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{{Short description|State of matter}}
{{Other uses|Plasma (disambiguation){{!}}Plasma}}
{{Pp|small=yes}}
{{Use dmy dates|date=March 2015}}
{{Use dmy dates|date=September 2024}}
{{infobox
{{Multiple image
| title = Plasma
| perrow = 2
| data1 = {{nowrap|] ]}}
| total_width = 300
| data2 = {{nowrap|] ]}}
| image1 = Lightning3.jpg
| data3 = Top: ] and ] are commonplace generators of plasma. Bottom left: A ], illustrating some of the more complex plasma phenomena, including ]. Bottom right: A plasma trail from the ] ] during re-entry into ], as seen from the ].}}
| image2 = Neon Internet Cafe open 24 hours.jpg
| image3 = Plasma-lamp 2.jpg
| image4 = Space Shuttle Atlantis in the sky on July 21, 2011, to its final landing.jpg
| image5 = Fire in a fire pit.jpg
| image6 = Solar eclipse 1999 4.jpg
| footer = Top: ] and ] are commonplace generators of plasma. Center left: A ], illustrating some of the more complex plasma phenomena, including ]. Center right: A plasma trail from the ] ] during re-entry into ], as seen from the ]. Bottom left: A ] in a fire pit; fires may produce plasma if hot enough. Bottom right: The ]'s ] as seen from a ] in ].
}}


'''Plasma''' ({{etymology|grc|''{{wikt-lang|grc|πλάσμα}}'' ({{grc-transl|πλάσμα}})|moldable substance}}<ref name="πλάσμα">{{Cite book|first1=Henry George |last1=Liddell |first2=Robert |last2=Scott |title=A Greek-English Lexicon |chapter=πλάσμα|chapter-url=http://www.perseus.tufts.edu/hopper/text?doc=Perseus%3Atext%3A1999.04.0057%3Aentry%3Dpla%2Fsma|access-date=10 February 2023|publisher=Clarendon Press |year=1940}}</ref>) is one of four fundamental ] (the other three being ], ], and ]) characterized by the presence of a significant portion of ]s in any combination of ]s or ]s. It is the most abundant form of ] in the ], mostly in ]s (including the ]), but also dominating the rarefied ] and ].<ref name="Itptma2013a">{{cite book
'''Plasma''' ({{ety|grc|''πλάσμα''&#8203;|moldable substance}}<ref name="πλάσμα"> {{webarchive|url=https://web.archive.org/web/20130618012819/http://www.perseus.tufts.edu/hopper/text?doc=Perseus%3Atext%3A1999.04.0057%3Aentry%3Dpla%2Fsma |date=18 June 2013 }}, Henry George Liddell, Robert Scott, ''A Greek English Lexicon'', on Perseus</ref>) is one of ], and was first described by chemist ]<ref name="Itpp1995"/> in the 1920s.<ref name=Itpd2012a>{{cite book |last1=Morozov |first1=A.I.|date=2012 |title=Introduction to Plasma Dynamics |page=17 |publisher=CRC Press| isbn=978-1-4398-8132-3 |url=https://books.google.com/?id=DB0L6P3TwiYC&printsec=frontcover&dq=Introduction+to+Plasma+Dynamics+morozov#v=onepage&q&f=false}}</ref> Plasma can be artificially generated by heating or subjecting a neutral gas to a strong ] to the point where an ionised gaseous substance becomes increasingly ], and long-range electromagnetic fields dominate the behaviour of the matter.<ref name=Itpd2012b>{{cite book |last1=Morozov |first1=A.I.|date=2012 |title=Introduction to Plasma Dynamics |page=30 |publisher=CRC Press| isbn=978-1-4398-8132-3}}</ref>
|last1=Chu

|first1=P.K.|last2=Lu
Plasma and ionised gases have properties and display behaviours unlike those of the other states, and the ] between them is mostly a matter of nomenclature<ref name="Itpp1995"/> and subject to interpretation.<ref name=Itpd2012>{{cite book |last1=Morozov |first1=A.I.|date=2012 |title=Introduction to Plasma Dynamics |page=4−5 |publisher=CRC Press|isbn=978-1-4398-8132-3}}</ref> Based on the surrounding environmental ] and ], partially ] or fully ionised forms of plasma may be produced. ]s and ] are examples of partially ionised plasma.<ref>{{Cite web | title = How Lightning Works | publisher = HowStuffWorks | url = http://science.howstuffworks.com/nature/natural-disasters/lightning2.htm | deadurl = no | archiveurl = https://web.archive.org/web/20140407080201/http://science.howstuffworks.com/nature/natural-disasters/lightning2.htm | archivedate = 7 April 2014 | df = dmy-all }}</ref> The Earth's ] is a plasma and the ] contains plasma in the Earth's surrounding ]. The interior of the ] is an example of fully ionised plasma,<ref name=Phillips1995>
|first2=XinPel
|date=2013
|title=Low Temperature Plasma Technology: Methods and Applications
| page=3
|publisher=CRC Press
|isbn=978-1-4665-0990-0}}</ref><ref name="Piel2010">{{Cite book
|last =Piel
|first=A.
|date=2010
|title= Plasma Physics: An Introduction to Laboratory, Space, and Fusion Plasmas
|pages= 4–5
|publisher=]
|url=https://books.google.com/books?id=9cA0DwAAQBAJ&pg=PR8
|isbn=978-3-642-10491-6
|url-status=live
|archive-url=https://web.archive.org/web/20160105142523/https://books.google.com/books?hl=en
|archive-date=5 January 2016
|df = dmy-all
}}</ref><ref name="Phillips1995">
{{Cite book {{Cite book
|last=Phillips |last=Phillips
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|page=295 |page=295
|publisher=] |publisher=]
|url=https://books.google.com/?id=idwBChjVP0gC&printsec=frontcover&dq=Guide+to+the+Sun+phillips#v=onepage&q&f=false |url=https://books.google.com/books?id=idwBChjVP0gC&q=Guide+to+the+Sun+phillips
|isbn=978-0-521-39788-9 |isbn=978-0-521-39788-9
|url-status=live
|deadurl=no
|archiveurl= https://web.archive.org/web/20180115215631/https://books.google.com/books?id=idwBChjVP0gC&printsec=frontcover&dq=Guide+to+the+Sun+phillips&hl=en&sa=X&ved=0ahUKEwiBj4Gbj5bXAhXrrVQKHfnAAKUQ6AEIKDAA#v=onepage&q&f=false |archive-url= https://web.archive.org/web/20180115215631/https://books.google.com/books?id=idwBChjVP0gC&printsec=frontcover&dq=Guide+to+the+Sun+phillips&hl=en&sa=X&ved=0ahUKEwiBj4Gbj5bXAhXrrVQKHfnAAKUQ6AEIKDAA
|archivedate=15 January 2018 |archive-date=15 January 2018
|df=dmy-all}}</ref> along with the ]<ref name="Aschwanden2004">{{cite book }}</ref><ref name="Aschwanden2004">{{cite book
|last=Aschwanden |last=Aschwanden
|first=M. J. |first=M. J.
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|title=Physics of the Solar Corona. An Introduction |title=Physics of the Solar Corona. An Introduction
|publisher=Praxis Publishing |publisher=Praxis Publishing
|isbn=978-3-540-22321-4}}</ref> and ]s.<ref name="Piel2010">{{Cite book |isbn=978-3-540-22321-4}}</ref>
Plasma can be artificially generated, for example, by heating a neutral gas or subjecting it to a strong ].<ref name="BoPA2015">{{cite book
|last =Piel
|last1=Chiuderi
|first=A.
|first1=C.
|date=2010
|last2=Velli
|title= Plasma Physics: An Introduction to Laboratory, Space, and Fusion Plasmas
|first2=M.
|pages= 4–5
|date=2015
|title=Basics of Plasma Astrophysics
|page=17
|publisher=] |publisher=]
|isbn=978-88-470-5280-2}}</ref>
|url=https://books.google.com/?id=9cA0DwAAQBAJ&pg=PR8#v=onepage&q&f=false
|isbn=978-3-642-10491-6
|deadurl= no
|archiveurl=https://web.archive.org/web/20160105142523/https://books.google.com/books?hl=en#v=onepage&q&f=false
|archivedate=5 January 2016
|df = dmy-all
}}</ref>


Positive ] in ] are achieved by stripping away ] orbiting the atomic nuclei, where the total number of electrons removed is related to either increasing temperature or the local density of other ionised matter. This also can be accompanied by the dissociation of ]s<ref name="Sturrock" />, though this process is distinctly different from ] of ] or the behaviour of shared ions in ]s. The response of plasma to electromagnetic fields is used in many modern technological devices, such as ] or ].<ref name=Itptma2013>{{cite book The presence of ]s makes plasma ], with the dynamics of individual particles and macroscopic plasma motion governed by collective electromagnetic fields and very sensitive to externally applied fields.<ref name="Itpd2012b">{{cite book |last1=Morozov |first1=A.I.|date=2012 |title=Introduction to Plasma Dynamics |page=30 |publisher=CRC Press| isbn=978-1-4398-8132-3}}</ref> The response of plasma to electromagnetic fields is used in many modern devices and technologies, such as ] or ].<ref name="Itptma2013">{{cite book
|last1=Chu |last1=Chu
|first1=P.K. |first1=P.K.
Line 53: Line 76:
|isbn=978-1-4665-0990-0}}</ref> |isbn=978-1-4665-0990-0}}</ref>


Depending on temperature and density, a certain number of neutral particles may also be present, in which case plasma is called ]. ]s and ] are examples of partially ionized plasmas.<ref>{{Cite web | title = How Lightning Works | publisher = HowStuffWorks | url = http://science.howstuffworks.com/nature/natural-disasters/lightning2.htm | url-status=live | archive-url = https://web.archive.org/web/20140407080201/http://science.howstuffworks.com/nature/natural-disasters/lightning2.htm | archive-date = 7 April 2014 | df = dmy-all | date = April 2000 }}</ref>
Plasma may be the most abundant form of ] in the ],<ref name=Itptma2013a>{{cite book
Unlike the ]s between the other three states of matter, the transition to plasma is not well defined and is a matter of interpretation and context.<ref name="Itpd2012">{{cite book |last1=Morozov |first1=A.I.|date=2012 |title=Introduction to Plasma Dynamics |page=4−5 |publisher=CRC Press|isbn=978-1-4398-8132-3}}</ref> Whether a given degree of ionization suffices to call a substance "plasma" depends on the specific phenomenon being considered.
|last1=Chu
|first1=P.K.
|last2=Lu
|first2=XinPel
|date=2013
|title=Low Temperature Plasma Technology: Methods and Applications
| page=3
|publisher=CRC Press
|isbn=978-1-4665-0990-0}}</ref> although this hypothesis is currently tentative based on the existence and unknown properties of ]. Plasma is mostly associated with ]s, extending to the rarefied ] and possibly the ].<ref name=BoPA2015>{{cite book
|last1=Chiuderi
|first1=C.
|last2=Velli
|first2=M.
|date=2015
|title=Basics of Plasma Astrophysics
|page=17
|publisher=]
|isbn=978-88-470-5280-2}}</ref>


==History== ==Early history==


] calculated by an ] ]. Note the fast moving electrons and slow ions, resembling a ].]]
The word ''plasma'' comes {{ety|grc|''πλάσμα''&#8203;|moldable substance}}<ref name="πλάσμα"/> or 'jelly',<ref name=Itpp1995>{{cite book |last1=Goldston |first1=R.J. |last2=Rutherford |first2=P.H. |date=1995 |title=Introduction to Plasma Physics |page=1−2 |publisher=Taylor & Francis |isbn=978-0-7503-0183-1 |url=https://books.google.com/?id=7kM7yEFUGnAC&printsec=frontcover&dq=chen+%22introduction+to+plasma+physics%22#v=onepage&q&f=false}}</ref> and describes the behaviour of the Ionised atomic nuclei and the electrons within the surrounding region of the plasma. Very simply, each of these nuclei are suspended in a movable sea of electrons. Plasma was first identified in a ], and so described by ] in 1879 (he called it "radiant matter").<ref>Crookes presented a ] to the ], in Sheffield, on Friday, 22 August 1879 {{cite web |url=http://www.worldcatlibraries.org/wcpa/top3mset/5dcb9349d366f8ec.html |title=Archived copy |accessdate=2006-05-24 |deadurl=no |archiveurl=https://web.archive.org/web/20060709162459/http://www.worldcatlibraries.org/wcpa/top3mset/5dcb9349d366f8ec.html |archivedate=9 July 2006 |df=dmy-all }} {{cite web |url=http://www.tfcbooks.com/mall/more/315rm.htm |title=Archived copy |accessdate=2006-05-24 |deadurl=no |archiveurl=https://web.archive.org/web/20060613212651/http://tfcbooks.com/mall/more/315rm.htm |archivedate=13 June 2006 |df=dmy-all }}</ref> The nature of this "]" matter was subsequently identified by British physicist ] in 1897.<ref>Announced in his evening lecture to the ] on Friday, 30 April 1897, and published in {{cite journal|journal=]|volume=44|issue=269|pages=293–316|title=J. J. Thomson (1856–1940)|url=http://web.lemoyne.edu/~GIUNTA/thomson1897.html|date=1897|doi=10.1080/14786449708621070|last1=Thomson|first1=J. J.|deadurl=no|archiveurl=https://web.archive.org/web/20150812112129/http://web.lemoyne.edu/%7EGIUNTA/thomson1897.html|archivedate=12 August 2015|df=dmy-all}}</ref>


Plasma was first identified in laboratory by ]. Crookes presented a ] on what he called "radiant matter" to the ], in Sheffield, on Friday, 22 August 1879.<ref>{{cite web |url=http://www.worldcatlibraries.org/wcpa/top3mset/5dcb9349d366f8ec.html |title=Find in a Library: On radiant matter a lecture delivered to the British Association for the Advancement of Science, at Sheffield, Friday, August 22, 1879 |access-date=24 May 2006 |url-status=live |archive-url=https://web.archive.org/web/20060709162459/http://www.worldcatlibraries.org/wcpa/top3mset/5dcb9349d366f8ec.html |archive-date=9 July 2006 }} {{cite web |url=http://www.tfcbooks.com/mall/more/315rm.htm |title=Radiant Matter |access-date=24 May 2006 |url-status=live |archive-url=https://web.archive.org/web/20060613212651/http://tfcbooks.com/mall/more/315rm.htm |archive-date=13 June 2006 }}</ref>
The term "plasma" was coined by ] in 1928.<ref name="langmuir1928">{{Cite journal | last1 = Langmuir | first1 = I. | title = Oscillations in Ionized Gases | doi = 10.1073/pnas.14.8.627 | journal = Proceedings of the National Academy of Sciences | volume = 14 | issue = 8 | pages = 627–637 | year = 1928 | pmid = 16587379| pmc = 1085653| bibcode = 1928PNAS...14..627L | url = http://www.pnas.org/content/14/8/627 | deadurl = no | archiveurl = https://web.archive.org/web/20170707054853/http://www.pnas.org/content/14/8/627 | archivedate = 7 July 2017 | df = dmy-all }}</ref> ] and Harold Mott-Smith, both of whom worked with Irving Langmuir in the 1920s, recall that Langmuir first used the word "plasma" in analogy with blood.<ref>{{cite article |first=Lewi |last=Tonks |title=The birth of "plasma" |year=1967 |journal=American Journal of Physics |volume=35 |pages=857–858 |doi=10.1119/1.1974266|bibcode=1967AmJPh..35..857T }}</ref><ref>{{cite book|author=Brown, Sanborn C.|chapter=Chapter 1: A Short History of Gaseous Electronics|editors=HIRSH, Merle N. e OSKAM, H. J.|title=Gaseous Electronics|volume=1|publisher=Academic Press|date=1978|isbn=978-0-12-349701-7|url=https://books.google.com/?id=C1UmeQ_E0_AC&pg=PA1#v=onepage&q=blood&f=false|deadurl=no|archiveurl=https://web.archive.org/web/20171023230956/https://books.google.co.uk/books?hl=en&lr=&id=C1UmeQ_E0_AC&oi=fnd&pg=PA1&ots=vwabB53YqL&sig=SI8DiBRSQI_yGy_DrspkxNLR0rs#v=onepage&q=blood&f=false|archivedate=23 October 2017|df=dmy-all}}</ref> Mott-Smith recalls, in particular, that the transport of electrons from thermionic filaments reminded Langmuir of "the way blood plasma carries red and white corpuscles and germs."<ref>{{cite article |first=Harold M.|last=Mott-Smith |journal=Nature |volume=233 |page=219 |year=1971 |title=History of "plasmas" |url=https://www.nature.com/nature/journal/v233/n5316/pdf/233219a0.pdf|bibcode=1971Natur.233..219M |doi=10.1038/233219a0 }}</ref>
Systematic studies of plasma began with the research of ] and his colleagues in the 1920s. Langmuir also introduced the term "plasma" as a description of ionized gas in 1928:<ref name="langmuir1928">{{Cite journal | last1 = Langmuir | first1 = I. | title = Oscillations in Ionized Gases | doi = 10.1073/pnas.14.8.627 | journal = Proceedings of the National Academy of Sciences | volume = 14 | issue = 8 | pages = 627–637 | year = 1928 | pmid = 16587379| pmc = 1085653| bibcode = 1928PNAS...14..627L | df = dmy-all | doi-access = free }}</ref>


{{Blockquote|Except near the electrodes, where there are ''sheaths'' containing very few electrons, the ionized gas contains ions and electrons in about equal numbers so that the resultant space charge is very small. We shall use the name ''plasma'' to describe this region containing balanced charges of ions and electrons.}}
Langmuir described the plasma he observed as follows:
:"''Except near the electrodes, where there are ''sheaths'' containing very few electrons, the ionised gas contains ions and electrons in about equal numbers so that the resultant space charge is very small. We shall use the name ''plasma'' to describe this region containing balanced charges of ions and electrons.''"<ref name="langmuir1928" />


] and Harold Mott-Smith, both of whom worked with Langmuir in the 1920s, recall that Langmuir first used the term by analogy with the ].<ref>{{cite journal |first=Lewi |last=Tonks |title=The birth of "plasma" |year=1967 |journal=American Journal of Physics |volume=35 |issue=9 |pages=857–858 |doi=10.1119/1.1974266|bibcode=1967AmJPh..35..857T }}</ref><ref>{{cite book|author=Brown, Sanborn C.|chapter=Chapter 1: A Short History of Gaseous Electronics|editor1=Hirsh, Merle N. |editor2=Oskam, H. J.|title=Gaseous Electronics|volume=1|publisher=Academic Press|date=1978|isbn=978-0-12-349701-7|chapter-url=https://books.google.com/books?id=C1UmeQ_E0_AC&pg=PA1|url-status=live|archive-url=https://web.archive.org/web/20171023230956/https://books.google.co.uk/books?hl=en&lr=&id=C1UmeQ_E0_AC&oi=fnd&pg=PA1&ots=vwabB53YqL&sig=SI8DiBRSQI_yGy_DrspkxNLR0rs#v=onepage&q=blood&f=false|archive-date=23 October 2017}}</ref> Mott-Smith recalls, in particular, that the transport of electrons from thermionic filaments reminded Langmuir of "the way blood plasma carries red and white corpuscles and germs."<ref>{{cite journal |first=Harold M.|last=Mott-Smith |journal=Nature |volume=233 |issue=5316 |page=219 |year=1971 |title=History of "plasmas" |bibcode=1971Natur.233..219M |doi=10.1038/233219a0 |pmid=16063290 |doi-access=free }}</ref>
{{Continuum mechanics}}


{{Continuum mechanics|fluid}}
==Properties and parameters==
] of the Earth's ], showing oxygen, helium, and hydrogen ions that gush into space from regions near the Earth's poles. The faint yellow area shown above the north pole represents gas lost from Earth into space; the green area is the ], where plasma energy pours back into the atmosphere.<ref>Plasma fountain {{webarchive|url=https://web.archive.org/web/20080906131534/http://pwg.gsfc.nasa.gov/istp/news/9812/solar1.html |date=6 September 2008 }}, press release: {{webarchive|url=https://web.archive.org/web/20090320143601/http://pwg.gsfc.nasa.gov/istp/news/9812/solarwind.html |date=20 March 2009 }}</ref>]]


===Definition=== ==Definitions==
===The fourth state of matter===
Plasma is called the ''fourth ]'' after ], ], and ].<ref>{{cite book
|last = Frank-Kamenetskii
|first = David A.
|author-link = David A. Frank-Kamenetskii
|orig-year = 1961–1963
|year = 1972
|edition = 3rd
|title = Plasma-The Fourth State of Matter
|language = en
|publisher = Plenum Press
|url = https://books.google.com/books?id=Q_vpBwAAQBAJ&q=%22Plasma-The+Fourth+State+of+Matter%22+Frank-Kamenetskii
|place = New York
|url-status = live
|archive-url = https://web.archive.org/web/20180115215631/https://books.google.com/books?id=Q_vpBwAAQBAJ&printsec=frontcover&dq=%22Plasma-The+Fourth+State+of+Matter%22+Frank-Kamenetskii&hl=en&sa=X&ved=0ahUKEwi8gerahpbXAhXT31QKHdlfB5oQ6AEIKDAA
|archive-date = 15 January 2018
|df = dmy-all
|isbn = 9781468418965
}}</ref><ref>Yaffa Eliezer, Shalom Eliezer, ''The Fourth State of Matter: An Introduction to the Physics of Plasma'', Publisher: Adam Hilger, 1989, {{ISBN|978-0-85274-164-1}}, 226 pages, page 5</ref><ref>{{cite book|author=Bittencourt, J.A.|title=Fundamentals of Plasma Physics|publisher=Springer|date=2004|isbn=9780387209753|page=1|url=https://books.google.com/books?id=qCA64ys-5bUC&pg=PA1|url-status=live|archive-url=https://web.archive.org/web/20170202072845/https://books.google.com/books?id=qCA64ys-5bUC&pg=PA1|archive-date=2 February 2017}}</ref> It is a state of matter in which an ] substance becomes highly ] to the point that long-range ] dominate its behaviour.<ref name="Chen, Francis F. 2016 2–3">{{cite book | title=Introduction to Plasma Physics and controlled fusion | author=Chen, Francis F. | year=1984 | publisher=Springer International Publishing | url=https://books.google.com/books?id=WGbaBwAAQBAJ&q=editions:9PGss7GnX-MC | pages=2–3 | url-status=live | archive-url=https://web.archive.org/web/20180115215631/https://books.google.com/books?id=WGbaBwAAQBAJ&printsec=frontcover&dq=editions:9PGss7GnX-MC&hl=en&sa=X&ved=0ahUKEwimuOfm_pXXAhVrzFQKHTrOCaUQ6AEIKDAA | archive-date=15 January 2018 | df=dmy-all | isbn=9781475755954 }}</ref><ref name="Freidberg, Jeffrey P. 2008 121">{{cite book | title=Plasma Physics and Fusion Energy | author=Freidberg, Jeffrey P. | year=2008 | publisher=Cambridge University Press | url=https://books.google.com/books?id=Vyoe88GEVz4C | page=121 | url-status=live | archive-url=https://web.archive.org/web/20161224204205/https://books.google.com/books?id=Vyoe88GEVz4C | archive-date=24 December 2016 | df=dmy-all | isbn=9781139462150 }}</ref>


Plasma is typically an electrically quasineutral medium of unbound positive and negative ]s (i.e., the overall charge of a plasma is roughly zero). Although these particles are unbound, they are not "free" in the sense of not experiencing forces. Moving charged particles generate ]s, and any movement of a ] plasma particle affects and is affected by the ] created by the other charges. In turn, this governs collective behaviour with many degrees of variation.<ref name="Sturrock">{{cite book |title=Plasma Physics: An Introduction to the Theory of Astrophysical, Geophysical & Laboratory Plasmas |last=Sturrock |first=Peter A. |date=1994 |publisher=Cambridge University Press |isbn=978-0-521-44810-9}}</ref><ref>{{cite book |title=The Framework of Plasma Physics |author=Hazeltine, R.D. |author2=Waelbroeck, F.L. |date=2004 |publisher=Westview Press |isbn=978-0-7382-0047-7}}
Plasma is a ] in which an ionised gaseous substance becomes highly ] to the point that long-range ] dominate the behaviour of the matter.<ref name="Chen, Francis F. 2016 2–3">{{cite book | title=Introduction to Plasma Physics and controlled fusion | author=Chen, Francis F. | year=1984 | publisher=Springer International Publishing | url=https://books.google.com/?id=WGbaBwAAQBAJ&printsec=frontcover&dq=editions:9PGss7GnX-MC#v=onepage&q&f=false | pages=2–3 | deadurl=no | archiveurl=https://web.archive.org/web/20180115215631/https://books.google.com/books?id=WGbaBwAAQBAJ&printsec=frontcover&dq=editions:9PGss7GnX-MC&hl=en&sa=X&ved=0ahUKEwimuOfm_pXXAhVrzFQKHTrOCaUQ6AEIKDAA#v=onepage&q&f=false | archivedate=15 January 2018 | df=dmy-all | isbn=9781475755954 }}</ref><ref name="Freidberg, Jeffrey P. 2008 121">{{cite book | title=Plasma Physics and Fusion Energy | author=Freidberg, Jeffrey P. | year=2008 | publisher=Cambridge University Press | url=https://books.google.com/books?id=Vyoe88GEVz4C | page=121 | deadurl=no | archiveurl=https://web.archive.org/web/20161224204205/https://books.google.com/books?id=Vyoe88GEVz4C | archivedate=24 December 2016 | df=dmy-all | isbn=9781139462150 }}</ref> The plasma state can be contrasted with the ]: ], ], and ].
</ref>


Plasma is distinct from the other states of matter. In particular, describing a low-density plasma as merely an "ionized gas" is wrong and misleading, even though it is similar to the gas phase in that both assume no definite shape or volume. The following table summarizes some principal differences:
Plasma is an electrically neutral medium of unbound positive and negative particles (i.e. the overall charge of a plasma is roughly zero). Although these particles are unbound, they are not "free" in the sense of not experiencing forces. Moving charged particles generate an electric current within a magnetic field, and any movement of a charged plasma particle affects and is affected by the fields created by the other charges. In turn this governs collective behaviour with many degrees of variation.<ref name="Sturrock">{{cite book |title=Plasma Physics: An Introduction to the Theory of Astrophysical, Geophysical & Laboratory Plasmas |last=Sturrock |first=Peter A. |date=1994 |publisher=Cambridge University Press |isbn=978-0-521-44810-9}}</ref><ref>{{cite book |title=The Framework of Plasma Physics |author=Hazeltine, R.D. |author2=Waelbroeck, F.L. |date=2004 |publisher=Westview Press |isbn=978-0-7382-0047-7}}
</ref> Three factors define a plasma:<ref name="Hazeltine">{{cite book|author=Dendy, R. O.|title=Plasma Dynamics|url=https://books.google.com/?id=puuQM4Dx0zYC&pg=PR19&dq=plasma+dynamics+dendy#v=onepage&q&f=false|publisher=Oxford University Press|date=1990|isbn=978-0-19-852041-2|deadurl=no|archiveurl=https://web.archive.org/web/20180115215631/https://books.google.com/books?id=puuQM4Dx0zYC&pg=PR19&dq=plasma+dynamics+dendy&hl=en&sa=X&ved=0ahUKEwjlvfbU_JXXAhVJxVQKHVSwC5kQ6AEILTAB#v=onepage&q&f=false|archivedate=15 January 2018|df=dmy-all}}</ref><ref>{{cite book|author=Hastings, Daniel|author2=Garrett, Henry|last-author-amp=yes |title=Spacecraft-Environment Interactions|isbn=978-0-521-47128-2|publisher=Cambridge University Press|date=2000}}</ref>


{| class="wikitable"
#'''The plasma approximation''': The plasma approximation applies when the plasma parameter, Λ,<ref>{{Cite book|url=https://books.google.com/?id=WGbaBwAAQBAJ&printsec=frontcover&dq=editions:9PGss7GnX-MC#v=onepage&q&f=false|title=Introduction to plasma physics and controlled fusion|last=1929-|first=Chen, Francis F.,|date=1984|publisher=Plenum Press|others=Chen, Francis F., 1929-|year=|isbn=978-0306413322|edition=2nd|location=New York|pages=|oclc=9852700|deadurl=no|archiveurl=https://web.archive.org/web/20180115215631/https://books.google.com/books?id=WGbaBwAAQBAJ&printsec=frontcover&dq=editions:9PGss7GnX-MC&hl=en&sa=X&ved=0ahUKEwimuOfm_pXXAhVrzFQKHTrOCaUQ6AEIKDAA#v=onepage&q&f=false|archivedate=15 January 2018|df=dmy-all}}</ref> representing the number of charge carriers within a sphere (called the Debye sphere whose radius is the Debye screening length) surrounding a given charged particle, is sufficiently high as to shield the electrostatic influence of the particle outside of the sphere.<ref name="Chen, Francis F. 2016 2–3"/><ref name="Freidberg, Jeffrey P. 2008 121"/>
|-
#'''Bulk interactions''': The Debye screening length (defined above) is short compared to the physical size of the plasma. This criterion means that interactions in the bulk of the plasma are more important than those at its edges, where boundary effects may take place. When this criterion is satisfied, the plasma is quasineutral.<ref>{{Cite web|url=http://www.plasma-universe.com/Quasi-neutrality|title=Quasi-neutrality - The Plasma Universe theory (Misplaced Pages-like Encyclopedia)|website=www.plasma-universe.com|language=en|access-date=2017-10-25|deadurl=no|archiveurl=https://web.archive.org/web/20171026001653/http://www.plasma-universe.com/Quasi-neutrality|archivedate=26 October 2017|df=dmy-all}}</ref>
! {{diagonal split header|Property|State}} !! Gas !! Plasma
#'''Plasma frequency''': The electron plasma frequency (measuring ]s of the electrons) is large compared to the electron-neutral collision frequency (measuring frequency of collisions between electrons and neutral particles). When this condition is valid, electrostatic interactions dominate over the processes of ordinary gas kinetics.<ref>{{Cite web|url=http://homepage.physics.uiowa.edu/~rmerlino/129Fall12/129_Fall_2012%20Daily%20Topics.htm|title=Plasma Oscillations— An application of electrostatics and classical mechanics|last=Merlino|first=Robert L.|date=October 3, 2012|website=homepage.physics.uiowa.edu|pages=See October 3 notes|archive-url=https://web.archive.org/web/20171026002410/http://homepage.physics.uiowa.edu/~rmerlino/129Fall12/129_Fall_2012%20Daily%20Topics.htm|archive-date=26 October 2017|dead-url=no|access-date=2017-10-25|df=dmy-all}}</ref>
|-
! Interactions
| '''Short-range''': Two-particle (binary) ]s are the rule.
| '''Long-range''': Collective motion of particles is ubiquitous in plasma, resulting in various ] and other types of collective phenomena.
|-
! Electrical conductivity
| '''Very low''': Gases are excellent ] up to electric field strengths of tens of kilovolts per centimetre.<ref>{{cite web
| url=https://hypertextbook.com/facts/2000/AliceHong.shtml
| title=Dielectric Strength of Air
| first=Alice
| last=Hong
| year=2000
| website=The Physics Factbook
| editor-last=Elert
| editor-first=Glenn
| access-date=6 July 2018
}}</ref>
| '''Very high''': For many purposes, the conductivity of a plasma may be treated as infinite.
|-
! Independently acting species
| '''One''': All gas particles behave in a similar way, largely influenced by collisions with one another and by ].
| '''Two or more''': ]s and ]s possess different ]s and vastly different masses, so that they behave differently in many circumstances, with various types of plasma-specific waves and ] emerging as a result.
|}


===Temperature=== ===Ideal plasma===
Three factors define an ideal plasma:<ref name="Hazeltine">{{cite book|author=Dendy, R. O.|title=Plasma Dynamics|url=https://books.google.com/books?id=puuQM4Dx0zYC&q=plasma+dynamics+dendy&pg=PR19|publisher=Oxford University Press|date=1990|isbn=978-0-19-852041-2|url-status=live|archive-url=https://web.archive.org/web/20180115215631/https://books.google.com/books?id=puuQM4Dx0zYC&pg=PR19&dq=plasma+dynamics+dendy&hl=en&sa=X&ved=0ahUKEwjlvfbU_JXXAhVJxVQKHVSwC5kQ6AEILTAB|archive-date=15 January 2018}}</ref><ref>{{cite book|author=Hastings, Daniel|author2=Garrett, Henry|name-list-style=amp |title=Spacecraft-Environment Interactions|isbn=978-0-521-47128-2|publisher=Cambridge University Press|date=2000}}</ref>
Plasma temperature is commonly measured in ] or ]s and is, informally, a measure of the thermal kinetic energy per particle. High temperatures are usually needed to sustain ionisation, which is a defining feature of a plasma. The degree of plasma ionisation is determined by the ] relative to the ] (and more weakly by the density), in a relationship called the ]. At low temperatures, ions and electrons tend to recombine into bound states—atoms<ref name="Nicholson">{{cite book |title=Introduction to Plasma Theory |last=Nicholson |first= Dwight R. |date=1983 |publisher=John Wiley & Sons |isbn=978-0-471-09045-8}}</ref>—and the plasma will eventually become a gas.


*'''The plasma approximation''': The plasma approximation applies when the ] Λ,<ref>{{Cite book|url=https://books.google.com/books?id=WGbaBwAAQBAJ&q=editions:9PGss7GnX-MC|title=Introduction to plasma physics and controlled fusion|author=Chen, Francis F.|date=1984|publisher=Plenum Press|others=Chen, Francis F., 1929-|isbn=978-0306413322|edition=2nd|location=New York|oclc=9852700|url-status=live|archive-url=https://web.archive.org/web/20180115215631/https://books.google.com/books?id=WGbaBwAAQBAJ&printsec=frontcover&dq=editions:9PGss7GnX-MC&hl=en&sa=X&ved=0ahUKEwimuOfm_pXXAhVrzFQKHTrOCaUQ6AEIKDAA|archive-date=15 January 2018}}</ref> representing the number of charge carriers within the ] is much higher than unity.<ref name="Chen, Francis F. 2016 2–3"/><ref name="Freidberg, Jeffrey P. 2008 121"/> It can be readily shown that this criterion is equivalent to smallness of the ratio of the plasma electrostatic and thermal energy densities. Such plasmas are called weakly coupled.<ref>{{Cite book| publisher = WORLD SCIENTIFIC| isbn = 978-981-02-3305-1|id={{isbnt| 978-981-281-554-5}}| last1 = Fortov| first1 = Vladimir E| last2 = Iakubov| first2 = Igor T| title = The Physics of Non-Ideal Plasma| access-date = 19 March 2021| date = November 1999| doi = 10.1142/3634| url = http://www.worldscientific.com/worldscibooks/10.1142/3634}}</ref>
In most cases the electrons are close enough to ] that their temperature is relatively well-defined, even when there is a significant deviation from a ] energy ], for example, due to ], energetic particles, or strong ]. Because of the large difference in mass, the electrons come to thermodynamic equilibrium amongst themselves much faster than they come into equilibrium with the ions or neutral atoms. For this reason, the ion temperature may be very different from (usually lower than) the electron temperature. This is especially common in weakly ionised technological plasmas, where the ions are often near the ].
*'''Bulk interactions''': The ] is much smaller than the physical size of the plasma. This criterion means that interactions in the bulk of the plasma are more important than those at its edges, where boundary effects may take place. When this criterion is satisfied, the plasma is quasineutral.<ref>{{Cite web|url=http://www.plasma-universe.com/Quasi-neutrality|title=Quasi-neutrality - The Plasma Universe theory (Misplaced Pages-like Encyclopedia)|website=www.plasma-universe.com|language=en|access-date=25 October 2017|url-status=live|archive-url=https://web.archive.org/web/20171026001653/http://www.plasma-universe.com/Quasi-neutrality|archive-date=26 October 2017}}</ref>
*'''Collisionlessness''': The electron plasma frequency (measuring ]s of the electrons) is much larger than the electron–neutral collision frequency. When this condition is valid, electrostatic interactions dominate over the processes of ordinary gas kinetics. Such plasmas are called collisionless.<ref>{{Cite journal| doi = 10.1070/PU1997v040n01ABEH000200| issn = 1063-7869| volume = 40| issue = 1| pages = 21–51| last = Klimontovich| first = Yu L.| title = Physics of collisionless plasma| journal = Physics-Uspekhi| access-date = 19 March 2021| date = 31 January 1997| s2cid = 250739485| url = http://iopscience.iop.org/article/10.1070/PU1997v040n01ABEH000200/meta}}</ref>


===Non-neutral plasma===
====Fully vs. partially (weakly) ionized gases====
{{main|Degree of ionization}} {{main|Non-neutral plasmas}}
The strength and range of the electric force and the good conductivity of plasmas usually ensure that the densities of positive and negative charges in any sizeable region are equal ("quasineutrality"). A plasma with a significant excess of charge density, or, in the extreme case, is composed of a single species, is called a ]. In such a plasma, electric fields play a dominant role. Examples are charged ]s, an electron cloud in a ] and positron plasmas.<ref>{{Cite journal | last1 = Greaves | first1 = R. G. | last2 = Tinkle | first2 = M. D. | last3 = Surko | first3 = C. M. | doi = 10.1063/1.870693 | title = Creation and uses of positron plasmas | journal = Physics of Plasmas | volume = 1 | issue = 5 | pages = 1439 | year = 1994 |bibcode = 1994PhPl....1.1439G }}</ref>
{{see also|Spitzer resistivity}}
For plasma to exist, ] is necessary. The term "plasma density" by itself usually refers to the "electron density", that is, the number of free electrons per unit volume. The ] of a plasma is the proportion of atoms that have lost or gained electrons, and is controlled by the electron and ion temperatures and electron-ion vs electron-neutral collision frequencies. The degree of ionisation, <math>\alpha</math>, is defined as <math>\alpha = \frac{n_i}{n_i + n_n}</math>, where <math>n_i</math> is the number density of ions and <math>n_n</math> is the number density of neutral atoms. The ''electron density'' is related to this by the average charge state{{Explain|date=August 2018}} <math>\langle Z\rangle</math> of the ions through <math>n_e = \langle Z\rangle n_i</math>, where <math>n_e</math> is the number density of electrons.


===Dusty plasma===
In a plasma, the electron-ion collision frequency <math>\nu_{ei}</math> is much greater than the electron-neutral collision frequency <math>\nu_{en}</math>. Therefore, with a weak degree of ionization <math>\alpha</math>, the electron-ion collision frequency can equal the electron-neutral collision frequency: <math>\nu_{ei} = \nu_{en}</math> is the limit separating a plasma from being partially or fully ionized.
{{main|Dusty plasma}}
A ] contains tiny charged particles of dust (typically found in space). The dust particles acquire high charges and interact with each other. A plasma that contains larger particles is called grain plasma. Under laboratory conditions, dusty plasmas are also called ''complex plasmas''.<ref>{{cite journal |last1=Morfill |first1=G. E. |title= Complex plasmas: An interdisciplinary research field |journal=Reviews of Modern Physics |volume=81 |date=2009 |pages=1353–1404 |doi=10.1103/RevModPhys.81.1353|bibcode = 2009RvMP...81.1353M |first2=Alexei V. |last2=Ivlev |issue=4 }}</ref>


==Properties and parameters==
* The term ''fully ionized gas'' introduced by ] does not mean the degree of ionization is unity, but only that the plasma is in a ''Coulomb-collision dominated regime'', i.e. when <math>\nu_{ei} > \nu_{en}</math>, which can correspond to a degree of ionization as low as 0.01%.<ref name="Chapman 1980">{{cite book |last=Chapman |first=Brian |date=25 September 1980 |title=Glow Discharge Processes: Sputtering and Plasma Etching |url=https://fr.scribd.com/document/150525600/Brian-Chapman-Glow-Discharge-Processes |location=New York |publisher=John Wiley & Sons |page=49 |chapter=Chapter 3: Plasmas |isbn=978-0471078289}}</ref>
] of the Earth's ], showing oxygen, helium, and hydrogen ions that gush into space from regions near the Earth's poles. The faint yellow area shown above the north pole represents gas lost from Earth into space; the green area is the ], where plasma energy pours back into the atmosphere.<ref>{{Cite web|title=Plasma Fountain|url=https://pwg.gsfc.nasa.gov/istp/news/9812/solar1.html|access-date=10 February 2023|website=pwg.gsfc.nasa.gov}}</ref>]]


===Density and ionization degree===
* A ''partially'' or ''weakly ionized gas'' means the plasma is not dominated by ]s, i.e. when <math>\nu_{ei} < \nu_{en}</math>.
For plasma to exist, ] is necessary. The term "plasma density" by itself usually refers to the electron density <math>n_e</math>, that is, the number of charge-contributing electrons per unit volume. The degree of ionization <math>\alpha</math> is defined as fraction of neutral particles that are ionized:


<math display="block">\alpha = \frac{n_i}{n_i + n_n},</math>
Most of "technological" (engineered) plasmas are weakly ionized gases.


where <math>n_i</math> is the ion density and <math>n_n</math> the neutral density (in number of particles per unit volume). In the case of fully ionized matter, <math>\alpha = 1</math>. Because of the quasineutrality of plasma, the electron and ion densities are related by <math>n_e = \langle Z_i\rangle n_i</math>, where <math>\langle Z_i\rangle</math> is the average ion charge (in units of the ]).
====Thermal vs. nonthermal (cold) plasmas====
{{main|Nonthermal plasma}}
{{see also|Anisothermal plasma}}
Based on the relative temperatures of the electrons, ions and neutrals, plasmas are classified as "thermal" or "non-thermal" (also referred to as "cold plasmas").


===Temperature===
* ''Thermal plasmas'' have electrons and the heavy particles at the same temperature, i.e. they are in thermal equilibrium with each other.
Plasma temperature, commonly measured in ] or ]s, is a measure of the thermal kinetic energy per particle. High temperatures are usually needed to sustain ionization, which is a defining feature of a plasma. The degree of plasma ionization is determined by the ] relative to the ] (and more weakly by the density). In ], the relationship is given by the ]. At low temperatures, ions and electrons tend to recombine into bound states—atoms<ref name="Nicholson">{{cite book |title=Introduction to Plasma Theory |last=Nicholson |first= Dwight R. |date=1983 |publisher=John Wiley & Sons |isbn=978-0-471-09045-8}}</ref>—and the plasma will eventually become a gas.


In most cases, the electrons and heavy plasma particles (ions and neutral atoms) separately have a relatively well-defined temperature; that is, their energy ] is close to a ] even in the presence of strong ] or ] fields. However, because of the large difference in mass between electrons and ions, their temperatures may be different, sometimes significantly so. This is especially common in weakly ionized technological plasmas, where the ions are often near the ] while electrons reach thousands of kelvin.<ref>{{Cite book |last=Hamrang |first=Abbas |title=Advanced Non-Classical Materials with Complex Behavior: Modeling and Applications, Volume 1 |publisher=CRC Press |year=2014 |pages=10}}</ref> The opposite case is the ] plasma where the ion temperature may exceed that of electrons.<ref>{{Cite journal| doi = 10.1063/5.0009432| issn = 1070-664X| volume = 27| issue = 6| pages = 060901| last = Maron| first = Yitzhak| title = Experimental determination of the thermal, turbulent, and rotational ion motion and magnetic field profiles in imploding plasmas| journal = Physics of Plasmas| date = 1 June 2020| bibcode = 2020PhPl...27f0901M| doi-access = free}}</ref>
* ''Nonthermal plasmas'' on the other hand are non-equilibrium ionized gases, with two temperatures: ions and neutrals stay at a low temperature (sometimes ]), whereas electrons are much hotter. (<math>T_e \gg T_n</math>).<ref>von Engel, A. and Cozens, J.R. (1976) "Flame Plasma" in ''Advances in electronics and electron physics'', L. L. Marton (ed.), Academic Press, {{ISBN|978-0-12-014520-1}}, {{webarchive|url=https://web.archive.org/web/20161202013244/https://books.google.com/books?id=0Mndi2cCMuUC&lpg=PA99 |date=2 December 2016 }}</ref> A kind of common nonthermal plasma is the ] within a ], where the "electrons gas" reaches a temperature of 10,000 kelvins while the rest of the gas stays barely above room temperature, so the ] can even be touched with hands while operating.


{{see also|Nonthermal plasma|Anisothermal plasma}}
A particular and unusual case of "inverse" nonthermal plasma is the very high temperature plasma produced by the ], where ions are much hotter than electrons.<ref name="haines_a">{{cite journal
|last1=Haines |first1=M. G.
|last2=LePell |first2=P. D.
|last3=Coverdale |first3=C. A.
|last4=Jones |first4=B.
|last5=Deeney |first5=C.
|last6=Apruzese |first6=J. P.
|title=Ion Viscous Heating in a Magnetohydrodynamically Unstable Pinch at Over 2 × 10{{sup|9}} Kelvin
|date=23 February 2006
|journal=Physical Review Letters
|volume=96
|issue=7
|pages=075003
|url=http://ayuba.fr/pdf/haines2006.pdf
|format=PDF
|doi=10.1103/PhysRevLett.96.075003
|pmid=16606100
|bibcode=2006PhRvL..96g5003H}}</ref><ref name="haines_b">{{cite web|url=http://ayuba.fr/pdf/comments_on_haines_paper.pdf |last1=Petit |first1=J.-P. |format=PDF |title=The Z Machine: Over two billion degrees! Malcolm Haines' paper |accessdate=2018-04-07}}</ref>


===Plasma potential=== ===Plasma potential===
] as an example of plasma present at Earth's surface: ] as an example of plasma present at Earth's surface:
Typically, lightning discharges 30 kiloamperes at up to 100 megavolts, and emits radio waves, light, X- and even gamma rays.<ref>See {{webarchive|url=https://web.archive.org/web/20140707164546/http://www.nasa.gov/vision/universe/solarsystem/rhessi_tgf.html |date=7 July 2014 }}</ref> Plasma temperatures can approach 30000 K and electron densities may exceed 10<sup>24</sup> m<sup>−3</sup>.]] Typically, lightning discharges 30 kiloamperes at up to 100 megavolts, and emits radio waves, light, X- and even gamma rays.<ref>{{Cite web | author= NASA Administrator |date=7 June 2013 |title=Flashes in the Sky: Earth's Gamma-Ray Bursts Triggered by Lightning |url=http://www.nasa.gov/vision/universe/solarsystem/rhessi_tgf.html |access-date=10 February 2023 |website=NASA |language=en}}</ref> Plasma temperatures can approach 30000 K and electron densities may exceed 10<sup>24</sup> m<sup>−3</sup>.]]
Since plasmas are very good ]s, electric potentials play an important role.{{clarify|what role?|date=October 2017}} The average potential in the space between charged particles, independent of how it can be measured, is called the "plasma potential", or the "space potential". If an electrode is inserted into a plasma, its potential will generally lie considerably below the plasma potential due to what is termed a ]. The good electrical conductivity of plasmas makes their electric fields very small. This results in the important concept of "quasineutrality", which says the density of negative charges is approximately equal to the density of positive charges over large volumes of the plasma (<math>n_e = \langle Z\rangle n_i</math>), but on the scale of the ] there can be charge imbalance. In the special case that '']'' are formed, the charge separation can extend some tens of Debye lengths.{{citation needed|date=February 2017}} Since plasmas are very good ]s, electric potentials play an important role.{{clarify|what role?|date=October 2017}} The average potential in the space between charged particles, independent of how it can be measured, is called the "plasma potential", or the "space potential". If an electrode is inserted into a plasma, its potential will generally lie considerably below the plasma potential due to what is termed a ]. The good electrical conductivity of plasmas makes their electric fields very small. This results in the important concept of "quasineutrality", which says the density of negative charges is approximately equal to the density of positive charges over large volumes of the plasma (<math>n_e = \langle Z\rangle n_i</math>), but on the scale of the ], there can be charge imbalance. In the special case that '']'' are formed, the charge separation can extend some tens of Debye lengths.<ref>{{Cite journal| doi = 10.1007/BF00642580 | issn = 1572-946X| volume = 55| issue = 1| pages = 59–83| last = Block| first = Lars P.| title = A double layer review| journal = Astrophysics and Space Science| accessdate = 15 July 2021| date = 1978| s2cid = 122977170| url = https://doi.org/10.1007/BF00642580}}</ref>


The magnitude of the potentials and electric fields must be determined by means other than simply finding the net ]. A common example is to assume that the electrons satisfy the ]: The magnitude of the potentials and electric fields must be determined by means other than simply finding the net ]. A common example is to assume that the electrons satisfy the ]:
:<math>n_e \propto e^{e\Phi/k_BT_e}.</math> <math display="block">n_e \propto \exp(e\Phi/k_\text{B} T_e).</math>


Differentiating this relation provides a means to calculate the electric field from the density: Differentiating this relation provides a means to calculate the electric field from the density:
:<math>\vec{E} = (k_BT_e/e)(\nabla n_e/n_e).</math> <math display="block">\vec{E} = \frac{k_\text{B} T_e}{e} \frac{\nabla n_e}{n_e}.</math>


It is possible to produce a plasma that is not quasineutral. An electron beam, for example, has only negative charges. The density of a non-neutral plasma must generally be very low, or it must be very small, otherwise, it will be dissipated by the repulsive ].<ref>{{Cite book|url=https://www.worldcat.org/oclc/42854229|title=Plasma science : from fundamental research to technological applications|last=|first=|date=1995|publisher=National Academy Press|others=National Research Council (U.S.). Panel on Opportunities in Plasma Science and Technology.|year=|isbn=9780309052313|location=Washington, D.C.|pages=51|oclc=42854229}}</ref> It is possible to produce a plasma that is not quasineutral. An electron beam, for example, has only negative charges. The density of a non-neutral plasma must generally be very low, or it must be very small, otherwise, it will be dissipated by the repulsive ].<ref>{{Cite book|title=Plasma science: from fundamental research to technological applications |date=1995 | publisher=National Academy Press | others=National Research Council (U.S.). Panel on Opportunities in Plasma Science and Technology |isbn=9780309052313 |location=Washington, D.C. |pages=51 |oclc=42854229}}</ref>

In ] plasmas, ] prevents ]s from directly affecting the plasma over large distances, i.e., greater than the ]. However, the existence of charged particles causes the plasma to generate, and be affected by, ]s. This can and does cause extremely complex behaviour, such as the generation of plasma double layers, an object that separates charge over a few tens of ]s. The dynamics of plasmas interacting with external and self-generated ]s are studied in the ] of ].<ref>{{Cite journal |last=Dorch |first=Søren |date=2007-04-13 |title=Magnetohydrodynamics |url=http://www.scholarpedia.org/article/Magnetohydrodynamics |journal=Scholarpedia |language=en |volume=2 |issue=4|pages=2295 |doi=10.4249/scholarpedia.2295 |issn=1941-6016 |deadurl=no |archiveurl=https://web.archive.org/web/20080402043642/http://www.scholarpedia.org/article/Magnetohydrodynamics |archivedate=2 April 2008 |df=dmy-all |bibcode=2007SchpJ...2.2295D}}</ref>


===Magnetization=== ===Magnetization===
Plasma with a magnetic field strong enough to influence the motion of the charged particles is said to be magnetized. A common quantitative criterion is that a particle on average completes at least one gyration around the magnetic field before making a collision, i.e., <math>\omega_{\mathrm{ce}} / v_{\mathrm{coll}} > 1</math>, where <math>\omega_{\mathrm{ce}}</math> is the "electron gyrofrequency" and <math>v_{\mathrm{coll}}</math> is the "electron collision rate". It is often the case that the electrons are magnetized while the ions are not. Magnetized plasmas are '']'', meaning that their properties in the direction parallel to the magnetic field are different from those perpendicular to it. While electric fields in plasmas are usually small due to the high conductivity, the electric field associated with a plasma moving in a magnetic field is given by <math>\mathbf{E} = -v\times\mathbf{B}</math> (where <math>\mathbf{E}</math> is the electric field, <math>\mathbf{v}</math> is the velocity, and <math>\mathbf{B}</math> is the magnetic field), and is not affected by ].<ref>Richard Fitzpatrick, ''Introduction to Plasma Physics'', {{webarchive|url=https://web.archive.org/web/20060301073703/http://farside.ph.utexas.edu/teaching/plasma/lectures/node10.html |date=1 March 2006 }}</ref> The existence of charged particles causes the plasma to generate, and be affected by, ]s. Plasma with a magnetic field strong enough to influence the motion of the charged particles is said to be magnetized. A common quantitative criterion is that a particle on average completes at least one gyration around the magnetic-field line before making a collision, i.e., <math>\nu_{\mathrm{ce}} / \nu_{\mathrm{coll}} > 1</math>, where <math>\nu_{\mathrm{ce}}</math> is the electron ] and <math>\nu_{\mathrm{coll}}</math> is the electron collision rate. It is often the case that the electrons are magnetized while the ions are not. Magnetized plasmas are '']'', meaning that their properties in the direction parallel to the magnetic field are different from those perpendicular to it. While electric fields in plasmas are usually small due to the plasma high conductivity, the electric field associated with a plasma moving with velocity <math>\mathbf{v}</math> in the magnetic field <math>\mathbf{B}</math> is given by the usual ] <math>\mathbf{E} = -\mathbf{v}\times\mathbf{B}</math>, and is not affected by ].<ref>{{Cite web|first=Richard |last=Fitzpatrick |website=Introduction to Plasma Physics |title=Magnetized Plasmas|url=https://farside.ph.utexas.edu/teaching/plasma/lectures/node10.html|access-date=10 February 2023}}</ref>


==Mathematical descriptions==
===Comparison of plasma and gas phases===
] that can develop in a plasma.<ref>{{Cite web|title=chapter 15|url=https://history.nasa.gov/SP-345/ch15.htm#250|access-date=10 February 2023|website=history.nasa.gov|date=January 1976 |last1=Alfven |first1=H. |last2=Arrhenius |first2=G. }}</ref>]]
Plasma is often called the ''fourth state of matter'' after solid, liquids and gases, despite plasma typically being an ionised gas.<ref>{{cite book
{{main|Plasma modeling}}
|last = Frank-Kamenetskii
To completely describe the state of a plasma, all of the particle locations and velocities that describe the electromagnetic field in the plasma region would need to be written down. However, it is generally not practical or necessary to keep track of all the particles in a plasma.{{Citation needed|date=January 2021}} Therefore, plasma physicists commonly use less detailed descriptions, of which there are two main types:
|first = David A.
|authorlink = David A. Frank-Kamenetskii
|orig-year = 1961–1963
|year = 1972
|edition = 3rd
|title = Plasma-The Fourth State of Matter
|language = English translation from Russian
|publisher = Plenum Press
|url = https://books.google.com/?id=Q_vpBwAAQBAJ&printsec=frontcover&dq=%22Plasma-The+Fourth+State+of+Matter%22+Frank-Kamenetskii#v=onepage&q&f=false
|place = New York
|deadurl = no
|archiveurl = https://web.archive.org/web/20180115215631/https://books.google.com/books?id=Q_vpBwAAQBAJ&printsec=frontcover&dq=%22Plasma-The+Fourth+State+of+Matter%22+Frank-Kamenetskii&hl=en&sa=X&ved=0ahUKEwi8gerahpbXAhXT31QKHdlfB5oQ6AEIKDAA#v=onepage&q&f=false
|archivedate = 15 January 2018
|df = dmy-all
|isbn = 9781468418965
}}</ref><ref>Yaffa Eliezer, Shalom Eliezer, ''The Fourth State of Matter: An Introduction to the Physics of Plasma'', Publisher: Adam Hilger, 1989, {{ISBN|978-0-85274-164-1}}, 226 pages, page 5</ref><ref>{{cite book|author=Bittencourt, J.A.|title=Fundamentals of Plasma Physics|publisher=Springer|date=2004|isbn=9780387209753|page=1|url=https://books.google.com/books?id=qCA64ys-5bUC&pg=PA1|deadurl=no|archiveurl=https://web.archive.org/web/20170202072845/https://books.google.com/books?id=qCA64ys-5bUC&pg=PA1|archivedate=2 February 2017|df=dmy-all}}</ref> It is distinct from these and other lower-energy ]. Although it is closely related to the gas phase in that it also has no definite form or volume, it differs in a number of ways, including the following:


===Fluid model===
{| class="wikitable"
Fluid models describe plasmas in terms of smoothed quantities, like density and averaged velocity around each position (see ]). One simple fluid model, ], treats the plasma as a single fluid governed by a combination of ] and the ]. A more general description is the two-fluid plasma,<ref>{{cite journal |last1=Roy |first1=Subrata |last2=Pandey |first2=B. P. |title=Numerical investigation of a Hall thruster plasma |journal=Physics of Plasmas |date=September 2002 |volume=9 |issue=9 |pages=4052–4060 |doi=10.1063/1.1498261|bibcode=2002PhPl....9.4052R |hdl=2027.42/70486 |hdl-access=free }}</ref> where the ions and electrons are described separately. Fluid models are often accurate when collisionality is sufficiently high to keep the plasma velocity distribution close to a ]. Because fluid models usually describe the plasma in terms of a single flow at a certain temperature at each spatial location, they can neither capture velocity space structures like beams or ]s, nor resolve wave-particle effects.{{Citation needed|date=January 2021}}
|-
! Property !! Gas !! Plasma
|-
! ]
| '''Very low''': Air is an excellent insulator until it breaks down into plasma at electric field strengths above 30 kilovolts per centimeter.<ref>{{cite web
| url=https://hypertextbook.com/facts/2000/AliceHong.shtml
| title=Dielectric Strength of Air
| first=Alice
| last=Hong
| year=2000
| website=The Physics Factbook
| editor-last=Elert
| editor-first=Glenn
| accessdate=2018-07-06
}}</ref>
| '''Usually very high''': For many purposes, the conductivity of a plasma may be treated as infinite.
|-
! Independently acting species
| '''One''': All gas particles behave in a similar way, influenced by ] and by ]s with one another.
| '''Two or three''': ]s, ]s, ]s and ]s can be distinguished by the sign and value of their ] so that they behave independently in many circumstances, with different bulk velocities and temperatures, allowing phenomena such as new types of ] and ].
|-
! Velocity distribution
| ''']''': Collisions usually lead to a Maxwellian velocity distribution of all gas particles, with very few relatively fast particles.
| '''Often non-Maxwellian''': Collisional interactions are often weak in hot plasmas and external forcing can drive the plasma far from local equilibrium and lead to a significant population of unusually fast particles.
|-
! Interactions
| '''Binary''': Two-particle collisions are the rule, three-body collisions extremely rare.
| '''Collective''': Waves, or organized motion of plasma, are very important because the particles can interact at long ranges through the electric and magnetic forces.
|}


===Kinetic model===
==Plasmas in space science and astronomy==
Kinetic models describe the particle velocity distribution function at each point in the plasma and therefore do not need to assume a ]. A kinetic description is often necessary for collisionless plasmas. There are two common approaches to kinetic description of a plasma. One is based on representing the smoothed distribution function on a grid in velocity and position. The other, known as the ] (PIC) technique, includes kinetic information by following the trajectories of a large number of individual particles. Kinetic models are generally more computationally intensive than fluid models. The ] may be used to describe the dynamics of a system of charged particles interacting with an electromagnetic field.

In magnetized plasmas, a ] approach can substantially reduce the computational expense of a fully kinetic simulation.{{Citation needed|date=January 2021}}
{{further information|Astrophysical plasma|Interstellar medium|Intergalactic space}}
{{see also|Magnetohydrodynamics}}
Plasmas are by far the most common ] in the universe, both by mass and by volume.<ref>It is assumed that more than 99% the visible universe is made of some form of plasma.{{cite book|author=Gurnett, D. A.|author2=Bhattacharjee, A.|last-author-amp=yes |title=Introduction to Plasma Physics: With Space and Laboratory Applications|date=2005|url=https://books.google.com/?id=VcueZlunrbcC&pg=PA2|page=2|isbn=978-0-521-36483-6|publisher=Cambridge University Press|location=Cambridge, UK}} {{cite book|author=Scherer, K|author2=Fichtner, H|author3=Heber, B|last-author-amp=yes |title=Space Weather: The Physics Behind a Slogan|date=2005|url=https://books.google.com/?id=irHgIUtLi0gC&pg=PA138|page=138|isbn=978-3-540-22907-0|publisher=Springer|location=Berlin}}.</ref>


==Plasma science and technology==
Above the Earth's surface, the ionosphere is a plasma,<ref>{{cite book |last=Kelley |first=M. C. |title=The Earth's Ionosphere: Plasma Physics and Electrodynamics |date=2009 |publisher=Academic Press |isbn=9780120884254 |edition=2nd}}</ref> and the magnetosphere contains plasma.<ref>{{cite journal|last=Russell|first=C.T.|title=The Magnetopause|journal=Physics of Magnetic Flux Ropes|date=1990|pages=439–453|url=http://www-ssc.igpp.ucla.edu/ssc/tutorial/magnetopause.html}}</ref> Within our Solar System, ] is filled with the plasma expelled via the ], extending from the Sun's surface out to the ]. Furthermore, all the distant ]s, and much of ] or ] is also likely filled with plasma, albeit at very low densities. ]s are also observed in ]s around stars or compact objects like ]s, ]s, or ] in close ] systems.<ref>Mészáros, Péter (2010) ''The High Energy Universe: Ultra-High Energy Events in Astrophysics and Cosmology'', Publisher: Cambridge University Press, {{ISBN|978-0-521-51700-3}}, {{webarchive|url=https://web.archive.org/web/20170202061841/https://books.google.com/books?id=NXvE_zQX5kAC&lpg=PA99&dq=%22Black%20hole%22%20plasma%20acreting&pg=PA99 |date=2 February 2017 }}.</ref> Plasma is associated with ejection of material in ], which have been observed with accreting black holes<ref>Raine, Derek J. and Thomas, Edwin George (2010) ''Black Holes: An Introduction'', Publisher: Imperial College Press, {{ISBN|978-1-84816-382-9}}, {{webarchive|url=https://web.archive.org/web/20161202104848/https://books.google.com/books?id=O3puAMw5U3UC&lpg=PA160 |date=2 December 2016 }}</ref> or in active ] like ] that possibly extends out to 5,000 light-years.<ref>Nemiroff, Robert and Bonnell, Jerry (11 December 2004) {{webarchive|url=https://web.archive.org/web/20121018162924/http://apod.nasa.gov/apod/ap041211.html |date=18 October 2012 }}, nasa.gov</ref>


Plasmas are studied by the vast ] of ''plasma science'' or ''plasma physics'', including several sub-disciplines such as ].
==Common plasmas==


Plasmas can appear in nature in various forms and locations, which can be usefully broadly summarised in the following Table: Plasmas can appear in nature in various forms and locations, with a few examples given in the following table:


{{clear}} {{clear}}
Line 235: Line 221:
|- style="vertical-align: top;" |- style="vertical-align: top;"
| |
*Those found in ], including TV screens. *In ], including TV screens.
*Inside ]s (low energy lighting), ]s<ref> {{webarchive|url=https://web.archive.org/web/20080308225731/http://ippex.pppl.gov/fusion/glossary.html |date=8 March 2008 }}. Ippex.pppl.gov. Retrieved on 2011-11-19.</ref> *Inside ]s (low energy lighting), ]s
*Rocket exhaust and ]s *Rocket exhaust and ]s
*The area in front of a ]'s ] during ] into the ] *The area in front of a ]'s ] during ] into the ]
*Plasmas in ] research
*Inside a corona discharge ] generator
*] (sometimes called plasma sphere or plasma ball)
*] research
*]-produced plasmas (LPP), found when high power lasers interact with materials
*The ] in an ], an arc ] or ]
*Plasma ball (sometimes called a plasma sphere or ])
*Arcs produced by ]s (resonant air core transformer or disruptor coil that produces arcs similar to lightning, but with ] rather than ])
*Plasmas used in ] including ], ], ] and ]
*]-produced plasmas (LPP), found when high power lasers interact with materials.
*]s (ICP), formed typically in ] gas for optical emission ] or ]
*Magnetically induced plasmas (MIP), typically produced using microwaves as a resonant coupling method
*]
*]s (CCP)
*]s (DBD)
| |
*] *]
*The ] contains plasma in the Earth's surrounding space environment *The ] contains plasma in the Earth's surrounding space environment
*The ] *The ]
*The ]
*The ] *The ]
*], including ], blue jets, blue starters, gigantic jets, ELVESs
*The ], a plasma fountain
*] (e.g. Blue jets, Blue starters, Gigantic jets, ELVES)
*]
*] *]
*] (if sufficiently hot)
| |
*]s<br />(plasmas heated by ]) *]s (plasmas heated by ])
*The ] *The ]
*The ]<br />(space between planets) *The ] (space between planets)
*The ]<br />(space between star systems) *The ] (space between star systems)
*The ]<br />(space between galaxies) *The ]<br />(space between galaxies)
*]s
*The ]-] ]
*]s
*Interstellar ]e *Interstellar ]e
|} |}


===Space and astrophysics===
==Complex plasma phenomena==


{{further|Astrophysical plasma}}
Although the underlying equations governing plasmas are relatively simple, plasma behaviour is extraordinarily varied and subtle: the emergence of unexpected behaviour from a simple model is a typical feature of a ]. Such systems lie in some sense on the boundary between ordered and disordered behaviour and cannot typically be described either by simple, smooth, mathematical functions, or by pure randomness. The spontaneous formation of interesting spatial features on a wide range of length scales is one manifestation of plasma complexity. The features are interesting, for example, because they are very sharp, spatially intermittent (the distance between features is much larger than the features themselves), or have a ] form. Many of these features were first studied in the laboratory, and have subsequently been recognized throughout the universe. Examples of complexity and complex structures in plasmas include:
Plasmas are by far the most common ] in the universe, both by mass and by volume.<ref>{{Cite book|last1=Gurnett|first1=D. A.|url=https://books.google.com/books?id=VcueZlunrbcC&pg=PA2%257CPAGE=2%257CISBN=978-0-521-36483-6%257CPUBLISHER|title=Introduction to Plasma Physics: With Space and Laboratory Applications|last2=Bhattacharjee|first2=A.|date=6 January 2005|publisher=Cambridge University Press|isbn=978-0-521-36483-6|language=en}}{{cite book|last1=Scherer |first1=K. |last2=Fichtner |first2=H. |last3=Heber |first3=B. |title=Space Weather: The Physics Behind a Slogan|date=2005|url=https://books.google.com/books?id=irHgIUtLi0gC&pg=PA138|page=138|isbn=978-3-540-22907-0|publisher=Springer|location=Berlin}}.</ref>


Above the Earth's surface, the ionosphere is a plasma,<ref>{{cite book |last=Kelley |first=M. C. |title=The Earth's Ionosphere: Plasma Physics and Electrodynamics |date=2009 |publisher=Academic Press |isbn=9780120884254 |edition=2nd}}</ref> and the magnetosphere contains plasma.<ref>{{cite book|last=Russell|first=C.T. |title=Physics of Magnetic Flux Ropes |chapter=The magnetopause |series=Geophysical Monograph Series|date=1990|volume=58|pages=439–453|doi=10.1029/GM058p0439|bibcode=1990GMS....58..439R|isbn=0-87590-026-7|url=http://www-ssc.igpp.ucla.edu/ssc/tutorial/magnetopause.html|access-date=25 August 2018|archive-url=https://web.archive.org/web/20120503220342/http://www-ssc.igpp.ucla.edu/ssc/tutorial/magnetopause.html|archive-date=3 May 2012|url-status=dead}}</ref> Within our Solar System, ] is filled with the plasma expelled via the ], extending from the Sun's surface out to the ]. Furthermore, all the distant ]s, and much of ] or ] is also filled with plasma, albeit at very low densities. ]s are also observed in ]s around stars or compact objects like ]s, ]s, or ] in close ] systems.<ref>{{Cite book|last=Mészáros|first=Péter|url=https://books.google.com/books?id=NXvE_zQX5kAC&dq=%2522Black%2520hole%2522%2520plasma%2520acreting&pg=PA99|title=The High Energy Universe: Ultra-High Energy Events in Astrophysics and Cosmology|date=16 September 2010|publisher=Cambridge University Press|isbn=978-1-139-49072-6|language=en}}</ref> Plasma is associated with ejection of material in ], which have been observed with accreting black holes<ref>{{Cite book|last1=Raine|first1=Derek J.|url=https://books.google.com/books?id=O3puAMw5U3UC&pg=PA160|title=Black Holes: An Introduction|last2=Thomas|first2=Edwin George|date=2010|publisher=Imperial College Press|isbn=978-1-84816-382-9|language=en}}</ref> or in active ] like ] that possibly extends out to 5,000 light-years.<ref>{{Cite web|title=APOD: 2004 December 11 - M87's Energetic Jet|url=https://apod.nasa.gov/apod/ap041211.html|access-date=10 February 2023|website=apod.nasa.gov}}</ref>
===Filamentation===
Striations or string-like structures,<ref>{{cite journal|author=Dickel, J. R.|bibcode=1990BAAS...22..832D |title=The Filaments in Supernova Remnants: Sheets, Strings, Ribbons, or?|date=1990|journal=Bulletin of the American Astronomical Society|volume= 22|page=832}}</ref> also known as ]s, are seen in many plasmas, like the ], the ],<ref>{{Cite journal | last1 = Grydeland | first1 = T. | doi = 10.1029/2002GL016362 | title = Interferometric observations of filamentary structures associated with plasma instability in the auroral ionosphere | journal = Geophysical Research Letters | volume = 30 | issue = 6 | pages = 1338 | year = 2003 | pmid = | pmc = | bibcode=2003GeoRL..30.1338G}}</ref> ],<ref>{{Cite journal | last1 = Moss | first1 = G. D. | last2 = Pasko | first2 = V. P. | last3 = Liu | first3 = N. | last4 = Veronis | first4 = G. | title = Monte Carlo model for analysis of thermal runaway electrons in streamer tips in transient luminous events and streamer zones of lightning leaders | doi = 10.1029/2005JA011350 | journal = Journal of Geophysical Research | volume = 111 | issue = A2 | pages = A02307 | year = 2006 | pmid = | pmc = | bibcode=2006JGRA..111.2307M}}</ref> ]s, ],<ref>{{cite journal|author=Doherty, Lowell R.|doi=10.1086/148107|title=Filamentary Structure in Solar Prominences|date=1965|journal=The Astrophysical Journal|volume=141|page=251|last2=Menzel|first2=Donald H.|bibcode=1965ApJ...141..251D}}</ref> and ]s.<ref>{{cite web |url=http://seds.lpl.arizona.edu/messier/more/m001_hst.html |title=Hubble views the Crab Nebula M1: The Crab Nebula Filaments |accessdate=2017-01-26 |deadurl=bot: unknown |archiveurl=https://web.archive.org/web/20091005084515/http://seds.lpl.arizona.edu/messier/more/m001_hst.html |archivedate=5 October 2009 |df=dmy-all }}. The University of Arizona</ref> They are sometimes associated with larger current densities, and the interaction with the magnetic field can form a ] structure.<ref>{{Cite journal | last1 = Zhang | first1 = Y. A. | last2 = Song | first2 = M. T. | last3 = Ji | first3 = H. S. | doi = 10.1016/S0275-1062(02)00095-4 | title = A rope-shaped solar filament and a IIIb flare | journal = Chinese Astronomy and Astrophysics | volume = 26 | issue = 4 | pages = 442–450 | year = 2002 | pmid = | pmc = |bibcode = 2002ChA&A..26..442Z }}</ref> High power microwave breakdown at atmospheric pressure also leads to the formation of filamentary structures.<ref name="mwbrkdwn">{{Cite journal | last1 = Boeuf | first1 = J. P. | last2 = Chaudhury | first2 = B. | last3 = Zhu | first3 = G. Q. | title = Theory and Modeling of Self-Organization and Propagation of Filamentary Plasma Arrays in Microwave Breakdown at Atmospheric Pressure | doi = 10.1103/PhysRevLett.104.015002 | journal = Physical Review Letters | volume = 104 | issue = 1 | pages = 015002 | year = 2010 | pmid = 20366367| pmc = | bibcode=2010PhRvL.104a5002B}}</ref> (See also ])

Filamentation also refers to the self-focusing of a high power laser pulse. At high powers, the nonlinear part of the index of refraction becomes important and causes a higher index of refraction in the center of the laser beam, where the laser is brighter than at the edges, causing a feedback that focuses the laser even more. The tighter focused laser has a higher peak brightness (irradiance) that forms a plasma. The plasma has an index of refraction lower than one, and causes a defocusing of the laser beam. The interplay of the focusing index of refraction, and the defocusing plasma makes the formation of a long filament of plasma that can be ] to kilometers in length.<ref>{{Cite book|author=Chin, S. L. |url=http://icpr.snu.ac.kr/resource/wop.pdf/J01/2006/049/S01/J012006049S010281.pdf|journal=Journal of the Korean Physical Society|volume=49|date=2006|page=281|title=Some Fundamental Concepts of Femtosecond Laser Filamentation|bibcode=2008pui3.book..243C|doi=10.1007/978-3-540-73794-0_12|series=Springer Series in Chemical Physics|isbn=978-3-540-73793-3}}</ref> One interesting aspect of the filamentation generated plasma is the relatively low ion density due to defocusing effects of the ionised electrons.<ref>{{Cite journal | last1 = Talebpour | first1 = A. | last2 = Abdel-Fattah | first2 = M. | last3 = Chin | first3 = S. L. | doi = 10.1016/S0030-4018(00)00903-2 | title = Focusing limits of intense ultrafast laser pulses in a high pressure gas: Road to new spectroscopic source | journal = Optics Communications | volume = 183 | issue = 5–6 | pages = 479–484 | year = 2000 | pmid = | pmc = | bibcode=2000OptCo.183..479T}}</ref> (See also ])

===Non-neutral plasma===
The strength and range of the electric force and the good conductivity of plasmas usually ensure that the densities of positive and negative charges in any sizeable region are equal ("quasineutrality"). A plasma with a significant excess of charge density, or, in the extreme case, is composed of a single species, is called a ]. In such a plasma, electric fields play a dominant role. Examples are charged ]s, an electron cloud in a ] and positron plasmas.<ref>{{Cite journal | last1 = Greaves | first1 = R. G. | last2 = Tinkle | first2 = M. D. | last3 = Surko | first3 = C. M. | doi = 10.1063/1.870693 | title = Creation and uses of positron plasmas | journal = Physics of Plasmas | volume = 1 | issue = 5 | pages = 1439 | year = 1994 | pmid = | pmc = |bibcode = 1994PhPl....1.1439G }}</ref>

===Dusty plasma/grain plasma===
A ] contains tiny charged particles of dust (typically found in space). The dust particles acquire high charges and interact with each other. A plasma that contains larger particles is called grain plasma. Under laboratory conditions, dusty plasmas are also called ''complex plasmas''.<ref>{{cite journal |last=Morfill |first=G. E. |title= Complex plasmas: An interdisciplinary research field |journal=Reviews of Modern Physics |volume=81 |date=2009 |pages=1353–1404 |doi=10.1103/RevModPhys.81.1353|bibcode = 2009RvMP...81.1353M |first2=Alexei V. |last2=Ivlev |issue=4 }}</ref>

===Impermeable plasma===
Impermeable plasma is a type of thermal plasma which acts like an impermeable solid with respect to gas or cold plasma and can be physically pushed. Interaction of cold gas and thermal plasma was briefly studied by a group led by ] in 1960s and 1970s for its possible applications in insulation of ] plasma from the reactor walls.<ref>{{cite journal |last1=Alfvén |first1=H. |last2=Smårs |first2=E.|title= Gas-Insulation of a Hot Plasma |journal=Nature |volume=188 |date=1960 |pages=801–802 |doi=10.1038/188801a0|bibcode = 1960Natur.188..801A |issue=4753 }}</ref> However, later it was found that the external ] in this configuration could induce ] in the plasma and subsequently lead to an unexpectedly high heat loss to the walls.<ref>{{cite journal |last1=Braams |first1=C.M. |title= Stability of Plasma Confined by a Cold-Gas Blanket |journal=Physical Review Letters |volume=17 |issue=9 |date=1966 |pages=470–471 |doi=10.1103/PhysRevLett.17.470|bibcode = 1966PhRvL..17..470B }}</ref>
In 2013, a group of materials scientists reported that they have successfully generated stable impermeable plasma with no ] using only an ultrahigh-pressure blanket of cold gas. While spectroscopic data on the characteristics of plasma were claimed to be difficult to obtain due to the high pressure, the passive effect of plasma on ] of different ] clearly suggested the effective confinement. They also showed that upon maintaining the impermeability for a few tens of seconds, screening of ] at the plasma-gas interface could give rise to a strong secondary mode of heating (known as viscous heating) leading to different kinetics of reactions and formation of complex ].<ref>{{cite journal |last1=Yaghoubi |first1=A. |last2=Mélinon |first2=P.|title= Tunable synthesis and in situ growth of silicon-carbon mesostructures using impermeable plasma |journal=Scientific Reports |volume=3 |pages=1083 |date=2013 |doi=10.1038/srep01083|bibcode = 2013NatSR...3E1083Y |pmid=23330064 |pmc=3547321}}</ref>

==Mathematical descriptions==
] that can develop in a plasma.<ref>See {{webarchive|url=https://web.archive.org/web/20171225232939/https://history.nasa.gov/SP-345/ch15.htm |date=25 December 2017 }}'', 1976''</ref>]]
{{main article|Plasma modeling}}
To completely describe the state of a plasma, all of the
particle locations and velocities that describe the electromagnetic field in the plasma region would need to be written down.
However, it is generally not practical or necessary to keep track of all the particles in a plasma.
Therefore, plasma physicists commonly use less detailed descriptions, of which
there are two main types:

===Fluid model===
Fluid models describe plasmas in terms of smoothed quantities, like density and averaged velocity around each position (see ]). One simple fluid model, ], treats the plasma as a single fluid governed by a combination of ] and the ]. A more general description is the ] picture, where the ions and electrons are described separately. Fluid models are often accurate when collisionality is sufficiently high to keep the plasma velocity distribution close to a ]. Because fluid models usually describe the plasma in terms of a single flow at a certain temperature at each spatial location, they can neither capture velocity space structures like beams or ]s, nor resolve wave-particle effects.

===Kinetic model===
Kinetic models describe the particle velocity distribution function at each point in the plasma and therefore do not need to assume a ]. A kinetic description is often necessary for collisionless plasmas. There are two common approaches to kinetic description of a plasma. One is based on representing the smoothed distribution function on a grid in velocity and position. The other, known as the ] (PIC) technique, includes kinetic information by following the trajectories of a large number of individual particles. Kinetic models are generally more computationally intensive than fluid models. The ] may be used to describe the dynamics of a system of charged particles interacting with an electromagnetic field.
In magnetized plasmas, a ] approach can substantially reduce the computational expense of a fully kinetic simulation.


==Artificial plasmas== ===Artificial plasmas===
Most artificial plasmas are generated by the application of electric and/or magnetic fields through a gas. Plasma generated in a laboratory setting and for industrial use can be generally categorized by: Most artificial plasmas are generated by the application of electric and/or magnetic fields through a gas. Plasma generated in a laboratory setting and for industrial use can be generally categorized by:
*The type of power source used to generate the plasma—DC, RF and microwave *The type of power source used to generate the plasma—DC, AC (typically with ] (RF)) and microwave{{Citation needed|date=January 2021}}
*The pressure they operate at—vacuum pressure (< 10&nbsp;mTorr or 1 Pa), moderate pressure (≈1&nbsp;Torr or 100 Pa), atmospheric pressure (760&nbsp;Torr or 100 kPa) *The pressure they operate at—vacuum pressure (< 10&nbsp;mTorr or 1 Pa), moderate pressure (≈1&nbsp;Torr or 100 Pa), atmospheric pressure (760&nbsp;Torr or 100 kPa){{Citation needed|date=January 2021}}
*The degree of ionisation within the plasma—fully, partially, or weakly ionised *The degree of ionization within the plasma—fully, partially, or weakly ionized{{Citation needed|date=January 2021}}
*The temperature relationships within the plasma—thermal plasma (<math>T_e = T_i = T_{gas}</math>), non-thermal or "cold" plasma (<math>T_e \gg T_i = T_{gas}</math>) *The temperature relationships within the plasma—thermal plasma (<math>T_e = T_i = T_\text{gas}</math>), non-thermal or "cold" plasma (<math>T_e \gg T_i = T_\text{gas}</math>){{Citation needed|date=January 2021}}
*The electrode configuration used to generate the plasma *The electrode configuration used to generate the plasma{{Citation needed|date=January 2021}}
*The magnetization of the particles within the plasma—magnetized (both ion and electrons are trapped in ] by the magnetic field), partially magnetized (the electrons but not the ions are trapped by the magnetic field), non-magnetized (the magnetic field is too weak to trap the particles in orbits but may generate ]s){{citation needed|date=February 2017}} *The magnetization of the particles within the plasma—magnetized (both ion and electrons are trapped in ] by the magnetic field), partially magnetized (the electrons but not the ions are trapped by the magnetic field), non-magnetized (the magnetic field is too weak to trap the particles in orbits but may generate ]s){{citation needed|date=February 2017}}


===Generation of artificial plasma=== ====Generation of artificial plasma====
] ]
]]] ]]]
Just like the many uses of plasma, there are several means for its generation, however, one principle is common to all of them: there must be energy input to produce and sustain it.<ref name="Hippler" /> For this case, plasma is generated when an ] is applied across a ] or fluid (an electrically ] material) as can be seen in the adjacent image, which shows a ] as a simple example (] used for simplicity). Just like the many uses of plasma, there are several means for its generation. However, one principle is common to all of them: there must be energy input to produce and sustain it.<ref name="Hippler" /> For this case, plasma is generated when an ] is applied across a ] or fluid (an electrically ] material) as can be seen in the adjacent image, which shows a ] as a simple example (] used for simplicity).{{Citation needed|date=January 2021}}


The ] and subsequent ] pull the bound electrons (negative) toward the ] (positive electrode) while the ] (negative electrode) pulls the nucleus.<ref name="Chen">{{cite book |title=Plasma Physics and Controlled Fusion |last=Chen |first=Francis F. |date=1984 |publisher=Plenum Press |isbn=978-0-306-41332-2 |url=https://books.google.com/?id=WGbaBwAAQBAJ&printsec=frontcover&dq=editions:9PGss7GnX-MC#v=onepage&q&f=false |deadurl=no |archiveurl=https://web.archive.org/web/20180115215631/https://books.google.com/books?id=WGbaBwAAQBAJ&printsec=frontcover&dq=editions:9PGss7GnX-MC&hl=en&sa=X&ved=0ahUKEwimuOfm_pXXAhVrzFQKHTrOCaUQ6AEIKDAA#v=onepage&q&f=false |archivedate=15 January 2018 |df=dmy-all }}</ref> As the ] increases, the current stresses the material (by ]) beyond its ] (termed strength) into a stage of ], marked by an ], where the material transforms from being an ] into a ] (as it becomes increasingly ]). The underlying process is the ], where collisions between electrons and neutral gas atoms create more ions and electrons (as can be seen in the figure on the right). The first impact of an electron on an atom results in one ion and two electrons. Therefore, the number of charged particles increases rapidly (in the millions) only "after about 20 successive sets of collisions",<ref name="Leal-Quiros" /> mainly due to a small mean free path (average distance travelled between collisions). The ] and subsequent ] pull the bound electrons (negative) toward the ] (positive electrode) while the ] (negative electrode) pulls the nucleus.<ref name="Chen">{{cite book |title=Plasma Physics and Controlled Fusion |last=Chen |first=Francis F. |date=1984 |publisher=Plenum Press |isbn=978-0-306-41332-2 |url=https://books.google.com/books?id=WGbaBwAAQBAJ&q=editions:9PGss7GnX-MC |url-status=live |archive-url=https://web.archive.org/web/20180115215631/https://books.google.com/books?id=WGbaBwAAQBAJ&printsec=frontcover&dq=editions:9PGss7GnX-MC&hl=en&sa=X&ved=0ahUKEwimuOfm_pXXAhVrzFQKHTrOCaUQ6AEIKDAA |archive-date=15 January 2018 }}</ref> As the ] increases, the current stresses the material (by ]) beyond its ] (termed strength) into a stage of ], marked by an ], where the material transforms from being an ] into a ] (as it becomes increasingly ]). The underlying process is the ], where collisions between electrons and neutral gas atoms create more ions and electrons (as can be seen in the figure on the right). The first impact of an electron on an atom results in one ion and two electrons. Therefore, the number of charged particles increases rapidly (in the millions) only "after about 20 successive sets of collisions",<ref name="Leal-Quiros" /> mainly due to a small mean free path (average distance travelled between collisions).{{Citation needed|date=January 2021}}


====Electric arc==== =====Electric arc=====
] ]
] ]
] is a continuous electric discharge between two electrodes, similar to ].
With ample current density and ionisation, this forms a luminous ] (a continuous electric discharge similar to ]) between the electrodes.{{#tag:ref|The material undergoes various "regimes" or stages (e.g. saturation, breakdown, glow, transition and thermal arc) as the voltage is increased under the voltage-current relationship. The voltage rises to its maximum value in the saturation stage, and thereafter it undergoes fluctuations of the various stages; while the current progressively increases throughout.<ref name="Leal-Quiros">{{cite journal |author=Leal-Quirós, Edbertho |date=2004 |title=Plasma Processing of Municipal Solid Waste |journal= Brazilian Journal of Physics |volume=34 |issue=4B |pages=1587–1593 |bibcode = 2004BrJPh..34.1587L |doi=10.1590/S0103-97332004000800015}}</ref>|group="Note"}} ] along the continuous electric arc creates ], which dissociates more gas molecules and ionises the resulting atoms (where degree of ionisation is determined by temperature), and as per the sequence: ]-]-]-plasma, the gas is gradually turned into a thermal plasma.{{#tag:ref|Across literature, there appears to be no strict definition on where the boundary is between a gas and plasma. Nevertheless, it is enough to say that at 2,000°C the gas molecules become atomized, and ionised at 3,000 °C and "in this state, gas has a liquid like viscosity at atmospheric pressure and the free electric charges confer relatively high electrical conductivities that can approach those of metals."<ref name="Gomez" />|group="Note"}} A thermal plasma is in ], which is to say that the temperature is relatively homogeneous throughout the heavy particles (i.e. atoms, molecules and ions) and electrons. This is so because when thermal plasmas are generated, ] is given to electrons, which, due to their great mobility and large numbers, are able to disperse it rapidly and by ] (without energy loss) to the heavy particles.<ref name="Gomez" /><ref group="Note">Note that non-thermal, or non-equilibrium plasmas are not as ionised and have lower energy densities, and thus the temperature is not dispersed evenly among the particles, where some heavy ones remain "cold".</ref>
With ample current density, the discharge forms a luminous arc, where the inter-electrode material (usually, a gas) undergoes various stages — saturation, breakdown, glow, transition, and thermal arc. The voltage rises to its maximum in the saturation stage, and thereafter it undergoes fluctuations of the various stages, while the current progressively increases throughout.<ref name="Leal-Quiros">{{cite journal |author=Leal-Quirós, Edbertho |date=2004 |title=Plasma Processing of Municipal Solid Waste |journal= Brazilian Journal of Physics |volume=34 |issue=4B |pages=1587–1593 |bibcode = 2004BrJPh..34.1587L |doi=10.1590/S0103-97332004000800015|doi-access=free }}</ref> ] along the arc creates ], which dissociates more gas molecules and ionizes the resulting atoms. Therefore, the ] is given to electrons, which, due to their great mobility and large numbers, are able to disperse it rapidly by ]s to the heavy particles.<ref name="Gomez" />


===Examples of industrial/commercial plasma=== ====Examples of industrial plasma====
Because of their sizable temperature and density ranges, plasmas find applications in many fields of research, technology and industry. For example, in: industrial and extractive ],<ref name="Gomez">{{Cite journal | last1 = Gomez | first1 = E. | last2 = Rani | first2 = D. A. | last3 = Cheeseman | first3 = C. R. | last4 = Deegan | first4 = D. | last5 = Wise | first5 = M. | last6 = Boccaccini | first6 = A. R. | doi = 10.1016/j.jhazmat.2008.04.017 | title = Thermal plasma technology for the treatment of wastes: A critical review | journal = Journal of Hazardous Materials | volume = 161 | issue = 2–3 | pages = 614–626 | year = 2009 | pmid = 18499345| pmc = }}</ref><ref name="Szałatkiewicz">{{Cite journal | last1 = Szałatkiewicz | first1 = J. | doi = 10.3390/ma9080683 | title = Metals Recovery from Artificial Ore in Case of Printed Circuit Boards, Using Plasmatron Plasma Reactor | journal = Materials | volume = 9 | issue = 8| pages = 683–696 | year = 2016 | pmid = 28773804| pmc = 5512349| bibcode = 2016Mate....9..683S}}</ref> surface treatments such as ] (coating), ] in microelectronics,<ref name="NRC">{{cite book |author= National Research Council |date=1991 |title=Plasma Processing of Materials : Scientific Opportunities and Technological Challenges |publisher=National Academies Press |isbn= 978-0-309-04597-1}}</ref> metal cutting<ref name="Nemchinsky">{{Cite journal | last1 = Nemchinsky | first1 = V. A. | last2 = Severance | first2 = W. S. | doi = 10.1088/0022-3727/39/22/R01 | title = What we know and what we do not know about plasma arc cutting | journal = Journal of Physics D: Applied Physics | volume = 39 | issue = 22 | pages = R423 | year = 2006 | pmid = | pmc = |bibcode = 2006JPhD...39R.423N }}</ref> and ]; as well as in everyday ] and ]/] lamps,<ref name="Hippler">{{cite book |editor=Hippler, R. |editor2=Kersten, H. |editor3=Schmidt, M. |editor4=Schoenbach, K.M. |date=2008 |title=Low Temperature Plasmas: Fundamentals, Technologies, and Techniques |chapter=Plasma Sources |publisher=Wiley-VCH |edition=2nd |isbn=978-3-527-40673-9}}</ref>, fuel ignition, while even playing a part in ] for ].<ref name="Peretich">{{cite journal |author=Peretich, M.A. |author2=O'Brien, W.F. |author3=Schetz, J.A. |date=2007 |title=Plasma torch power control for scramjet application |publisher=Virginia Space Grant Consortium |url=http://www.vsgc.odu.edu/src/SRC07/SRC07papers/Mark%20Peretich%20_%20PaperFinal%20Report.pdf |accessdate=12 April 2010 |deadurl=no |archiveurl=https://web.archive.org/web/20100629193719/http://www.vsgc.odu.edu/src/SRC07/SRC07papers/Mark%20Peretich%20_%20PaperFinal%20Report.pdf |archivedate=29 June 2010 |df=dmy-all }}</ref> Plasmas find applications in many fields of research, technology and industry, for example, in industrial and extractive ],<ref name="Gomez">{{Cite journal | last1 = Gomez | first1 = E. | last2 = Rani | first2 = D. A. | last3 = Cheeseman | first3 = C. R. | last4 = Deegan | first4 = D. | last5 = Wise | first5 = M. | last6 = Boccaccini | first6 = A. R. | doi = 10.1016/j.jhazmat.2008.04.017 | title = Thermal plasma technology for the treatment of wastes: A critical review | journal = Journal of Hazardous Materials | volume = 161 | issue = 2–3 | pages = 614–626 | year = 2009 | pmid = 18499345| bibcode = 2009JHzM..161..614G | s2cid = 206069219 }}</ref><ref name="Szałatkiewicz">{{Cite journal | last1 = Szałatkiewicz | first1 = J. | doi = 10.3390/ma9080683 | title = Metals Recovery from Artificial Ore in Case of Printed Circuit Boards, Using Plasmatron Plasma Reactor | journal = Materials | volume = 9 | issue = 8| pages = 683–696 | year = 2016 | pmid = 28773804| pmc = 5512349| bibcode = 2016Mate....9..683S| doi-access = free }}</ref> surface treatments such as ] (coating), ] in microelectronics,<ref name="NRC">{{cite book |author= National Research Council |date=1991 |title=Plasma Processing of Materials : Scientific Opportunities and Technological Challenges |publisher=National Academies Press |isbn= 978-0-309-04597-1}}</ref> metal cutting<ref name="Nemchinsky">{{Cite journal | last1 = Nemchinsky | first1 = V. A. | last2 = Severance | first2 = W. S. | doi = 10.1088/0022-3727/39/22/R01 | title = What we know and what we do not know about plasma arc cutting | journal = Journal of Physics D: Applied Physics | volume = 39 | issue = 22 | pages = R423 | year = 2006 |bibcode = 2006JPhD...39R.423N | s2cid = 116995929 }}</ref> and ]; as well as in everyday ] and ]/] lamps,<ref name="Hippler">{{cite book |editor=Hippler, R. |editor2=Kersten, H. |editor3=Schmidt, M. |editor4=Schoenbach, K.M. |date=2008 |title=Low Temperature Plasmas: Fundamentals, Technologies, and Techniques |chapter=Plasma Sources |publisher=Wiley-VCH |edition=2nd |isbn=978-3-527-40673-9}}</ref> fuel ignition, and even in ] for ].<ref name="Peretich">{{cite journal |author=Peretich, M.A. |author2=O'Brien, W.F. |author3=Schetz, J.A. |date=2007 |title=Plasma torch power control for scramjet application |publisher=Virginia Space Grant Consortium |url=http://www.vsgc.odu.edu/src/SRC07/SRC07papers/Mark%20Peretich%20_%20PaperFinal%20Report.pdf |access-date=12 April 2010 |url-status=dead |archive-url=https://web.archive.org/web/20100629193719/http://www.vsgc.odu.edu/src/SRC07/SRC07papers/Mark%20Peretich%20_%20PaperFinal%20Report.pdf |archive-date=29 June 2010 }}</ref>


====Low-pressure discharges==== =====Low-pressure discharges=====
*''] plasmas'': non-thermal plasmas generated by the application of DC or low frequency RF (<100&nbsp;kHz) electric field to the gap between two metal electrodes. Probably the most common plasma; this is the type of plasma generated within ] tubes.<ref>{{cite web |url=http://www-spof.gsfc.nasa.gov/Education/wfluor.html |title=The Fluorescent Lamp: A plasma you can use |author=Stern, David P. |accessdate=2010-05-19 |deadurl=no |archiveurl=https://web.archive.org/web/20100530165958/http://www-spof.gsfc.nasa.gov/Education/wfluor.html |archivedate=30 May 2010 |df=dmy-all }}</ref> *''] plasmas'': non-thermal plasmas generated by the application of DC or low frequency RF (<100&nbsp;kHz) electric field to the gap between two metal electrodes. Probably the most common plasma; this is the type of plasma generated within ] tubes.<ref>{{cite web |url=http://www-spof.gsfc.nasa.gov/Education/wfluor.html |title=The Fluorescent Lamp: A plasma you can use |author=Stern, David P. |access-date=19 May 2010 |url-status=live |archive-url=https://web.archive.org/web/20100530165958/http://www-spof.gsfc.nasa.gov/Education/wfluor.html |archive-date=30 May 2010 }}</ref>
*''] (CCP)'': similar to glow discharge plasmas, but generated with high frequency RF electric fields, typically ]. These differ from glow discharges in that the sheaths are much less intense. These are widely used in the microfabrication and integrated circuit manufacturing industries for plasma etching and plasma enhanced chemical vapor deposition.<ref>{{cite journal |last1=Sobolewski |first1=M.A. |last2=Langan & Felker |first2=J.G. & B.S. |date=1997 |title=Electrical optimization of plasma-enhanced chemical vapor deposition chamber cleaning plasmas |journal=Journal of Vacuum Science and Technology B |volume=16 |issue=1 |pages=173–182 |url=http://physics.nist.gov/MajResProj/rfcell/Publications/MAS_JVSTB16_1.pdf | archiveurl=https://web.archive.org/web/20090118212957/http://www.physics.nist.gov/MajResProj/rfcell/Publications/MAS_JVSTB16_1.pdf | archivedate=18 January 2009 |doi=10.1116/1.589774|bibcode = 1998JVSTB..16..173S }}</ref> *''] (CCP)'': similar to glow discharge plasmas, but generated with high frequency RF electric fields, typically ]. These differ from glow discharges in that the sheaths are much less intense. These are widely used in the microfabrication and integrated circuit manufacturing industries for plasma etching and plasma enhanced chemical vapor deposition.<ref>{{cite journal |last1=Sobolewski |first1=M.A. |last2=Langan & Felker |first2=J.G. & B.S. |date=1997 |title=Electrical optimization of plasma-enhanced chemical vapor deposition chamber cleaning plasmas |journal=Journal of Vacuum Science and Technology B |volume=16 |issue=1 |pages=173–182 |url=http://physics.nist.gov/MajResProj/rfcell/Publications/MAS_JVSTB16_1.pdf | archive-url=https://web.archive.org/web/20090118212957/http://www.physics.nist.gov/MajResProj/rfcell/Publications/MAS_JVSTB16_1.pdf | archive-date=18 January 2009 |doi=10.1116/1.589774|bibcode = 1998JVSTB..16..173S }}</ref>
*'']'': a device to produce low temperature (≈1eV) high density plasmas (HDP). *'']'': a device to produce low temperature (≈1eV) high density plasmas (HDP).
*''] (ICP)'': similar to a CCP and with similar applications but the electrode consists of a coil wrapped around the chamber where plasma is formed.<ref>{{Cite journal | last1 = Okumura | first1 = T. | doi = 10.1155/2010/164249 | title = Inductively Coupled Plasma Sources and Applications | journal = Physics Research International | volume = 2010 | pages = 1–14 | year = 2010 | pmid = | pmc = }}</ref> *''] (ICP)'': similar to a CCP and with similar applications but the electrode consists of a coil wrapped around the chamber where plasma is formed.<ref>{{Cite journal | last1 = Okumura | first1 = T. | doi = 10.1155/2010/164249 | title = Inductively Coupled Plasma Sources and Applications | journal = Physics Research International | volume = 2010 | pages = 1–14 | year = 2010 | doi-access = free }}</ref>
*'']'': similar to CCP and ICP in that it is typically RF (or microwave). Examples include ] and ] (ECR).<ref>{{cite book|title=Plasma Chemistry|date=2008|publisher=Cambridge University Press|page=229|url=https://books.google.com/books?id=ZzmtGEHCC9MC&pg=PA229#v=onepage&q&f=false|isbn=9781139471732|deadurl=no|archiveurl=https://web.archive.org/web/20170202060021/https://books.google.com/books?id=ZzmtGEHCC9MC&pg=PA229#v=onepage&q&f=false|archivedate=2 February 2017|df=dmy-all}}</ref> *'']'': similar to CCP and ICP in that it is typically RF (or microwave). Examples include ] and ] (ECR).<ref>{{cite book|title=Plasma Chemistry|date=2008|publisher=Cambridge University Press|page=229|url=https://books.google.com/books?id=ZzmtGEHCC9MC&pg=PA229|isbn=9781139471732|url-status=live|archive-url=https://web.archive.org/web/20170202060021/https://books.google.com/books?id=ZzmtGEHCC9MC&pg=PA229|archive-date=2 February 2017}}</ref>


====Atmospheric pressure==== =====Atmospheric pressure=====
*'']:'' this is a high power thermal discharge of very high temperature (≈10,000 K). It can be generated using various power supplies. It is commonly used in ] processes. For example, it is used to smelt minerals containing Al<sub>2</sub>O<sub>3</sub> to produce ]. *'']:'' this is a high power thermal discharge of very high temperature (≈10,000 K). It can be generated using various power supplies. It is commonly used in ] processes. For example, it is used to smelt minerals containing Al<sub>2</sub>O<sub>3</sub> to produce ].{{Citation needed|date=January 2021}}
*'']:'' this is a non-thermal discharge generated by the application of high voltage to sharp electrode tips. It is commonly used in ] generators and particle precipitators. *'']:'' this is a non-thermal discharge generated by the application of high voltage to sharp electrode tips. It is commonly used in ] generators and particle precipitators.{{Citation needed|date=January 2021}}
*''] (DBD):'' this is a non-thermal discharge generated by the application of high voltages across small gaps wherein a non-conducting coating prevents the transition of the plasma discharge into an arc. It is often mislabeled 'Corona' discharge in industry and has similar application to corona discharges. It is also widely used in the web treatment of fabrics.<ref>{{Cite journal | last1 = Leroux | first1 = F. | last2 = Perwuelz | first2 = A. | last3 = Campagne | first3 = C. | last4 = Behary | first4 = N. | title = Atmospheric air-plasma treatments of polyester textile structures | doi = 10.1163/156856106777657788 | journal = Journal of Adhesion Science and Technology | volume = 20 | issue = 9 | pages = 939–957 | year = 2006 | pmid = | pmc = }}</ref> The application of the discharge to synthetic fabrics and plastics functionalizes the surface and allows for paints, glues and similar materials to adhere.<ref>{{Cite journal *''] (DBD):'' this is a non-thermal discharge generated by the application of high voltages across small gaps wherein a non-conducting coating prevents the transition of the plasma discharge into an arc. It is often mislabeled "Corona" discharge in industry and has similar application to corona discharges. A common usage of this discharge is in a ] for vehicle drag reduction.<ref>{{Cite journal | last1 = Roy | first1 = S. | last2 = Zhao | first2 = P. | last3 = Dasgupta | first3 = A. | last4 = Soni | first4 = J. | title = Dielectric barrier discharge actuator for vehicle drag reduction at highway speeds| doi = 10.1063/1.4942979 | journal = AIP Advances | volume = 6 | issue = 2 | pages = 025322 | year = 2016 | bibcode = 2016AIPA....6b5322R | doi-access = free }}</ref> It is also widely used in the web treatment of fabrics.<ref>{{Cite journal | last1 = Leroux | first1 = F. | last2 = Perwuelz | first2 = A. | last3 = Campagne | first3 = C. | last4 = Behary | first4 = N. | s2cid = 137392051 | title = Atmospheric air-plasma treatments of polyester textile structures | doi = 10.1163/156856106777657788 | journal = Journal of Adhesion Science and Technology | volume = 20 | issue = 9 | pages = 939–957 | year = 2006 }}</ref> The application of the discharge to synthetic fabrics and plastics functionalizes the surface and allows for paints, glues and similar materials to adhere.<ref>{{Cite journal
| last1 = Leroux | first1 = F. D. R. | last1 = Leroux | first1 = F. D. R.
| last2 = Campagne | first2 = C. | last2 = Campagne | first2 = C.
Line 354: Line 301:
| year = 2008 | year = 2008
| pmid = 18930244 | pmid = 18930244
| pmc =
| bibcode = 2008JCIS..328..412L | bibcode = 2008JCIS..328..412L
}}</ref> The dielectric barrier discharge was used in the mid-1990s to show that low temperature atmospheric pressure plasma is effective in inactivating bacterial cells.<ref>{{cite journal|doi=10.1109/27.533129|title=Sterilization of contaminated matter with an atmospheric pressure plasma|journal=IEEE Transactions on Plasma Science|volume=24|issue=3|pages=1188–1191|year=1996|last1=Laroussi|first1=M.|bibcode=1996ITPS...24.1188L}}</ref> This work and later experiments using mammalian cells led to the establishment of a new field of research known as ]. The dielectric barrier discharge configuration was also used in the design of low temperature plasma jets. These plasma jets are produced by fast propagating guided ionisation waves known as plasma bullets.<ref>{{cite journal|doi=10.1016/j.physrep.2014.02.006|title=Guided ionization waves: Theory and experiments|journal=Physics Reports|volume=540|issue=3|pages=123|year=2014|last1=Lu|first1=X.|last2=Naidis|first2=G.V.|last3=Laroussi|first3=M.|last4=Ostrikov|first4=K.|bibcode=2014PhR...540..123L}}</ref> }}</ref> The dielectric barrier discharge was used in the mid-1990s to show that low temperature atmospheric pressure plasma is effective in inactivating bacterial cells.<ref>{{cite journal|doi=10.1109/27.533129|title=Sterilization of contaminated matter with an atmospheric pressure plasma|journal=IEEE Transactions on Plasma Science|volume=24|issue=3|pages=1188–1191|year=1996|last1=Laroussi|first1=M.|bibcode=1996ITPS...24.1188L}}</ref> This work and later experiments using mammalian cells led to the establishment of a new field of research known as ]. The dielectric barrier discharge configuration was also used in the design of low temperature plasma jets. These plasma jets are produced by fast propagating guided ionization waves known as plasma bullets.<ref>{{cite journal|doi=10.1016/j.physrep.2014.02.006|title=Guided ionization waves: Theory and experiments|journal=Physics Reports|volume=540|issue=3|pages=123|year=2014|last1=Lu|first1=X.|last2=Naidis|first2=G.V.|last3=Laroussi|first3=M.|last4=Ostrikov|first4=K.|bibcode=2014PhR...540..123L}}</ref>
*'']:'' this is a ] generated by the application of RF power (e.g., ]) to one powered electrode, with a grounded electrode held at a small separation distance on the order of 1&nbsp;cm. Such discharges are commonly stabilized using a noble gas such as helium or argon.<ref>{{Cite journal | last1 = Park | first1 = J. | last2 = Henins | first2 = I. | last3 = Herrmann | first3 = H. W. | last4 = Selwyn | first4 = G. S. | last5 = Hicks | first5 = R. F. | title = Discharge phenomena of an atmospheric pressure radio-frequency capacitive plasma source | doi = 10.1063/1.1323753 | journal = Journal of Applied Physics | volume = 89 | issue = 1 | pages = 20 | year = 2001 | pmid = | pmc = |bibcode = 2001JAP....89...20P | url = https://zenodo.org/record/1231852 }}</ref> *'']:'' this is a ] generated by the application of RF power (e.g., ]) to one powered electrode, with a grounded electrode held at a small separation distance on the order of 1&nbsp;cm. Such discharges are commonly stabilized using a noble gas such as helium or argon.<ref>{{Cite journal | last1 = Park | first1 = J. | last2 = Henins | first2 = I. | last3 = Herrmann | first3 = H. W. | last4 = Selwyn | first4 = G. S. | last5 = Hicks | first5 = R. F. | title = Discharge phenomena of an atmospheric pressure radio-frequency capacitive plasma source | doi = 10.1063/1.1323753 | journal = Journal of Applied Physics | volume = 89 | issue = 1 | pages = 20 | year = 2001 |bibcode = 2001JAP....89...20P | url = https://zenodo.org/record/1231852 }}</ref>
*"]:" is a ] generated at the high-side of a piezoelectric transformer (PT). This generation variant is particularly suited for high efficient and compact devices where a separate high voltage power supply is not desired. *"]:" is a ] generated at the high side of a piezoelectric transformer (PT). This generation variant is particularly suited for high efficient and compact devices where a separate high voltage power supply is not desired.{{Citation needed|date=January 2021}}


===MHD converters=== ====MHD converters====
{{main|magnetohydrodynamic converter|magnetohydrodynamic generator|magnetohydrodynamic drive}} {{main|magnetohydrodynamic converter|magnetohydrodynamic generator|magnetohydrodynamic drive}}
{{see also|Electrothermal instability}} {{see also|Electrothermal instability}}
A world effort was triggered in the 1960s to study ]s in order to bring ] to market with commercial power plants of a new kind, converting the ] of a high velocity plasma into ] with no ] at a high ]. Research was also conducted in the field of supersonic and hypersonic aerodynamics to study plasma interaction with magnetic fields to eventually achieve passive and even active ] around vehicles or projectiles, in order to soften and mitigate ]s, lower thermal transfer and reduce ]. A world effort was triggered in the 1960s to study ]s in order to bring ] to market with commercial power plants of a new kind, converting the ] of a high velocity plasma into ] with no ] at a high ]. Research was also conducted in the field of supersonic and hypersonic aerodynamics to study plasma interaction with magnetic fields to eventually achieve passive and even active ] around vehicles or projectiles, in order to soften and mitigate ]s, lower thermal transfer and reduce ].{{Citation needed|date=January 2021}}


Such ionized gases used in "plasma technology" ("technological" or "engineered" plasmas) are usually ''weakly ionized gases'' in the sense that only a tiny fraction of the gas molecules are ionized.<ref>{{Cite book|url=https://www.worldcat.org/oclc/690642377|title=Plasma scattering of electromagnetic radiation : theory and measurement techniques|last=|first=|date=2011|publisher=Academic Press/Elsevier|others=Froula, Dustin H.|year=|isbn=978-0080952031|edition=1st ed., 2nd|location=Burlington, MA|pages=273|oclc=690642377}}</ref> These kinds of weakly ionized gases are also nonthermal "cold" plasmas. In the presence of magnetics fields, the study of such magnetized nonthermal weakly ionized gases involves ] with low ], a challenging field of plasma physics where calculations require ]s in a ] ]. When used in combination with a high ], a critical value triggers the problematic ] which limited these technological developments. Such ionized gases used in "plasma technology" ("technological" or "engineered" plasmas) are usually ''weakly ionized gases'' in the sense that only a tiny fraction of the gas molecules are ionized.<ref>{{Cite book|title=Plasma Scattering of Electromagnetic Radiation: Theory and Measurement Techniques |date=2011|publisher=Academic Press/Elsevier |url=https://books.google.com/books?id=1NS5Fxam1lkC&pg=PA273 |first1=J. |last1=Sheffield |first2=D. |last2=Froula |first3=S. H. |last3=Glenzer |first4=N. C. Jr. |last4=Luhmann |isbn=978-0080952031|edition=1st ed., 2nd|location=Burlington, MA|pages=273|oclc=690642377}}</ref> These kinds of weakly ionized gases are also nonthermal "cold" plasmas. In the presence of magnetics fields, the study of such magnetized nonthermal weakly ionized gases involves ] with low ], a challenging field of plasma physics where calculations require ]s in a ] ]. When used in combination with a high ], a critical value triggers the problematic ] which limited these technological developments.{{Citation needed|date=January 2021}}


==Complex plasma phenomena==
==Research{{anchor|Fields of active research}}==
{{Tone|section|talk=Opinionated judgemental language|date=June 2024}}


Although the underlying equations governing plasmas are relatively simple, plasma behaviour is extraordinarily varied and subtle: the emergence of unexpected behaviour from a simple model is a typical feature of a ]. Such systems lie in some sense on the boundary between ordered and disordered behaviour and cannot typically be described either by simple, smooth, mathematical functions, or by pure randomness. The spontaneous formation of interesting spatial features on a wide range of length scales is one manifestation of plasma complexity. The features are interesting, for example, because they are very sharp, spatially intermittent (the distance between features is much larger than the features themselves), or have a ] form. Many of these features were first studied in the laboratory, and have subsequently been recognized throughout the universe.{{Citation needed|date=January 2021}} Examples of complexity and complex structures in plasmas include:
Plasmas are the object of study of the ] of ''plasma science'' or ''plasma physics'', including sub-disciplines such as ]. It currently involves the following fields of active research and features across many ], whose interest includes:


===Filamentation===
<!--This list needs organization and pruning!-->
Striations or string-like structures<ref>{{cite journal|author=Dickel, J. R.|bibcode=1990BAAS...22..832D |title=The Filaments in Supernova Remnants: Sheets, Strings, Ribbons, or?|date=1990|journal=Bulletin of the American Astronomical Society|volume= 22|page=832}}</ref> are seen in many plasmas, like the ], the ],<ref>{{Cite journal | last1 = Grydeland | first1 = T. | doi = 10.1029/2002GL016362 | title = Interferometric observations of filamentary structures associated with plasma instability in the auroral ionosphere | journal = Geophysical Research Letters | volume = 30 | issue = 6 | pages = 1338 | year = 2003 | bibcode=2003GeoRL..30.1338G| doi-access = free }}</ref> ],<ref>{{Cite journal | last1 = Moss | first1 = G. D. | last2 = Pasko | first2 = V. P. | last3 = Liu | first3 = N. | last4 = Veronis | first4 = G. | title = Monte Carlo model for analysis of thermal runaway electrons in streamer tips in transient luminous events and streamer zones of lightning leaders | doi = 10.1029/2005JA011350 | journal = Journal of Geophysical Research | volume = 111 | issue = A2 | pages = A02307 | year = 2006 | bibcode=2006JGRA..111.2307M| doi-access = free }}</ref> ]s, ],<ref>{{cite journal|author=Doherty, Lowell R.|doi=10.1086/148107|title=Filamentary Structure in Solar Prominences|date=1965|journal=The Astrophysical Journal|volume=141|page=251|last2=Menzel|first2=Donald H.|bibcode=1965ApJ...141..251D}}</ref> and ]s.<ref>{{cite web |url=http://seds.lpl.arizona.edu/messier/more/m001_hst.html |title=Hubble views the Crab Nebula M1: The Crab Nebula Filaments |access-date=26 January 2017 |url-status=bot: unknown |archive-url=https://web.archive.org/web/20091005084515/http://seds.lpl.arizona.edu/messier/more/m001_hst.html |archive-date=5 October 2009 }}. The University of Arizona</ref> They are sometimes associated with larger current densities, and the interaction with the magnetic field can form a ] structure.<ref>{{Cite journal | last1 = Zhang | first1 = Y. A. | last2 = Song | first2 = M. T. | last3 = Ji | first3 = H. S. | doi = 10.1016/S0275-1062(02)00095-4 | title = A rope-shaped solar filament and a IIIb flare | journal = Chinese Astronomy and Astrophysics | volume = 26 | issue = 4 | pages = 442–450 | year = 2002 |bibcode = 2002ChA&A..26..442Z }}</ref> (See also ])
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Filamentation also refers to the self-focusing of a high power laser pulse. At high powers, the nonlinear part of the ] becomes important and causes a higher index of refraction in the center of the laser beam, where the laser is brighter than at the edges, causing a feedback that focuses the laser even more. The tighter focused laser has a higher peak brightness (irradiance) that forms a plasma. The plasma has an index of refraction lower than one, and causes a defocusing of the laser beam. The interplay of the focusing index of refraction, and the defocusing plasma makes the formation of a long filament of plasma that can be ] to kilometers in length.<ref>{{Cite book|author=Chin, S. L. |title=Progress in Ultrafast Intense Laser Science III|url=http://icpr.snu.ac.kr/resource/wop.pdf/J01/2006/049/S01/J012006049S010281.pdf|journal=Journal of the Korean Physical Society|volume=49|date=2006|page=281|chapter=Some Fundamental Concepts of Femtosecond Laser Filamentation|bibcode=2008pui3.book..243C|doi=10.1007/978-3-540-73794-0_12|series=Springer Series in Chemical Physics|isbn=978-3-540-73793-3}}</ref> One interesting aspect of the filamentation generated plasma is the relatively low ion density due to defocusing effects of the ionized electrons.<ref>{{Cite journal | last1 = Talebpour | first1 = A. | last2 = Abdel-Fattah | first2 = M. | last3 = Chin | first3 = S. L. | doi = 10.1016/S0030-4018(00)00903-2 | title = Focusing limits of intense ultrafast laser pulses in a high pressure gas: Road to new spectroscopic source | journal = Optics Communications | volume = 183 | issue = 5–6 | pages = 479–484 | year = 2000 | bibcode=2000OptCo.183..479T}}</ref> (See also ])
*Plasma theory

**]
===Impermeable plasma===
**Plasma interactions with waves and beams
Impermeable plasma is a type of thermal plasma which acts like an impermeable solid with respect to gas or cold plasma and can be physically pushed. Interaction of cold gas and thermal plasma was briefly studied by a group led by ] in 1960s and 1970s for its possible applications in insulation of ] plasma from the reactor walls.<ref>{{cite journal |last1=Alfvén |first1=H. |last2=Smårs |first2=E.|s2cid=26797662 |title= Gas-Insulation of a Hot Plasma |journal=Nature |volume=188 |date=1960 |pages=801–802 |doi=10.1038/188801a0|bibcode = 1960Natur.188..801A |issue=4753 }}</ref> However, later it was found that the external ] in this configuration could induce ] in the plasma and subsequently lead to an unexpectedly high heat loss to the walls.<ref>{{cite journal |last1=Braams |first1=C.M. |title= Stability of Plasma Confined by a Cold-Gas Blanket |journal=Physical Review Letters |volume=17 |issue=9 |date=1966 |pages=470–471 |doi=10.1103/PhysRevLett.17.470|bibcode = 1966PhRvL..17..470B }}</ref>
**]
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*Plasmas in nature
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**The Earth's ]
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**Planetary ]s
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*Industrial plasmas
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*Plasma applications
**]
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***] (MFE)&nbsp;—
****]
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***] (ICF)
***]s
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**] (Implosion experiments)
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**Food processing
***] or "cold plasma"
**], recycling.
**]
**] (e. g. Dentistry<ref name="tws44">{{cite news
|title = High-tech dentistry&nbsp;– "St Elmo's frier"&nbsp;– Using a plasma torch to clean your teeth
|publisher = The Economist print edition
|date = Jun 17, 2009
|url = http://www.economist.com/displaystory.cfm?story_id=13794903&fsrc=rss
|accessdate = 2009-09-07
|deadurl = no
|archiveurl = https://web.archive.org/web/20090620234324/http://www.economist.com/displaystory.cfm?story_id=13794903&fsrc=rss
|archivedate = 20 June 2009
|df = dmy-all
}}</ref>)
**]


In 2013, a group of materials scientists reported that they have successfully generated stable impermeable plasma with no ] using only an ultrahigh-pressure blanket of cold gas. While spectroscopic data on the characteristics of plasma were claimed to be difficult to obtain due to the high pressure, the passive effect of plasma on ] of different ] clearly suggested the effective confinement. They also showed that upon maintaining the impermeability for a few tens of seconds, screening of ] at the plasma-gas interface could give rise to a strong secondary mode of heating (known as viscous heating) leading to different kinetics of reactions and formation of complex ].<ref>{{cite journal |last1=Yaghoubi |first1=A. |last2=Mélinon |first2=P.|title= Tunable synthesis and in situ growth of silicon-carbon mesostructures using impermeable plasma |journal=Scientific Reports |volume=3 |pages=1083 |date=2013 |doi=10.1038/srep01083|bibcode = 2013NatSR...3.1083Y|pmid=23330064 |pmc=3547321}}</ref>
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==Gallery==
==Research examples==
<gallery> <gallery>
File:HallThruster 2.jpg|]. The electric field in a plasma ] is so effective at accelerating ions that electric fields are used in ]s. File:HallThruster 2.jpg|]
File:Wispy 'Plasma Dancer' on the limb of the Sun.ogv|Solar plasma File:Wispy 'Plasma Dancer' on the limb of the Sun.ogv|Solar plasma
File:Plasma Spraying Process.jpg|Plasma spraying File:Plasma Spraying Process.jpg|Plasma spraying
File:MAST plasma image.jpg|Tokamak plasma in nuclear fusion research File:MAST plasma image.jpg|Plasma in a ]
File:Argon Plasma.jpg|Laboratory plasma
</gallery> </gallery>


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==Notes==
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==References== ==References==
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==External links== ==External links==
{{Sister project links | wikt=plasma | commons=Category:Plasma physics | b=Wikijunior:The Elements/Plasma | q=no | s=Special:Search/Plasma physics | v=Plasma | d=Q10251 | n=Special:Search/Plasma physics}} {{Sister project links | wikt=plasma | commons=Category:Plasma physics | b=Wikijunior:The Elements/Plasma | q=no | s=Special:Search/Plasma physics | v=Plasma | d=y| n=Special:Search/Plasma physics}}
* {{Webarchive|url=https://web.archive.org/web/20190930230004/http://fusedweb.llnl.gov/CPEP/Chart_Pages/5.Plasma4StateMatter.html |date=30 September 2019 }}
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*&nbsp;– a list of plasma related links.
*Introduction to Plasma Physics: | *Introduction to Plasma Physics: |
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*| * {{Webarchive|url=https://web.archive.org/web/20050906205014/http://c3po.barnesos.net/homepage/lpl/grapeplasma/ |date=6 September 2005 }}|
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{{States of matter}}
{{Branches of physics}} {{Branches of physics}}
{{Nuclear Technology}}


{{Authority control}} {{Authority control}}


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Latest revision as of 20:50, 13 December 2024

State of matter

Top: Lightning and neon lights are commonplace generators of plasma. Center left: A plasma globe, illustrating some of the more complex plasma phenomena, including filamentation. Center right: A plasma trail from the Space Shuttle Atlantis during re-entry into Earth's atmosphere, as seen from the International Space Station. Bottom left: A fire in a fire pit; fires may produce plasma if hot enough. Bottom right: The Sun's corona as seen from a solar eclipse in France.

Plasma (from Ancient Greek πλάσμα (plásma) 'moldable substance') is one of four fundamental states of matter (the other three being solid, liquid, and gas) characterized by the presence of a significant portion of charged particles in any combination of ions or electrons. It is the most abundant form of ordinary matter in the universe, mostly in stars (including the Sun), but also dominating the rarefied intracluster medium and intergalactic medium. Plasma can be artificially generated, for example, by heating a neutral gas or subjecting it to a strong electromagnetic field.

The presence of charged particles makes plasma electrically conductive, with the dynamics of individual particles and macroscopic plasma motion governed by collective electromagnetic fields and very sensitive to externally applied fields. The response of plasma to electromagnetic fields is used in many modern devices and technologies, such as plasma televisions or plasma etching.

Depending on temperature and density, a certain number of neutral particles may also be present, in which case plasma is called partially ionized. Neon signs and lightning are examples of partially ionized plasmas. Unlike the phase transitions between the other three states of matter, the transition to plasma is not well defined and is a matter of interpretation and context. Whether a given degree of ionization suffices to call a substance "plasma" depends on the specific phenomenon being considered.

Early history

Plasma microfields calculated by an N-body simulation. Note the fast moving electrons and slow ions, resembling a bodily fluid.

Plasma was first identified in laboratory by Sir William Crookes. Crookes presented a lecture on what he called "radiant matter" to the British Association for the Advancement of Science, in Sheffield, on Friday, 22 August 1879. Systematic studies of plasma began with the research of Irving Langmuir and his colleagues in the 1920s. Langmuir also introduced the term "plasma" as a description of ionized gas in 1928:

Except near the electrodes, where there are sheaths containing very few electrons, the ionized gas contains ions and electrons in about equal numbers so that the resultant space charge is very small. We shall use the name plasma to describe this region containing balanced charges of ions and electrons.

Lewi Tonks and Harold Mott-Smith, both of whom worked with Langmuir in the 1920s, recall that Langmuir first used the term by analogy with the blood plasma. Mott-Smith recalls, in particular, that the transport of electrons from thermionic filaments reminded Langmuir of "the way blood plasma carries red and white corpuscles and germs."

Part of a series on
Continuum mechanics
J = D d φ d x {\displaystyle J=-D{\frac {d\varphi }{dx}}} Fick's laws of diffusion
Laws
Conservations
Inequalities
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Fluids
Liquids
Gases
Plasma
Rheology
Smart fluids
Scientists

Definitions

The fourth state of matter

Plasma is called the fourth state of matter after solid, liquid, and gas. It is a state of matter in which an ionized substance becomes highly electrically conductive to the point that long-range electric and magnetic fields dominate its behaviour.

Plasma is typically an electrically quasineutral medium of unbound positive and negative particles (i.e., the overall charge of a plasma is roughly zero). Although these particles are unbound, they are not "free" in the sense of not experiencing forces. Moving charged particles generate electric currents, and any movement of a charged plasma particle affects and is affected by the fields created by the other charges. In turn, this governs collective behaviour with many degrees of variation.

Plasma is distinct from the other states of matter. In particular, describing a low-density plasma as merely an "ionized gas" is wrong and misleading, even though it is similar to the gas phase in that both assume no definite shape or volume. The following table summarizes some principal differences:

StateProperty Gas Plasma
Interactions Short-range: Two-particle (binary) collisions are the rule. Long-range: Collective motion of particles is ubiquitous in plasma, resulting in various waves and other types of collective phenomena.
Electrical conductivity Very low: Gases are excellent insulators up to electric field strengths of tens of kilovolts per centimetre. Very high: For many purposes, the conductivity of a plasma may be treated as infinite.
Independently acting species One: All gas particles behave in a similar way, largely influenced by collisions with one another and by gravity. Two or more: Electrons and ions possess different charges and vastly different masses, so that they behave differently in many circumstances, with various types of plasma-specific waves and instabilities emerging as a result.

Ideal plasma

Three factors define an ideal plasma:

  • The plasma approximation: The plasma approximation applies when the plasma parameter Λ, representing the number of charge carriers within the Debye sphere is much higher than unity. It can be readily shown that this criterion is equivalent to smallness of the ratio of the plasma electrostatic and thermal energy densities. Such plasmas are called weakly coupled.
  • Bulk interactions: The Debye length is much smaller than the physical size of the plasma. This criterion means that interactions in the bulk of the plasma are more important than those at its edges, where boundary effects may take place. When this criterion is satisfied, the plasma is quasineutral.
  • Collisionlessness: The electron plasma frequency (measuring plasma oscillations of the electrons) is much larger than the electron–neutral collision frequency. When this condition is valid, electrostatic interactions dominate over the processes of ordinary gas kinetics. Such plasmas are called collisionless.

Non-neutral plasma

Main article: Non-neutral plasmas

The strength and range of the electric force and the good conductivity of plasmas usually ensure that the densities of positive and negative charges in any sizeable region are equal ("quasineutrality"). A plasma with a significant excess of charge density, or, in the extreme case, is composed of a single species, is called a non-neutral plasma. In such a plasma, electric fields play a dominant role. Examples are charged particle beams, an electron cloud in a Penning trap and positron plasmas.

Dusty plasma

Main article: Dusty plasma

A dusty plasma contains tiny charged particles of dust (typically found in space). The dust particles acquire high charges and interact with each other. A plasma that contains larger particles is called grain plasma. Under laboratory conditions, dusty plasmas are also called complex plasmas.

Properties and parameters

Artist's rendition of the Earth's plasma fountain, showing oxygen, helium, and hydrogen ions that gush into space from regions near the Earth's poles. The faint yellow area shown above the north pole represents gas lost from Earth into space; the green area is the aurora borealis, where plasma energy pours back into the atmosphere.

Density and ionization degree

For plasma to exist, ionization is necessary. The term "plasma density" by itself usually refers to the electron density n e {\displaystyle n_{e}} , that is, the number of charge-contributing electrons per unit volume. The degree of ionization α {\displaystyle \alpha } is defined as fraction of neutral particles that are ionized:

α = n i n i + n n , {\displaystyle \alpha ={\frac {n_{i}}{n_{i}+n_{n}}},}

where n i {\displaystyle n_{i}} is the ion density and n n {\displaystyle n_{n}} the neutral density (in number of particles per unit volume). In the case of fully ionized matter, α = 1 {\displaystyle \alpha =1} . Because of the quasineutrality of plasma, the electron and ion densities are related by n e = Z i n i {\displaystyle n_{e}=\langle Z_{i}\rangle n_{i}} , where Z i {\displaystyle \langle Z_{i}\rangle } is the average ion charge (in units of the elementary charge).

Temperature

Plasma temperature, commonly measured in kelvin or electronvolts, is a measure of the thermal kinetic energy per particle. High temperatures are usually needed to sustain ionization, which is a defining feature of a plasma. The degree of plasma ionization is determined by the electron temperature relative to the ionization energy (and more weakly by the density). In thermal equilibrium, the relationship is given by the Saha equation. At low temperatures, ions and electrons tend to recombine into bound states—atoms—and the plasma will eventually become a gas.

In most cases, the electrons and heavy plasma particles (ions and neutral atoms) separately have a relatively well-defined temperature; that is, their energy distribution function is close to a Maxwellian even in the presence of strong electric or magnetic fields. However, because of the large difference in mass between electrons and ions, their temperatures may be different, sometimes significantly so. This is especially common in weakly ionized technological plasmas, where the ions are often near the ambient temperature while electrons reach thousands of kelvin. The opposite case is the z-pinch plasma where the ion temperature may exceed that of electrons.

See also: Nonthermal plasma and Anisothermal plasma

Plasma potential

Lightning as an example of plasma present at Earth's surface: Typically, lightning discharges 30 kiloamperes at up to 100 megavolts, and emits radio waves, light, X- and even gamma rays. Plasma temperatures can approach 30000 K and electron densities may exceed 10 m.

Since plasmas are very good electrical conductors, electric potentials play an important role. The average potential in the space between charged particles, independent of how it can be measured, is called the "plasma potential", or the "space potential". If an electrode is inserted into a plasma, its potential will generally lie considerably below the plasma potential due to what is termed a Debye sheath. The good electrical conductivity of plasmas makes their electric fields very small. This results in the important concept of "quasineutrality", which says the density of negative charges is approximately equal to the density of positive charges over large volumes of the plasma ( n e = Z n i {\displaystyle n_{e}=\langle Z\rangle n_{i}} ), but on the scale of the Debye length, there can be charge imbalance. In the special case that double layers are formed, the charge separation can extend some tens of Debye lengths.

The magnitude of the potentials and electric fields must be determined by means other than simply finding the net charge density. A common example is to assume that the electrons satisfy the Boltzmann relation: n e exp ( e Φ / k B T e ) . {\displaystyle n_{e}\propto \exp(e\Phi /k_{\text{B}}T_{e}).}

Differentiating this relation provides a means to calculate the electric field from the density: E = k B T e e n e n e . {\displaystyle {\vec {E}}={\frac {k_{\text{B}}T_{e}}{e}}{\frac {\nabla n_{e}}{n_{e}}}.}

It is possible to produce a plasma that is not quasineutral. An electron beam, for example, has only negative charges. The density of a non-neutral plasma must generally be very low, or it must be very small, otherwise, it will be dissipated by the repulsive electrostatic force.

Magnetization

The existence of charged particles causes the plasma to generate, and be affected by, magnetic fields. Plasma with a magnetic field strong enough to influence the motion of the charged particles is said to be magnetized. A common quantitative criterion is that a particle on average completes at least one gyration around the magnetic-field line before making a collision, i.e., ν c e / ν c o l l > 1 {\displaystyle \nu _{\mathrm {ce} }/\nu _{\mathrm {coll} }>1} , where ν c e {\displaystyle \nu _{\mathrm {ce} }} is the electron gyrofrequency and ν c o l l {\displaystyle \nu _{\mathrm {coll} }} is the electron collision rate. It is often the case that the electrons are magnetized while the ions are not. Magnetized plasmas are anisotropic, meaning that their properties in the direction parallel to the magnetic field are different from those perpendicular to it. While electric fields in plasmas are usually small due to the plasma high conductivity, the electric field associated with a plasma moving with velocity v {\displaystyle \mathbf {v} } in the magnetic field B {\displaystyle \mathbf {B} } is given by the usual Lorentz formula E = v × B {\displaystyle \mathbf {E} =-\mathbf {v} \times \mathbf {B} } , and is not affected by Debye shielding.

Mathematical descriptions

The complex self-constricting magnetic field lines and current paths in a field-aligned Birkeland current that can develop in a plasma.
Main article: Plasma modeling

To completely describe the state of a plasma, all of the particle locations and velocities that describe the electromagnetic field in the plasma region would need to be written down. However, it is generally not practical or necessary to keep track of all the particles in a plasma. Therefore, plasma physicists commonly use less detailed descriptions, of which there are two main types:

Fluid model

Fluid models describe plasmas in terms of smoothed quantities, like density and averaged velocity around each position (see Plasma parameters). One simple fluid model, magnetohydrodynamics, treats the plasma as a single fluid governed by a combination of Maxwell's equations and the Navier–Stokes equations. A more general description is the two-fluid plasma, where the ions and electrons are described separately. Fluid models are often accurate when collisionality is sufficiently high to keep the plasma velocity distribution close to a Maxwell–Boltzmann distribution. Because fluid models usually describe the plasma in terms of a single flow at a certain temperature at each spatial location, they can neither capture velocity space structures like beams or double layers, nor resolve wave-particle effects.

Kinetic model

Kinetic models describe the particle velocity distribution function at each point in the plasma and therefore do not need to assume a Maxwell–Boltzmann distribution. A kinetic description is often necessary for collisionless plasmas. There are two common approaches to kinetic description of a plasma. One is based on representing the smoothed distribution function on a grid in velocity and position. The other, known as the particle-in-cell (PIC) technique, includes kinetic information by following the trajectories of a large number of individual particles. Kinetic models are generally more computationally intensive than fluid models. The Vlasov equation may be used to describe the dynamics of a system of charged particles interacting with an electromagnetic field. In magnetized plasmas, a gyrokinetic approach can substantially reduce the computational expense of a fully kinetic simulation.

Plasma science and technology

Plasmas are studied by the vast academic field of plasma science or plasma physics, including several sub-disciplines such as space plasma physics.

Plasmas can appear in nature in various forms and locations, with a few examples given in the following table:

Common forms of plasma
Artificially produced Terrestrial plasmas Space and astrophysical plasmas

Space and astrophysics

Further information: Astrophysical plasma

Plasmas are by far the most common phase of ordinary matter in the universe, both by mass and by volume.

Above the Earth's surface, the ionosphere is a plasma, and the magnetosphere contains plasma. Within our Solar System, interplanetary space is filled with the plasma expelled via the solar wind, extending from the Sun's surface out to the heliopause. Furthermore, all the distant stars, and much of interstellar space or intergalactic space is also filled with plasma, albeit at very low densities. Astrophysical plasmas are also observed in accretion disks around stars or compact objects like white dwarfs, neutron stars, or black holes in close binary star systems. Plasma is associated with ejection of material in astrophysical jets, which have been observed with accreting black holes or in active galaxies like M87's jet that possibly extends out to 5,000 light-years.

Artificial plasmas

Most artificial plasmas are generated by the application of electric and/or magnetic fields through a gas. Plasma generated in a laboratory setting and for industrial use can be generally categorized by:

  • The type of power source used to generate the plasma—DC, AC (typically with radio frequency (RF)) and microwave
  • The pressure they operate at—vacuum pressure (< 10 mTorr or 1 Pa), moderate pressure (≈1 Torr or 100 Pa), atmospheric pressure (760 Torr or 100 kPa)
  • The degree of ionization within the plasma—fully, partially, or weakly ionized
  • The temperature relationships within the plasma—thermal plasma ( T e = T i = T gas {\displaystyle T_{e}=T_{i}=T_{\text{gas}}} ), non-thermal or "cold" plasma ( T e T i = T gas {\displaystyle T_{e}\gg T_{i}=T_{\text{gas}}} )
  • The electrode configuration used to generate the plasma
  • The magnetization of the particles within the plasma—magnetized (both ion and electrons are trapped in Larmor orbits by the magnetic field), partially magnetized (the electrons but not the ions are trapped by the magnetic field), non-magnetized (the magnetic field is too weak to trap the particles in orbits but may generate Lorentz forces)

Generation of artificial plasma

Artificial plasma produced in air by a Jacob's Ladder
Artificial plasma produced in air by a Jacob's Ladder

Just like the many uses of plasma, there are several means for its generation. However, one principle is common to all of them: there must be energy input to produce and sustain it. For this case, plasma is generated when an electric current is applied across a dielectric gas or fluid (an electrically non-conducting material) as can be seen in the adjacent image, which shows a discharge tube as a simple example (DC used for simplicity).

The potential difference and subsequent electric field pull the bound electrons (negative) toward the anode (positive electrode) while the cathode (negative electrode) pulls the nucleus. As the voltage increases, the current stresses the material (by electric polarization) beyond its dielectric limit (termed strength) into a stage of electrical breakdown, marked by an electric spark, where the material transforms from being an insulator into a conductor (as it becomes increasingly ionized). The underlying process is the Townsend avalanche, where collisions between electrons and neutral gas atoms create more ions and electrons (as can be seen in the figure on the right). The first impact of an electron on an atom results in one ion and two electrons. Therefore, the number of charged particles increases rapidly (in the millions) only "after about 20 successive sets of collisions", mainly due to a small mean free path (average distance travelled between collisions).

Electric arc
Cascade process of ionization. Electrons are "e−", neutral atoms "o", and cations "+".
Avalanche effect between two electrodes. The original ionization event liberates one electron, and each subsequent collision liberates a further electron, so two electrons emerge from each collision: the ionizing electron and the liberated electron.

Electric arc is a continuous electric discharge between two electrodes, similar to lightning. With ample current density, the discharge forms a luminous arc, where the inter-electrode material (usually, a gas) undergoes various stages — saturation, breakdown, glow, transition, and thermal arc. The voltage rises to its maximum in the saturation stage, and thereafter it undergoes fluctuations of the various stages, while the current progressively increases throughout. Electrical resistance along the arc creates heat, which dissociates more gas molecules and ionizes the resulting atoms. Therefore, the electrical energy is given to electrons, which, due to their great mobility and large numbers, are able to disperse it rapidly by elastic collisions to the heavy particles.

Examples of industrial plasma

Plasmas find applications in many fields of research, technology and industry, for example, in industrial and extractive metallurgy, surface treatments such as plasma spraying (coating), etching in microelectronics, metal cutting and welding; as well as in everyday vehicle exhaust cleanup and fluorescent/luminescent lamps, fuel ignition, and even in supersonic combustion engines for aerospace engineering.

Low-pressure discharges
  • Glow discharge plasmas: non-thermal plasmas generated by the application of DC or low frequency RF (<100 kHz) electric field to the gap between two metal electrodes. Probably the most common plasma; this is the type of plasma generated within fluorescent light tubes.
  • Capacitively coupled plasma (CCP): similar to glow discharge plasmas, but generated with high frequency RF electric fields, typically 13.56 MHz. These differ from glow discharges in that the sheaths are much less intense. These are widely used in the microfabrication and integrated circuit manufacturing industries for plasma etching and plasma enhanced chemical vapor deposition.
  • Cascaded arc plasma source: a device to produce low temperature (≈1eV) high density plasmas (HDP).
  • Inductively coupled plasma (ICP): similar to a CCP and with similar applications but the electrode consists of a coil wrapped around the chamber where plasma is formed.
  • Wave heated plasma: similar to CCP and ICP in that it is typically RF (or microwave). Examples include helicon discharge and electron cyclotron resonance (ECR).
Atmospheric pressure
  • Arc discharge: this is a high power thermal discharge of very high temperature (≈10,000 K). It can be generated using various power supplies. It is commonly used in metallurgical processes. For example, it is used to smelt minerals containing Al2O3 to produce aluminium.
  • Corona discharge: this is a non-thermal discharge generated by the application of high voltage to sharp electrode tips. It is commonly used in ozone generators and particle precipitators.
  • Dielectric barrier discharge (DBD): this is a non-thermal discharge generated by the application of high voltages across small gaps wherein a non-conducting coating prevents the transition of the plasma discharge into an arc. It is often mislabeled "Corona" discharge in industry and has similar application to corona discharges. A common usage of this discharge is in a plasma actuator for vehicle drag reduction. It is also widely used in the web treatment of fabrics. The application of the discharge to synthetic fabrics and plastics functionalizes the surface and allows for paints, glues and similar materials to adhere. The dielectric barrier discharge was used in the mid-1990s to show that low temperature atmospheric pressure plasma is effective in inactivating bacterial cells. This work and later experiments using mammalian cells led to the establishment of a new field of research known as plasma medicine. The dielectric barrier discharge configuration was also used in the design of low temperature plasma jets. These plasma jets are produced by fast propagating guided ionization waves known as plasma bullets.
  • Capacitive discharge: this is a nonthermal plasma generated by the application of RF power (e.g., 13.56 MHz) to one powered electrode, with a grounded electrode held at a small separation distance on the order of 1 cm. Such discharges are commonly stabilized using a noble gas such as helium or argon.
  • "Piezoelectric direct discharge plasma:" is a nonthermal plasma generated at the high side of a piezoelectric transformer (PT). This generation variant is particularly suited for high efficient and compact devices where a separate high voltage power supply is not desired.

MHD converters

Main articles: magnetohydrodynamic converter, magnetohydrodynamic generator, and magnetohydrodynamic drive See also: Electrothermal instability

A world effort was triggered in the 1960s to study magnetohydrodynamic converters in order to bring MHD power conversion to market with commercial power plants of a new kind, converting the kinetic energy of a high velocity plasma into electricity with no moving parts at a high efficiency. Research was also conducted in the field of supersonic and hypersonic aerodynamics to study plasma interaction with magnetic fields to eventually achieve passive and even active flow control around vehicles or projectiles, in order to soften and mitigate shock waves, lower thermal transfer and reduce drag.

Such ionized gases used in "plasma technology" ("technological" or "engineered" plasmas) are usually weakly ionized gases in the sense that only a tiny fraction of the gas molecules are ionized. These kinds of weakly ionized gases are also nonthermal "cold" plasmas. In the presence of magnetics fields, the study of such magnetized nonthermal weakly ionized gases involves resistive magnetohydrodynamics with low magnetic Reynolds number, a challenging field of plasma physics where calculations require dyadic tensors in a 7-dimensional phase space. When used in combination with a high Hall parameter, a critical value triggers the problematic electrothermal instability which limited these technological developments.

Complex plasma phenomena

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Although the underlying equations governing plasmas are relatively simple, plasma behaviour is extraordinarily varied and subtle: the emergence of unexpected behaviour from a simple model is a typical feature of a complex system. Such systems lie in some sense on the boundary between ordered and disordered behaviour and cannot typically be described either by simple, smooth, mathematical functions, or by pure randomness. The spontaneous formation of interesting spatial features on a wide range of length scales is one manifestation of plasma complexity. The features are interesting, for example, because they are very sharp, spatially intermittent (the distance between features is much larger than the features themselves), or have a fractal form. Many of these features were first studied in the laboratory, and have subsequently been recognized throughout the universe. Examples of complexity and complex structures in plasmas include:

Filamentation

Striations or string-like structures are seen in many plasmas, like the plasma ball, the aurora, lightning, electric arcs, solar flares, and supernova remnants. They are sometimes associated with larger current densities, and the interaction with the magnetic field can form a magnetic rope structure. (See also Plasma pinch)

Filamentation also refers to the self-focusing of a high power laser pulse. At high powers, the nonlinear part of the index of refraction becomes important and causes a higher index of refraction in the center of the laser beam, where the laser is brighter than at the edges, causing a feedback that focuses the laser even more. The tighter focused laser has a higher peak brightness (irradiance) that forms a plasma. The plasma has an index of refraction lower than one, and causes a defocusing of the laser beam. The interplay of the focusing index of refraction, and the defocusing plasma makes the formation of a long filament of plasma that can be micrometers to kilometers in length. One interesting aspect of the filamentation generated plasma is the relatively low ion density due to defocusing effects of the ionized electrons. (See also Filament propagation)

Impermeable plasma

Impermeable plasma is a type of thermal plasma which acts like an impermeable solid with respect to gas or cold plasma and can be physically pushed. Interaction of cold gas and thermal plasma was briefly studied by a group led by Hannes Alfvén in 1960s and 1970s for its possible applications in insulation of fusion plasma from the reactor walls. However, later it was found that the external magnetic fields in this configuration could induce kink instabilities in the plasma and subsequently lead to an unexpectedly high heat loss to the walls.

In 2013, a group of materials scientists reported that they have successfully generated stable impermeable plasma with no magnetic confinement using only an ultrahigh-pressure blanket of cold gas. While spectroscopic data on the characteristics of plasma were claimed to be difficult to obtain due to the high pressure, the passive effect of plasma on synthesis of different nanostructures clearly suggested the effective confinement. They also showed that upon maintaining the impermeability for a few tens of seconds, screening of ions at the plasma-gas interface could give rise to a strong secondary mode of heating (known as viscous heating) leading to different kinetics of reactions and formation of complex nanomaterials.

Gallery

See also

Phase transitions of matter ()
ToFrom Solid Liquid Gas Plasma
Solid Melting Sublimation
Liquid Freezing Vaporization
Gas Deposition Condensation Ionization
Plasma Recombination

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