Electromagnetic spectrum - wikipedia Electromagnetic spectrum Class Freq - uency Wave - length Energy Ionizing radiation γ Gamma rays 300 EHz 1 pm 1.24 M eV 30 EHz 10 pm 124 k eV HX Hard X-rays 3 EHz 100 pm 12.4 keV SX Soft X-rays 300 PHz 1 nm 1.24 keV 30 PHz 10 nm 124 eV EUV Extreme ultraviolet 3 PHz 100 nm 12.4 eV NUV Near ultraviolet Visible 300 THz 1 μm 1.24 eV NIR Near infrared 30 THz 10 μm 124 m eV MIR Mid infrared 3 THz 100 μm 12.4 meV FIR Far infrared 300 GHz 1 mm 1.24 meV Micro - waves and radio waves EHF Extremely high frequency 30 GHz 1 cm 124 μ eV SHF Super high frequency 3 GHz 1 dm 12.4 μeV UHF Ultra high frequency 300 MHz 1 m 1.24 μeV VHF Very high frequency 30 MHz 10 m 124 n eV HF High frequency 3 MHz 100 m 12.4 neV MF Medium frequency 300 kHz 1 km 1.24 neV LF Low frequency 30 kHz 10 km 124 p eV VLF Very low frequency 3 kHz 100 km 12.4 peV ULF Ultra low frequency 300 Hz 1 Mm 1.24 peV SLF Super low frequency 30 Hz 10 Mm 124 f eV ELF Extremely low frequency 3 Hz 100 Mm 12.4 feV Sources : File : Light spectrum. svg Legend γ = Gamma rays MIR = Mid infrared HF = High freq. HX = Hard X-rays FIR = Far infrared MF = Medium freq. SX = Soft X-rays Radio waves LF = Low freq. EUV = Extreme ultraviolet EHF = Extremely high freq. VLF = Very low freq. NUV = Near ultraviolet SHF = Super high freq. VF / ULF = Voice freq. Visible light UHF = Ultra high freq. SLF = Super low freq. NIR = Near Infrared VHF = Very high freq. ELF = Extremely low freq. Freq = Frequency The electromagnetic spectrum is the range of frequencies ( the spectrum ) of electromagnetic radiation and their respective wavelengths and photon energies. The electromagnetic spectrum covers electromagnetic waves with frequencies ranging from below one hertz to above 10 hertz, corresponding to wavelengths from thousands of kilometers down to a fraction of the size of an atomic nucleus. This frequency range is divided into separate bands, and the electromagnetic waves within each frequency band are called by different names ; beginning at the low frequency ( long wavelength ) end of the spectrum these are : radio waves, microwaves, terahertz waves, infrared, visible light, ultraviolet, X-rays, and gamma rays at the high - frequency ( short wavelength ) end. The electromagnetic waves in each of these bands have different characteristics, such as how they are produced, how they interact with matter, and their practical applications. The limit for long wavelengths is the size of the universe itself, while it is thought that the short wavelength limit is in the vicinity of the Planck length. Gamma rays, X-rays, and high ultraviolet are classified as ionizing radiation as their photons have enough energy to ionize atoms, causing chemical reactions. Exposure to these rays can be a health hazard, causing radiation sickness, DNA damage and cancer. Radiation of visible light wavelengths and lower are called nonionizing radiation as they can not cause these effects. In most of the frequency bands above, a technique called spectroscopy can be used to physically separate waves of different frequencies, producing a spectrum showing the constituent frequencies. Spectroscopy is used to study the interactions of electromagnetic waves with matter. Other technological uses are described under electromagnetic radiation. Contents 1 History and discovery 2 Range 3 Regions 3.1 Rationale for names 4 Types of radiation 4.1 Radio frequency 4.2 Microwaves 4.3 Terahertz radiation 4.4 Infrared radiation 4.5 Visible radiation ( light ) 4.6 Ultraviolet radiation 4.7 X-rays 4.8 Gamma rays 5 See also 6 Notes and references 7 External links History and discovery See also : History of electromagnetism, History of radio, History of electrical engineering, and History of optics For most of history, visible light was the only known part of the electromagnetic spectrum. The ancient Greeks recognized that light traveled in straight lines and studied some of its properties, including reflection and refraction. The study of light continued, and during the 16th and 17th centuries conflicting theories regarded light as either a wave or a particle. The first discovery of electromagnetic radiation other than visible light came in 1800, when William Herschel discovered infrared radiation. He was studying the temperature of different colors by moving a thermometer through light split by a prism. He noticed that the highest temperature was beyond red. He theorized that this temperature change was due to `` calorific rays '' that were a type of light ray that could not be seen. The next year, Johann Ritter, working at the other end of the spectrum, noticed what he called `` chemical rays '' ( invisible light rays that induced certain chemical reactions ). These behaved similarly to visible violet light rays, but were beyond them in the spectrum. They were later renamed ultraviolet radiation. Electromagnetic radiation was first linked to electromagnetism in 1845, when Michael Faraday noticed that the polarization of light traveling through a transparent material responded to a magnetic field ( see Faraday effect ). During the 1860s James Maxwell developed four partial differential equations for the electromagnetic field. Two of these equations predicted the possibility and behavior of waves in the field. Analyzing the speed of these theoretical waves, Maxwell realized that they must travel at a speed that was about the known speed of light. This startling coincidence in value led Maxwell to make the inference that light itself is a type of electromagnetic wave. Maxwell 's equations predicted an infinite number of frequencies of electromagnetic waves, all traveling at the speed of light. This was the first indication of the existence of the entire electromagnetic spectrum. Maxwell 's predicted waves included waves at very low frequencies compared to infrared, which in theory might be created by oscillating charges in an ordinary electrical circuit of a certain type. Attempting to prove Maxwell 's equations and detect such low frequency electromagnetic radiation, in 1886 the physicist Heinrich Hertz built an apparatus to generate and detect what are now called radio waves. Hertz found the waves and was able to infer ( by measuring their wavelength and multiplying it by their frequency ) that they traveled at the speed of light. Hertz also demonstrated that the new radiation could be both reflected and refracted by various dielectric media, in the same manner as light. For example, Hertz was able to focus the waves using a lens made of tree resin. In a later experiment, Hertz similarly produced and measured the properties of microwaves. These new types of waves paved the way for inventions such as the wireless telegraph and the radio. In 1895 Wilhelm Röntgen noticed a new type of radiation emitted during an experiment with an evacuated tube subjected to a high voltage. He called these radiations x-rays and found that they were able to travel through parts of the human body but were reflected or stopped by denser matter such as bones. Before long, many uses were found for them in the field of medicine. The last portion of the electromagnetic spectrum was filled in with the discovery of gamma rays. In 1900 Paul Villard was studying the radioactive emissions of radium when he identified a new type of radiation that he first thought consisted of particles similar to known alpha and beta particles, but with the power of being far more penetrating than either. However, in 1910, British physicist William Henry Bragg demonstrated that gamma rays are electromagnetic radiation, not particles, and in 1914, Ernest Rutherford ( who had named them gamma rays in 1903 when he realized that they were fundamentally different from charged alpha and beta particles ) and Edward Andrade measured their wavelengths, and found that gamma rays were similar to X-rays, but with shorter wavelengths and higher frequencies. Range Electromagnetic waves are typically described by any of the following three physical properties : the frequency f, wavelength λ, or photon energy E. Frequencies observed in astronomy range from 7023239999999999999 ♠ 2.4 × 10 Hz ( 1 GeV gamma rays ) down to the local plasma frequency of the ionized interstellar medium ( ~ 1 kHz ). Wavelength is inversely proportional to the wave frequency, so gamma rays have very short wavelengths that are fractions of the size of atoms, whereas wavelengths on the opposite end of the spectrum can be as long as the universe. Photon energy is directly proportional to the wave frequency, so gamma ray photons have the highest energy ( around a billion electron volts ), while radio wave photons have very low energy ( around a femtoelectronvolt ). These relations are illustrated by the following equations : f = c λ, or f = E h, or E = h c λ, ( displaystyle f = ( \frac ( c ) ( lambda ) ), quad ( \text ( or ) ) quad f = ( \frac ( E ) ( h ) ), quad ( \text ( or ) ) quad E = ( \frac ( hc ) ( lambda ) ), ) where : c = 7008299792458000000 ♠ 299 792 458 m / s is the speed of light in a vacuum h = 6966662606895999999 ♠ 6.626 068 96 ( 33 ) × 10 J s = 6985413566733000000 ♠ 4.135 667 33 ( 10 ) × 10 eV s is Planck 's constant. Whenever electromagnetic waves exist in a medium with matter, their wavelength is decreased. Wavelengths of electromagnetic radiation, no matter what medium they are traveling through, are usually quoted in terms of the vacuum wavelength, although this is not always explicitly stated. Generally, electromagnetic radiation is classified by wavelength into radio wave, microwave, terahertz ( or sub-millimeter ) radiation, infrared, the visible region that is perceived as light, ultraviolet, X-rays and gamma rays. The behavior of EM radiation depends on its wavelength. When EM radiation interacts with single atoms and molecules, its behavior also depends on the amount of energy per quantum ( photon ) it carries. Spectroscopy can detect a much wider region of the EM spectrum than the visible range of 400 nm to 700 nm. A common laboratory spectroscope can detect wavelengths from 2 nm to 2500 nm. Detailed information about the physical properties of objects, gases, or even stars can be obtained from this type of device. Spectroscopes are widely used in astrophysics. For example, many hydrogen atoms emit a radio wave photon that has a wavelength of 21.12 cm. Also, frequencies of 30 Hz and below can be produced by and are important in the study of certain stellar nebulae and frequencies as high as 7027290000000000000 ♠ 2.9 × 10 Hz have been detected from astrophysical sources. Regions The electromagnetic spectrum A diagram of the electromagnetic spectrum, showing various properties across the range of frequencies and wavelengths The types of electromagnetic radiation are broadly classified into the following classes ( regions, bands or types ) : Gamma radiation X-ray radiation Ultraviolet radiation Visible radiation Infrared radiation Terahertz radiation Microwave radiation Radio waves This classification goes in the increasing order of wavelength, which is characteristic of the type of radiation. While, in general, the classification scheme is accurate, in reality there is often some overlap between neighboring types of electromagnetic energy. For example, SLF radio waves at 60 Hz may be received and studied by astronomers, or may be ducted along wires as electric power, although the latter is, in the strict sense, not electromagnetic radiation at all ( see near and far field ). Note that there are no precisely defined boundaries between the bands of the electromagnetic spectrum ; rather they fade into each other like the bands in a rainbow ( which is the sub-spectrum of visible light ). Radiation of each frequency and wavelength ( or in each band ) has a mix of properties of the two regions of the spectrum that bound it. For example, red light resembles infrared radiation in that it can excite and add energy to some chemical bonds and indeed must do so to power the chemical mechanisms responsible for photosynthesis and the working of the visual system. The distinction between X-rays and gamma rays is partly based on sources : the photons generated from nuclear decay or other nuclear and subnuclear / particle process, are always termed gamma rays, whereas X-rays are generated by electronic transitions involving highly energetic inner atomic electrons. In general, nuclear transitions are much more energetic than electronic transitions, so gamma - rays are more energetic than X-rays, but exceptions exist. By analogy to electronic transitions, muonic atom transitions are also said to produce X-rays, even though their energy may exceed 6 megaelectronvolts ( 0.96 pJ ), whereas there are many ( 77 known to be less than 10 keV ( 1.6 fJ ) ) low - energy nuclear transitions ( e.g., the 7.6 eV ( 1.22 aJ ) nuclear transition of thorium - 229 ), and, despite being one million-fold less energetic than some muonic X-rays, the emitted photons are still called gamma rays due to their nuclear origin. The convention that EM radiation that is known to come from the nucleus, is always called `` gamma ray '' radiation is the only convention that is universally respected, however. Many astronomical gamma ray sources ( such as gamma ray bursts ) are known to be too energetic ( in both intensity and wavelength ) to be of nuclear origin. Quite often, in high energy physics and in medical radiotherapy, very high energy EMR ( in the > 10 MeV region ) -- which is of higher energy than any nuclear gamma ray -- is not called X-ray or gamma - ray, but instead by the generic term of `` high energy photons. '' The region of the spectrum where a particular observed electromagnetic radiation falls, is reference frame - dependent ( due to the Doppler shift for light ), so EM radiation that one observer would say is in one region of the spectrum could appear to an observer moving at a substantial fraction of the speed of light with respect to the first to be in another part of the spectrum. For example, consider the cosmic microwave background. It was produced, when matter and radiation decoupled, by the de-excitation of hydrogen atoms to the ground state. These photons were from Lyman series transitions, putting them in the ultraviolet ( UV ) part of the electromagnetic spectrum. Now this radiation has undergone enough cosmological red shift to put it into the microwave region of the spectrum for observers moving slowly ( compared to the speed of light ) with respect to the cosmos. Rationale for names Electromagnetic radiation interacts with matter in different ways across the spectrum. These types of interaction are so different that historically different names have been applied to different parts of the spectrum, as though these were different types of radiation. Thus, although these `` different kinds '' of electromagnetic radiation form a quantitatively continuous spectrum of frequencies and wavelengths, the spectrum remains divided for practical reasons related to these qualitative interaction differences. Electromagnetic radiation interaction with matter Region of the spectrum Main interactions with matter Radio Collective oscillation of charge carriers in bulk material ( plasma oscillation ). An example would be the oscillatory travels of the electrons in an antenna. Microwave through far infrared Plasma oscillation, molecular rotation Near infrared Molecular vibration, plasma oscillation ( in metals only ) Visible Molecular electron excitation ( including pigment molecules found in the human retina ), plasma oscillations ( in metals only ) Ultraviolet Excitation of molecular and atomic valence electrons, including ejection of the electrons ( photoelectric effect ) X-rays Excitation and ejection of core atomic electrons, Compton scattering ( for low atomic numbers ) Gamma rays Energetic ejection of core electrons in heavy elements, Compton scattering ( for all atomic numbers ), excitation of atomic nuclei, including dissociation of nuclei High - energy gamma rays Creation of particle - antiparticle pairs. At very high energies a single photon can create a shower of high - energy particles and antiparticles upon interaction with matter. Types of radiation Radio frequency Main articles : Radio frequency, Radio spectrum, and Radio waves Radio waves are emitted and received by antennas, which consist of conductors such as metal rod resonators. In artificial generation of radio waves, an electronic device called a transmitter generates an AC electric current which is applied to an antenna. The oscillating electrons in the antenna generate oscillating electric and magnetic fields that radiate away from the antenna as radio waves. In reception of radio waves, the oscillating electric and magnetic fields of a radio wave couple to the electrons in an antenna, pushing them back and forth, creating oscillating currents which are applied to a radio receiver. Earth 's atmosphere is mainly transparent to radio waves, except for layers of charged particles in the ionosphere which can reflect certain frequencies. Radio waves are extremely widely used to transmit information across distances in radio communication systems such as radio broadcasting, television, two way radios, mobile phones, communication satellites, and wireless networking. In a radio communication system, a radio frequency current is modulated with an information - bearing signal in a transmitter by varying either the amplitude, frequency or phase, and applied to an antenna. The radio waves carry the information across space to a receiver, where they are received by an antenna and the information extracted by demodulation in the receiver. Radio waves are also used for navigation in systems like Global Positioning System ( GPS ) and navigational beacons, and locating distant objects in radiolocation and radar. They are also used for remote control, and for industrial heating. The use of the radio spectrum is strictly regulated by governments, coordinated by a body called the International Telecommunications Union ( ITU ) which allocates frequencies to different users for different uses. Microwaves Main article : Microwaves Plot of Earth 's atmospheric transmittance ( or opacity ) to various wavelengths of electromagnetic radiation. Microwaves are radio waves of short wavelength, from about 10 centimeters to one millimeter, in the SHF and EHF frequency bands. Microwave energy is produced with klystron and magnetron tubes, and with solid state devices such as Gunn and IMPATT diodes. Although they are emitted and absorbed by short antennas, they are also absorbed by polar molecules, coupling to vibrational and rotational modes, resulting in bulk heating. Unlike higher frequency waves such as infrared and light which are absorbed mainly at surfaces, microwaves can penetrate into materials and deposit their energy below the surface. This effect is used to heat food in microwave ovens, and for industrial heating and medical diathermy. Microwaves are the main wavelengths used in radar, and are used for satellite communication, and wireless networking technologies such as Wifi, although this is at intensity levels unable to cause thermal heating. The copper cables ( transmission lines ) which are used to carry lower frequency radio waves to antennas have excessive power losses at microwave frequencies, and metal pipes called waveguides are used to carry them. Although at the low end of the band the atmosphere is mainly transparent, at the upper end of the band absorption of microwaves by atmospheric gasses limits practical propagation distances to a few kilometers. Terahertz radiation Main article : Terahertz radiation Terahertz radiation is a region of the spectrum between far infrared and microwaves. Until recently, the range was rarely studied and few sources existed for microwave energy at the high end of the band ( sub-millimeter waves or so - called terahertz waves ), but applications such as imaging and communications are now appearing. Scientists are also looking to apply terahertz technology in the armed forces, where high - frequency waves might be directed at enemy troops to incapacitate their electronic equipment. Terahertz radiation is strongly absorbed by atmospheric gases, making this frequency range useless for long distance communication. Infrared radiation Main article : Infrared radiation The infrared part of the electromagnetic spectrum covers the range from roughly 300 GHz to 400 THz ( 1 mm - 750 nm ). It can be divided into three parts : Far - infrared, from 300 GHz to 30 THz ( 1 mm -- 10 μm ). The lower part of this range may also be called microwaves or terahertz waves. This radiation is typically absorbed by so - called rotational modes in gas - phase molecules, by molecular motions in liquids, and by phonons in solids. The water in Earth 's atmosphere absorbs so strongly in this range that it renders the atmosphere in effect opaque. However, there are certain wavelength ranges ( `` windows '' ) within the opaque range that allow partial transmission, and can be used for astronomy. The wavelength range from approximately 200 μm up to a few mm is often referred to as `` sub-millimeter '' in astronomy, reserving far infrared for wavelengths below 200 μm. Mid-infrared, from 30 to 120 THz ( 10 -- 2.5 μm ). Hot objects ( black - body radiators ) can radiate strongly in this range, and human skin at normal body temperature radiates strongly at the lower end of this region. This radiation is absorbed by molecular vibrations, where the different atoms in a molecule vibrate around their equilibrium positions. This range is sometimes called the fingerprint region, since the mid-infrared absorption spectrum of a compound is very specific for that compound. Near - infrared, from 120 to 400 THz ( 2,500 -- 750 nm ). Physical processes that are relevant for this range are similar to those for visible light. The highest frequencies in this region can be detected directly by some types of photographic film, and by many types of solid state image sensors for infrared photography and videography. Visible radiation ( light ) Main article : Visible spectrum Above infrared in frequency comes visible light. The Sun emits its peak power in the visible region, although integrating the entire emission power spectrum through all wavelengths shows that the Sun emits slightly more infrared than visible light. By definition, visible light is the part of the EM spectrum the human eye is the most sensitive to. Visible light ( and near - infrared light ) is typically absorbed and emitted by electrons in molecules and atoms that move from one energy level to another. This action allows the chemical mechanisms that underlie human vision and plant photosynthesis. The light that excites the human visual system is a very small portion of the electromagnetic spectrum. A rainbow shows the optical ( visible ) part of the electromagnetic spectrum ; infrared ( if it could be seen ) would be located just beyond the red side of the rainbow with ultraviolet appearing just beyond the violet end. Electromagnetic radiation with a wavelength between 380 nm and 760 nm ( 400 -- 790 terahertz ) is detected by the human eye and perceived as visible light. Other wavelengths, especially near infrared ( longer than 760 nm ) and ultraviolet ( shorter than 380 nm ) are also sometimes referred to as light, especially when the visibility to humans is not relevant. White light is a combination of lights of different wavelengths in the visible spectrum. Passing white light through a prism splits it up into the several colors of light observed in the visible spectrum between 400 nm and 780 nm. If radiation having a frequency in the visible region of the EM spectrum reflects off an object, say, a bowl of fruit, and then strikes the eyes, this results in visual perception of the scene. The brain 's visual system processes the multitude of reflected frequencies into different shades and hues, and through this insufficiently - understood psychophysical phenomenon, most people perceive a bowl of fruit. At most wavelengths, however, the information carried by electromagnetic radiation is not directly detected by human senses. Natural sources produce EM radiation across the spectrum, and technology can also manipulate a broad range of wavelengths. Optical fiber transmits light that, although not necessarily in the visible part of the spectrum ( it is usually infrared ), can carry information. The modulation is similar to that used with radio waves. Ultraviolet radiation Main article : Ultraviolet The amount of penetration of UV relative to altitude in Earth 's ozone Next in frequency comes ultraviolet ( UV ). The wavelength of UV rays is shorter than the violet end of the visible spectrum but longer than the X-ray. UV is the longest wavelength radiation whose photons are energetic enough to ionize atoms, separating electrons from them, and thus causing chemical reactions. Short wavelength UV and the shorter wavelength radiation above it ( X-rays and gamma rays ) are called ionizing radiation, and exposure to them can damage living tissue, making them a health hazard. UV can also cause many substances to glow with visible light ; this is called fluorescence. At the middle range of UV, UV rays can not ionize but can break chemical bonds, making molecules unusually reactive. Sunburn, for example, is caused by the disruptive effects of middle range UV radiation on skin cells, which is the main cause of skin cancer. UV rays in the middle range can irreparably damage the complex DNA molecules in the cells producing thymine dimers making it a very potent mutagen. The Sun emits significant UV radiation ( about 10 % of its total power ), including extremely short wavelength UV that could potentially destroy most life on land ( ocean water would provide some protection for life there ). However, most of the Sun 's damaging UV wavelengths are absorbed by the atmosphere before they reach the surface. The higher energy ( shortest wavelength ) ranges of UV ( called `` vacuum UV '' ) are absorbed by nitrogen and, at longer wavelengths, by simple diatomic oxygen in the air. Most of the UV in the mid-range of energy is blocked by the ozone layer, which absorbs strongly in the important 200 -- 315 nm range, the lower energy part of which is too long for ordinary dioxygen in air to absorb. This leaves less than 3 % of sunlight at sea level in UV, with all of this remainder at the lower energies. The remainder is UV - A, along with some UV - B. The very lowest energy range of UV between 315 nm and visible light ( called UV - A ) is not blocked well by the atmosphere, but does not cause sunburn and does less biological damage. However, it is not harmless and does create oxygen radicals, mutations and skin damage. See ultraviolet for more information. X-rays Main article : X-rays After UV come X-rays, which, like the upper ranges of UV are also ionizing. However, due to their higher energies, X-rays can also interact with matter by means of the Compton effect. Hard X-rays have shorter wavelengths than soft X-rays and as they can pass through many substances with little absorption, they can be used to ' see through ' objects with ' thicknesses ' less than that equivalent to a few meters of water. One notable use is diagnostic X-ray imaging in medicine ( a process known as radiography ). X-rays are useful as probes in high - energy physics. In astronomy, the accretion disks around neutron stars and black holes emit X-rays, enabling studies of these phenomena. X-rays are also emitted by the coronas of stars and are strongly emitted by some types of nebulae. However, X-ray telescopes must be placed outside the Earth 's atmosphere to see astronomical X-rays, since the great depth of the atmosphere of Earth is opaque to X-rays ( with areal density of 1000 grams per cm ), equivalent to 10 meters thickness of water. This is an amount sufficient to block almost all astronomical X-rays ( and also astronomical gamma rays -- see below ). Gamma rays Main article : Gamma rays After hard X-rays come gamma rays, which were discovered by Paul Ulrich Villard in 1900. These are the most energetic photons, having no defined lower limit to their wavelength. In astronomy they are valuable for studying high - energy objects or regions, however as with X-rays this can only be done with telescopes outside the Earth 's atmosphere. Gamma rays are used experimentally by physicists for their penetrating ability and are produced by a number of radioisotopes. They are used for irradiation of foods and seeds for sterilization, and in medicine they are occasionally used in radiation cancer therapy. More commonly, gamma rays are used for diagnostic imaging in nuclear medicine, an example being PET scans. The wavelength of gamma rays can be measured with high accuracy through the effects of Compton scattering. See also Electromagnetism portal Electronics portal Telecommunication portal Bandplan Cosmic ray Digital dividend after digital television transition Electroencephalography Infrared window Ionizing radiation List of international common standards Optical window Ozone layer Radiant energy Radiation Radio window Spectroscopy V band W band Notes and references ^ Jump up to : What is Light ? Archived December 5, 2013, at the Wayback Machine. -- UC Davis lecture slides ^ Jump up to : Elert, Glenn. `` The Electromagnetic Spectrum, The Physics Hypertextbook ''. Hypertextbook.com. Retrieved 2010 - 10 - 16. ^ Jump up to : `` Definition of frequency bands on ''. Vlf.it. Retrieved 2010 - 10 - 16. Jump up ^ Bakshi, U.A. ; Godse, A.P. ( 2009 ). Basic Electronics Engineering. Technical Publications. pp. 8 -- 10. ISBN 978 - 81 - 8431 - 580 - 6. ^ Jump up to : Mehta, Akul. `` Introduction to the Electromagnetic Spectrum and Spectroscopy ''. Pharmaxchange.info. Retrieved 2011 - 11 - 08. Jump up ^ Haitel, Gary ( 2014 - 05 - 15 ). Origins and Grand Finale : How the Bible and Science relate to the Origin of Everything, Abuses of Political Authority, and End Times Predictions. iUniverse. ISBN 9781491732571. Jump up ^ `` Herschel Discovers Infrared Light ''. Cool Cosmos Classroom activities. Archived from the original on 2012 - 02 - 25. Retrieved 4 March 2013. He directed sunlight through a glass prism to create a spectrum (... ) and then measured the temperature of each colour. (... ) He found that the temperatures of the colors increased from the violet to the red part of the spectrum. (... ) Herschel decided to measure the temperature just beyond the red of the spectrum in a region where no sunlight was visible. To his surprise, he found that this region had the highest temperature of all. Jump up ^ Davidson, Michael W. `` Johann Wilhelm Ritter ( 1776 -- 1810 ) ''. The Florida State University. Retrieved 5 March 2013. Ritter (... ) hypothesized that there must also be invisible radiation beyond the violet end of the spectrum and commenced experiments to confirm his speculation. He began working with silver chloride, a substance decomposed by light, measuring the speed at which different colors of light broke it down. (... ) Ritter (... ) demonstrated that the fastest rate of decomposition occurred with radiation that could not be seen, but that existed in a region beyond the violet. Ritter initially referred to the new type of radiation as chemical rays, but the title of ultraviolet radiation eventually became the preferred term. Jump up ^ Mohr, Peter J. ; Taylor, Barry N. ; Newell, David B. ( 2008 ). `` CODATA Recommended Values of the Fundamental Physical Constants : 2006 ''. Reviews of Modern Physics. 80 ( 2 ) : 633 -- 730. arXiv : 0801.0028. Bibcode : 2008RvMP... 80... 633M. doi : 10.1103 / RevModPhys. 80.633. Direct link to value. Jump up ^ Condon, J.J. ; Ransom, S.M. `` Essential Radio Astronomy : Pulsar Properties ''. National Radio Astronomy Observatory. Retrieved 2008 - 01 - 05. Jump up ^ Abdo, A.A. ; Allen, B. ; Berley, D. ; Blaufuss, E. ; Casanova, S. ; Chen, C. ; Coyne, D.G. ; Delay, R.S. ; Dingus, B.L. ; Ellsworth, R.W. ; Fleysher, L. ; Fleysher, R. ; Gebauer, I. ; Gonzalez, M.M. ; Goodman, J.A. ; Hays, E. ; Hoffman, C.M. ; Kolterman, B.E. ; Kelley, L.A. ; Lansdell, C.P. ; Linnemann, J.T. ; McEnery, J.E. ; Mincer, A.I. ; Moskalenko, I.V. ; Nemethy, P. ; Noyes, D. ; Ryan, J.M. ; Samuelson, F.W. ; Saz Parkinson, P.M. ; et al. ( 2007 ). `` Discovery of TeV Gamma - Ray Emission from the Cygnus Region of the Galaxy ''. The Astrophysical Journal. 658 ( 1 ) : L33 -- L36. arXiv : astro - ph / 0611691. Bibcode : 2007ApJ... 658L... 33A. doi : 10.1086 / 513696. Jump up ^ Feynman, Richard ; Leighton, Robert ; Sands, Matthew ( 1963 ). The Feynman Lectures on Physics, Vol. 1. USA : Addison - Wesley. pp. 2 -- 5. ISBN 978 - 0 - 201 - 02116 - 5. Jump up ^ L'Annunziata, Michael ; Baradei, Mohammad ( 2003 ). Handbook of Radioactivity Analysis. Academic Press. p. 58. ISBN 978 - 0 - 12 - 436603 - 9. Jump up ^ Grupen, Claus ; Cowan, G. ; Eidelman, S.D. ; Stroh, T. ( 2005 ). Astroparticle Physics. Springer. p. 109. ISBN 978 - 3 - 540 - 25312 - 9. Jump up ^ Corrections to muonic X-rays and a possible proton halo slac - pub - 0335 ( 1967 ) Jump up ^ `` Gamma - Rays ''. Hyperphysics.phy-astr.gsu.edu. Retrieved 2010 - 10 - 16. Jump up ^ `` Advanced weapon systems using lethal Short - pulse terahertz radiation from high - intensity - laser - produced plasmas ''. India Daily. March 6, 2005. Archived from the original on 6 January 2010. Retrieved 2010 - 09 - 27. Jump up ^ `` Reference Solar Spectral Irradiance : Air Mass 1.5 ''. Retrieved 2009 - 11 - 12. Jump up ^ Koontz, Steve ( 26 June 2012 ) Designing Spacecraft and Mission Operations Plans to Meet Flight Crew Radiation Dose. NASA / MIT Workshop. See pages I - 7 ( atmosphere ) and I - 23 ( for water ). Jump up ^ Uses of Electromagnetic Waves gcse - revision, physics, waves, uses - electromagnetic - waves Revision World External links Wikimedia Commons has media related to Electromagnetic spectrum. UnwantedEmissions.com ( U.S. radio spectrum allocations resource ) Australian Radiofrequency Spectrum Allocations Chart ( from Australian Communications and Media Authority ) Canadian Table of Frequency Allocations ( from Industry Canada ) U.S. Frequency Allocation Chart -- Covering the range 3 kHz to 300 GHz ( from Department of Commerce ) UK frequency allocation table ( from Ofcom, which inherited the Radiocommunications Agency 's duties, pdf format ) Flash EM Spectrum Presentation / Tool -- Very complete and customizable. How to render the color spectrum / Code -- Only approximately right. Poster `` Electromagnetic Radiation Spectrum '' ( 992 kB ) Electromagnetic Spectrum presentation Electromagnetic Spectrum Strategy : A Call to Action U.S. Department of Defense Electromagnetic spectrum Gamma rays X-rays Ultraviolet Visible Infrared Terahertz radiation Microwave Radio ← higher frequencies longer wavelengths → Visible ( optical ) Violet Blue Green Yellow Orange Red Microwaves W band V band Q band K band K band K band X band C band S band L band Radio EHF SHF UHF VHF HF MF LF VLF ULF SLF ELF Wavelength types Microwave Shortwave Medium wave Longwave Color topics Red Orange Yellow Green Cyan Blue Indigo Violet Purple Magenta Pink Brown White Gray Black Color science Color physics Electromagnetic spectrum Light Rainbow Visible Spectral colors Chromophore Structural coloration Animal coloration On Vision and Colors Metamerism Spectral power distribution Color perception Color vision Color blindness Achromatopsia test Tetrachromacy Color constancy Color term Color depth Color photography Spot color Color printing Web colors Color mapping Color code Color management Chrominance False color Chroma key Color balance Color cast Color temperature Eigengrau Color psychology Color symbolism Color preferences Lüscher color test Kruithof curve Political color National colors Chromophobia Chromotherapy Color philosophy Color space Color model additive subtractive Color mixing Primary color Secondary color Tertiary color ( intermediate ) Quaternary color Quinary color Aggressive color ( warm ) Receding color ( cool ) Pastel colors Color gradient Color scheme Color tool Monochromatic colors Complementary colors Analogous colors Achromatic colors ( Neutral ) Polychromatic colors Impossible colors Light - on - dark Tinctures in heraldry Color theory Chromaticity diagram Color solid Color wheel Color triangle Color analysis ( art ) Color realism ( art style ) Color terms Basic terms Blue Green Red Yellow Pink Purple Orange Black Gray White Brown Cultural differences Linguistic relativity and the color naming debate Blue -- green distinction in language Color history Color in Chinese culture Traditional colors of Japan Human skin color Color dimensions Hue Dichromatism Colorfulness ( chroma and saturation ) Tints and shades Lightness ( tone and value ) Grayscale Color organizations Pantone Color Marketing Group The Color Association of the United States International Colour Authority International Commission on Illumination ( CIE ) International Color Consortium International Colour Association Lists List of colors : A -- F List of colors : G -- M List of colors : N -- Z List of colors ( compact ) List of colors by shade List of color palettes List of color spaces List of Crayola crayon colors history Color chart List of fictional colors List of RAL colors List of web colors Related Vision Image processing Multi-primary color display Quattron Qualia Lighting Local color ( visual art ) Portal Index of color - related articles Retrieved from `` https://en.wikipedia.org/w/index.php?title=Electromagnetic_spectrum&oldid=864925501 '' Categories : Electromagnetic spectrum Waves Hidden categories : Webarchive template wayback links Wikipedia semi-protected pages All articles with unsourced statements Articles with unsourced statements from November 2015 Talk View source Contents About Wikipedia Afrikaans Aragonés Asturianu Azərbaycanca বাংলা Български Bosanski Català Čeština Dansk Deutsch Eesti Ελληνικά Español Esperanto Euskara فارسی Français Gaeilge Galego 한국어 हिन्दी Hrvatski Bahasa Indonesia Italiano עברית Basa Jawa Қазақша Kiswahili Kreyòl ayisyen Latviešu Lëtzebuergesch Македонски മലയാളം Bahasa Melayu Nederlands 日本 語 Norsk Norsk nynorsk Polski Português Română Русиньскый Русский Sardu Scots Shqip සිංහල Simple English Slovenčina Slovenščina کوردی Српски / srpski Srpskohrvatski / српскохрватски Basa Sunda Suomi Svenska தமிழ் తెలుగు ไทย Türkçe Українська Tiếng Việt Winaray 中文 57 more Edit links This page was last edited on 20 October 2018, at 13 : 45 ( UTC ). 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Question: what type of radiation is light with a wavelength of 1nm
Answer: Soft X-rays