Lasers and the electromagnetic spectrum

The color of light you choose will have a big effect on what your laser beam can do. Let’s discuss various colors of light, both visible and invisible, to get an overview of what each is good for and what limitations each may have. After all, choosing the right color is the key to really making your laser shine.

Radio

Radio waves are essentially useless for lasers. Sure, they get through the air okay, but diffraction makes them almost impossible to focus enough to cause damage. So without further ado, we’ll move on.

Color	Frequency	Wavelength	Energy
Radio	30 Hz - 30 MHz	10,000 km - 1 m	< 1.25 μeV

Microwaves

Microwaves, at least, focus better than radio waves. They still don’t focus well enough to make practical weapons - at least not if your intent is cooking or burning or blasting your enemy. They are useful at projecting destructive currents into electronic circuits. Such high power microwave devices operating in a counter-electronics role are usually considered a different class of weapon than lasers, so we will leave them for now.

Color	Frequency	Wavelength	Energy
Microwave	30 MHz - 300 GHz	1 m - 1 mm	1.25 μeV - 1.25 meV

Terahertz waves

Terahertz waves are all the rage these days for remote scanning and a new window for material spectroscopy. Unfortunately, they are absorbed by the air within a few tens of meters, so they are a poor choice for a weapon.

Color	Frequency	Wavelength	Energy
Terahertz wave	300 GHz - 10 THz	1 mm - 30 μm	1.25 meV - 40 meV

Far infrared

Far infrared is a sort of orphan band of the electromagnetic spectrum, because it is hard for us to get sources and detectors in this range. As a result, we don’t have a lot of experience with what it can do. In principle, your high-tech sci-fi society could be able to make fiercely high power far infrared lasers. But they’re still not a good choice for a weapon because the diffraction limit makes them hard to focus to damaging intensities without huge focal apertures and they’d have bad issues with cascade breakdown of the air.

Color	Frequency	Wavelength	Energy
Far infrared	10 THz - 20 THz	30 μm - 15 μm	40 meV - 80 meV

Long-wave infrared

This is the electromagnetic band where most thermal radiation from room-temperature and body-temperature objects occur. When someone is seeing heat with infrared vision, this is the color they are seeing with. The atmosphere is quite transparent to long-wave infrared radiation. Unfortunately, these long wavelengths are still difficult to focus at any useful distance, and they tend to cause cascade breakdown in the air when high powers are put into tight focal spots. The main reason they pop up in talking about lasers is that one of the first kinds of high power lasers, and still one of the cheapest and simplest to build, is the carbon dioxide laser which operates in the long-wave infrared.

Color	Frequency	Wavelength	Energy
Long-wave infrared	20 THz - 38 THz	30 μm - 15 μm	80 meV - 160 meV

Mid-wave infrared

A lot of the mid-wave infrared spectrum is absorbed quickly by air. However, there is a “window” between 3.5 and 4 μm where the light can get through. This window was investigated by early laser weapon designers, using chemical deuterium fluoride lasers. Chemical laser weapons were nasty, toxin-spewing, noisy monstrosities of machines with abysmal beam quality and long logistics chains to supply their highly toxic, corrosive, flammable, and explosive chemicals. And even when they were the only game in town, the deuterium fluoride laser was replaced as soon as they could by chemical oxygen iodine lasers that at least operated in the near infrared and so could be focused three times as far. Today we have far better choices, so don’t expect mid-wave infrared lasers to get much love.

Color	Frequency	Wavelength	Energy
Mid-wave infrared	38 THz - 100 THz	8 μm - 3 μm	160 meV - 410 meV

Short-wave infrared

Short-wave infrared is a good choice when you are looking for a color of light that focuses well, can get through air, can maintain a tight focus without two-photon ionization messing it up, and that won’t pose a severe blinding hazard to anyone nearby. It is the shortest wavelength (and thus longest ranged) color of infrared that is eye-safe. You won’t get eye-safe colors again until you are up into the ultraviolet.

Some modern lasers can output high power short-wave infrared beams, primarily fiber lasers.

Color	Frequency	Wavelength	Energy
Short-wave infrared	100 THz - 215 THz	3 μm - 1.4 μm	410 meV - 900 meV

Near infrared

This is the color that almost all modern combat lasers operate. The air is nicely transparent to light at this color, the beams focus well enough, and you can get crazy high powers out of fiber lasers these days. Sure - look at the thing they are shooting and you might go blind, but there are bigger hazards in the military.

Color	Frequency	Wavelength	Energy
Near infrared	215 THz - 430 THz	1.4 μm - 0.7 μm	900 meV - 1.8 eV

Visible

Yeah baby! Now we’re talkin’! Flashing beams lighting up the sky for stunning visual effects, strobing flashes where the beams hit. These are the beams you can really see! Except for the minor detail that if you ever do actually see one in person, there’s a good chance you won’t ever see anything again. But we’ll ignore that for the sake of a good special effects loaded sci-fi extravaganza.

The air is very transparent to visible light. It turns out that water is also at around its optimal transparency to visible light in the green, blue, and violet colors, so lasers of these colors might be the choice for underwater combat (or at least, underwater combat where you are close enough to see your enemy). If you want maximum range in air without two photon absorption making your life miserable when your beam reaches close focus, visible light is the color choice for you.

Visible light is where you start having significant losses due to Raighleh scattering for light going all the way through an Earth-like atmosphere. Shorter wavelengths (the closer to violet) are scattered more than longer wavelengths (closer to red). But still, the shorter wavelengths focus better because of diffraction. When shooting straight down through Earth’s atmosphere, you still get the best laser intensity with violet light (even though your beam will have less energy, that energy will still be more concentrated). But as you shoot at more and more of an angle, the best choice goes toward longer and longer wavelengths. And for alien planets, all bets are off.

Color	Frequency	Wavelength	Energy
Red	430 THz - 480 THz	0.7 μm - 0.62 μm	1.8 eV - 2 eV
Orange	480 THz - 510 THz	0.62 μm - 0.59 μm	2 eV - 2.1 eV
Yellow	510 THz - 530 THz	0.59 μm - 0.57 μm	2.1 eV - 2.2 eV
Green	530 THz - 610 THz	0.57 μm - 0.49 μm	2.2 eV - 2.5 eV
Blue	610 THz - 670 THz	0.49 μm - 0.45 μm	2.5 eV - 2.7 eV
Violet	670 THz - 750 THz	0.45 μm - 0.4 μm	2.7 eV - 3.1 eV

Near ultraviolet

This region of the spectrum is made up of invisible colors with shorter wavelengths than we can see that can still go through air. But although these colors can get through sea level air, ozone in the upper atmosphere does a pretty good job of absorbing ultraviolet light with wavelengths shorter than 0.34 μm. So if you want to use your laser to shoot things on the ground from your spacecraft, choose a wavelength longer than 0.34 μm. Ultraviolet light is scattered more by air than visible light, which makes it more favorable to use visible light for shooting things on Earth from a spacecraft. But on an alien planet, the scales may tip in favor of ultraviolet. And if you are shooting down within the atmosphere, the optimum color depends on the range to the target. And there is also the issue that high powered ultraviolet pulses are likely to be absorbed due to two-photon absorption before they get to their target.

Ultraviolet light is eye-safe at wavelengths shorter than 0.35 μm. Some ultraviolet-A colored light can get through window glass, but ultraviolet-B or C cannot. So if you are shooting your laser gun at someone on the other side of a window, choose ultraviolet-A or longer wavelengths.

Color	Frequency	Wavelength	Energy
Ultraviolet-A	750 THz - 950 THz	0.4 μm - 0.315 μm	3.1 eV - 3.9 eV
Ultraviolet-B	950 THz - 1.1 PHz	0.315 μm - 0.28 μm	3.9 eV - 4.4 eV
Ultraviolet-C	1.1 PHz - 1.5 PHz	0.28 μm - 0.2 μm	4.4 eV - 6.2 eV

Vacuum ultraviolet

Wavelengths shorter than 0.2 μm can’t go through oxygen. Hence, these wavelengths are called “vacuum” frequencies because they can’t go through air, only vacuum. Other atmospheres may let through slightly shorter wavelengths, but not by much. Anything shorter than 0.1 μm won’t be able to go through any matter (except perhaps a pure helium atmosphere - which can let stuff through down to 0.05 μm).

Still, as much as vacuum ultraviolet can’t be used in air, it focuses really well in vacuum. If you can make it in your laser, and if you can focus it, it’s a great choice for shooting things in space. In today’s world, our ultraviolet optics are not great and a lot of the light will get absorbed when we want it to be reflected. But a science fiction setting might have solved this, allowing their spaceships to mount devastating long range ultraviolet lasers.

Color	Frequency	Wavelength	Energy
Vacuum ultraviolet	1.5 PHz - 30 PHz	0.2 μm - 10 nm	6.2 eV - 125 eV

Soft x-ray

The boundary between ultraviolet and x-ray is kind of fuzzy - there is no strict line with ultraviolet on one side and x-rays on the other. The lower energy-per-photon sorts of x-rays act a lot like vacuum ultraviolet. Sure, they focus better because of their shorter wavelengths but they still get almost immediately absorbed by air. The best way we can find to focus soft x-rays is by using a complicated grazing incidence mirror.

Color	Frequency	Wavelength	Energy
Soft x-ray	30 PHz - 3 EHz	10 nm - 0.1 nm	125 eV - 12.5 keV

Hard x-rays

At higher energies-per-photon, x-rays start being able to go some distance through matter before they can be absorbed. There is no hard and fast rule on what is a soft x-ray and what is a hard x-ray. But these little photons can zip through tens of meters of air, or stand a reasonable chance of making it through a person’s body. This still makes them impractical for use in an atmosphere, however. But they can really allow your spacecraft to reach out and touch someone if you can somehow figure out a way to make and focus these little guys. Grazing incidence telescopes can work, but become more and more difficult the more energetic the x-rays get.

If you shoot a hard x-ray beam through an enemy spacecraft, expect the people that were in the compartments the beam penetrated to die from radiation poisoning if the blast and heat don’t get them.

Color	Frequency	Wavelength	Energy
Hard x-ray	3 EHz - 30 EHz	0.1 nm - 0.01 nm	12.5 keV - 125 keV

Gamma rays

The highest energy photons are called gamma rays. As with a lot of this high energy-per-photon light, there isn’t really a sharp distinction between high energy x-rays and low energy gamma rays. Gamma rays can get through several hundred meters of air. But don’t use a gamma ray laser if you are in air - the scattered radiation will come back to give you radiation sickness. Much like with hard x-ray, anyone even near where a gamma ray laser goes through matter will be dosed with dangerous levels of ionizing radiation. Also like hard x-rays, we have no idea how we would focus gamma rays.

Color	Frequency	Wavelength	Energy
Gamma ray	> 30 EHz	< 0.01 nm	> 125 keV