Pyranometers
by Chris Woodford. Last updated: August 16, 2011.
They say the Sun shines on the righteous—and if you want to know precisely how righteous you are, you'd better invest in a pyranometer! Widely used by weather and climate scientists, these strange looking instruments measure the amount of sunlight hitting Earth's surface at a particular place and time. How do they work? Let's take a closer look!
Photo: Sunrise seen through the glass dome of a pyranometer. Photo by Steve Wilcox courtesy of US Department of Energy/National Renewable Energy Laboratory (US DOE/NREL).What does a pyranometer do?
Unless you're lucky enough to live in a tropical paradise, you probably see quite a bit less of the Sun than you might like. Earth orbits the Sun and, at the same time, spins around on a tilted axis, so we get variations in sunlight across our planet each hour of the day and each day of the year. That's essentially what gives us our seasons and climate.
Now suppose you had the job of comparing how much sunlight different places receive. How would you go about it? You could lounge about in the Sun all day in different places and see how brown you get, but unless you wear copious amounts of sunscreen, that'll be very dangerous—and it's not exactly scientific! What about rigging up a small solar panel to an electricity meter? You could carry the panel round the world with you, measure how much electricity it generates in each place, and use that to compare the amount of sunlight.
Photo: Sunlight varies all the time, from its theoretical minimum at sunrise (as here) and sunset to its theoretical maximum at midday. But how can you measure it more precisely?.
Very roughly speaking, this is what pyranometers do—although they work in a much more precise and scientific way. What they measure is the solar radiation falling on a horizontal surface in watts (the amount of energy received each second) per square meter. Technically that's known as insolation.
What is a pyranometer?
If you're good with your Greek, you'll know that pyr means fire, ano indicates something up above, and meter suggests measurement, so a pyr-ano-meter measures "fire from up above"—sunlight, in other words. A typical, laboratory-grade pyranometer is essentially just a thermopile (a collection of thermocouples, perhaps 50-100 in the best instruments) mounted on a black carbon disc, which generates electricity according to how hot it gets (how much solar radiation falls on it).
That's not quite all there is to it, however! Scientists are serious people who like to be sure that when they measure something, other things aren't getting in the way and spoiling their data. So pyranometers have some extra features. Most noticeably, there's a dome made from one or two layers of ground and polished optical glass or acrylic plastic covering the thermopile, which eliminates air movements and dirt that might affect the measurements (the curved outer surface also ensures any raindrops fall away quickly). A small, replaceable cartridge of silica gel (or other dessicant) inside the dome absorbs any dew. Since a thermopile typically sits outside in an exposed position, its case has to be made from something like toughened, rustproof, anodized aluminum. Typically, there's a built-in spirit level so you can be sure your pyranometer is flat (though some are designed to be used on inclined surfaces as well).
Photo: A pyranometer quietly going about its job, measuring solar radiation. Note the double glass in the dome and the weatherproof cable coming out of the side that carries electrical signals, corresponding to the strength of the solar radiation, out to a computer. (Strictly, this is a pyroheliometer: a pyranometer that measures direct solar radiation over a narrow field of view.) Photo by Steve Wilcox courtesy of US Department of Energy/National Renewable Energy Laboratory (US DOE/NREL).How does a pyranometer work?
When sunlight falls on a pyranometer, the thermopile sensor produces a proportional response typically in 30 seconds or less: the more sunlight, the hotter the sensor gets and the greater the electric current it generates. The thermopile is designed to be precisely linear (so a doubling of solar radiation produces twice as much current) and also has a directional response: it produces maximum output when the Sun is directly overhead (at midday) and zero output when the Sun is on the horizon (at dawn or dusk). This is called a cosine response (or cosine correction), because the electrical signal from the pyranometer varies with the cosine of the angle between the Sun's rays and the vertical.
Sunlight may look yellow, but it actually consists of a very broad spectrum of electromagnetic radiation, ranging in wavelength from about 280 nanometers (nm) up to about 4000 nanometers. This includes both visible "white light" (the familiar rainbow spectrum ranging from red and orange through to indigo and violet) and invisible electromagnetic radiation, including ultraviolet (UV) and infrared (IR). Although our eyes can't see much of this light, pyranometers do their best to detect as much of it as possible, because it all counts as sunlight. The best ones are designed to respond more or less equally to a substantial band of incoming light wavelengths (this is sometimes described as a flat wavelength response).
Types of pyranometers
Instruments like the ones we've discussed above are laboratory-grade pyranometers, usually described as secondary standard (ISO) or high quality (WMO)—the very best, in other words. Slightly lesser instruments are described as first class (ISO) or good quality (WMO), while second class (ISO) are the next best grade.
Not all pyranometers use thermopiles. You can also get less sophisticated (and considerably cheaper) solar-cell pyranometers that give more approximate measurements using tiny photovoltaic cells instead of thermopiles. Their main drawback is that they don't respond linearly to a broad band of solar radiation but only to a limited range of wavelengths; so while a high-quality pyranometer might measure wavelengths from 280-2800 nanometers, a solar-cell version might respond to wavelengths in a much narrower band from about 300-1100 nanometers (with a peak in the infrared region from around 800-1100nm). But unless you're making really detailed measurements in a laboratory, that may be perfectly fine for your needs.
Further reading
On this website
On other sites
- Measuring Sunlight at Earth's Surface: Build Your Own Pyranometer: There's nothing like doing some experiments to get a grip of the science behind things. This is a great activity you can try from solar scientist Dr David Brooks, whose Institute for Earth Science Research and Education website is a mine of fascinating information about sunlight measurements and their use in climate and weather science. See also his great little book, below.
- Photovoltaic Geographical Information System (PVGIS): How does sunlight vary across Europe? This website gives you comparative mapping data.
Books
- Bringing the Sun Down to Earth: Designing Inexpensive Instruments for Monitoring the Atmosphere by David R. Brooks. Springer, 2008. A great introduction to the science of how the Sun interacts with Earth's atmosphere, followed by details of how to make solar measurements and some simple measuring instruments you can build yourself.
- Solar Radiation & Daylight Models by Tariq Muneer. Elsevier Butterworth Heinemann, 2004. A guide to how measurements of solar radiation are used in such things as building design.
