The first prototype ammonia maser in front of its inventor Charles H. Townes. The ammonia nozzle is at left in the box, the four brass rods at center are the quadrupole state selector, and the resonant cavity is at right. The 24 GHz microwaves exit through the vertical waveguide Townes is adjusting. At bottom are the vacuum pumps.
A hydrogen radio frequency discharge, the first element inside a hydrogen maser (see description below)

A maser is a device that produces coherent electromagnetic waves (microwaves), through amplification by stimulated emission. The term is an acronym for microwave amplification by stimulated emission of radiation. First suggested by Joseph Weber, the first maser was built by Charles H. Townes, James P. Gordon, and Herbert J. Zeiger at Columbia University in 1953. Townes, Nikolay Basov and Alexander Prokhorov were awarded the 1964 Nobel Prize in Physics for theoretical work leading to the maser. Masers are used as the timekeeping device in atomic clocks, and as extremely low-noise microwave amplifiers in radio telescopes and deep-space spacecraft communication ground stations.

Modern masers can be designed to generate electromagnetic waves at microwave frequencies and radio and infrared frequencies. For this reason, Townes suggested replacing "microwave" with "molecular" as the first word in the acronym "maser".[1]

The laser works by the same principle as the maser, but produces higher frequency coherent radiation at visible wavelengths. The maser was the precursor to the laser, inspiring theoretical work by Townes and Arthur Leonard Schawlow that led to the invention of the laser in 1960 by Theodore Maiman. When the coherent optical oscillator was first imagined in 1957, it was originally called the "optical maser". This was ultimately changed to laser, for "light amplification by stimulated emission of radiation". Gordon Gould is credited with creating this acronym in 1957.


The theoretical principles governing the operation of a maser were first described by Joseph Weber of the University of Maryland, College Park at the Electron Tube Research Conference in June 1952 in Ottawa,[2] with a summary published in the June 1953 Transactions of the Institute of Radio Engineers Professional Group on Electron Devices,[3] and simultaneously by Nikolay Basov and Alexander Prokhorov from Lebedev Institute of Physics, at an All-Union Conference on Radio-Spectroscopy held by the USSR Academy of Sciences in May 1952, published in October 1954.

Independently, Charles Hard Townes, James P. Gordon, and H. J. Zeiger built the first ammonia maser at Columbia University in 1953. This device used stimulated emission in a stream of energized ammonia molecules to produce amplification of microwaves at a frequency of about 24.0 gigahertz.[4] Townes later worked with Arthur L. Schawlow to describe the principle of the optical maser, or laser,[5] of which Theodore H. Maiman created the first working model in 1960.

For their research in the field of stimulated emission, Townes, Basov and Prokhorov were awarded the Nobel Prize in Physics in 1964.[6]


The maser is based on the principle of stimulated emission proposed by Albert Einstein in 1917. When atoms have been induced into an excited energy state, they can amplify radiation at a frequency particular to the element or molecule used as the masing medium (similar to what occurs in the lasing medium in a laser).

By putting such an amplifying medium in a resonant cavity, feedback is created that can produce coherent radiation.

Some common types

21st-century developments

In 2012, a research team from the National Physical Laboratory and Imperial College London developed a solid-state maser that operated at room temperature by using optically pumped, pentacene-doped p-Terphenyl as the amplifier medium.[8][9][10] It produced pulses of maser emission lasting for a few hundred microseconds.

In 2018, a research team from Imperial College London and University College London demonstrated continuous-wave maser oscillation using synthetic diamonds containing nitrogen-vacancy defects.[11][12]


Masers serve as high precision frequency references. These "atomic frequency standards" are one of the many forms of atomic clocks. Masers were also used as low-noise microwave amplifiers in radio telescopes, though these have largely been replaced by amplifiers based on FETs.[13]

During the early 1960s, the Jet Propulsion Laboratory developed a maser to provide ultra-low-noise amplification of S-band microwave signals received from deep space probes.[14] This maser used deeply refrigerated helium to chill the amplifier down to a temperature of 4 kelvin. Amplification was achieved by exciting a ruby comb with a 12.0 gigahertz klystron. In the early years, it took days to chill and remove the impurities from the hydrogen lines.

Refrigeration was a two-stage process, with a large Linde unit on the ground, and a crosshead compressor within the antenna. The final injection was at 21 MPa (3,000 psi) through a 150 μm (0.006 in) micrometer-adjustable entry to the chamber. The whole system noise temperature looking at cold sky (2.7 kelvin in the microwave band) was 17 kelvin. This gave such a low noise figure that the Mariner IV space probe could send still pictures from Mars back to the Earth, even though the output power of its radio transmitter was only 15 watts, and hence the total signal power received was only −169 decibels with respect to a milliwatt (dBm).

Hydrogen maser

Main article: Hydrogen maser

A hydrogen maser.

The hydrogen maser is used as an atomic frequency standard. Together with other kinds of atomic clocks, these help make up the International Atomic Time standard ("Temps Atomique International" or "TAI" in French). This is the international time scale coordinated by the International Bureau of Weights and Measures. Norman Ramsey and his colleagues first conceived of the maser as a timing standard. More recent masers are practically identical to their original design. Maser oscillations rely on the stimulated emission between two hyperfine energy levels of atomic hydrogen.

Here is a brief description of how they work:

Astrophysical masers

Main article: Astrophysical maser

Maser-like stimulated emission has also been observed in nature from interstellar space, and it is frequently called "superradiant emission" to distinguish it from laboratory masers. Such emission is observed from molecules such as water (H2O), hydroxyl radicals (•OH), methanol (CH3OH), formaldehyde (HCHO), silicon monoxide (SiO), and carbodiimide (HNCNH).[16] Water molecules in star-forming regions can undergo a population inversion and emit radiation at about 22.0 GHz, creating the brightest spectral line in the radio universe. Some water masers also emit radiation from a rotational transition at a frequency of 96 GHz.[17][18]

Extremely powerful masers, associated with active galactic nuclei, are known as megamasers and are up to a million times more powerful than stellar masers.


The meaning of the term maser has changed slightly since its introduction. Initially the acronym was universally given as "microwave amplification by stimulated emission of radiation", which described devices which emitted in the microwave region of the electromagnetic spectrum.

The principle and concept of stimulated emission has since been extended to more devices and frequencies. Thus, the original acronym is sometimes modified, as suggested by Charles H. Townes,[1] to "molecular amplification by stimulated emission of radiation." Some have asserted that Townes's efforts to extend the acronym in this way were primarily motivated by the desire to increase the importance of his invention, and his reputation in the scientific community.[19]

When the laser was developed, Townes and Schawlow and their colleagues at Bell Labs pushed the use of the term optical maser, but this was largely abandoned in favor of laser, coined by their rival Gordon Gould.[20] In modern usage, devices that emit in the X-ray through infrared portions of the spectrum are typically called lasers, and devices that emit in the microwave region and below are commonly called masers, regardless of whether they emit microwaves or other frequencies.

Gould originally proposed distinct names for devices that emit in each portion of the spectrum, including grasers (gamma ray lasers), xasers (x-ray lasers), uvasers (ultraviolet lasers), lasers (visible lasers), irasers (infrared lasers), masers (microwave masers), and rasers (RF masers). Most of these terms never caught on, however, and all have now become (apart from in science fiction) obsolete except for maser and laser.[citation needed]

See also


  1. ^ a b Townes, Charles H. (1964-12-11). "Production of coherent radiation by atoms and molecules - Nobel Lecture" (PDF). The Nobel Prize. p. 63. Archived (pdf) from the original on 2020-08-27. Retrieved 2020-08-27. We called this general type of system the maser, an acronym for microwave amplification by stimulated emission of radiation. The idea has been successfully extended to such a variety of devices and frequencies that it is probably well to generalize the name - perhaps to mean molecular amplification by stimulated emission of radiation.
  2. ^ American Institute of Physics Oral History Interview with Weber
  3. ^ Mario Bertolotti (2004). The History of the Laser. CRC Press. p. 180. ISBN 978-1420033403.
  4. ^ Gordon, J. P.; Zeiger, H. J.; Townes, C. H. (1955). "The Maser—New Type of Microwave Amplifier, Frequency Standard, and Spectrometer". Phys. Rev. 99 (4): 1264. Bibcode:1955PhRv...99.1264G. doi:10.1103/PhysRev.99.1264.
  5. ^ Schawlow, A.L.; Townes, C.H. (15 December 1958). "Infrared and Optical Masers". Physical Review. 112 (6): 1940–1949. Bibcode:1958PhRv..112.1940S. doi:10.1103/PhysRev.112.1940.
  6. ^ "The Nobel Prize in Physics 1964". Retrieved 2020-08-27.
  7. ^ The Dual Noble Gas Maser, Harvard University, Department of Physics
  8. ^ Brumfiel, G. (2012). "Microwave laser fulfills 60 years of promise". Nature. doi:10.1038/nature.2012.11199. S2CID 124247048.
  9. ^ Palmer, Jason (16 August 2012). "'Maser' source of microwave beams comes out of the cold". BBC News. Archived from the original on July 29, 2016. Retrieved 23 August 2012.
  10. ^ Microwave Laser Fulfills 60 Years of Promise
  11. ^ Liu, Ren-Bao (March 2018). "A diamond age of masers". Nature. 555 (7697): 447–449. Bibcode:2018Natur.555..447L. doi:10.1038/d41586-018-03215-3. PMID 29565370.
  12. ^ Scientists use diamond in world's first continuous room-temperature solid-state maser,
  13. ^ "Low Noise Amplifiers – Pushing the limits of low noise". National Radio Astronomy Observatory (NRAO).
  14. ^ Macgregor S. Reid, ed. (2008). "Low-Noise Systems in the Deep Space Network" (PDF). JPL.
  15. ^ "Time and Frequency From A to Z: H". NIST. 12 May 2010.
  16. ^ McGuire, Brett A.; Loomis, Ryan A.; Charness, Cameron M.; Corby, Joanna F.; Blake, Geoffrey A.; Hollis, Jan M.; Lovas, Frank J.; Jewell, Philip R.; Remijan, Anthony J. (2012-10-20). "Interstellar Carbodiimide (HNCNH): A New Astronomical Detection from the GBT Primos Survey Via Maser Emission Features". The Astrophysical Journal. 758 (2): L33. arXiv:1209.1590. Bibcode:2012ApJ...758L..33M. doi:10.1088/2041-8205/758/2/L33. ISSN 2041-8205. S2CID 26146516.
  17. ^ Neufeld, David A.; Melnick, Gary J. (1991). "Excitation of Millimeter and Submillimeter Water Masers in Warm Astrophysical Gas". Atoms, Ions and Molecules: New Results in Spectral Line Astrophysics, ASP Conference Series (ASP: San Francisco). 16: 163. Bibcode:1991ASPC...16..163N.
  18. ^ Tennyson, Jonathan; et al. (March 2013). "IUPAC critical evaluation of the rotational–vibrational spectra of water vapor, Part III: Energy levels and transition wavenumbers for H216O". Journal of Quantitative Spectroscopy and Radiative Transfer. 117: 29–58. Bibcode:2013JQSRT.117...29T. doi:10.1016/j.jqsrt.2012.10.002. hdl:10831/91303.
  19. ^ Taylor, Nick (2000). LASER: The inventor, the Nobel laureate, and the thirty-year patent war. New York: Simon & Schuster. ISBN 978-0-684-83515-0.
  20. ^ Taylor, Nick (2000). LASER: The inventor, the Nobel laureate, and the thirty-year patent war. New York: Simon & Schuster. pp. 66–70. ISBN 978-0-684-83515-0.

Further reading