by Chris Woodford. Last updated: November 5, 2018.
Have you ever done one of those spot-the-difference newspaper puzzles where
you have to find the missing details using two very similar cartoons?
The quick way to solve them is to cut out the two images, place one
on top of the other, and shine a light through the paper. It might
sound like cheating but it's actually science: you're using the light
pattern from one image to show up differences in the other.
Scientists use a very similar process called interferometry to
measure small things with incredibly high accuracy by comparing
light or radio beams. Let's take a closer look at how it works!
Photo: A laser interferometer. The laser beam is split into two parts. One part travels straight to a detector while the other undergoes a change of some sort. By comparing the two beams again at the end, you can measure the extent of the change very precisely. Photo courtesy of NASA Glenn Research Center (NASA-GRC).
What is interference?
To understand interferometry, you need to understand interference.
In everyday life, interference simply means getting in the way or
meddling, but in physics it has a much more specific meaning.
Interference is what happens when two waves carrying energy meet up
and overlap. The energy they carry gets mixed up together so, instead
of two waves, you get a third wave whose shape and size depends on
the patterns of the original two waves. When waves combine like this,
the process is called superposition.
If you've ever sat making waves in a bath-tub, you'll have seen
interference and superposition in action. If you push your hand back
and forth, you can send waves of energy out from the center of the
water to the walls of the tub. When the waves get to the walls, they
bounce back off the hard surface more or less unchanged in size but
with their velocity reversed. Each wave reflects off the tub just as if
you'd kicked a rubber ball at the wall. Once the waves come back to
where your hand is, you can make them much bigger by moving
your hand in step with them. In effect, you create new waves that add
themselves to the original ones and increase the size of their peaks
(amplitude). When waves add together to make bigger waves, scientists call it
If you move your hands a different way, you can create waves that are
out of step with your original waves. When these new waves add to the
originals, they subtract energy from them and make them smaller. This
is what scientists call destructive interference.
It's just a phase
The extent to which one wave is in step with another is known as its
phase. If two identical waves are "in phase," it means their
peaks align so, if we add them together, we get a new wave that's
twice as big but otherwise exactly the same as the original waves.
Similarly, if two waves are completely out of phase (in what we call antiphase),
the peaks of one exactly coincide with the troughs of the other so
adding the waves together gives you nothing at all. In between these
two extremes are all sorts of other possibilities where one wave is
partly in phase with the other. Adding two waves like this
creates a third wave that has an unusual, rising and falling pattern of peaks and
troughs. Shine a wave like this onto a screen and you get a
characteristic pattern of light and dark areas called interference
fringes. This pattern is what you study and measure with an interferometer.
How do interferometers work?
An interferometer is a really precise scientific instrument designed to
measure things with extraordinary accuracy. The basic idea of
interferometry involves taking a beam of light
(or another type of electromagnetic radiation) and splitting it into two equal halves
using what's called a beam-splitter (also called a half-transparent
mirror or half-mirror). This is simply a piece of glass whose surface is very thinly coated with silver. If you shine light at it, half the light passes straight through and half of it reflects back—so the beam-splitter is like a cross between an ordinary piece of glass and
a mirror. One of the beams (known as the reference beam) shines onto a mirror and from there to a screen, camera,
or other detector. The other beam shines at or through something you want to measure, onto a second mirror, back through the beam splitter, and onto the same screen. This second beam travels an extra distance
(or in some other slightly different way) to the first beam, so it gets slightly out of step (out of phase).
Artwork: How a basic (Michelson) interferometer works. If we take the green
beam to be the reference beam, we'd subject the blue beam to some sort of change we wanted to measure.
The interferometer combines the two beams and the interference fringes that appear on the screen
are a visual representation of the difference between them.
When the two light beams meet up at the screen, they overlap and interfere, and the phase difference between them creates a pattern of light and dark areas (in other words, a set
of interference fringes). The light areas are places where the two
beams have added together (constructively) and become brighter; the
dark areas are places where the beams have subtracted from one
another (destructively). The exact pattern of interference depends on
the different way or the extra distance that one of the beams has
traveled. By inspecting and measuring the fringes, you can calculate
this with great accuracy—and that gives you an exact measurement of
whatever it is you're trying to find.
Instead of the interference fringes falling on a simple screen, often they're directed into
a camera to produce a permanent image called an interferogram. In another arrangement,
the interferogram is made by a detector
(like the CCD image sensor used in older digital cameras) that converts the pattern of fluctuating optical interference fringes into
an electrical signal that can be very easily analyzed with a computer.
What are the different types of interferometers?
Photo: Albert Einstein solved the "failed" Michelson-Morley interferometer experiment with his theory of relativity. Photo courtesy of US Library of Congress.
Interferometers became popular toward the end of the 19th century and there are several
different kinds, each based roughly on the principle we've outlined
above and named for the scientist who perfected it. Six
common types are the Michelson, Fabry-Perot, Fizeau,
Mach-Zehnder, Sagnac, and Twyman-Green interferometers:
- The Michelson interferometer (named for Albert Michelson,
1853–1931) is probably best known for the part it played in the
famous Michelson-Morley experiment in 1881. That was when Michelson and his
colleague Edward Morley (1838–1923) disproved the existence of a mysterious invisible fluid called "the ether" that physicists had believed filled empty space. The Michelson-Morley experiment was an important stepping-stone toward Albert Einstein's theory of relativity.
- The Fabry-Perot interferometer (invented in 1897 by Charles
Fabry, 1867–1945, and Alfred Perot, 1863–1925), also known as an
etalon, evolved from the Michelson interferometer. It makes clearer and sharper fringes that are easier to see and measure.
- The Fizeau interferometer (named for French physicist Hippolyte
Fizeau, 1819–1896) is another variation and is generally easier to use than a Fabry-Perot. It's widely used for making optical and engineering measurements.
- The Mach-Zehnder interferometer (invented by German Ludwig Mach and Swissman Ludwig Zehnder) uses two beam splitters instead of one and produces two output beams, which can be analyzed separately. It's widely used in fluid dynamics and aerodynamics—the fields for which it was originally developed.
- The Sagnac interferometer (named for Georges Sagnac, a French physicist) splits light into two beams that travel in opposite directions around a closed loop or ring (hence its alternative name, the ring interferometer). It's widely used in navigational equipment, such as
ring-laser gyroscopes (optical versions of gyroscopes that use laser beams instead of spinning wheels).
- The Twyman-Green interferometer (developed by Frank Twyman and Arthur Green in 1916) is a modified
Michelson mainly used for testing optical devices.
Most modern interferometers use laser light because it's more regular and
precise than ordinary light and produces coherent beams (in
which all the light waves travel in phase). The pioneers of interferometry didn't have access to lasers (which weren't developed until the mid-20th century) so they had to use beams of light passed through slits and lenses instead.
Artwork: Fiber-optic interferometry. Most interferometers pass their beams through the open air, but local temperature and pressure variations can sometimes be a source of error. If that matters,
one option is to use a fiber-optic interferometer like this. A laser (red, 12) shoots its beam through lenses (gray, 16a/b) into a pair of fiber-optic cables. One of them (blue, 18) becomes the reference beam, bouncing its light straight onto a screen (orange, 22). The other (green, 20) allows its beam to reflect off something that's being measured (such as a vibrating surface) into a third cable (green, 30). The reference and reflected beams meet up and interfere on the screen in the usual way. Artwork from
US Patent 4,380,394: Fiber optic interferometer by David Stowe, Gould Inc., April 19, 1983, courtesy of US Patent and Trademark Office.
How accurate are interferometers?
A state-of-the-art interferometer can measure distances to within 1 nanometer (one billionth of a meter,
which is about the width of 10 hydrogen atoms), but like any other kind
of measurement, it's subject to errors. The biggest source of error is likely to come from changes in the
wavelength of the laser light, which depends on the refractive index of the material through which it's
traveling. The temperature, pressure, humidity, and concentration of different gases in the air all
change its refractive index, altering the wavelength of the laser light passing through it and potentially
introducing measurement errors. Fortunately, good interferometers can compensate for this. Some have
separate lasers that measure the air's refractive index, while others measure air
temperature, pressure, and humidity and calculate the effect on the refractive index indirectly; either way,
measurements can be corrected and the overall error is reduced to perhaps one or two parts per million.
What are interferometers used for?
Photo: Interferometry in action: These 3D topographical maps of Long Valley, California were made from the Space Shuttle using a technique called radar interferometry, in which beams of microwaves are reflected off Earth's contours and then recombined. Photo courtesy of NASA Jet Propulsion Laboratory (NASA-JPL).
Interferometers are widely used in all kinds of scientific and engineering applications for making precise measurements. By scanning interferometers over objects, you can also make very detailed maps of surfaces.
By "precise" and "detailed", I really do mean precise and detailed. The interference fringes that an optical (light-based) interferometer produces are made by light waves traveling fractionally out of step. Since the wavelength
of visible light is in the hundreds of nanometers, interferometers can theoretically measure lengths a couple of hundred times smaller than a human hair. In practice, everyday laboratory constraints sometimes make that kind of precision hard to achieve. Albert Michelson, for example, found his ether-detecting apparatus was affected by traffic movements about a third of a kilometer away!
Astronomers also use interferometers to combine signals from telescopes so they
work in the same way as larger and much more powerful instruments
that can penetrate deeper into space. Some of these interferometers
work with light waves; others use radio waves (similar to light waves
but with much longer wavelengths and lower frequencies).
Photo: The Keck interferometer. Astronomers have linked the two 10-m (33-ft) optical telescopes in these domes on Mauna Kea, Hawaii to make what is effectively a single, much more powerful telescope. Photo courtesy of NASA Jet Propulsion Laboratory (NASA-JPL).
Interferometry is also helping us to figure out the secrets of gravity. In 2017, three US physicists (Rainer Weiss, Barry Barish, and Kip Thorne) shared the Nobel Prize in Physics for the discovery of gravitational waves ("ripples in spacetime"), originally predicted by Albert Einstein over a century ago.
Their experiment is called LIGO (Laser Interferometer Gravitational-Wave Observatory) and uses two very large laser interferometers with arms 4km (2.5 miles) long, located in two different places 3000km (1800 miles) apart, at opposite ends of the United States (Hanford, Washington and Livingston, Louisiana).