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{{Short description|State of matter}} | |||
{{Other uses|Plasma (disambiguation){{!}}Plasma}} | |||
{{Pp|small=yes}} | |||
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{{Use dmy dates|date=September 2024}} | |||
], illustrating some of the more complex phenomena of a plasma, including '']''. The colors are a result of relaxation of electrons in excited states to lower energy states after they have recombined with ions. These processes emit light in a ] characteristic of the gas being excited.]] | |||
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| image1 = Lightning3.jpg | |||
| 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 | |||
In ] and ], '''plasma''' is a ] similar to ] in which a certain portion of the particles are ]ized. After sufficient heating a gas dissociates its ]s, rendering it into constituent ]s. However, further heating may also lead to ] (a loss or gain of ]) of the molecules or atoms of the gas, thus turning it into a plasma, containing ]d particles: positive ] and negative electrons.<ref name="Sturrock" /> | |||
|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><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 | |||
|last=Phillips | |||
|first=K. J. H. | |||
|date=1995 | |||
|title=Guide to the Sun | |||
|page=295 | |||
|publisher=] | |||
|url=https://books.google.com/books?id=idwBChjVP0gC&q=Guide+to+the+Sun+phillips | |||
|isbn=978-0-521-39788-9 | |||
|url-status=live | |||
|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 | |||
|archive-date=15 January 2018 | |||
}}</ref><ref name="Aschwanden2004">{{cite book | |||
|last=Aschwanden | |||
|first=M. J. | |||
|year=2004 | |||
|title=Physics of the Solar Corona. An Introduction | |||
|publisher=Praxis Publishing | |||
|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 | |||
|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> | |||
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 | |||
The presence of a non-negligible number of ]s makes the plasma ] so that it responds strongly to ]s. Plasma, therefore, has properties quite unlike those of ]s, ]s, or ]es and is considered a distinct ]. Like gas, plasma does not have a definite shape or a definite volume unless enclosed in a container; unlike gas, under the influence of a magnetic field, it may form structures such as filaments, beams and double layers. Some common plasmas are ]s and ]s. In the ], plasma is the most common ] for ], most of which is in the rarefied ] (particularly ]) and in stars. | |||
|last1=Chu | |||
|first1=P.K. | |||
|last2=Lu | |||
|first2=XinPel | |||
|date=2013 | |||
|title=Low Temperature Plasma Technology: Methods and Applications | |||
|publisher=CRC Press | |||
|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 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 </ref> The nature of the Crookes tube "]" matter was subsequently identified by British physicist ] in 1897,<ref>Announced in his evening lecture to the ] on Friday, 30th April 1897, and published in {{cite journal|journal=]|volume=44|page=293|url=http://web.lemoyne.edu/~GIUNTA/thomson1897.html|year=1897}}</ref> and dubbed "plasma" by ] in 1928,<ref name="langmuir1928">{{cite journal|author=I. Langmuir|doi=10.1073/pnas.14.8.627|title=Oscillations in ionized gases|journal=Proc. Nat. Acad. Sci. U.S.|volume=14|issue=8|page=628|year=1928|bibcode = 1928PNAS...14..627L }}</ref> perhaps because it characteristic that the glowing discharge mold itself to any shape into which the tube is formed.<ref>{{cite book|author=BROWN, Sanborn C.|chapter=Chapter 1: A Short History of Gaseous Electronics|editor=HIRSH, Merle N. e OSKAM, H. J.|title=Gaseous Electronics|volume=1|local=Nova Yorque|publisher=Academic Press|year=1978|ISBN=0-12-349701-9}}</ref> Langmuir wrote: | |||
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. | |||
==Early history== | |||
<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.<ref name="langmuir1928" /></blockquote> | |||
] calculated by an ] ]. Note the fast moving electrons and slow ions, resembling a ].]] | |||
==Common plasmas== | |||
{{see|Astrophysical plasma|Interstellar medium|Intergalactic space}} | |||
Plasmas are by far the most common ] in the universe, both by mass and by volume.<ref>It is often stated that more than 99% of the material in the visible universe is plasma. See, for example, {{cite book|author=D. A. Gurnett, A. Bhattacharjee|title=Introduction to Plasma Physics: With Space and Laboratory Applications|year=2005|url=http://books.google.com/?id=VcueZlunrbcC&pg=PA2|page=2|isbn=0521364833|publisher=Cambridge University Press|location=Cambridge, UK}} and {{cite book|author=K Scherer, H Fichtner, B Heber|title=Space Weather: The Physics Behind a Slogan|year=2005|url=http://books.google.com/?id=irHgIUtLi0gC&pg=PA138|page=138|isbn=3540229078|publisher=Springer|location=Berlin}}. Essentially, all of the visible light from space comes from stars, which are plasmas with a temperature such that they radiate strongly at visible wavelengths. Most of the ordinary (or ]ic) matter in the universe, however, is found in the ], which is also a plasma, but much hotter, so that it radiates primarily as X-rays. The current scientific consensus is that about 96% of the total energy density in the universe is not plasma or any other form of ordinary matter, but a combination of ] and ].</ref> All the ]s are made of plasma, and even the space between the stars is filled with a plasma, albeit a very sparse one. In our solar system, the planet ] accounts for most of the ''non''-plasma, only about 0.1% of the mass and 10<sup>−15</sup>% of the volume within the orbit of ]. Very small grains within a gaseous plasma will also pick up a net negative charge, so that they in turn may act like a very heavy negative ion component of the plasma (see ]s). | |||
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> | |||
{| class="wikitable" | |||
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> | |||
|+ Common forms of plasma | |||
|- | |||
! Artificially produced | |||
! style="width: 11em;" | ] plasmas | |||
! style="width: 18em;" | Space and ] plasmas | |||
|- style="vertical-align: top;" | |||
| | |||
*Those found in ], including TVs | |||
*Inside ]s (low energy lighting), ]s<ref></ref> | |||
*Rocket exhaust and ]s | |||
*The area in front of a ]'s ] during re-entry into the ] | |||
*Inside a corona discharge ] generator | |||
*] research | |||
*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 | |||
| | |||
*] | |||
*] | |||
*] | |||
*] | |||
*The ] | |||
*The ] | |||
*Most ]s | |||
| | |||
*The ] and other ]s<br />(plasmas heated by ]) | |||
*The ] | |||
*The ]<br />(space between planets) | |||
*The ]<br />(space between star systems) | |||
*The ]<br />(space between galaxies) | |||
*The ]-] ] | |||
*]s | |||
*Interstellar ]e | |||
|} | |||
{{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.}} | |||
==Plasma properties and parameters== | |||
], 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 , press release: </ref>]] | |||
] 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> | |||
===Definition of a plasma=== | |||
Plasma is loosely described as an electrically neutral medium of positive and negative particles (i.e. the overall charge of a plasma is roughly zero). It is important to note that although they are unbound, these particles are not ‘free’. When the charges move they generate electrical currents with magnetic fields, and as a result, they are affected by each other’s fields. This governs their collective behavior with many degrees of freedom.<ref name="Sturrock">{{cite book |title=Plasma Physics: An Introduction to the Theory of Astrophysical, Geophysical & Laboratory Plasmas. |last=Sturrock |first=Peter A. |year=1994 |publisher=Cambridge University Press |isbn=0521448107}}</ref><ref>{{cite book |title=The Framework of Plasma Physics |author=Hazeltine, R.D.; Waelbroeck, F.L. |year=2004 |publisher=Westview Press. |isbn=0738200476 }} | |||
</ref> A definition can have three criteria:<ref name="Hazeltine">{{cite book|author=R. O. Dendy|title=Plasma Dynamics|url=http://books.google.com/?id=S1C6-4OBOeYC|publisher=Oxford University Press|year=1990|isbn=0198520417}}</ref><ref>{{cite book|author=Daniel Hastings, Henry Garrett|title=Spacecraft-Environment Interactions|isbn=0521471281|publisher=Cambridge University Press|year=2000}}</ref> | |||
{{Continuum mechanics|fluid}} | |||
#'''The plasma approximation''': Charged particles must be close enough together that each particle influences many nearby charged particles, rather than just interacting with the closest particle (these collective effects are a distinguishing feature of a plasma). The plasma approximation is valid when the number of charge carriers within the sphere of influence (called the ''Debye sphere'' whose radius is the ]) of a particular particle is higher than unity to provide collective behavior of the charged particles. The average number of particles in the Debye sphere is given by the ], "Λ" (the ] letter ]). | |||
#'''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. | |||
#'''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. | |||
==Definitions== | |||
===Ranges of plasma parameters=== | |||
===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 parameters can take on values varying by many ], but the properties of plasmas with apparently disparate parameters may be very similar (see ]). The following chart considers only conventional atomic plasmas and not exotic phenomena like ]s: | |||
</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: | |||
] | |||
{|class=wikitable | {| class="wikitable" | ||
! | |||
!colspan=2|Typical ranges of plasma parameters: orders of magnitude (OOM) | |||
|- | |- | ||
! {{diagonal split header|Property|State}} !! Gas !! Plasma | |||
!Characteristic | |||
!Terrestrial plasmas | |||
!Cosmic plasmas | |||
|- | |- | ||
! Interactions | |||
|'''Size'''<br>in meters | |||
| '''Short-range''': Two-particle (binary) ]s are the rule. | |||
|10<sup>−6</sup> m (lab plasmas) to<br>10<sup>2</sup> m (lightning) (~8 ]) | |||
| '''Long-range''': Collective motion of particles is ubiquitous in plasma, resulting in various ] and other types of collective phenomena. | |||
|10<sup>−6</sup> m (spacecraft sheath) to<br>10<sup>25</sup> m (intergalactic nebula) (~31 OOM) | |||
|- | |- | ||
! Electrical conductivity | |||
|'''Lifetime'''<br>in seconds | |||
| '''Very low''': Gases are excellent ] up to electric field strengths of tens of kilovolts per centimetre.<ref>{{cite web | |||
|10<sup>−12</sup> s (laser-produced plasma) to<br>10<sup>7</sup> s (fluorescent lights) (~19 OOM) | |||
| url=https://hypertextbook.com/facts/2000/AliceHong.shtml | |||
|10<sup>1</sup> s (solar flares) to<br>10<sup>17</sup> s (intergalactic plasma) (~16 OOM) | |||
| 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 | |||
|'''Density'''<br> in particles per<br>cubic meter | |||
| '''One''': All gas particles behave in a similar way, largely influenced by collisions with one another and by ]. | |||
|10<sup>7</sup> m<sup>−3</sup> to<br>10<sup>32</sup> m<sup>−3</sup> (inertial confinement plasma) | |||
| '''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. | |||
|1 m<sup>−3</sup> (intergalactic medium) to<br>10<sup>30</sup> m<sup>−3</sup> (stellar core) | |||
|- | |||
|'''Temperature'''<br>in kelvins | |||
|~0 K (crystalline non-neutral plasma<ref>See at the University of California, San Diego</ref>) to<br>10<sup>8</sup> K (magnetic fusion plasma) | |||
|10<sup>2</sup> K (aurora) to<br>10<sup>7</sup> K (solar core) | |||
|- | |||
|'''Magnetic fields'''<br>in teslas | |||
|10<sup>−4</sup> T (lab plasma) to<br>10<sup>3</sup> T (pulsed-power plasma) | |||
|10<sup>−12</sup> T (intergalactic medium) to<br>10<sup>11</sup> T (near neutron stars) | |||
|} | |} | ||
=== |
===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> | |||
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 mostly by the temperature. Even a partially ionized gas in which as little as 1% of the particles are ionized can have the characteristics of a plasma (i.e., response to magnetic fields and high ]). The degree of ionization, ''α'' is defined as ''α'' = ''n''<sub>i</sub>/(''n''<sub>i</sub> + ''n''<sub>a</sub>) where ''n''<sub>i</sub> is the number density of ions and ''n''<sub>a</sub> is the number density of neutral atoms. The ''electron density'' is related to this by the average charge state <Z> of the ions through ''n''<sub>e</sub> = <Z> ''n''<sub>i</sub> where ''n''<sub>e</sub> is the number density of electrons. | |||
*'''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> | |||
===Temperatures=== | |||
*'''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=== | |||
Plasma temperature is commonly measured in ]s or ]s and is, informally, a measure of the thermal kinetic energy per particle. Very 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 ], (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. |year=1983 |publisher=John Wiley & Sons |isbn=047109045X}}</ref> and the plasma will eventually become a gas. | |||
{{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> | |||
===Dusty plasma=== | |||
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 "]". This is especially common in weakly ionized technological plasmas, where the ions are often near the ]. | |||
{{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== | |||
Based on the relative temperatures of the electrons, ions and neutrals, plasmas are classified as "thermal" or "non-thermal". Thermal plasmas have electrons and the heavy particles at the same temperature, i.e., they are in thermal equilibrium with each other. Non-thermal plasmas on the other hand have the ions and neutrals at a much lower temperature, (normally room temperature), whereas electrons are much "hotter". | |||
] 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 plasma is sometimes referred to as being "hot" if it is nearly fully ionized, or "cold" if only a small fraction (for example 1%), of the gas molecules are ionized, but other definitions of the terms "hot plasma" and "cold plasma" are common. Even in a "cold" plasma, the electron temperature is still typically several thousand degrees Celsius. Plasmas utilized in "plasma technology" ("technological plasmas") are usually cold in this sense. | |||
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> | |||
===Potentials=== | |||
] | |||
is an example of plasma present at Earth's surface. | |||
Typically, lightning discharges 30,000 amperes at up to 100 million volts, and emits light, radio waves, X-rays and even gamma rays.<ref>See </ref> Plasma temperatures in lightning can approach ~28,000 kelvin and electron densities may exceed 10<sup>24</sup> m<sup>−3</sup>.]] | |||
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 ]). | |||
Since plasmas are very good conductors, electric potentials play an important role. | |||
The potential as it exists on average in the space between charged particles, independent of the question 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 (''n''<sub>e</sub> = <Z>''n''<sub>i</sub>), but on the scale of the Debye length there can be charge imbalance. In the special case that '']'' are formed, the charge separation can extend some tens of Debye lengths. | |||
===Temperature=== | |||
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 "]": | |||
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. | |||
:<math>n_e \propto e^{e\Phi/k_BT_e}</math>. | |||
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> | |||
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>. | |||
{{see also|Nonthermal plasma|Anisothermal plasma}} | |||
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 ]. | |||
===Plasma potential=== | |||
In ] plasmas, ] prevents ]s from directly affecting the plasma over large distances, i.e., greater than the ]. But the existence of charged particles causes the plasma to generate and can be affected by ]s. This can and does cause extremely complex behavior, 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 ]. | |||
] 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>{{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.<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 ]: | |||
===Magnetization=== | |||
<math display="block">n_e \propto \exp(e\Phi/k_\text{B} T_e).</math> | |||
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., ω<sub>ce</sub>/ν<sub>coll</sub> > 1, where ω<sub>ce</sub> is the "electron gyrofrequency" and ν<sub>coll</sub> 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 '''E''' = −'''v''' x '''B''' (where '''E''' is the electric field, '''v''' is the velocity, and '''B''' is the magnetic field), and is not affected by ].<ref>Richard Fitzpatrick, ''Introduction to Plasma Physics'', </ref> | |||
Differentiating this relation provides a means to calculate the electric field from the density: | |||
===Comparison of plasma and gas phases=== | |||
<math display="block">\vec{E} = \frac{k_\text{B} T_e}{e} \frac{\nabla n_e}{n_e}.</math> | |||
Plasma is often called the ''fourth state of matter''. It is distinct from other lower-energy ]; most commonly ], ], and ]. 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: | |||
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> | |||
<table class="wikitable"> | |||
===Magnetization=== | |||
<tr style="background:#eee; text-align:center; vertical-align:top;"> | |||
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> | |||
<td>'''Property'''</td> | |||
<td>'''Gas'''</td> | |||
<td>'''Plasma'''</td> | |||
</tr> | |||
==Mathematical descriptions== | |||
<tr valign=top> | |||
] 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>]] | |||
<td style="background:#eee;">''']'''</td> | |||
{{main|Plasma modeling}} | |||
<td>'''Very low''' | |||
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: | |||
:Air is an excellent insulator until it breaks down into plasma at electric field strengths above 30 kilovolts per centimeter.<ref>{{cite web|url=http://hypertextbook.com/facts/2000/AliceHong.shtml|title=Dielectric Strength of Air|year=2000|first=Alice|last=Hong|work=The Physics Factbook}}</ref> | |||
<td>'''Usually very high''' | |||
:For many purposes, the conductivity of a plasma may be treated as infinite. | |||
</td> | |||
</tr> | |||
<tr valign=top> | |||
<td style="background:#eee;">'''Independently acting species'''</td> | |||
<td>'''One''' | |||
:All gas particles behave in a similar way, influenced by ] and by ]s with one another.</td> | |||
<td>'''Two or three''' | |||
:], ], ] and ] 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 ]. | |||
</td> | |||
</tr> | |||
===Fluid model=== | |||
<tr valign=top> | |||
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}} | |||
<td style="background:#eee;">'''Velocity distribution'''</td> | |||
<td>''']''' | |||
:Collisions usually lead to a Maxwellian velocity distribution of all gas particles, with very few relatively fast particles. </td> | |||
<td>'''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. | |||
</td> | |||
</tr> | |||
<tr valign=top> | |||
<td style="background:#eee;">'''Interactions'''</td> | |||
<td>'''Binary''' | |||
:Two-particle collisions are the rule, three-body collisions extremely rare.</td> | |||
<td>'''Collective''' | |||
:Waves, or organized motion of plasma, are very important because the particles can interact at long ranges through the electric and magnetic forces. | |||
</td> | |||
</tr> | |||
===Kinetic model=== | |||
</table> | |||
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}} | |||
==Plasma science and technology== | |||
==Complex plasma phenomena== | |||
] of "]", a huge ball of expanding plasma. The outer shell shown in blue is X-ray emission by high-speed electrons.]] | |||
Plasmas are studied by the vast ] of ''plasma science'' or ''plasma physics'', including several sub-disciplines such as ]. | |||
Although the underlying equations governing plasmas are relatively simple, plasma behavior is extraordinarily varied and subtle: the emergence of unexpected behavior from a simple model is a typical feature of a ]. Such systems lie in some sense on the boundary between ordered and disordered behavior 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 can appear in nature in various forms and locations, with a few examples given in the following table: | |||
===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?|year=1990|journal=Bulletin of the American Astronomical Society|volume= 22|page=832}}</ref> are seen in many plasmas, like the plasma ball, the ],<ref>{{cite journal|author=Grydeland, T., ''et al.''|doi=10.1029/2002GL016362|title=Interferometric observations of filamentary structures associated with plasma instability in the auroral ionosphere|year=2003|journal=Geophysical Research Letters|volume=30|issue=6|page=71|bibcode=2003GeoRL..30f..71G}}</ref> ],<ref>{{cite journal|author=Moss, Gregory D., ''et al.''|doi=10.1029/2005JA011350|title=Monte Carlo model for analysis of thermal runaway electrons in streamer tips in transient luminous events and streamer zones of lightning leaders|year=2006|journal=Journal of Geophysical Research|volume=111|issue=A2|pages=A02307|bibcode=2006JGRA..11102307M}}</ref> ]s, ],<ref>{{cite journal|author=Doherty, Lowell R.|doi=10.1086/148107|title=Filamentary Structure in Solar Prominences|year=1965|journal=The Astrophysical Journal|volume=141|page=251|last2=Menzel|first2=Donald H.|bibcode=1965ApJ...141..251D}}</ref> and ]s.<ref></ref> They are sometimes associated with larger current densities, and the interaction with the magnetic field can form a ] structure.<ref>{{cite journal|author=Zhang, Yan-An, ''et al.''|bibcode=2002ChA&A..26..442Z |title=A rope-shaped solar filament and a IIIb flare|year=2002|journal=Chinese Astronomy and Astrophysics|volume=26|issue=4|pages=442–450|doi=10.1016/S0275-1062(02)00095-4}}</ref> High power microwave breakdown at atmospheric pressure also leads to the formation of filamentary structures.<ref name="mwbrkdwn">{{cite journal | author=Jean-Pierre Boeuf, Bhaskar Chaudhury, and Guo Qiang Zhu | |||
| title=Theory and Modeling of Self-Organization and Propagation of Filamentary Plasma Arrays in Microwave Breakdown at Atmospheric Pressure | year=2010 | journal=] | volume=104 | issue=1 | page=015002 | doi= 10.1103/PhysRevLett.104.015002 | bibcode=2010PhRvL.104a5002B | |||
}}</ref> (See also ]) | |||
{{clear}} | |||
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 journal|author=S. L. Chin|url=http://icpr.snu.ac.kr/resource/wop.pdf/J01/2006/049/S01/J012006049S010281.pdf|journal=Journal of the Korean Physical Society|volume=49|year=2006|page=281|title=Some Fundamental Concepts of Femtosecond Laser Filamentation}}</ref> | |||
{| class="wikitable" | |||
===Shocks or double layers=== | |||
|+ Common forms of plasma | |||
Plasma properties change rapidly (within a few ] lengths) across a two-dimensional sheet in the presence of a (moving) shock or (stationary) ]. Double layers involve localized charge separation, which causes a large potential difference across the layer, but does not generate an electric field outside the layer. Double layers separate adjacent plasma regions with different physical characteristics, and are often found in current carrying plasmas. They accelerate both ions and electrons. | |||
|- | |||
! style="width: 40%;"|Artificially produced | |||
! style="width: 30%;"|Terrestrial plasmas | |||
! style="width: 30%;"|Space and astrophysical plasmas | |||
|- style="vertical-align: top;" | |||
| | |||
*In ], including TV screens. | |||
*Inside ]s (low energy lighting), ]s | |||
*Rocket exhaust and ]s | |||
*The area in front of a ]'s ] during ] into the ] | |||
*Plasmas in ] research | |||
*] (sometimes called plasma sphere or plasma ball) | |||
*]-produced plasmas (LPP), found when high power lasers interact with materials | |||
| | |||
*] | |||
*The ] contains plasma in the Earth's surrounding space environment | |||
*The ] | |||
*The ] | |||
*], including ], blue jets, blue starters, gigantic jets, ELVESs | |||
*] | |||
*] (if sufficiently hot) | |||
| | |||
*]s (plasmas heated by ]) | |||
*The ] | |||
*The ] (space between planets) | |||
*The ] (space between star systems) | |||
*The ]<br />(space between galaxies) | |||
*]s | |||
*Interstellar ]e | |||
|} | |||
=== |
===Space and astrophysics=== | ||
Quasineutrality of a plasma requires that plasma currents close on themselves in electric circuits. Such circuits follow ] and possess a ] and ]. These circuits must generally be treated as a strongly coupled system, with the behavior in each plasma region dependent on the entire circuit. It is this strong coupling between system elements, together with nonlinearity, which may lead to complex behavior. Electrical circuits in plasmas store inductive (magnetic) energy, and should the circuit be disrupted, for example, by a plasma instability, the inductive energy will be released as plasma heating and acceleration. This is a common explanation for the heating that takes place in the ]. Electric currents, and in particular, magnetic-field-aligned electric currents (which are sometimes generically referred to as "]s"), are also observed in the Earth's aurora, and in plasma filaments. | |||
{{further|Astrophysical plasma}} | |||
===Cellular structure=== | |||
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> | |||
Narrow sheets with sharp gradients may separate regions with different properties such as magnetization, density and temperature, resulting in cell-like regions. Examples include the ], ], and ]. Hannes Alfvén wrote: "From the cosmological point of view, the most important new space research discovery is probably the cellular structure of space. As has been seen in every region of space accessible to in situ measurements, there are a number of 'cell walls', sheets of electric currents, which divide space into compartments with different magnetization, temperature, density, etc."<ref>{{cite book|author=Hannes Alfvén|title=Cosmic Plasma|year=1981|chapter=section VI.13.1. Cellular Structure of Space|isbn=9027711518|publisher=Dordrecht}}</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> | |||
===Critical ionization velocity=== | |||
The ] is the relative velocity between an ionized plasma and a neutral gas, above which a runaway ionization process takes place. The critical ionization process is a quite general mechanism for the conversion of the kinetic energy of a rapidly streaming gas into ionization and plasma thermal energy. Critical phenomena in general are typical of complex systems, and may lead to sharp spatial or temporal features. | |||
=== |
===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: | |||
Ultracold plasmas are created in a ] (MOT) by trapping and cooling neutral ], to temperatures of 1 ] or lower, and then using another ] to ] the atoms by giving each of the outermost electrons just enough energy to escape the electrical attraction of its parent ion. | |||
*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 mTorr or 1 Pa), moderate pressure (≈1 Torr or 100 Pa), atmospheric pressure (760 Torr or 100 kPa){{Citation needed|date=January 2021}} | |||
*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_\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{{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}} | |||
====Generation of artificial plasma==== | |||
One advantage of ultracold plasmas are their well characterized and tunable initial conditions, including their size and electron temperature. By adjusting the wavelength of the ionizing laser, the kinetic energy of the liberated electrons can be tuned as low as 0.1 K, a limit set by the frequency bandwidth of the laser pulse. The ions inherit the millikelvin temperatures of the neutral atoms, but are quickly heated through a process known as disorder induced heating (DIH). This type of non-equilibrium ultracold plasma evolves rapidly, and displays many other interesting phenomena.<ref>{{cite book|url=http://books.google.com/?id=rHo6IbakG2kC&pg=PA190|pages=190–193|title=Plasma science: advancing knowledge in the national interest|author=National Research Council (U.S.). Plasma 2010 Committee|publisher=National Academies Press|year=2007|isbn=0309109434}}</ref> | |||
] | |||
]]] | |||
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/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}} | |||
One of the metastable states of a strongly nonideal plasma is ], which forms upon condensation of excited atoms. | |||
=== |
=====Electric arc===== | ||
] | |||
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 ]s, an electron cloud in a ] and positron plasmas.<ref>{{cite journal|author=R. G. Greaves, M. D. Tinkle, and C. M. Surko|doi=10.1063/1.870693|title=Creation and uses of positron plasmas|year=1994|journal=Physics of Plasmas|volume=1|issue=5|page=1439|bibcode = 1994PhPl....1.1439G }}</ref> | |||
] | |||
] is a continuous electric discharge between two electrodes, similar to ]. | |||
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 plasma==== | ||
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> | |||
A ] contains tiny charged particles of dust (typically found in space), which also behave like a plasma. A plasma that contains larger particles is called grain plasma. | |||
=====Low-pressure discharges===== | |||
==Mathematical descriptions== | |||
*''] 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 ] 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> | |||
] that can develop in a plasma.<ref>See '', 1976)</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> | |||
{{main|Plasma modeling}} | |||
*'']'': a device to produce low temperature (≈1eV) high density plasmas (HDP). | |||
To completely describe the state of a plasma, we would need to write down all the | |||
*''] (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> | |||
particle locations and velocities and describe the electromagnetic field in the plasma region. | |||
*'']'': 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> | |||
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: | |||
=== |
=====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 ].{{Citation needed|date=January 2021}} | |||
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. | |||
*'']:'' 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. 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. | |||
| last2 = Campagne | first2 = C. | |||
| last3 = Perwuelz | first3 = A. | |||
| last4 = Gengembre | first4 = L. O. | |||
| title = Polypropylene film chemical and physical modifications by dielectric barrier discharge plasma treatment at atmospheric pressure | |||
| doi = 10.1016/j.jcis.2008.09.062 | |||
| journal = Journal of Colloid and Interface Science | |||
| volume = 328 | |||
| issue = 2 | |||
| pages = 412–420 | |||
| year = 2008 | |||
| pmid = 18930244 | |||
| 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 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 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.{{Citation needed|date=January 2021}} | |||
=== |
====MHD converters==== | ||
{{main|magnetohydrodynamic converter|magnetohydrodynamic generator|magnetohydrodynamic drive}} | |||
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. | |||
{{see also|Electrothermal instability}} | |||
In magnetized plasmas, a ] approach can substantially reduce the computational expense of a fully kinetic simulation. | |||
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|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}} | |||
==Artificial plasmas== | |||
Most artificial plasmas are generated by the application of electric and/or magnetic fields. 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 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<sub>e</sub>'' = ''T''<sub>ion</sub> = ''T''<sub>gas</sub>), non-thermal or "cold" plasma (''T<sub>e</sub>'' >> ''T''<sub>ion</sub> = ''T''<sub>gas</sub>) | |||
*The electrode configuration used to generate the plasma | |||
*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) | |||
*The application | |||
==Complex plasma phenomena== | |||
===Generation of artificial plasma=== | |||
{{Tone|section|talk=Opinionated judgemental language|date=June 2024}} | |||
]]] | |||
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 image below, which shows a ] as a simple example (] used for simplicity). | |||
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: | |||
] | |||
===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> 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 ]) | |||
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. |year=1984 |publisher=Plenum Press |isbn=0306413329}}</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 ]). This is a stage of avalanching ionization, 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). | |||
With ample current density and ionization, this forms a luminous ] (essentially ]) 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 |year=2004 |title=Plasma Processing of Municipal Solid Waste |journal= Brazilian Journal of Physics |volume=34 |issue=4B |page=1587 |bibcode = 2004BrJPh..34.1587L }}</ref>|group="Note"}} ] along the continuous electric arc creates ], which ionizes more gas molecules (where degree of ionization 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 2000°C the gas molecules become atomized, and ionized at 3000°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 ionized and have lower energy densities, and thus the temperature is not dispersed evenly among the particles, where some heavy ones remain ‘cold’.</ref> | |||
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 ]) | |||
===Examples of industrial/commercial 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 |doi=10.1016/j.jhazmat.2008.04.017 |author=Gomez, E., Rani, D.A., Cheeseman, C.R., Deegan, D., Wise, M., Boccaccini, A.R. |year=2009 |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 |pmid=18499345 }}</ref> surface treatments such as ] (coating), ] in microelectronics,<ref name="NRC">{{cite book |author= National Research Council |year=1991 |title=Plasma Processing of Materials : Scientific Opportunities and Technological Challenges. |publisher=National Academies Press |isbn= 0309045975 }}</ref> metal cutting<ref name="Nemchinsky">{{cite journal |doi=10.1088/0022-3727/39/22/R01 |author=Nemchinsky, V.A., Severance, W.S. |year=2006 |title=What we know and what we do not know about plasma arc cutting |journal=J. Phys. D: Appl. Phys. |volume=39 |issue=22 |pages=R423–R438 |bibcode = 2006JPhD...39R.423N }}</ref> and ]; as well as in everyday ] and ]/] lamps,<ref name="Hippler">{{cite book |editor=Hippler, R., Kersten, H., Schmidt, M., Schoenbach, K.M. |year=2008 |title=Low Temperature Plasmas: Fundamentals, Technologies, and Techniques |chapter=Plasma Sources |publisher=Wiley-VCH |edition=2 |isbn=3527406735 }}</ref> while even playing a part in ] for ].<ref name="Peretich">{{cite journal |author=Peretich, M.A., O’Brien, W.F., Schetz, J.A. |year=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 }}</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.|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> | |||
*''] 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 ] tubes.<ref>{{cite web |url=http://www-spof.gsfc.nasa.gov/Education/wfluor.html |title=The Fluorescent Lamp: A plasma you can use. |author=Dr. David P. Stern |accessdate=2010-05-19}}</ref> | |||
*''] (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.<ref>{{cite journal |last1=Sobolewski |first1=M.A. |last2=Langan & Felker |first2=J.G. & B.S. |year=1997 |title=Electrical optimization of plasma-enhanced chemical vapor deposition chamber cleaning plasmas |publisher=J. Vac. Sci. Technol. B |volume=16 |issue=1 |pages=173–182 |url=http://physics.nist.gov/MajResProj/rfcell/Publications/MAS_JVSTB16_1.pdf}}</ref> | |||
*''] (ICP)'': similar to a CCP and with similar applications but the electrode consists of a coil wrapped around the discharge volume that inductively excites the plasma.{{Citation needed|date=August 2008}} | |||
*'']'': similar to CCP and ICP in that it is typically RF (or microwave), but is heated by both electrostatic and electromagnetic means. Examples are ], ] (ECR), and ] (ICR). These typically require a coaxial magnetic field for wave propagation.{{Citation needed|date=August 2008}} | |||
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> | |||
====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 melt rocks containing Al<sub>2</sub>O<sub>3</sub> to produce ]. | |||
*'']:'' 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. | |||
*''] (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|author=F. Leroux et al. |title=Atmospheric air plasma treatments of polyester textile structures|journal=Journal of Adhesion Science and Technology|volume=20|issue=9|pages=939–957|year=2006|doi=10.1163/156856106777657788}}</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|author=F. Leroux et al.|doi=10.1016/j.jcis.2008.09.062|title=Polypropylene film chemical and physical modifications by dielectric barrier discharge plasma treatment at atmospheric pressure|year=2008|journal=Journal of Colloid and Interface Science|volume=328|page=412|pmid=18930244|issue=2}}</ref> | |||
*'']:'' this is a ] 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.<ref>{{cite journal|author=J. Park et al.|doi=10.1063/1.1323753|title=Discharge phenomena of an atmospheric pressure radio-frequency capacitive plasma source|year=2001|journal=Journal of Applied Physics|volume=89|issue=1|page=20|bibcode = 2001JAP....89...20P }}</ref> | |||
==Gallery== | |||
==Fields of active research== | |||
<gallery> | |||
]. The electric field in a plasma ] is so effective at accelerating ions that electric fields are used in ]s.]] | |||
File:HallThruster 2.jpg|] | |||
<!--This list needs organization and pruning!--> | |||
File:Wispy 'Plasma Dancer' on the limb of the Sun.ogv|Solar plasma | |||
This is just a partial list of topics. A more complete and organized list can be found on the web site Plasma science and technology.<ref>Web site for </ref> | |||
File:Plasma Spraying Process.jpg|Plasma spraying | |||
<table><tr valign=top><td> | |||
File:MAST plasma image.jpg|Plasma in a ] | |||
*Plasma theory | |||
File:Argon Plasma.jpg|Laboratory plasma | |||
**] | |||
</gallery> | |||
**Plasma interactions with waves and beams | |||
**] | |||
**] | |||
**] | |||
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*Plasmas in nature | |||
**The Earth's ] | |||
**] | |||
**Space plasmas, e.g. Earth's ] (an inner portion of the ] dense with plasma) | |||
**] | |||
*Industrial plasmas | |||
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**] radar | |||
*Plasma applications | |||
**] | |||
***] (MFE) — ], ], ], ], ] | |||
***] (IFE) (also Inertial confinement fusion — ICF) | |||
***] | |||
**] | |||
**] | |||
**] | |||
**Food processing (], aka "cold plasma") | |||
**], convert waste into reusable material with plasma. | |||
**] | |||
**] (e. g. Dentistry <ref name=tws44>{{cite news | |||
| author = | |||
| title = High-tech dentistry – "St Elmo's frier" – Using a plasma torch to clean your teeth | |||
| publisher = The Economist print edition | |||
| date = Jun 17th 2009 | |||
| url = http://www.economist.com/displaystory.cfm?story_id=13794903&fsrc=rss | |||
| accessdate = 2009-09-07 | |||
}}</ref>) | |||
**] | |||
</table> | |||
==See also== | ==See also== | ||
{{portal|Physics}} | {{portal|Physics}} | ||
{{colbegin|colwidth=20em}} | |||
{{Commons category|Plasma physics}} | |||
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{{colend}} | |||
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{{Table_of_phase_transitions}} | |||
==Notes== | |||
<references group="Note" /> | |||
==References== | ==References== | ||
{{ |
{{Reflist|30em}} | ||
==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=y| n=Special:Search/Plasma physics}} | |||
{{wiktionary|plasma}} | |||
* {{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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*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 }}| | |||
* - a list of plasma related links. | |||
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*Introduction to Plasma Physics: | | |||
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Latest revision as of 20:50, 13 December 2024
State of matterTop: 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 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."
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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 plasmasThe 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 plasmaA 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
Density and ionization degree
For plasma to exist, ionization is necessary. The term "plasma density" by itself usually refers to the electron density , that is, the number of charge-contributing electrons per unit volume. The degree of ionization is defined as fraction of neutral particles that are ionized:
where is the ion density and the neutral density (in number of particles per unit volume). In the case of fully ionized matter, . Because of the quasineutrality of plasma, the electron and ion densities are related by , where 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 plasmaPlasma potential
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 (), 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:
Differentiating this relation provides a means to calculate the electric field from the density:
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., , where is the electron gyrofrequency and 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 in the magnetic field is given by the usual Lorentz formula , and is not affected by Debye shielding.
Mathematical descriptions
Main article: Plasma modelingTo 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:
Artificially produced | Terrestrial plasmas | Space and astrophysical plasmas |
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|
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Space and astrophysics
Further information: Astrophysical plasmaPlasmas 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 (), non-thermal or "cold" plasma ()
- 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
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
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 instabilityA 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
- Hall-effect thruster
- Solar plasma
- Plasma spraying
- Plasma in a tokamak
- Laboratory plasma
See also
ToFrom | Solid | Liquid | Gas | Plasma |
---|---|---|---|---|
Solid | Melting | Sublimation | ||
Liquid | Freezing | Vaporization | ||
Gas | Deposition | Condensation | Ionization | |
Plasma | Recombination |
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- Alfvén, H.; Smårs, E. (1960). "Gas-Insulation of a Hot Plasma". Nature. 188 (4753): 801–802. Bibcode:1960Natur.188..801A. doi:10.1038/188801a0. S2CID 26797662.
- Braams, C.M. (1966). "Stability of Plasma Confined by a Cold-Gas Blanket". Physical Review Letters. 17 (9): 470–471. Bibcode:1966PhRvL..17..470B. doi:10.1103/PhysRevLett.17.470.
- Yaghoubi, A.; Mélinon, P. (2013). "Tunable synthesis and in situ growth of silicon-carbon mesostructures using impermeable plasma". Scientific Reports. 3: 1083. Bibcode:2013NatSR...3.1083Y. doi:10.1038/srep01083. PMC 3547321. PMID 23330064.
External links
- Plasmas: the Fourth State of Matter Archived 30 September 2019 at the Wayback Machine
- Introduction to Plasma Physics: Graduate course given by Richard Fitzpatrick|M.I.T. Introduction by I.H.Hutchinson
- Plasma Material Interaction
- How to make a glowing ball of plasma in your microwave with a grape Archived 6 September 2005 at the Wayback Machine|More (Video)
- OpenPIC3D – 3D Hybrid Particle-In-Cell simulation of plasma dynamics
- Plasma Formulary Interactive
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