more expensive than silicon photocell pyranometers.
Silicon photocell pyranometers produce a µA output current similar to how a solar panel converts the sun’s energy into electricity. When the current passes through a shunt resistor (for example, 100 ohm), it is converted to a voltage signal with a sensitivity of several µV/W/m2. A plastic diffuser is used to provide a uniform cosine response at varying sun angles.
The spectral response of silicon photocell pyranometers is limited to just a portion of the solar spectrum from 0.4 to 1.1 µm. Although these pyranometers only sample a portion of the short-wave radiation, they are calibrated to provide an output similar to thermopile sensors under clear, sunny skies. Silicon photocell pyranometers are often used in all sky conditions, but measurement errors are higher when clouds are present. The uniformity of the daylight spectrum under most sky conditions limits errors typically to less than ±3%, with maximum errors of ±10%. The error is usually positive under cloudy conditions.
Silicon photocell pyranometers are typically several times less expensive than thermopile pyranometers. For environmental researchers, the accuracy of silicon photocell pyranometers is often sufficient for their requirements.
The disadvantage of silicon photocell pyranometers is that their spectral response is limited to a smaller portion of the solar spectrum from 0.4 to 1.1 µm. These pyranometers perform their best when they are used to measure global solar radiation under the same clear sky conditions used to calibrate them. They should not be used within vegetation canopies or greenhouses, or to measure reflected radiation.
The following graph shows a comparison between the measured output of an inexpensive silicon-cell pyranometer and a secondary-standard blackbody thermopile reference sensor on both sunny and overcast days:
Because the silicon-cell sensor is calibrated under sunny, clear-sky conditions, it closely matches the higher-end sensor in those conditions. However, because the silicon-cell sensor only subsamples solar short-wave radiation (0.4 to 1.1 µm), errors are introduced when the sky conditions change. This particular sensor reported a positive 8% difference from the reference on an overcast day.
The WMO (World Meteorological Organization) has established the World Radiometric Reference (WRR) as a “collective standard.” "The WRR is accepted as representing the physical units of total irradiance within 0.3 per cent (99 percent uncertainty of the measured value).” All pyranometer calibrations trace back to the WRR.
Not all pyranometers are of the same quality. Three pyranometer categories have been established by the WMO (World Meteorological Organization) and the International Organization for Standardization (ISO) for different applications. The following table shows the WMO pyranometer categories (Jarraud, M. “Guide to meteorological instruments and methods of observation," 233). The ISO categories named “secondary standard,” “first class,” and “second class” closely correspond to the WMO categories named “High quality,” “Good quality,” and “Moderate quality.”
There are a few differences in the WMO and ISO specifications. For example, the ISO standard for solar energy (ISO 9060) specifies a spectral range of .35 to 1.5 μm, whereas the WMO standard’s spectral range is 0.30 to 3.0 μm. In addition, the ISO secondary standard specifies 3% spectral sensitivity, whereas the WMO High Quality specifies a 2% spectral sensitivity. In the table image above, the WMO specifies “Resolution” and “Achievable uncertainty,” which are not mentioned in the ISO standard.
I hope this introductory article has helped familiarize you with pyranometers and what they do. I also hope you have a better understanding as to the type of pyranometer that may be most suitable for your application’s needs. If you have any questions or comments about pyranometers, please post them below.
Credits: References used to write this article include the following: