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Running Time: 5m 22s
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Electromagnetic Spectrum
The electromagnetic – or EM – spectrum is made up of seven kinds of electromagnetic energy with each corresponding to a different range. From lowest energy to highest energy, the seven groupings along the spectrum are: Radio Waves, Microwaves, Infrared, Visible Light, Ultraviolet, X-rays, and Gamma Rays. Electromagnetic energy travels in waves and spans a broad spectrum from very long radio waves to very short gamma rays. Read in the order listed above, waves increase in frequency and decrease in wavelength. The visible range, which is the only portion of the spectrum the human eye can detect, represents only a very tiny portion of the entire electromagnetic spectrum.
All electromagnetic radiation is made up of up of fields of electricity and magnetism interacting with each other. Electric fields can be static – like the static electricity that can hold a balloon to the wall. Magnetic fields can be static, too – like what holds a refrigerator magnet in place. However, electric and magnetic fields can also change and move together, and when that happens, the interaction produces waves: electromagnetic waves. EM energy can be described by frequency, wavelength, or energy, all of which are inter-related by the expression E = Frequency / Wavelength. Frequency is directly proportional to energy (they increase and decrease together) while wavelength is inversely proportional to energy (as wavelength increases, energy decreases).
Radio and microwaves are usually described by frequency (units of Hertz), infrared and visible light by wavelength (units of meters), and x-rays and gamma rays by energy (units of electron-volts). Though referred to by different names – light, EM radiation, or rays – all EM energy is made up of the same kinds of waves. The convention of using different units for different parts of the spectrum is simply a convenience that has to do with using numbers that are neither too large nor too small. The distinctions between the energy bands are simply a convention that eases communication. The EM spectrum doesn’t actually have breaks or chapters.
When you think of a water wave in the ocean, it might be easy to imagine the water oscillating up and down, creating a traveling waveform across the water. Even easier to imagine: making waves travel along a jump-rope secured to a wall at one end. In that case, it’s easy to see that the wave’s oscillation is perpendicular to the direction of its forward movement. In other words, the movement of the rope may be up and down, but the wave that travels through the rope is moving forward or backward—two perpendicular directions. These kinds of waves are called “transverse” waves. In transverse waves, the direction of the wave is perpendicular to the direction of applied energy. Another type of wave is a “longitudinal” wave, in which the wave moves parallel to the applied energy. With sound waves and other longitudinal waves, molecules vibrate and bump into one another, passing energy along the same direction the wave is moving.
While some transverse waves and some longitudinal waves might be easy to imagine, electromagnetic wave are harder to visualize. Because the wave is traveling in a direction that’s perpendicular to both the electric field and the magnetic field, thinking about EM waves requires three-dimensional visualization. Transverse waves like the jump-rope example give a close approximation, but electromagnetic radiation is more complex. One important feature of EM radiation is that, since its movement is based on the interaction of electric and magnetic fields, and electric and magnetic forces are possible over long distances, EM waves can travel through a vacuum. No material medium is necessary. Remember that low-energy EM radiation has longer wavelengths, corresponding to lower frequencies. High-energy EM radiation has shorter wavelengths, corresponding to higher frequencies.
All EM radiation travels at the same speed: the speed of light.
The categories along the spectrum – Radio, Microwave, Infrared, Visible, Ultraviolet, X-ray, Gamma Ray - represent a useful breakdown of EM radiation that helps scientists understand and visualize energy sources on, in, and under the Earth as well as throughout our solar system, galaxy, and universe.
Infrared
In our everyday lives, we use infrared energy in many ways – in TV remote controls, night vision goggles, satellite images of vegetation patterns. Infrared waves have wavelengths about the size of the diameter of a human hair. That seems small to us, but, along the EM spectrum, infrared radiation has relatively low energy and long wavelengths.
Infrared energy was discovered in 1800 when William Herschel conducted a now-famous experiment to measure the temperature differences between colors in the visible part of the spectrum. (The visible band is “next to” infrared on the EM spectrum.) He found that temperature increased going from the blue end of the visible spectrum to the red end. Luckily, he also measured beyond red, because in that region, he found that the temperature increased even more! He had discovered infrared energy.
Though humans can’t see infrared energy, we can sense it as heat. A fire, solar energy, heat lamps, your dog, other humans – all emit infrared energy. Because infrared radiation can pass through dust without getting scattered, astronomers can get clear images of space from areas not visible at optical wavelengths. NASA scientists have discovered many stars and newborn planets by collecting data at infrared wavelengths.
For scientists studying Earth, infrared images are very important. As solar energy hits the Earth, some gets absorbed and warms the planet. The heat then gets emitted and can be “seen” by infrared sensors on satellites circling the Earth. Scientists use infrared data to study changes in vegetation, ocean movements and temperatures, lava flows, locations of forest fires, and other environmental features.
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NARRATION: When you use a remote control to change channels on your TV, your remote is using light waves. But, this light is beyond the visible spectrum of light you can see.
Back in 1800, William Herschel conducted an experiment measuring the temperature changes between the colors of the spectrum plus one measurement beyond visible red. When that thermometer registered a temperature warmer than all the other colors, Herschel had discovered another region of the electromagnetic spectrum: infrared light. This region consists of short wavelengths around 760 nanometers to longer wavelengths about 1 million nanometers, or about 1 thousand micrometers in length.
We can sense some of this infrared energy as heat. Some objects are so hot they also emit visible light, such as a fire. Other objects, such as humans, are not as hot, and only emit infrared waves. We cannot see these infrared waves with our eyes alone. However, instruments that can sense infrared energy, such as night-vision goggles or infrared cameras, allow us to see these infrared waves from warm objects like humans and animals.
Infrared energy can also reveal objects in the universe that cannot be seen with optical telescopes. Infrared waves have longer wavelengths than visible light and can pass through dense regions of gas and dust with lower scattering and absorption. When you look up at the constellation Orion, you see only the visible light. But, NASA’s Spitzer telescope was able to detect nearly 23 hundred planet-forming disks in the Orion Nebula by sensing the infrared glow of their warm dust. Each disk has the potential to form planets and its own solar system.
Incoming ultraviolet, visible, and a limited portion of infrared energy, together sometimes called short wave radiation from the Sun, drives our Earth system. Some of this radiation is reflected off of clouds and some is absorbed in the atmosphere. Larger aerosol particles in the atmosphere interact with and absorb some of the radiation, causing the atmosphere to warm. The heat generated by this absorption is emitted as long wave infrared radiation, some of which radiates out to space. The solar radiation that does pass through Earth’s atmosphere is either reflected off snow, ice, or other surfaces, or is absorbed by the Earth’s surface. This absorption of radiation warms the Earth’s surface and this heat is emitted as long wave radiation into the atmosphere, which allows only a small amount to radiate out to space.
Greenhouses gases in the atmosphere, such as water vapor and carbon dioxide, absorb most of this emitted long wave infrared radiation, and this absorption heats the lower atmosphere. In turn, the warmed atmosphere emits long wave radiation, some of which radiates towards the Earth’s surface, keeping our planet warm and generally comfortable. The energy entering, energy reflected, energy absorbed, and energy emitted by the Earth system constitutes the components of the Earth radiation budget. A budget that’s out of balance can cause the temperature of the atmosphere to increase and eventually affect our climate.
For scientists to understand climate, they must also determine what drives the changes within the Earth’s radiation budget. The CERES instrument, aboard NASA’s Aqua and Terra satellites, can measure the reflected short wave and emitted long wave radiation into space accurately enough for scientists to determine the Earth’s total radiation budget. Other NASA instruments monitor the changes in other aspects of the Earth’s climate system such as clouds, aerosol particles, or surface reflectivity, and scientists are examining their many interactions with the energy budget.
A portion of solar radiation from the Sun that is just beyond the visible spectrum is referred to as near-infrared. Scientists can study how this radiation reflects off the Earth’s surface to understand changes in land cover, such as growth of cities or changes in vegetation. Our eyes perceive a leaf as green, because wavelengths in the green region of the visible light spectrum are reflected, while other visible wavelengths are absorbed. Yet, the chlorophyll and the cell structure of the leaf are also reflecting near-infrared light, light we cannot see. This reflected near-infrared radiation can be sensed by satellites, allowing scientists to study vegetation from space. Using these data, scientists can identify some types of trees, can examine the health of forests, and can even monitor the health of vegetation, such as forests infested with pine beetles or crops affected by drought.
Studying the emission and reflection of infrared waves helps us to understand the Earth system and its energy budget. Near-infrared data can also help scientists study land cover such as changes in snow, ice, forests, urbanization, and agriculture. Scientists are beginning to unlock the mysteries of cooler objects across the universe, such as planets, cool stars, nebulae, and much more, using infrared waves.
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