Microwave
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Microwave is a form of electromagnetic radiation with wavelengths shorter than other radio waves but longer than infrared waves. Its wavelength ranges from about one meter to one millimeter, corresponding to frequencies between 300 MHz and 300 GHz, broadly construed.[1][2][3] A more common definition in radio-frequency engineering is the range between 1 and 100 GHz (wavelengths between 30 cm and 3 mm),[4]: 3 or between 1 and 3000 GHz (30 cm and 0.1 mm).[5][6] In all cases, microwaves include the entire super high frequency (SHF) band (3 to 30 GHz, or 10 to 1 cm) at minimum. The boundaries between far infrared, terahertz radiation, microwaves, and ultra-high-frequency (UHF) are fairly arbitrary and differ between different fields of study.[4]: 3
The prefix micro- in microwave indicates that microwaves are small (having shorter wavelengths), compared to the radio waves used in prior radio technology. Frequencies in the microwave range are often referred to by their IEEE radar band designations: S, C, X, Ku, K, or Ka band, or by similar NATO or EU designations.
Microwaves travel by line-of-sight; unlike lower frequency radio waves, they do not diffract around hills, follow the Earth's surface as ground waves, or reflect from the ionosphere, so terrestrial microwave communication links are limited by the visual horizon to about 40 miles (64 km). At the high end of the band, they are absorbed by gases in the atmosphere, limiting practical communication distances to around a kilometer.
Microwaves are widely used in modern technology, for example in point-to-point communication links, wireless networks, microwave radio relay networks, radar, satellite and spacecraft communication, medical diathermy and cancer treatment, remote sensing, radio astronomy, particle accelerators, spectroscopy, industrial heating, collision avoidance systems, garage door openers and keyless entry systems, and for cooking food in microwave ovens.
Electromagnetic spectrum
[edit]Microwaves occupy a place in the electromagnetic spectrum with frequency above ordinary radio waves, and below infrared light:
| Electromagnetic spectrum | ||||
|---|---|---|---|---|
| Name | Wavelength | Frequency (Hz) | Photon energy (eV) | |
| Gamma ray | < 0.01 nm | > 30 EHz | > 124 keV | |
| X-ray | 0.01 nm – 10 nm | 30 EHz – 30 PHz | 124 keV – 124 eV | |
| Ultraviolet | 10 nm – 400 nm | 30 PHz – 750 THz | 124 eV – 3 eV | |
| Visible light | 400 nm – 750 nm | 750 THz – 400 THz | 3 eV – 1.7 eV | |
| Infrared | 750 nm – 1 mm | 400 THz – 300 GHz | 1.7 eV – 1.24 meV | |
| Microwave | 1 mm – 1 m | 300 GHz – 300 MHz | 1.24 meV – 1.24 μeV | |
| Radio | ≥ 1 m | ≤ 300 MHz | ≤ 1.24 μeV | |
In descriptions of the electromagnetic spectrum, some sources classify microwaves as radio waves, a subset of the radio wave band, while others classify microwaves and radio waves as distinct types of radiation.[1] This is an arbitrary distinction.
Frequency bands
[edit]Bands of frequencies in the microwave spectrum are designated by letters. Unfortunately, there are several incompatible band designation systems, and even within a system the frequency ranges corresponding to some of the letters vary somewhat between different application fields.[7][8] The letter system had its origin in World War 2 in a top-secret U.S. classification of bands used in radar sets; this is the origin of the oldest letter system, the IEEE radar bands. One set of microwave frequency bands designations by the Radio Society of Great Britain (RSGB), is tabulated below:
| Radio bands | ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| ITU | ||||||||||||
|
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| EU / NATO / US ECM | ||||||||||||
| IEEE | ||||||||||||
| Other TV and radio | ||||||||||||
| Designation | Frequency range | Wavelength range | Typical uses |
|---|---|---|---|
| L band | 1 to 2 GHz | 15 cm to 30 cm | military telemetry, GPS, mobile phones (GSM), amateur radio |
| S band | 2 to 4 GHz | 7.5 cm to 15 cm | weather radar, surface ship radar, some communications satellites, microwave ovens, microwave devices/communications, radio astronomy, mobile phones, wireless LAN, Bluetooth, ZigBee, GPS, amateur radio |
| C band | 4 to 8 GHz | 3.75 cm to 7.5 cm | long-distance radio telecommunications, wireless LAN, amateur radio |
| X band | 8 to 12 GHz | 25 mm to 37.5 mm | satellite communications, radar, terrestrial broadband, space communications, amateur radio, molecular rotational spectroscopy |
| Ku band | 12 to 18 GHz | 16.7 mm to 25 mm | satellite communications, molecular rotational spectroscopy |
| K band | 18 to 26.5 GHz | 11.3 mm to 16.7 mm | radar, satellite communications, astronomical observations, automotive radar, molecular rotational spectroscopy |
| Ka band | 26.5 to 40 GHz | 5.0 mm to 11.3 mm | satellite communications, molecular rotational spectroscopy |
| Q band | 33 to 50 GHz | 6.0 mm to 9.0 mm | satellite communications, terrestrial microwave communications, radio astronomy, automotive radar, molecular rotational spectroscopy |
| U band | 40 to 60 GHz | 5.0 mm to 7.5 mm | |
| V band | 50 to 75 GHz | 4.0 mm to 6.0 mm | millimeter wave radar research, molecular rotational spectroscopy and other kinds of scientific research |
| W band | 75 to 110 GHz | 2.7 mm to 4.0 mm | satellite communications, millimeter-wave radar research, military radar targeting and tracking applications, and some non-military applications, automotive radar |
| F band | 90 to 140 GHz | 2.1 mm to 3.3 mm | SHF transmissions: Radio astronomy, microwave devices/communications, wireless LAN, most modern radars, communications satellites, satellite television broadcasting, DBS, amateur radio |
| D band | 110 to 170 GHz | 1.8 mm to 2.7 mm | EHF transmissions: Radio astronomy, high-frequency microwave radio relay, microwave remote sensing, amateur radio, directed-energy weapon, millimeter wave scanner |
Other definitions exist.[9]
The term P band is sometimes used for UHF frequencies below the L band but is now obsolete per IEEE Std 521.
When radars were first developed at K band during World War 2, it was not known that there was a nearby absorption band (due to water vapor and oxygen in the atmosphere). To avoid this problem, the original K band was split into a lower band, Ku, and upper band, Ka.[10]
Propagation
[edit]
Microwaves travel solely by line-of-sight paths; unlike lower frequency radio waves, they do not travel as ground waves which follow the contour of the Earth, or reflect off the ionosphere (skywaves).[11] Although at the low end of the band, they can pass through building walls enough for useful reception, usually rights of way cleared to the first Fresnel zone are required. Therefore, on the surface of the Earth, microwave communication links are limited by the visual horizon to about 30–40 miles (48–64 km). Microwaves are absorbed by moisture in the atmosphere, and the attenuation increases with frequency, becoming a significant factor (rain fade) at the high end of the band. Beginning at about 40 GHz, atmospheric gases also begin to absorb microwaves, so above this frequency microwave transmission is limited to a few kilometers. A spectral band structure causes absorption peaks at specific frequencies (see graph at right). Above 100 GHz, the absorption of electromagnetic radiation by Earth's atmosphere is so effective that it is in effect opaque, until the atmosphere becomes transparent again in the so-called infrared and optical window frequency ranges.
Troposcatter
[edit]In a microwave beam directed at an angle into the sky, a small amount of the power will be randomly scattered as the beam passes through the troposphere.[11] A sensitive receiver beyond the horizon with a high gain antenna focused on that area of the troposphere can pick up the signal. This technique has been used at frequencies between 0.45 and 5 GHz in tropospheric scatter (troposcatter) communication systems to communicate beyond the horizon, at distances up to 300 km.
Antennas
[edit]
The short wavelengths of microwaves allow omnidirectional antennas for portable devices to be made very small, from 1 to 20 centimeters long, so microwave frequencies are widely used for wireless devices such as cell phones, cordless phones, and wireless LANs (Wi-Fi) access for laptops, and Bluetooth earphones. Antennas used include short whip antennas, rubber ducky antennas, sleeve dipoles, patch antennas, and increasingly the printed circuit inverted F antenna (PIFA) used in cell phones.
Their short wavelength also allows narrow beams of microwaves to be produced by conveniently small high gain antennas from a half meter to 5 meters in diameter. Therefore, beams of microwaves are used for point-to-point communication links, and for radar. An advantage of narrow beams is that they do not interfere with nearby equipment using the same frequency, allowing frequency reuse by nearby transmitters. Parabolic ("dish") antennas are the most widely used directive antennas at microwave frequencies, but horn antennas, slot antennas and lens antennas are also used. Flat microstrip antennas are being increasingly used in consumer devices. Another directive antenna practical at microwave frequencies is the phased array, a computer-controlled array of antennas that produces a beam that can be electronically steered in different directions.
At microwave frequencies, the transmission lines which are used to carry lower frequency radio waves to and from antennas, such as coaxial cable and parallel wire lines, have excessive power losses, so when low attenuation is required, microwaves are carried by metal pipes called waveguides. Due to the high cost and maintenance requirements of waveguide runs, in many microwave antennas the output stage of the transmitter or the RF front end of the receiver is located at the antenna.
Design and analysis
[edit]The term microwave also has a more technical meaning in electromagnetics and circuit theory.[12][13] Apparatus and techniques may be described qualitatively as "microwave" when the wavelengths of signals are roughly the same as the dimensions of the circuit, so that lumped-element circuit theory is inaccurate, and instead distributed circuit elements and transmission-line theory are more useful methods for design and analysis.
As a consequence, practical microwave circuits tend not to use the discrete resistors, capacitors, and inductors used with lower-frequency radio waves. Open-wire and coaxial transmission lines used at lower frequencies are replaced by waveguides and stripline, and lumped-element tuned circuits are replaced by cavity resonators or resonant stubs.[12] In turn, at even higher frequencies, where the wavelength of the electromagnetic waves becomes small in comparison to the size of the structures used to process them, microwave techniques become inadequate, and the methods of optics are used.
Sources
[edit]
High-power microwave sources use specialized vacuum tubes to generate microwaves. These devices operate on different principles from low-frequency vacuum tubes, using the ballistic motion of electrons in a vacuum under the influence of controlling electric or magnetic fields, and include the magnetron (used in microwave ovens), klystron, traveling-wave tube (TWT), and gyrotron. These devices work in the density modulated mode, rather than the current modulated mode. This means that they work on the basis of clumps of electrons flying ballistically through them, rather than using a continuous stream of electrons.
Low-power microwave sources use solid-state devices such as the field-effect transistor (at least at lower frequencies), tunnel diodes, Gunn diodes, and IMPATT diodes.[14] Low-power sources are available as benchtop instruments, rackmount instruments, embeddable modules and in card-level formats. A maser is a solid-state device that amplifies microwaves using similar principles to the laser, which amplifies higher-frequency light waves.
All warm objects emit low level microwave black-body radiation, depending on their temperature, so in meteorology and remote sensing, microwave radiometers are used to measure the temperature of objects or terrain.[15] The sun[16] and other astronomical radio sources such as Cassiopeia A emit low level microwave radiation which carries information about their makeup, which is studied by radio astronomers using receivers called radio telescopes.[15] The cosmic microwave background radiation (CMBR), for example, is a weak microwave noise filling empty space which is a major source of information on cosmology's Big Bang theory of the origin of the Universe.
Applications
[edit]Microwave technology is extensively used for point-to-point telecommunications (i.e., non-broadcast uses). Microwaves are especially suitable for this use since they are more easily focused into narrower beams than radio waves, allowing frequency reuse; their comparatively higher frequencies allow broad bandwidth and high data transmission rates, and antenna sizes are smaller than at lower frequencies because antenna size is inversely proportional to the transmitted frequency. Microwaves are used in spacecraft communication, and much of the world's data, TV, and telephone communications are transmitted long distances by microwaves between ground stations and communications satellites. Microwaves are also employed in microwave ovens and in radar technology.
Communication
[edit]
Before the advent of fiber-optic transmission, most long-distance telephone calls were carried via networks of microwave radio relay links run by carriers such as AT&T Long Lines. Starting in the early 1950s, frequency-division multiplexing was used to send up to 5,400 telephone channels on each microwave radio channel, with as many as ten radio channels combined into one antenna for the hop to the next site, up to 70 km away.
Wireless LAN protocols, such as Bluetooth and the IEEE 802.11 specifications used for Wi-Fi, also use microwaves in the 2.4 GHz ISM band, although 802.11a uses ISM band and U-NII frequencies in the 5 GHz range. Licensed long-range (up to about 25 km) Wireless Internet Access services have been used for almost a decade in many countries in the 3.5–4.0 GHz range. The FCC recently[when?] carved out spectrum for carriers that wish to offer services in this range in the U.S. — with emphasis on 3.65 GHz. Dozens of service providers across the country are securing or have already received licenses from the FCC to operate in this band. The WIMAX service offerings that can be carried on the 3.65 GHz band will give business customers another option for connectivity.
Metropolitan area network (MAN) protocols, such as WiMAX (Worldwide Interoperability for Microwave Access) are based on standards such as IEEE 802.16, designed to operate between 2 and 11 GHz. Commercial implementations are in the 2.3 GHz, 2.5 GHz, 3.5 GHz and 5.8 GHz ranges.
Mobile Broadband Wireless Access (MBWA) protocols based on standards specifications such as IEEE 802.20 or ATIS/ANSI HC-SDMA (such as iBurst) operate between 1.6 and 2.3 GHz to give mobility and in-building penetration characteristics similar to mobile phones but with vastly greater spectral efficiency.[17]
Some mobile phone networks, like GSM, use the low-microwave/high-UHF frequencies around 1.8 and 1.9 GHz in the Americas and elsewhere, respectively. DVB-SH and S-DMB use 1.452 to 1.492 GHz, while proprietary/incompatible satellite radio in the U.S. uses around 2.3 GHz for DARS.
Microwave radio is used in point-to-point telecommunications transmissions because, due to their short wavelength, highly directional antennas are smaller and therefore more practical than they would be at longer wavelengths (lower frequencies). There is also more bandwidth in the microwave spectrum than in the rest of the radio spectrum; the usable bandwidth below 300 MHz is less than 300 MHz while many GHz can be used above 300 MHz. Typically, microwaves are used in remote broadcasting of news or sports events as the backhaul link to transmit a signal from a remote location to a television station from a specially equipped van. See broadcast auxiliary service (BAS), remote pickup unit (RPU), and studio/transmitter link (STL).
Most satellite communications systems operate in the C, X, Ka, or Ku bands of the microwave spectrum. These frequencies allow large bandwidth while avoiding the crowded UHF frequencies and staying below the atmospheric absorption of EHF frequencies. Satellite TV either operates in the C band for the traditional large dish fixed satellite service or Ku band for direct-broadcast satellite. Military communications run primarily over X or Ku-band links, with Ka band being used for Milstar.
Navigation
[edit]Global Navigation Satellite Systems (GNSS) including the Chinese Beidou, the American Global Positioning System (introduced in 1978) and the Russian GLONASS broadcast navigational signals in various bands between about 1.2 GHz and 1.6 GHz.
Radar
[edit]
Radar is a radiolocation technique in which a beam of radio waves emitted by a transmitter bounces off an object and returns to a receiver, allowing the location, range, speed, and other characteristics of the object to be determined. The short wavelength of microwaves causes large reflections from objects the size of motor vehicles, ships and aircraft. Also, at these wavelengths, the high gain antennas such as parabolic antennas which are required to produce the narrow beamwidths needed to accurately locate objects are conveniently small, allowing them to be rapidly turned to scan for objects. Therefore, microwave frequencies are the main frequencies used in radar. Microwave radar is widely used for applications such as air traffic control, weather forecasting, navigation of ships, and speed limit enforcement. Long-distance radars use the lower microwave frequencies since at the upper end of the band atmospheric absorption limits the range, but millimeter waves are used for short-range radar such as collision avoidance systems.
Radio astronomy
[edit]Microwaves emitted by astronomical radio sources; planets, stars, galaxies, and nebulas are studied in radio astronomy with large dish antennas called radio telescopes. In addition to receiving naturally occurring microwave radiation, radio telescopes have been used in active radar experiments to bounce microwaves off planets in the Solar System, to determine the distance to the Moon or map the invisible surface of Venus through cloud cover.
A recently[when?] completed microwave radio telescope is the Atacama Large Millimeter Array, located at more than 5,000 meters (16,597 ft) altitude in Chile, which observes the universe in the millimeter and submillimeter wavelength ranges. The world's largest ground-based astronomy project to date, it consists of more than 66 dishes and was built in an international collaboration by Europe, North America, East Asia and Chile.[18][19]
A major recent[when?] focus of microwave radio astronomy has been mapping the cosmic microwave background radiation (CMBR) discovered in 1964 by radio astronomers Arno Penzias and Robert Wilson. This faint background radiation, which fills the universe and is almost the same in all directions, is "relic radiation" from the Big Bang, and is one of the few sources of information about conditions in the early universe. Due to the expansion and thus cooling of the Universe, the originally high-energy radiation has been shifted into the microwave region of the radio spectrum. Sufficiently sensitive radio telescopes can detect the CMBR as a faint signal that is not associated with any star, galaxy, or other object.[20]
Heating and power application
[edit]
A microwave oven passes microwave radiation at a frequency near 2.45 GHz (12 cm) through food, causing dielectric heating primarily by absorption of the energy in water. Microwave ovens became common kitchen appliances in Western countries in the late 1970s, following the development of less expensive cavity magnetrons. Water in the liquid state possesses many molecular interactions that broaden the absorption peak. In the vapor phase, isolated water molecules absorb at around 22 GHz, almost ten times the frequency of the microwave oven.
Microwave heating is used in industrial processes for drying and curing products.
Many semiconductor processing techniques use microwaves to generate plasma for such purposes as reactive ion etching and plasma-enhanced chemical vapor deposition (PECVD).
Microwaves are used in stellarators and tokamak experimental fusion reactors to help break down the gas into a plasma and heat it to very high temperatures. The frequency is tuned to the cyclotron resonance of the electrons in the magnetic field, anywhere between 2–200 GHz, hence it is often referred to as Electron Cyclotron Resonance Heating (ECRH). The upcoming ITER thermonuclear reactor[21] will use up to 20 MW of 170 GHz microwaves.
Microwaves can be used to transmit power over long distances, and post-World War 2 research was done to examine possibilities. NASA worked in the 1970s and early 1980s to research the possibilities of using solar power satellite (SPS) systems with large solar arrays that would beam power down to the Earth's surface via microwaves.
Less-than-lethal weaponry exists that uses millimeter waves to heat a thin layer of human skin to an intolerable temperature so as to make the targeted person move away. A two-second burst of the 95 GHz focused beam heats the skin to a temperature of 54 °C (129 °F) at a depth of 0.4 millimetres (1⁄64 in). The United States Air Force and Marines are currently using this type of active denial system in fixed installations.[22]
Spectroscopy
[edit]Microwave radiation is used in electron paramagnetic resonance (EPR or ESR) spectroscopy, typically in the X-band region (~9 GHz) in conjunction typically with magnetic fields of 0.3 T. This technique provides information on unpaired electrons in chemical systems, such as free radicals or transition metal ions such as Cu(II). Microwave radiation is also used to perform rotational spectroscopy and can be combined with electrochemistry as in microwave enhanced electrochemistry.
Frequency measurement
[edit]Microwave frequency can be measured by either electronic or mechanical techniques.
Frequency counters or high frequency heterodyne systems can be used. Here the unknown frequency is compared with harmonics of a known lower frequency by use of a low-frequency generator, a harmonic generator and a mixer. The accuracy of the measurement is limited by the accuracy and stability of the reference source.
Mechanical methods require a tunable resonator such as an absorption wavemeter, which has a known relation between a physical dimension and frequency.
In a laboratory setting, Lecher lines can be used to directly measure the wavelength on a transmission line made of parallel wires, the frequency can then be calculated. A similar technique is to use a slotted waveguide or slotted coaxial line to directly measure the wavelength. These devices consist of a probe introduced into the line through a longitudinal slot so that the probe is free to travel up and down the line. Slotted lines are primarily intended for measurement of the voltage standing wave ratio on the line. However, provided a standing wave is present, they may also be used to measure the distance between the nodes, which is equal to half the wavelength. The precision of this method is limited by the determination of the nodal locations.
Effects on health
[edit]Microwaves are non-ionizing radiation, which means that microwave photons do not contain sufficient energy to ionize molecules or break chemical bonds, or cause DNA damage, as ionizing radiation such as x-rays or ultraviolet can.[23] The word "radiation" refers to energy radiating from a source and not to radioactivity. The main effect of absorption of microwaves is to heat materials; the electromagnetic fields cause polar molecules to vibrate. It has not been shown conclusively that microwaves (or other non-ionizing electromagnetic radiation) have significant adverse biological effects at low levels. Some, but not all, studies suggest that long-term exposure may have a carcinogenic effect.[24]
During World War II, it was observed that individuals in the radiation path of radar installations experienced clicks and buzzing sounds in response to microwave radiation. Research by NASA in the 1970s has shown this to be caused by thermal expansion in parts of the inner ear. In 1955, Dr. James Lovelock was able to reanimate rats chilled to 0 and 1 °C (32 and 34 °F) using microwave diathermy.[25]
When injury from exposure to microwaves occurs, it usually results from dielectric heating induced in the body. The lens and cornea of the eye are especially vulnerable because they contain no blood vessels that can carry away heat. Exposure to microwave radiation can produce cataracts by this mechanism, because the microwave heating denatures proteins in the crystalline lens of the eye[26] (in the same way that heat turns egg whites white and opaque). Exposure to heavy doses of microwave radiation (as from an oven that has been tampered with to allow operation even with the door open) can produce heat damage in other tissues as well, up to and including serious burns that may not be immediately evident because of the tendency for microwaves to heat deeper tissues with higher moisture content.
History
[edit]The motivation for exploiting the microwave frequencies was the increasing congestion in the lower frequency bands, and the ability to use smaller antennas at higher frequencies[27]: 830
Hertzian optics
[edit]Microwaves were first generated in the 1890s in some of the earliest radio wave experiments by physicists who thought of them as a form of "invisible light".[28] James Clerk Maxwell in his 1873 theory of electromagnetism, now called Maxwell's equations, had predicted that a coupled electric field and magnetic field could travel through space as an electromagnetic wave, and proposed that light consisted of electromagnetic waves of short wavelength.[27]: 832 In 1888, physicist Heinrich Hertz was the first to demonstrate the existence of electromagnetic waves, generating radio waves using a primitive spark gap radio transmitter.[27]: 830 [29]
Hertz and the other early radio researchers were interested in exploring the similarities between radio waves and light waves, to test Maxwell's theory. They concentrated on producing short wavelength radio waves in the UHF and microwave ranges, with which they could duplicate classic optics experiments in their laboratories, using quasioptical components such as prisms and lenses made of paraffin, sulfur and pitch and wire diffraction gratings, to refract and diffract radio waves like light rays.[30] Hertz used frequencies at the threshold of the microwave region: 50, 100, and 430 MHz.[27]: 831 His directional 430 MHz transmitter consisted of a 26 cm brass rod dipole antenna with a spark gap between the ends, suspended at the focal line of a parabolic antenna made of a curved zinc sheet, powered by high voltage pulses from an induction coil.[27]: 845 [29] His historic experiments demonstrated that radio waves like light exhibited refraction, diffraction, polarization, interference and standing waves,[27]: 845-846 [30] proving that radio waves and light waves were both forms of Maxwell's electromagnetic waves. He also experimented with open wire and coaxial transmission lines.[27]: 841
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Heinrich Hertz's 430 MHz spark transmitter, 1888, consisting of 23 cm dipole and spark gap at the focus of a parabolic reflector
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Jagadish Chandra Bose in 1894 was the first person to produce millimeter waves; his spark oscillator (in box, right) generated 60 GHz (5 mm) waves using 3 mm metal ball resonators.
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3 mm spark ball oscillator Bose used to generate 60 GHz waves
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Microwave spectroscopy experiment by John Ambrose Fleming in 1897 showing refraction of 1.4 GHz microwaves by paraffin prism, duplicating earlier experiments by Bose and Righi.
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Augusto Righi's 12 GHz spark oscillator and receiver, 1895
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Oliver Lodge's 5 inch oscillator ball he used to generate 1.2 GHz microwaves in 1894
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1.2 GHz microwave spark transmitter (left) and coherer receiver (right) used by Guglielmo Marconi during his 1895 experiments had a range of 6.5 km (4.0 mi)
Beginning in 1894 Jagadish Chandra Bose performed the first experiments with microwaves. He was the first person to produce millimeter waves, generating frequencies up to 60 GHz (5 millimeter) using a 3 mm metal ball spark oscillator.[31][30] Bose also invented waveguide, horn antennas, and semiconductor crystal detectors for use in his experiments. Independently in 1894, Oliver Lodge and Augusto Righi experimented with 1.5 and 12 GHz microwaves respectively, generated by small metal ball spark resonators.[30] Russian physicist Pyotr Lebedev in 1895 generated 50 GHz millimeter waves.[30] In 1897 Lord Rayleigh solved the mathematical boundary-value problem of electromagnetic waves propagating through conducting tubes and dielectric rods of arbitrary shape[32][33][34][35] which gave the modes and cutoff frequency of microwaves propagating through a waveguide.[29]
However, since microwaves were limited to line-of-sight paths, they could not communicate beyond the visual horizon, and the low power of the spark transmitters then in use limited their practical range to a few miles. The subsequent development of radio communication after 1896 employed lower frequencies, which could travel beyond the horizon as ground waves and by reflecting off the ionosphere as skywaves, and microwave frequencies were not further explored at this time.
First microwave communication experiments
[edit]Practical use of microwave frequencies did not occur until the 1940s and 1950s due to a lack of adequate sources, since the triode vacuum tube (valve) electronic oscillator used in radio transmitters could not produce frequencies above a few hundred megahertz due to excessive electron transit time and interelectrode capacitance.[29] By the 1930s, the first low-power microwave vacuum tubes had been developed using new principles; the Barkhausen–Kurz tube and the split-anode magnetron.[27]: 849-850 [36][29] These could generate a few watts of power at frequencies up to a few gigahertz and were used in the first experiments in communication with microwaves.
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Antennas of 1931 experimental 1.7 GHz microwave relay link across the English Channel
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Experimental 3.3 GHz (9 cm) transmitter 1933 using split-anode magnetron, at Westinghouse labs [37]
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Southworth (at left) demonstrating waveguide at IRE meeting in 1938, showing 1.5 GHz microwaves passing through the 7.5 m flexible metal hose registering on a diode detector
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The first modern horn antenna in 1938 with inventor Wilmer L. Barrow
In 1931 an Anglo-French consortium headed by Andre C. Clavier demonstrated the first experimental microwave relay link, across the English Channel 40 miles (64 km) between Dover, UK and Calais, France.[38][39] The system transmitted telephony, telegraph and facsimile data over bidirectional 1.7 GHz beams with a power of one-half watt, produced by miniature Barkhausen–Kurz tubes at the focus of 10-foot (3 m) metal dishes.
A word was needed to distinguish these new shorter wavelengths, which had previously been lumped into the "short wave" band, which meant all waves shorter than 200 meters. The terms quasi-optical waves and ultrashort waves were used briefly[36][40][37] but did not catch on. The first usage of the word micro-wave occurred in 1931[39][41] in reporting of the Clavier Anglo-French microwave link.[27]: 849
Radar development
[edit]The development of radar, mainly in secrecy, before and during World War II, resulted in the technological advances which made microwaves practical.[27]: 851 [29] Microwave wavelengths in the centimeter range were required to give the small radar antennas which were compact enough to fit on aircraft a narrow enough beamwidth to localize enemy aircraft. It was found that conventional transmission lines used to carry radio waves had excessive power losses at microwave frequencies, and George Southworth at Bell Labs and Wilmer Barrow at MIT independently invented waveguide in 1936.[32] Barrow invented the horn antenna in 1938 as a means to efficiently radiate microwaves into or out of a waveguide. In a microwave receiver, a nonlinear component was needed that would act as a detector and mixer at these frequencies, as vacuum tubes had too much capacitance. To fill this need researchers resurrected an obsolete technology, the point contact crystal detector (cat whisker detector) which was used as a demodulator in crystal radios around the turn of the century before vacuum tube receivers.[29][42] The low capacitance of semiconductor junctions allowed them to function at microwave frequencies. The first modern silicon and germanium diodes were developed as microwave detectors in the 1930s, and the principles of semiconductor physics learned during their development led to semiconductor electronics after the war.[29]
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Randall and Boot's prototype cavity magnetron tube at the University of Birmingham, 1940. In use the tube was installed between the poles of an electromagnet
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First commercial klystron tube, by General Electric, 1940, sectioned to show internal construction
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British Mk. VIII, the first microwave air intercept radar, in nose of British fighter
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Mobile US Army microwave relay station 1945 demonstrating relay systems using frequencies from 100 MHz to 4.9 GHz which could transmit up to 8 phone calls on a beam
The first powerful sources of microwaves were invented at the beginning of World War II: the klystron tube by Russell and Sigurd Varian at Stanford University in 1937,[27]: 852-853 and the cavity magnetron tube by John Randall and Harry Boot at Birmingham University, UK in 1940.[27]: 853-855 [29] Ten centimeter (3 GHz) microwave radar powered by the magnetron tube was in use on British warplanes in late 1941 and proved to be a game changer. Britain's 1940 decision to share its microwave technology with its US ally (the Tizard Mission)[27]: 852 significantly shortened the war. The MIT Radiation Laboratory established secretly at Massachusetts Institute of Technology in 1940 to research radar, produced much of the theoretical knowledge necessary to use microwaves.[27]: 852 Microwave relay systems were developed by the Allied military in the war and used for secure battlefield communication networks in the European theater. The first was the British Wireless Set No. 10, a 5 GHz, 8 telephone line, time division multiplex system developed by the UK's Signals Research and Development Establishment in 1942.[27]: 855
Post World War II exploitation
[edit]After World War II, microwaves were rapidly exploited commercially.[29] Due to their high frequency they had a very large information-carrying capacity (bandwidth); a single microwave beam could carry tens of thousands of phone calls. In the 1950s and 60s transcontinental microwave relay networks were built in the US and Europe to exchange telephone calls between cities and distribute television programs. In the new television broadcasting industry, from the 1940s microwave dishes were used to transmit backhaul video feeds from mobile production trucks back to the studio, allowing the first remote TV broadcasts. The first communications satellites were launched in the 1960s, which relayed telephone calls and television between widely separated points on Earth using microwave beams. In 1964, Arno Penzias and Robert Woodrow Wilson while investigating noise in a satellite horn antenna at Bell Labs, Holmdel, New Jersey discovered cosmic microwave background radiation.
Microwave radar became the central technology used in air traffic control, maritime navigation, anti-aircraft defense, ballistic missile detection, and later many other uses. Radar and satellite communication motivated the development of modern microwave antennas; the parabolic antenna (the most common type), cassegrain antenna, lens antenna, slot antenna, and phased array.
The ability of short waves to quickly heat materials and cook food had been investigated in the 1930s by Ilia E. Mouromtseff at Westinghouse, and at the 1933 Chicago World's Fair demonstrated cooking meals with a 60 MHz radio transmitter.[43] In 1945 Percy Spencer, an engineer working on radar at Raytheon, noticed that microwave radiation from a magnetron oscillator melted a candy bar in his pocket. He investigated cooking with microwaves and invented the microwave oven, consisting of a magnetron feeding microwaves into a closed metal cavity containing food, which was patented by Raytheon on 8 October 1945. Due to their expense microwave ovens were initially used in institutional kitchens, but by 1986 roughly 25% of households in the U.S. owned one. Microwave heating became widely used as an industrial process in industries such as plastics fabrication, and as a medical therapy to kill cancer cells in microwave hyperthermy.
The traveling wave tube (TWT) developed in 1943 by Rudolph Kompfner and John Pierce provided a high-power tunable source of microwaves up to 50 GHz and became the most widely used microwave tube (besides the ubiquitous magnetron used in microwave ovens). The gyrotron tube family developed in Russia could produce megawatts of power up into millimeter wave frequencies and is used in industrial heating and plasma research, and to power particle accelerators and nuclear fusion reactors.
Solid state microwave devices
[edit]The development of semiconductor electronics in the 1950s led to the first solid state microwave devices which worked by a new principle; negative resistance (some of the prewar microwave tubes had also used negative resistance).[29] The feedback oscillator and two-port amplifiers which were used at lower frequencies became unstable at microwave frequencies, and negative resistance oscillators and amplifiers based on one-port devices like diodes worked better.
The tunnel diode invented in 1957 by Japanese physicist Leo Esaki could produce a few milliwatts of microwave power. Its invention set off a search for better negative resistance semiconductor devices for use as microwave oscillators, resulting in the invention of the IMPATT diode in 1956 by W.T. Read and Ralph L. Johnston and the Gunn diode in 1962 by J. B. Gunn.[29] Diodes are the most widely used microwave sources today.
Two low-noise solid state negative resistance microwave amplifiers were developed; the maser invented in 1953 by Charles H. Townes, James P. Gordon, and H. J. Zeiger, and the varactor parametric amplifier developed in 1956 by Marion Hines.[29] The parametric amplifier and the ruby maser, invented in 1958 by a team at Bell Labs headed by H.E.D. Scovil were used for low noise microwave receivers in radio telescopes and satellite ground stations. The maser led to the development of atomic clocks, which keep time using a precise microwave frequency emitted by atoms undergoing an electron transition between two energy levels. Negative resistance amplifier circuits required the invention of new nonreciprocal waveguide components, such as circulators, isolators, and directional couplers. In 1969 Kaneyuki Kurokawa derived mathematical conditions for stability in negative resistance circuits which formed the basis of microwave oscillator design.[44]
Microwave integrated circuits
[edit]Prior to the 1980s microwave devices and circuits were bulky and expensive, so microwave frequencies were generally limited to the output stage of transmitters and the RF front end of receivers, and signals were heterodyned to a lower intermediate frequency for processing. The period from the 1970s to the present has seen the development of tiny inexpensive active solid-state microwave components which can be mounted on circuit boards, allowing circuits to perform significant signal processing at microwave frequencies. This has made possible satellite television, cable television, GPS devices, and modern wireless devices, such as smartphones, Wi-Fi, and Bluetooth which connect to networks using microwaves.
Microstrip, a type of transmission line usable at microwave frequencies, was invented with printed circuits in the 1950s.[29] The ability to cheaply fabricate a wide range of shapes on printed circuit boards allowed microstrip versions of capacitors, inductors, resonant stubs, splitters, directional couplers, diplexers, filters and antennas to be made, thus allowing compact microwave circuits to be constructed.[29]
Transistors that operated at microwave frequencies were developed in the 1970s. The semiconductor gallium arsenide (GaAs) has a much higher electron mobility than silicon,[29] so devices fabricated with this material can operate at 4 times the frequency of similar devices of silicon. Beginning in the 1970s GaAs was used to make the first microwave transistors,[29] and it has dominated microwave semiconductors ever since. MESFETs (metal-semiconductor field-effect transistors), fast GaAs field effect transistors using Schottky junctions for the gate, were developed starting in 1968 and have reached cutoff frequencies of 100 GHz, and are now the most widely used active microwave devices.[29] Another family of transistors with a higher frequency limit is the HEMT (high electron mobility transistor), a field effect transistor made with two different semiconductors, AlGaAs and GaAs, using heterojunction technology, and the similar HBT (heterojunction bipolar transistor).[29]
GaAs can be made semi-insulating, allowing it to be used as a substrate on which circuits containing passive components, as well as transistors, can be fabricated by lithography.[29] By 1976 this led to the first integrated circuits (ICs) which functioned at microwave frequencies, called monolithic microwave integrated circuits (MMIC).[29] The word "monolithic" was added to distinguish these from microstrip PCB circuits, which were called "microwave integrated circuits" (MIC). Since then, silicon MMICs have also been developed. Today MMICs have become the workhorses of both analog and digital high-frequency electronics, enabling the production of single-chip microwave receivers, broadband amplifiers, modems, and microprocessors.
See also
[edit]- Block upconverter (BUC)
- Cosmic microwave background
- Electron cyclotron resonance
- International Microwave Power Institute
- Low-noise block converter (LNB)
- Maser
- Microwave auditory effect
- Microwave cavity
- Microwave chemistry
- Microwave radio relay
- Microwave transmission
- Rain fade
- RF switch matrix
- The Thing (listening device)
References
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External links
[edit]- EM Talk, Microwave Engineering Tutorials and Tools
- Millimeter Wave Archived 2013-06-09 at the Wayback Machine and Microwave Waveguide dimension chart.
Microwave
View on GrokipediaFundamentals
Definition and Characteristics
Microwaves are a form of electromagnetic radiation characterized by wavelengths ranging from 1 millimeter to 1 meter, corresponding to frequencies between 300 megahertz (MHz) and 300 gigahertz (GHz).[1][8] This range places microwaves as non-ionizing radiation, consisting of oscillating electric and magnetic fields that propagate through space perpendicular to each other and to the direction of wave travel.[9] As transverse electromagnetic (TEM) waves, microwaves exhibit key properties including polarization, which describes the orientation of the electric field vector and can be linear, circular, or elliptical depending on the wave's generation and propagation medium.[10] The phase velocity of microwaves in vacuum equals the speed of light, approximately m/s, representing the speed at which a point of constant phase travels.[11] Energy transport in microwave fields is quantified by the Poynting vector, , whose magnitude indicates the power flux density in watts per square meter and direction aligns with wave propagation.[12] Microwaves constitute a subset of radio waves, specifically at the higher-frequency end of the radio spectrum, but they are distinguished by behaviors such as increased directive properties and interaction with matter at shorter wavelengths, enabling applications like radar and communication.[4] The fundamental relationship between wavelength and frequency for microwaves (as for all electromagnetic waves) is given by , where is the speed of light in vacuum.[13]Position in Electromagnetic Spectrum
Microwaves are situated in the electromagnetic spectrum between infrared radiation and radio waves, occupying wavelengths from approximately 1 millimeter to 1 meter, which correspond to frequencies ranging from 300 MHz to 300 GHz./23:_Electromagnetic_Waves/23.1:_The_Electromagnetic_Spectrum) This positioning distinguishes microwaves from the shorter wavelengths of infrared (typically less than 1 mm) and the longer wavelengths of radio waves (greater than 1 m).[14] There is notable overlap at the boundaries of the microwave band. At the lower frequency end, microwaves extend into the ultra-high frequency (UHF) portion of the radio spectrum, which covers 300 MHz to 3 GHz (wavelengths of 1 m to 10 cm)./23:_Electromagnetic_Waves/23.1:_The_Electromagnetic_Spectrum) Similarly, the upper frequency range of microwaves overlaps with millimeter waves, defined as electromagnetic waves with wavelengths from 1 mm to 10 mm (frequencies of 30 GHz to 300 GHz).[15] In visual representations of the electromagnetic spectrum, such as standard diagrams, microwaves appear as a distinct band nestled between the broad radio wave region on the low-frequency side and the infrared region on the high-frequency side, highlighting their intermediate wavelength scale relative to visible light and longer radio transmissions.[16] The term "microwave" emerged in the early 1930s to describe these short-wavelength radio waves, with "micro-" emphasizing their relatively small size compared to the meter-scale wavelengths of conventional radio technology at the time; it was first documented in a 1931 paper by A. G. Clavier and appeared in print in an international journal in 1932.[17][18]Frequency Bands and Designations
Microwave frequencies are subdivided into standardized bands to facilitate technical communication, equipment design, and regulatory allocation, primarily through designations established by the International Telecommunication Union (ITU) and the Institute of Electrical and Electronics Engineers (IEEE). These letter-based bands, ranging from L to mm or D, cover the microwave spectrum from approximately 1 GHz to 300 GHz, with each band defined by specific frequency ranges that correspond to practical wavelength intervals.[19][20] The origins of these band names trace back to World War II, when Allied forces, particularly in radar development, adopted informal letter designations to classify microwave frequencies for secrecy and rapid communication among engineers; for instance, the X band was prominently used in fire-control radars. Post-war, these designations were formalized to resolve inconsistencies arising from their ad hoc military application, leading to the IEEE Standard 521 first issued in 1976 (revised in 2002) for radar-frequency bands, while the ITU's Recommendation ITU-R V.431 provides complementary nomenclature for radiocommunication services. The IEEE standard relates common letter terms to precise frequency ranges, emphasizing their use in radar while acknowledging broader microwave applications.[21][22][19] Despite standardization, some overlaps and ambiguities persist, particularly in the 26–40 GHz region where the K band (18–27 GHz) and Ka band (27–40 GHz) may adjoin without clear delineation in certain contexts, and the ITU notes that K and Ka are sometimes merged as "Ka" in space radiocommunications. Additionally, higher bands like V and W show variations between IEEE and ITU definitions, with non-standardized extensions occasionally applied. The mm or D band, encompassing 110–300 GHz, further illustrates this, as "D" is sometimes narrowly defined as 110–170 GHz in legacy radar contexts, while "mm" broadly covers millimeter waves up to 300 GHz.[19][20][23] The following table summarizes the primary IEEE and ITU microwave band designations, including frequency ranges, corresponding wavelengths, and brief notes on typical uses across radar, communications, and sensing applications:| Band | Frequency Range (GHz) | Wavelength Range | Common Uses |
|---|---|---|---|
| L | 1–2 | 30–15 cm | Long-range radar and mobile communications |
| S | 2–4 | 15–7.5 cm | Weather radar and air traffic control |
| C | 4–8 | 7.5–3.75 cm | Satellite communications and maritime radar |
| X | 8–12 | 3.75–2.5 cm | Military surveillance and missile guidance |
| Ku | 12–18 | 2.5–1.67 cm | Direct broadcast satellite and VSAT systems |
| K | 18–27 | 1.67–1.11 cm | Automotive radar and short-range wireless |
| Ka | 27–40 | 1.11–0.75 cm | High-resolution imaging and 5G backhaul |
| V | 40–75 | 7.5–4 mm | Experimental radar and millimeter-wave links |
| W | 75–110 | 4–2.7 mm | High-frequency sensing and security scanners |
| mm/D | 110–300 | 2.7–1 mm | Terahertz imaging and advanced research |
Propagation and Interaction
Propagation Mechanisms
Microwaves propagate through free space following the principles of electromagnetic wave theory, where the power density decreases according to the inverse square law due to the spreading of wavefronts from a point source. In ideal conditions without obstacles or atmospheric interference, the received power $ P_r $ between a transmitter and receiver is described by the Friis transmission equation:Absorption and Effects on Materials
Microwaves are absorbed by materials through dielectric heating, a process dominated by two mechanisms: dipolar polarization and ionic conduction. In dipolar polarization, the oscillating electric field of the microwave aligns the permanent dipole moments of polar molecules, such as water, causing rotational excitation and molecular friction that dissipates energy as heat. This effect is particularly pronounced in materials containing polar components, where the torque on the dipole moment is given by , leading to energy loss proportional to the dielectric loss factor . Ionic conduction contributes additionally by accelerating charged particles, resulting in collisions and Joule heating. These mechanisms are detailed in foundational analyses of microwave-material interactions.[27][28] The depth to which microwaves penetrate a material, known as the penetration depth , varies significantly depending on the material's properties and governs the extent of absorption. For conductive materials, penetration is limited by the skin effect, with , where is frequency, is magnetic permeability, and is electrical conductivity; this results in shallow penetration (e.g., 1–3 m in metals at 2.45 GHz), causing most energy to reflect at the surface. In dielectrics, penetration depth is deeper and given approximately by , where is the speed of light, is the real relative permittivity, and is the loss tangent; here, absorption occurs volumetrically until the power density drops to of its surface value. These formulations highlight how material conductivity and permittivity dictate energy transfer efficiency.[27][28] Materials are classified based on their microwave interaction: low-loss dielectrics (e.g., quartz or dry ceramics) exhibit minimal absorption and allow deep penetration with ; absorbers, such as carbon-loaded polyurethane foams, are engineered for high loss () to dissipate energy across broadband frequencies, often used in shielding applications; and reflectors, typically metals like copper or aluminum, have high conductivity ( S/m) leading to near-total reflection due to negligible penetration. Frequency dependence further modulates these behaviors: in dielectrics, absorption often increases with frequency up to relaxation peaks (e.g., around 2–10 GHz for water), enhancing heating efficiency, while in conductors, higher frequencies reduce , amplifying surface reflection and minimizing internal absorption.[27][29][28] Beyond thermal effects, microwaves can induce non-thermal phenomena such as dielectric breakdown, where intense electric fields exceed the material's intrinsic strength, triggering ionization, plasma formation, or arcing. Breakdown thresholds vary by material and conditions, typically ranging from 10–30 MV/m in solid dielectrics under microwave exposure, lower than DC values due to rapid field oscillations that promote electron avalanche. This can occur at metal-dielectric interfaces, leading to localized discharges with energy conversion efficiencies of 20–60%, distinct from uniform heating. Such effects are critical for high-power applications to avoid hotspots or system failure.[27][30]Components and Technology
Antennas and Waveguides
Antennas and waveguides form the backbone of microwave systems, enabling the efficient launch, guidance, and reception of electromagnetic waves in the 300 MHz to 300 GHz frequency range. These structures are optimized for low loss and high directivity, addressing the challenges of wavelength-scale dimensions that make traditional wires impractical at microwave frequencies. Antennas radiate or capture waves into free space, while waveguides confine them along defined paths, often integrating seamlessly to support applications from telecommunications to radar. Parabolic dish antennas, characterized by a curved reflector that directs microwaves to a focal point feed, achieve high gain through large apertures and are staples in long-haul microwave communication links operating in the 4-40 GHz bands. Their design leverages the reflective properties of the dish surface to collimate beams, providing narrow patterns essential for line-of-sight propagation over distances exceeding 50 km. Horn antennas, evolving from waveguide apertures with exponentially or linearly flaring sections, serve as versatile radiators or feeds, offering broadband performance and controlled radiation patterns in microwave test fixtures and satellite systems. Phased array antennas consist of numerous elements—such as patches or slots—whose phases are adjusted electronically to steer beams dynamically, facilitating rapid scanning in radar and multi-user 5G environments without moving parts. The gain $ G $ of such aperture-limited antennas is fundamentally expressed asMicrowave Sources
Microwave sources are specialized devices designed to generate or amplify electromagnetic signals in the microwave frequency range, typically from 300 MHz to 300 GHz. These sources play a crucial role in applications requiring high-frequency signal production, including radar systems, communication links, and scientific instrumentation. They can be broadly categorized into vacuum tube-based devices, which excel in high-power output; solid-state devices, which offer compactness and reliability; and quantum-based sources, which provide exceptional low-noise performance. The choice of source depends on factors such as required power, frequency bandwidth, efficiency, and noise characteristics. Vacuum tube sources represent classical high-power microwave generators, leveraging electron beam interactions within evacuated envelopes. Klystrons operate on the principle of velocity modulation, where an input signal modulates the velocity of electrons in a beam as they pass through resonant cavities, leading to bunching and subsequent energy extraction in output cavities for amplification. Multicavity klystrons can achieve gains exceeding 100 dB, making them suitable for high-power amplification in particle accelerators and radar transmitters. Magnetrons, in contrast, generate microwaves through cavity resonance, where electrons emitted from a central cathode interact with a perpendicular magnetic field and a series of resonant cavities in the anode block, converting electron kinetic energy into microwave oscillations at frequencies determined by cavity dimensions. These devices are renowned for their use in microwave ovens, producing continuous-wave outputs around 2.45 GHz. Traveling-wave tubes (TWTs) provide broadband amplification by propagating an RF signal along a slow-wave structure in synchronism with a helical electron beam, enabling wide frequency coverage—often octave or multi-octave bandwidths—essential for electronic warfare and satellite communications. Solid-state microwave sources utilize semiconductor materials to produce oscillations or amplification without vacuum tubes, offering advantages in size, cost, and integration. Gunn diodes exploit negative differential resistance arising from intervalley electron transfer in materials like gallium arsenide, enabling self-oscillation at microwave frequencies when biased in the negative resistance region; they typically serve as low-power oscillators in the 1-100 GHz range for local oscillators in receivers. IMPATT (impact ionization avalanche transit-time) diodes generate microwaves through impact ionization in a reverse-biased p-n junction, where avalanche multiplication of carriers creates a current pulse that transits the depletion region, producing negative resistance and high-power output at frequencies up to 100 GHz or more; they are valued for their efficiency in CW or pulsed radar applications. Quantum sources, such as masers (microwave amplification by stimulated emission of radiation), achieve ultra-low noise by using population inversion in atomic or molecular systems to amplify microwaves coherently, often approaching the quantum limit of added noise. Early masers employed gaseous or solid-state media like ammonia or ruby, but modern solid-state masers using nitrogen-vacancy centers in diamond operate at room temperature with minimal noise addition, suitable for sensitive applications like radio astronomy and quantum sensing. Power output from microwave sources varies widely: solid-state oscillators like Gunn diodes typically deliver milliwatts (mW) to watts (W), while amplifiers such as IMPATT diodes reach tens of watts; vacuum tube devices scale to kilowatts (kW), with TWTs providing 10 W to 1 kW broadband and klystrons or magnetrons exceeding 100 kW in pulsed modes. Efficiency and noise performance are key figures of merit for microwave sources. Vacuum tubes generally offer higher efficiencies—magnetrons up to 80%, klystrons 40-70%, and TWTs 10-30%—compared to solid-state devices, where Gunn diodes achieve 1-5% and IMPATT diodes 15-25%, though masers prioritize noise over efficiency, often operating below 1% but with quantum-limited performance. Noise is quantified by the noise figure (NF), defined asCircuits and Devices
Microwave circuits and devices encompass a range of passive and active components designed to process signals at frequencies typically from 300 MHz to 300 GHz, enabling functions such as filtering, power division, isolation, amplification, and frequency conversion.[38] These components are critical for applications in radar, communications, and sensing systems, where high-frequency performance demands compact, low-loss designs.[39] Passive components form the backbone of microwave signal routing and conditioning. Filters, essential for selecting desired frequency bands while rejecting others, include cavity filters that utilize resonant metallic enclosures to achieve high quality factors (Q > 1000) and low insertion loss in narrowband applications around 1-10 GHz.[40] Microstrip filters, implemented on planar substrates like alumina or PTFE, offer compact integration for broadband responses, with designs such as coupled-line or hairpin structures providing fractional bandwidths up to 50% at 2-18 GHz.[39] Couplers enable power splitting and sampling; directional couplers, which preferentially couple forward-propagating waves, are realized using coupled microstrip lines or waveguides, achieving 3 dB coupling (equal power split) over octave bandwidths with isolation better than 20 dB.[41] Circulators, ferrite-based non-reciprocal devices, use magnetized ferrite materials to route signals unidirectionally in three or four ports, providing isolation >20 dB at X-band (8-12 GHz) for duplexing in transmitters and receivers.[42] These ferrite circulators rely on the gyromagnetic properties of materials like yttrium iron garnet under an external magnetic field to break reciprocity.[43] Active devices introduce gain and nonlinear processing to microwave circuits. Transistors such as gallium arsenide (GaAs) field-effect transistors (FETs) serve as amplifiers and switches, with metal-semiconductor FETs (MESFETs) offering cutoff frequencies up to 100 GHz and power densities of 1-2 W/mm at 10 GHz.[44] High electron mobility transistors (HEMTs), featuring heterojunctions like AlGaAs/InGaAs on GaAs substrates, excel in millimeter-wave regimes (30-300 GHz), delivering noise figures as low as 1 dB and gains >10 dB at 60 GHz due to enhanced electron mobility (>8000 cm²/V·s).[45] Mixers perform frequency conversion by multiplying signals; diode-based mixers, using Schottky barrier diodes, enable downconversion with conversion losses of 6-10 dB at 10-60 GHz, leveraging the diode's nonlinear I-V characteristics for harmonic generation and image rejection.[46] Single-balanced and double-balanced configurations improve port-to-port isolation (>30 dB) and suppress LO leakage.[47] Monolithic microwave integrated circuits (MMICs) integrate multiple passive and active elements on a single chip, reducing size and parasitics for high-frequency operation. Fabricated on GaAs substrates using processes like ion implantation or epitaxial growth, MMICs support amplifiers, mixers, and phase shifters with operating frequencies up to 100 GHz and integration densities exceeding 100 components per mm².[48] Silicon-germanium (SiGe) substrates enable cost-effective MMICs for broadband applications, with heterojunction bipolar transistors (HBTs) in SiGe achieving cutoff frequencies >200 GHz and suitable for phased-array radar up to 20 GHz.[49] These substrates leverage silicon-compatible fabrication for yields >90% in production.[50] At microwave frequencies, losses and parasitics significantly impact performance; the skin effect confines current to a thin layer (depth δ ≈ 1/√(π f μ σ), where f is frequency, μ permeability, and σ conductivity) on conductors, increasing effective resistance by factors of 5-10 at 10 GHz compared to DC, leading to insertion losses of 0.1-1 dB/cm in microstrip lines.[51] This effect exacerbates ohmic losses in inductors and vias, necessitating wider traces or superconducting alternatives in high-Q designs.[52] Emerging hybrid approaches incorporate photonic integrated circuits (PICs) for microwave-optics interfacing, where silicon or indium phosphide platforms generate and process microwave signals via optical modulation, achieving phase noise <-100 dBc/Hz at 10 kHz offset for signals up to 40 GHz.[53] These PICs enable low-loss beamforming in arrays, with electro-optic modulators converting RF to optical domains for distribution over fiber.Analysis and Design
Modeling Techniques
Modeling techniques for microwave systems rely on solving Maxwell's equations to predict electromagnetic field behavior, wave propagation, and device performance. Analytical methods offer closed-form solutions for idealized structures, while numerical approaches address complex geometries and materials. These techniques enable the design and optimization of components such as antennas, waveguides, and circuits by simulating scattering, radiation, and transmission characteristics without physical prototyping.[54] Analytical methods begin with the frequency-domain formulation of Maxwell's equations, which describe time-harmonic fields in linear media:Measurement Methods
Microwave measurement methods encompass a range of experimental techniques designed to quantify signal characteristics, system performance, and electromagnetic interactions with high precision, often serving to validate computational modeling predictions from prior analysis stages. Frequency measurement in the microwave regime typically employs heterodyne techniques, where the unknown signal is mixed with a reference oscillator to generate a lower intermediate frequency amenable to direct counting or analysis.[62] This approach enables accurate determination of microwave frequencies by leveraging stable, traceable references down-converted from gigahertz ranges. Frequency counters, enhanced with microwave samplers or prescalers, extend direct measurements up to approximately 100 GHz, providing resolution on the order of 10^{-9} or better for timebase stability.[63] For enhanced precision, especially in calibration standards, cavity resonators are utilized; these devices operate by exciting electromagnetic modes within a high-Q resonant structure, where the resonant frequency shift due to perturbations yields absolute frequency values with uncertainties below 10^{-7}.[64] Power measurement relies on thermal and electronic detectors to capture incident energy across wide dynamic ranges. Bolometers, which detect power through resistive changes induced by absorbed heat, offer broadband response from DC to beyond 100 GHz with dynamic ranges exceeding 50 dB, though they exhibit slower response times on the order of milliseconds.[65] Calorimeters provide absolute power calibration by measuring total heat dissipation in an absorbing load, achieving accuracies of 0.5% or better up to 18 GHz, ideal for traceability in standards labs.[66] Diode detectors, operating in the square-law region for low powers, enable fast, video-bandwidth measurements but require careful consideration of dynamic range limitations—typically 20-40 dB—due to nonlinearity at higher inputs, often mitigated by attenuators or logarithmic amplifiers.[67] Network analysis employs vector network analyzers (VNAs) to characterize scattering parameters (S-parameters), which describe signal reflection and transmission in microwave circuits and devices. VNAs generate swept-frequency stimuli, measure amplitude and phase responses via coherent detection, and compute S-parameters such as return loss (S_{11}) and insertion loss (S_{21}) with trace noise floors below -80 dBm and phase stability under 0.1 degrees up to 67 GHz.[68] Accurate results demand calibration, commonly using the Short-Open-Load-Thru (SOLT) method, which applies known standards to de-embed systematic errors like directivity (typically <0.1 dB) and source match (>40 dB), ensuring measurement uncertainties below 0.05 dB in magnitude and 1 degree in phase for well-matched systems.[69] Field probing techniques, particularly near-field scanning, facilitate detailed mapping of antenna radiation patterns by positioning a small probe over a planar, cylindrical, or spherical surface close to the device under test. These scanners sample electric or magnetic field components at sub-wavelength spacings—often λ/10—to capture evanescent waves, followed by Fourier transform algorithms to extrapolate far-field patterns with angular resolutions better than 0.5 degrees and gain accuracies within 0.5 dB.[70] Standardized practices, such as those outlined in IEEE recommendations, guide probe positioning and data processing to minimize truncation errors in large apertures.[71] Recent advancements extend these methods into the terahertz regime for 6G testing, with VNAs incorporating frequency extenders to reach up to 1 THz, enabling S-parameter characterization of sub-THz components with bandwidths exceeding 100 GHz and supporting data rates beyond 200 Gbps in validation campaigns.[72][73]Applications
Telecommunications and Communication
Microwaves serve as a critical backbone for telecommunications through point-to-point (P2P) links, which provide high-capacity, line-of-sight connections between network nodes over distances up to 100 kilometers. These links operate in licensed frequency bands from 4 to 42 GHz and unlicensed bands including 2.4 GHz, 5 GHz, 17 GHz, 24 GHz, and 60 GHz, enabling transparent Ethernet extensions for telecom carriers, utilities, and corporate networks. Capacities reach up to 6 Gbps using advanced techniques like adaptive coding and modulation (ACM), which dynamically adjust to channel conditions for optimal performance.[74][75] To maximize spectral efficiency in these links, quadrature amplitude modulation (QAM) schemes encode data by varying both amplitude and phase of the carrier signal. Higher-order QAM, such as 256-QAM, 1024-QAM, and 2048-QAM, allows more bits per symbol, increasing throughput—for instance, 2048-QAM provides approximately 10% more capacity than 1024-QAM—while requiring higher carrier-to-interference (C/I) ratios and reducing system gain. The theoretical upper limit on channel capacity is given by Shannon's formula:Radar, Navigation, and Sensing
Microwave radars function by emitting electromagnetic waves in the frequency range of 300 MHz to 300 GHz and processing the backscattered signals to determine target location, velocity, and other attributes. A core principle is Pulse-Doppler radar, which transmits short microwave pulses and analyzes the time delay for range and the frequency shift for velocity, enabling detection of moving objects amid clutter. Another key method is Frequency-Modulated Continuous Wave (FMCW) radar, which sweeps the transmitted frequency linearly over time and measures the beat frequency between the transmitted and received signals to derive both range and Doppler information simultaneously, offering advantages in power efficiency and resolution for short-range applications. The range resolution in such systems is fundamentally limited by the signal bandwidth , expressed as , where is the speed of light, allowing finer discrimination between closely spaced targets with wider bandwidths.[82] Weather radars predominantly use S-band (2–4 GHz) for long-range detection of severe storms due to its lower attenuation by rain, or C-band (4–8 GHz) for higher resolution in moderate precipitation, mapping echo intensities to infer rainfall rates and wind patterns. Synthetic Aperture Radar (SAR), operating in microwave bands such as L- or X-band, exploits the relative motion between the radar platform and target to simulate a large antenna aperture, producing two-dimensional images with meter-scale resolution for terrain mapping and surveillance, even through clouds or at night.[83] In navigation, microwave radar altimeters transmit pulses toward the ground to measure round-trip time for precise height determination, typically in the 4.2–4.4 GHz C-band, providing a GPS-independent backup for low-altitude flight and terrain-following in GPS-denied scenarios.[84] These altimeters are frequently coupled with inertial navigation systems, which use gyroscopes and accelerometers aided by periodic microwave updates to maintain accurate positioning over extended periods without external signals.[85] Microwave proximity sensors operate on the Doppler principle, emitting continuous waves and detecting frequency shifts from reflected signals off nearby objects, enabling non-contact detection up to several meters for applications like automatic doors and intrusion alarms.[86] In automotive sensing, 77 GHz millimeter-wave radars, compliant with automotive standards, support Advanced Driver Assistance Systems (ADAS) by providing real-time range, velocity, and angle data for features such as blind-spot monitoring and emergency braking, with typical resolutions below 0.5 meters. Prototypes of quantum radars, utilizing entangled microwave photons generated via parametric down-conversion, aim to enhance stealth detection by correlating signal and idler beams to distinguish low-reflectivity targets from noise, potentially outperforming classical systems in adverse conditions, though practical ranges remain limited to under a kilometer.[87]Astronomy and Scientific Research
Microwaves play a crucial role in radio astronomy, enabling the detection of faint signals from distant cosmic phenomena through large parabolic dishes and arrays that focus electromagnetic waves in the frequency range of 300 MHz to 300 GHz. One of the most significant discoveries facilitated by microwave observations is the cosmic microwave background (CMB), the remnant radiation from the Big Bang, measured at a temperature of approximately 2.725 K. This uniform microwave glow across the sky was serendipitously detected in 1965 by Arno Penzias and Robert Wilson using a sensitive horn antenna operating at 4.08 GHz, providing key evidence for the hot, dense early universe. Subsequent microwave telescopes have mapped the CMB in exquisite detail, revealing tiny temperature fluctuations that seed the large-scale structure of the universe. Legacy instruments like the 305-meter Arecibo Observatory, operational from 1963 to 2020, contributed to microwave astronomy by observing radio emissions from pulsars and galaxies in the 1-10 GHz range, though its primary focus was lower frequencies. Modern facilities such as the Atacama Large Millimeter/submillimeter Array (ALMA) extend microwave capabilities into the millimeter-wave regime (up to 950 GHz), allowing astronomers to image protoplanetary disks and star-forming regions with unprecedented resolution. In astrophysical spectroscopy, microwaves are essential for studying the rotational transitions of interstellar molecules, which emit or absorb at specific frequencies to reveal the composition and dynamics of molecular clouds. For instance, the carbon monoxide (CO) molecule's J=1–0 rotational transition at 115.271 GHz serves as a primary tracer for molecular hydrogen in the interstellar medium, enabling mappings of galactic structure and star formation rates. Observations of such lines using microwave receivers on telescopes like the James Clerk Maxwell Telescope have identified over 200 molecular species in space, from simple diatomic gases to complex organics. Microwave technology also underpins pulsar timing arrays, where networks of radio telescopes monitor millisecond pulsars—rapidly rotating neutron stars emitting periodic microwave pulses—to detect low-frequency gravitational waves. Precision microwave receivers, often cooled to cryogenic temperatures for low noise, achieve timing accuracies of tens of nanoseconds, as demonstrated by the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) using facilities like the Green Bank Telescope at 1.4 GHz. These arrays have set limits on the gravitational wave background from supermassive black hole binaries. A landmark application of millimeter-wave microwaves is the Event Horizon Telescope (EHT), a global very-long-baseline interferometry array that captured the first images of black hole shadows in 2019 and beyond. Operating primarily at 230 GHz (1.3 mm wavelength), the EHT synthesized a telescope the size of Earth to resolve the supermassive black holes in Messier 87 and Sagittarius A*, revealing event horizons glowing with hot plasma emissions. This breakthrough relied on advanced microwave correlators and atmospheric calibration techniques to overcome Earth's variable conditions.Industrial and Consumer Uses
Microwave ovens represent one of the most widespread consumer applications of microwave technology, utilizing a magnetron to generate electromagnetic waves at a frequency of 2.45 GHz, which are directed into a resonant metal cavity where they form standing waves to heat food through dielectric absorption primarily in water molecules.[88] These standing waves create a pattern of nodes and antinodes within the cavity, with a rotating turntable or mode stirrer employed to distribute the energy more uniformly and prevent uneven heating.[88] Typical household models operate at power outputs ranging from 600 to 1200 watts, enabling rapid cooking times while maintaining efficiency through the magnetron's approximately 80% conversion rate from electrical to microwave energy.[89] In industrial settings, microwaves are extensively used for drying and curing processes, offering advantages over traditional convection methods such as faster volumetric heating, higher energy efficiency, and reduced processing times due to direct molecular excitation rather than surface heat transfer.[90] For polymers, microwave curing accelerates chemical reactions in resins and enables precise shaping or welding of materials like plastics, minimizing defects and energy consumption compared to convective ovens by achieving uniform temperature distribution throughout the material volume.[90] In food processing, microwave drying removes moisture from products such as grains, fruits, and pasta more selectively and rapidly than convection, preserving nutritional quality and texture while lowering operational costs through smaller equipment footprints and improved throughput.[90] Microwave diathermy serves as a key medical application for therapeutic deep heating, employing frequencies of 915 MHz or 2.45 GHz to penetrate subcutaneous tissues, muscles, and joints, thereby alleviating pain, reducing inflammation, and improving mobility without significantly raising skin temperature.[91] In treatments for conditions like knee osteoarthritis, sessions of 30 minutes three times per week over four weeks have demonstrated sustained reductions in pain and stiffness, enhancements in muscle strength, and better physical function lasting up to 12 weeks, outperforming superficial heat therapies.[92] This modality is particularly effective for muscle therapy, as it promotes tissue relaxation and repair by converting microwave energy into controlled heat within deeper structures.[91] Microwaves also facilitate plasma generation for advanced material synthesis, where high-power microwave sources ionize gases to create thermal plasmas that melt or vaporize precursors into fine particles for applications like producing metal powders and battery cathodes.[93] This process, as in the UniMelt system, enables rapid synthesis of materials such as titanium or nickel alloys with reduced waste and energy use compared to conventional methods, supporting scalable production for industries like additive manufacturing.[93] In 3D printing aids, microwave-assisted processing heats continuous fiber-reinforced thermoplastic composites during extrusion, allowing for efficient layer bonding and complex structure formation without traditional binders, thus enhancing mechanical properties and print speed.[94]Emerging Technologies
Recent advancements in microwave technology are pushing the boundaries of frequency ranges and applications, particularly with the exploration of terahertz (THz) waves above 100 GHz for next-generation wireless communication systems like 6G. THz microwaves offer ultra-high bandwidth potential, enabling data rates exceeding 100 Gbps, which is essential for supporting emerging demands in holographic communications, extended reality, and massive IoT connectivity. Research roadmaps highlight that THz systems address challenges such as high path loss and atmospheric absorption through advanced beamforming and integrated photonics, with prototypes demonstrating reliable transmission over short distances in indoor environments.[95] These developments, building on post-2010 progress, position THz as a cornerstone for 6G networks expected to deploy by 2030, focusing on seamless integration with lower microwave bands for hybrid architectures.[96] Microwave imaging has emerged as a non-ionizing alternative to traditional X-ray methods, particularly for medical diagnostics like breast cancer detection, where it exploits dielectric contrasts in tissue to identify tumors without harmful radiation. Clinical studies using systems like the SAFE microwave breast imaging device have shown detection sensitivities comparable to mammography, with pilot trials reporting accurate visualization of breast tissue inhomogeneities in diverse patient cohorts.[97] Recent innovations incorporate machine learning for image reconstruction, achieving up to 100% tumor detection success in simulated datasets by processing scattering parameters from multi-antenna arrays operating at 1-10 GHz.[98] Beyond medicine, microwave imaging is advancing security screening through real-time systems that penetrate clothing to detect concealed threats, as demonstrated by technologies like HEXWAVE, which provide high-resolution imaging at checkpoints without physical contact.[99] However, these surveillance applications raise ethical concerns regarding privacy invasion and data security, as body scanners capture detailed images that could be misused without strict retention policies and consent protocols.[100][101] In quantum computing, microwave photons serve as carriers for information in circuit quantum electrodynamics (cQED) platforms, where superconducting qubits—typically transmon or fluxonium types operating at 5-10 GHz—are coupled to high-quality microwave resonators to enable coherent control and readout. This strong light-matter interaction allows for gate operations with fidelities exceeding 99%, forming the basis for scalable quantum processors as seen in systems from IBM and Google.[102] Post-2010 breakthroughs have extended coherence times to microseconds via improved circuit designs, mitigating decoherence from environmental noise and paving the way for error-corrected quantum algorithms.[103] Microwave integration in cQED also facilitates hybrid quantum systems, such as linking superconducting qubits to spin-based ones for fault-tolerant computing.[104] The fusion of artificial intelligence with microwave systems is enhancing adaptability in dynamic environments, particularly through AI-driven adaptive beamforming that optimizes signal directionality in real-time for 5G and beyond networks. Machine learning algorithms, such as deep neural networks, predict channel states to adjust beam patterns, improving spectral efficiency by up to 30% in multi-user scenarios with crowded spectrum.[105] In spectrum management, AI enables cognitive radio techniques for opportunistic access, using reinforcement learning to detect idle bands and mitigate interference, which is critical for dense urban deployments.[106] These integrations, accelerated since 2015, also support microwave imaging by automating anomaly detection, though they introduce challenges in algorithmic bias and explainability for reliable deployment.[98]Health and Safety
Biological Effects
Microwaves interact with biological tissues primarily through thermal effects, where absorbed energy leads to heating via molecular agitation, particularly in water-rich structures. The specific absorption rate (SAR), defined as the rate of energy absorption per unit mass, quantifies this process and is calculated using the formula:Exposure Standards and Regulations
Exposure standards for microwave radiation, which falls within the radiofrequency (RF) electromagnetic field (EMF) spectrum from approximately 300 MHz to 300 GHz, are established to protect against known adverse health effects such as tissue heating. The International Commission on Non-Ionizing Radiation Protection (ICNIRP) provides globally influential guidelines that set reference levels for power density to ensure compliance with underlying basic restrictions on absorbed energy. For the frequency range of 2–300 GHz, ICNIRP 2020 guidelines specify a power density limit of 10 W/m² for general public exposure (averaged over 30 minutes for whole-body or 6 minutes for local exposure over 4 cm²) and 50 W/m² for occupational exposure (averaged over 6 minutes for local exposure over 4 cm², with an additional 100 W/m² limit over 1 cm² above 30 GHz).[113][114] In the United States, the Federal Communications Commission (FCC) enforces similar RF exposure limits under its rules, harmonized with standards from the Institute of Electrical and Electronics Engineers (IEEE) and the National Council on Radiation Protection and Measurements (NCRP). For uncontrolled environments (general public), the limit is 10 W/m² (1 mW/cm²) averaged over 30 minutes above 1.5 GHz up to 100 GHz, with proposals to extend constant limits to 300 GHz; for controlled environments (occupational), it is 50 W/m² (5 mW/cm²) averaged over 6 minutes.[115][116] These limits apply to microwave sources, ensuring that exposure from devices and antennas remains below thresholds that could cause significant heating.| Exposure Type | Frequency Range | Power Density Limit (General Public) | Power Density Limit (Occupational) | Averaging Time | Source |
|---|---|---|---|---|---|
| ICNIRP | 2–300 GHz | 10 W/m² (local: over 4 cm²) | 50 W/m² (local: over 4 cm²) | 6–30 min | ICNIRP 2020 Guidelines[113] |
| FCC | 1.5–100 GHz (extendable to 300 GHz) | 10 W/m² (1 mW/cm²) | 50 W/m² (5 mW/cm²) | 6–30 min | FCC Rules (47 CFR §1.1310)[115] |

