Gauss (unit)

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## Name, symbol, and metric prefixes

## Unit conversions

## Typical values

## See also

## Notes

## References

This article uses material from the Wikipedia page available here. It is released under the Creative Commons Attribution-Share-Alike License 3.0.

Gauss Unit

gauss | |
---|---|

Unit system | Gaussian and emu-cgs |

Unit of | magnetic flux density (also known as magnetic induction, or the B-field, or magnetic field) |

Symbol | G or Gs |

Named after | Carl Friedrich Gauss |

Conversions | |

SI derived units | ^{[a]} |

Gaussian base units | 1 cm^{-1/2}?^{1/2}?^{-1} |

esu-cgs | 1/c_{cgs} esu^{[b]} |

The **gauss**, symbol (sometimes Gs), is a unit of measurement of magnetic induction, also known as *magnetic flux density*. The unit is part of the Gaussian system of units, which inherited it from the older CGS-EMU system. It was named after the German mathematician and physicist Carl Friedrich Gauss in 1936. One gauss is defined as one maxwell per square centimetre.

As the cgs system has been superseded by the International System of Units (SI), the use of the gauss has been deprecated by the standards bodies, but is still regularly used in various subfields of science. The SI unit for magnetic flux density is the tesla (symbol T),^{[1]} which corresponds to 10,000gauss.

Albeit not a component of the International System of Units, the usage of the gauss generally follows the rules for SI units. Since the name is derived from a person's name, its symbol is the uppercase letter *G*. When the unit is spelled out, it is written in lowercase ("gauss"), unless it begins a sentence.^{[2]} The gauss may be combined with metric prefixes,^{[3]} such as in milligauss, mG (or mGs), or kilogauss, kGauss or kG.

The gauss is the unit of magnetic flux density **B** in the system of Gaussian units and is equal to Mx/cm^{2} or g/Bi/s^{2}, while the oersted is the unit of **H**-field. One tesla (T) corresponds to 10^{4} gauss, and one ampere (A) per metre corresponds to 4? × 10^{-3} oersted.

The units for magnetic flux ?, which is the integral of magnetic **B**-field over an area, are the weber (Wb) in the SI and the maxwell (Mx) in the CGS-Gaussian system. The conversion factor is , since flux is the integral of field over an area, area having the units of the square of distance, thus (magnetic field conversion factor) times the square of (linear distance conversion factor). 10^{8} Mx/Wb = 10^{4} G/T × (10^{2} cm/m)^{2}.

- 10
^{-9}-10^{-8}G - the magnetic field of the human brain - 10
^{-6}-10^{-3}G - the magnetic field of Galactic molecular clouds. Typical magnetic field strengths within the interstellar medium of the Milky Way are ~5 ?G. - 0.25-0.60 G - the Earth's magnetic field at its surface
- 4 G - near Jupiter's equator
- 25 G - the Earth's magnetic field in its core
^{[4]} - 50 G - a typical refrigerator magnet
- 100 G - an iron magnet
- 1500 G - within a sun spot
^{[5]} - 10000 to 13000 G - remanence of a neodymium-iron-boron (NIB) magnet
^{[6]} - 16000 to 22000 G - saturation of high permeability iron alloys used in transformers
^{[7]} - 3000-70000 G - a medical magnetic resonance imaging machine
- 10
^{12}-10^{13}G - the surface of a neutron star^{[8]} - 4 × 10
^{13}G - the Schwinger limit - 10
^{14}G - the magnetic field of SGR J1745-2900, orbiting the supermassive black hole Sgr A* in the center of the Milky Way. - 10
^{15}G - the magnetic field of some newly created magnetars^{[9]} - 10
^{17}G - the upper limit to neutron star magnetism^{[9]}

**^**The electromagnetic Gaussian and SI quantities*correspond*(symbol '?') rather than being*equal*(symbol '=').**^***c*_{cgs}= is the numeric part of the speed of light when expressed in cgs units.

**^***NIST Special Publication 1038*, Section 4.3.1**^***Le Système international d'unités*[*The International System of Units*] (PDF) (in French and English) (9th ed.), International Bureau of Weights and Measures, 2019, ISBN 978-92-822-2272-0**^**International Bureau of Weights and Measures (2006),*The International System of Units (SI)*(PDF) (8th ed.), ISBN 92-822-2213-6, archived (PDF) from the original on 2021-06-04, retrieved**^**Buffett, Bruce A. (2010), "Tidal dissipation and the strength of the Earth's internal magnetic field",*Nature*, volume 468, pages 952-954, doi:10.1038/nature09643**^**Hoadley, Rick. "How strong are magnets?".*www.coolmagnetman.com*. Retrieved .**^**Pyrhönen, Juha; Jokinen, Tapani; Hrabovcová, Valéria (2009).*Design of Rotating Electrical Machines*. John Wiley and Sons. p. 232. ISBN 978-0-470-69516-6.**^**Laughton, Michael A.; Warne, Douglas F., eds. (2003). "8".*Electrical Engineer's Reference Book*(Sixteenth ed.). Newnes. ISBN 0-7506-4637-3.**^**"How strong are magnets?".*Experiments with magnets and our surroundings*. Magcraft. Retrieved .- ^
^{a}^{b}Duncan, Robert C. (March 2003). "Magnetars, Soft Gamma Repeaters and Very Strong Magnetic Fields". University of Texas at Austin. Archived from the original on 2007-06-11. Retrieved .

This article uses material from the Wikipedia page available here. It is released under the Creative Commons Attribution-Share-Alike License 3.0.

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