<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://wiki.sarg.dev/api.php?action=feedcontributions&amp;feedformat=atom&amp;user=2001%3A9E8%3A6A86%3A3800%3A3C8%3AAE32%3AF4D4%3AF3CA</id>
	<title>Vero - Wikipedia - User contributions [en]</title>
	<link rel="self" type="application/atom+xml" href="https://wiki.sarg.dev/api.php?action=feedcontributions&amp;feedformat=atom&amp;user=2001%3A9E8%3A6A86%3A3800%3A3C8%3AAE32%3AF4D4%3AF3CA"/>
	<link rel="alternate" type="text/html" href="https://wiki.sarg.dev/index.php/Special:Contributions/2001:9E8:6A86:3800:3C8:AE32:F4D4:F3CA"/>
	<updated>2026-08-14T17:37:54Z</updated>
	<subtitle>User contributions</subtitle>
	<generator>MediaWiki 1.44.2</generator>
	<entry>
		<id>https://wiki.sarg.dev/index.php?title=Gauss_(unit)&amp;diff=7869</id>
		<title>Gauss (unit)</title>
		<link rel="alternate" type="text/html" href="https://wiki.sarg.dev/index.php?title=Gauss_(unit)&amp;diff=7869"/>
		<updated>2025-09-05T23:30:20Z</updated>

		<summary type="html">&lt;p&gt;2001:9E8:6A86:3800:3C8:AE32:F4D4:F3CA: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{{Short description|Unit of magnetic induction}}&lt;br /&gt;
{{Infobox unit&lt;br /&gt;
| name         = gauss&lt;br /&gt;
| image        = &lt;br /&gt;
| caption      = &lt;br /&gt;
| standard     = [[Gaussian units|Gaussian]] and [[Centimetre–gram–second_system_of_units#Electromagnetic_units_.28EMU.29|emu-cgs]]&lt;br /&gt;
| quantity     = [[magnetic flux]] density (also known as [[Magnetic_field#The_B-field|magnetic induction]], or the {{math|&#039;&#039;&#039;B&#039;&#039;&#039;}}-field, or magnetic field)&lt;br /&gt;
| symbol       = G &#039;&#039;or&#039;&#039; Gs&lt;br /&gt;
| symbol2      = &lt;br /&gt;
| namedafter   = [[Carl Friedrich Gauss]]&lt;br /&gt;
| extralabel   = &lt;br /&gt;
| extradata    = &lt;br /&gt;
| units1       = [[SI derived units]]&lt;br /&gt;
| inunits1     = {{val|e=-4|u=tesla}}{{efn|The electromagnetic Gaussian and SI quantities &#039;&#039;correspond&#039;&#039; (symbol &#039;≘&#039;) rather than being &#039;&#039;equal&#039;&#039; (symbol &#039;{{=}}&#039;).}}&lt;br /&gt;
| units2       = Gaussian base units&lt;br /&gt;
| inunits2     = 1&amp;amp;nbsp;cm&amp;lt;sup&amp;gt;−1/2&amp;lt;/sup&amp;gt;⋅&amp;lt;wbr/&amp;gt;g&amp;lt;sup&amp;gt;1/2&amp;lt;/sup&amp;gt;⋅&amp;lt;wbr/&amp;gt;s&amp;lt;sup&amp;gt;−1&amp;lt;/sup&amp;gt;&lt;br /&gt;
| units3       = [[Centimetre–gram–second system of units#Electrostatic units (ESU)|esu-cgs]]&lt;br /&gt;
| inunits3     = 1/{{math|&#039;&#039;c&#039;&#039;}}{{sub|cgs}}&amp;amp;nbsp;esu{{efn|{{math|&#039;&#039;c&#039;&#039;}}{{sub|cgs}} {{=}} {{val|2.99792458e10}} is the numeric part of the [[speed of light]] when expressed in cgs units.}}&lt;br /&gt;
}}&lt;br /&gt;
[[File:Bendixen_-_Carl_Friedrich_Gauß,_1828.jpg | thumb | right | Carl Friedrich Gauß in 1828, aged 50 years old]]&lt;br /&gt;
The &#039;&#039;&#039;gauss&#039;&#039;&#039; (symbol: &#039;&#039;&#039;{{val|u=G}}&#039;&#039;&#039;, sometimes &#039;&#039;&#039;Gs&#039;&#039;&#039;) is a unit of measurement of magnetic induction, also known as [[magnetic flux density]]. The unit is part of the [[Gaussian units|Gaussian system]] of units, which inherited it from the older [[centimetre–gram–second system of units#Electromagnetic units .28EMU.29|centimetre–gram–second electromagnetic units]] (CGS-EMU) system. It was named after the German mathematician and physicist [[Carl Friedrich Gauss]] in 1936. One gauss is defined as one [[maxwell (unit)|maxwell]] per square [[centimetre]].&lt;br /&gt;
&lt;br /&gt;
As the [[centimetre–gram–second system of units]] (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, and preferred in [[astrophysics]].&amp;lt;ref&amp;gt;J. B. Zirker, &#039;&#039;The Magnetic Universe.&#039;&#039;, Johns Hopkins University Press, Baltimore, 2009, p. 281.&amp;lt;/ref&amp;gt; The SI unit for magnetic flux density is the [[Tesla (unit)|tesla]] (symbol T),&amp;lt;ref&amp;gt;&#039;&#039;NIST Special Publication 1038&#039;&#039;, Section 4.3.1&amp;lt;/ref&amp;gt; which corresponds to {{gaps|10,000|gauss}}.&lt;br /&gt;
&lt;br /&gt;
==Name, symbol, and metric prefixes==&lt;br /&gt;
Although 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&#039;s name, its symbol is the uppercase letter &amp;quot;G&amp;quot;. When the unit is spelled out, it is written in lowercase (&amp;quot;gauss&amp;quot;), unless it begins a sentence.&amp;lt;ref name=&amp;quot;SIBrochure9thEd&amp;quot;&amp;gt;{{SIbrochure9th}}&amp;lt;/ref&amp;gt;{{rp|147–148}}  The gauss may be combined with [[metric prefix]]es,&amp;lt;ref name=&amp;quot;SIBrochure8th&amp;quot;&amp;gt;{{SIbrochure8th}}&amp;lt;/ref&amp;gt;{{rp|128}} such as in milligauss, mG (or mGs), or kilogauss, kG (or kGs).&lt;br /&gt;
&lt;br /&gt;
==Unit conversions==&lt;br /&gt;
&amp;lt;math display=&amp;quot;block&amp;quot;&amp;gt;\begin{align}&lt;br /&gt;
1\,{\rm G} &amp;amp;= {\rm Mx}{\cdot}{\rm cm}^{-2} = \frac{\rm g}{{\rm Bi}{\cdot}{\rm s}^2}\\&lt;br /&gt;
           &amp;amp;\text{ ≘ } 10^{-4}\,{\rm T} = 10^{-4}\frac{\rm kg}{{\rm A}{\cdot}{\rm s^2}}&lt;br /&gt;
\end{align}&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The gauss is the unit of magnetic flux density &#039;&#039;&#039;B&#039;&#039;&#039; in the system of [[Gaussian units]] and is equal to [[Maxwell (unit)|Mx]]/cm&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt; or [[gram (unit)|g]]/[[Abampere|Bi]]/s&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;, while the [[oersted]] is the unit of [[Magnetic_field#The_H-field|{{math|&#039;&#039;&#039;H&#039;&#039;&#039;}}-field]]. One [[tesla (unit)|tesla]] (T) corresponds to 10&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&amp;amp;nbsp;gauss, and one [[ampere]] (A) per metre corresponds to 4π&amp;amp;nbsp;×&amp;amp;nbsp;10&amp;lt;sup&amp;gt;−3&amp;lt;/sup&amp;gt; [[oersted]]. &lt;br /&gt;
&amp;lt;!--&lt;br /&gt;
 A [[Abampere|biot]] (or [[abampere]]) is equal to 10 [[ampere]]s.&amp;lt;ref name=&amp;quot;Hayt&amp;quot;&amp;gt;Hayt, Jr., William H. (1974), &#039;&#039;Engineering Electromagnetics, Third Edition&#039;&#039;, McGraw-Hill, {{ISBN|0-07-027390-1}}&amp;lt;/ref&amp;gt;&amp;lt;ref&amp;gt;Jackson, John (1975), &#039;&#039;Classical Electrodynamics, 2nd Ed.&#039;&#039;, John Wiley, {{ISBN|0-471-43132-X}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
--&amp;gt;&lt;br /&gt;
&lt;br /&gt;
The units for [[magnetic flux]]&amp;amp;nbsp;Φ, which is the [[integral]] of [[Magnetic_field#The_B-field|magnetic {{math|&#039;&#039;&#039;B&#039;&#039;&#039;}}-field]] over an [[area]], are the [[weber (unit)|weber]] (Wb) in the [[SI]] and the [[Maxwell (unit)|maxwell]] (Mx) in the CGS-Gaussian system. The conversion factor is {{val|e=8|u=maxwell per weber}}, since [[flux]] is the integral of field over an area, area having the units of the square of distance, thus {{val|e=4|u=G/T}} (magnetic field conversion factor) times the square of {{val|e=2|u=cm/m}} (linear distance conversion factor). 10&amp;lt;sup&amp;gt;8&amp;lt;/sup&amp;gt;&amp;amp;nbsp;Mx/Wb = 10&amp;lt;sup&amp;gt;4&amp;lt;/sup&amp;gt;&amp;amp;nbsp;G/T × (10&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;&amp;amp;nbsp;cm/m)&amp;lt;sup&amp;gt;2&amp;lt;/sup&amp;gt;.&lt;br /&gt;
&lt;br /&gt;
==Typical values==&lt;br /&gt;
{{main|Orders of magnitude (magnetic field)}}&lt;br /&gt;
* 10&amp;lt;sup&amp;gt;−9&amp;lt;/sup&amp;gt;–10&amp;lt;sup&amp;gt;−8&amp;lt;/sup&amp;gt; G – the magnetic field of the human brain&lt;br /&gt;
* 10&amp;lt;sup&amp;gt;−6&amp;lt;/sup&amp;gt;–10&amp;lt;sup&amp;gt;−3&amp;lt;/sup&amp;gt; G – the magnetic field of Galactic [[molecular clouds]]. Typical magnetic field strengths within the interstellar medium of the [[Milky Way]] are ~5 μG.&lt;br /&gt;
* 0.25–0.60 G – the [[Earth&#039;s magnetic field]] at its surface&lt;br /&gt;
* 4 G – near [[Jupiter]]&#039;s equator&lt;br /&gt;
* 25 G – the Earth&#039;s magnetic field in its [[Earth&#039;s outer core|core]]&amp;lt;ref name=&amp;quot;buff2010&amp;quot;&amp;gt;Buffett, Bruce A. (2010), &amp;quot;Tidal dissipation and the strength of the Earth&#039;s internal magnetic field&amp;quot;, &#039;&#039;Nature&#039;&#039;, volume 468, pages 952–954, {{doi|10.1038/nature09643}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* 50 G – a typical [[refrigerator magnet]]&lt;br /&gt;
* 100 G – an [[iron]] [[magnet]]&lt;br /&gt;
* 1500 G – within a [[sun spot]]&amp;lt;ref&amp;gt;{{Cite web |url=http://www.coolmagnetman.com/magflux.htm |title=How strong are magnets?|last=Hoadley |first=Rick |website=www.coolmagnetman.com |access-date=2017-01-26 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* 10000 to 13000 G – [[remanence]] of a [[neodymium magnet|neodymium-iron-boron (NIB) magnet]]&amp;lt;ref&amp;gt;{{cite book |url=https://books.google.com/books?id=_y3LSh1XTJYC&amp;amp;pg=PT232 |page=232 |title=Design of Rotating Electrical Machines |first1=Juha |last1=Pyrhönen |first2=Tapani |last2=Jokinen |first3=Valéria |last3=Hrabovcová |publisher=John Wiley and Sons |year=2009 |isbn=978-0-470-69516-6 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* 16000 to 22000 G – [[saturation (magnetic)|saturation]] of high permeability iron alloys used in transformers&amp;lt;ref&amp;gt;{{cite book |editor1-last=Laughton |editor1-first=Michael A. |editor2-last=Warne |editor2-first=Douglas F. |title=Electrical Engineer&#039;s Reference Book |edition=Sixteenth |publisher=Newnes |year=2003 |isbn=0-7506-4637-3 |chapter=8 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* 3000–70000 G – a medical [[magnetic resonance imaging|magnetic resonance imaging machine]] &lt;br /&gt;
* 10&amp;lt;sup&amp;gt;12&amp;lt;/sup&amp;gt;–10&amp;lt;sup&amp;gt;13&amp;lt;/sup&amp;gt; G – the surface of a [[neutron star]]&amp;lt;ref&amp;gt;{{cite web |title=How strong are magnets? |work=Experiments with magnets and our surroundings |publisher=Magcraft |url=http://www.coolmagnetman.com/magflux.htm |access-date=2007-12-14 }}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* 4 × 10&amp;lt;sup&amp;gt;13&amp;lt;/sup&amp;gt; G – the [[Schwinger limit]]&lt;br /&gt;
* 10&amp;lt;sup&amp;gt;14&amp;lt;/sup&amp;gt; G – the magnetic field of [[SGR J1745-2900]], orbiting the supermassive black hole [[Sagittarius A*|Sgr A*]] in the center of the Milky Way.&lt;br /&gt;
* 10&amp;lt;sup&amp;gt;15&amp;lt;/sup&amp;gt; G – the magnetic field of some newly created [[magnetar]]s&amp;lt;ref name=&amp;quot;sciam_article&amp;quot;&amp;gt;{{cite web &lt;br /&gt;
 |date        = March 2003&lt;br /&gt;
 |first       = Robert C. &lt;br /&gt;
 |last        = Duncan&lt;br /&gt;
 |url         = http://solomon.as.utexas.edu/~duncan/magnetar.html#Epilog&lt;br /&gt;
 |title       = Magnetars, Soft Gamma Repeaters and Very Strong Magnetic Fields&lt;br /&gt;
 |publisher   = University of Texas at Austin&lt;br /&gt;
 |access-date  = 2007-05-23&lt;br /&gt;
 |url-status     = dead&lt;br /&gt;
 |archive-url  = https://web.archive.org/web/20070611144512/http://solomon.as.utexas.edu/~duncan/magnetar.html#Epilog&lt;br /&gt;
 |archive-date = 2007-06-11&lt;br /&gt;
}}&amp;lt;/ref&amp;gt;&lt;br /&gt;
* 10&amp;lt;sup&amp;gt;17&amp;lt;/sup&amp;gt; G – the upper limit to neutron star magnetism&amp;lt;ref name=&amp;quot;sciam_article&amp;quot; /&amp;gt;&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
*[[Tesla (unit)]]&lt;br /&gt;
*[[Centimetre–gram–second system of units]]&lt;br /&gt;
*[[Gaussian units]]&lt;br /&gt;
&lt;br /&gt;
== Notes ==&lt;br /&gt;
{{notelist}}&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{reflist}}&lt;br /&gt;
&lt;br /&gt;
{{CGS units}}&lt;br /&gt;
&lt;br /&gt;
[[Category:Centimetre–gram–second system of units]]&lt;br /&gt;
[[Category:Units of magnetic flux density]]&lt;br /&gt;
[[Category:Carl Friedrich Gauss|Unit]]&lt;/div&gt;</summary>
		<author><name>2001:9E8:6A86:3800:3C8:AE32:F4D4:F3CA</name></author>
	</entry>
</feed>