
Pyranometers
Last updated: September 9, 2009.
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.
Photo: Sunlight varies all the time, but how can you measure it? Photo by Steve Wilcox courtesy of US Department of Energy/National Renewable Energy Laboratory (US DOE/NREL).
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.
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, it's 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