Plasma classification (types of plasma)

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Plasmas are described by many characteristics, such as temperature, degree of ionization, and density, the magnitude of which, and approximations of the model describing them, gives rise to plasmas that may be classified in different ways.

Contents

Pseudo-plasmas vs real plasmas

A real plasma may have complex characteristics that exhibited complex phenomena. To model it's behavior, scientists may approximate and simplify a real plasma's characteristics; this pseudo-plasma may or may not be a adequate representation of a real plasma. Pseudo-plasmas tend to neglect double layers, instabilities, filamentary structures, plasma beams, electric currents, and other potentially important properties.

Cold, warm and hot plasmas

In the laboratory in the positive column of a glow discharge tube:

"..there is a plasma composed of the same number of electrons and ions. [..] In low pressure gas discharge, the collision rate between electrons and gas molecules is not frequent enough for non-thermal equilibrium to exist between the energy of the electrons and the gas molecules. So the high-energy particles are mostly composed of electrons while the energy of the gas molecules is around room temperature. We have Te >> Ti >> Tg where Te, Ti and Tg are the temperatures of the electron, ion and gas molecules, respectively. This type of plasma is called a "cold plasma".
"In a high pressure gas discharge the collision between electrons and gas molecules occurs frequently. This causes thermal equilibrium between the electrons and gas molecules. We have Te ≃ Tg. We call this type of plasma a "hot plasma".
"In cold plasma, the degree of ionization is below 10-4."[1]

Hot plasma (thermal plasma)

A hot plasma in one which approaches a state of local thermodynamic equilibrium (LTE). A hot plasma is also called a thermal plasma, but in Russian literature, a "low temperature" plasma in order to distinguish it from a thermonuclear fusion plasma.[2] Such plasmas can be produced by atmospheric arcs, sparks and flames.[3]

Warm plasma

Cold plasma (non-thermal plasma)

A cold plasma is one in which the thermal motion of the ions can be ignored. Consequently there is no pressure force, the magnetic force can be ignored, and only the electric force is considered to act on the particles.[4] Examples of cold plasmas include the Earth's ionopshere (about 1000K compared to the Earth's ring current temperature of about 108K).[5], the flow discharge in a fluorescent tube, [6]

Ultracold plasma

An ultracold plasma is one which occurs at temperatures as low as 1K.[7] and may be formed by photoionizing laser-cooled atoms. Ultracold plasmas tend to be rather delicate, experiments being carried out in vacuum.[8]

Plasma ionization

The degree of ionization of a plasma is the proportion of charged particles to the total number of particles including neutrals and ions, and is defined as: α = n+/(n + n+) where n is the number of neutrals, and n+ is the number of charged particles. α is the Greek letter alpha.

Degree required to exhibit plasma behaviour

Umran S. Inan et al write:

"It turns out that a very low degree of ionization is sufficient for a gas to exhibit electromagnetic properties and behave as a plasma: a gas achieves an electrical conductivity of about half its possible maximum at about 0.1% ionization and had a conductivity nearly equal to that of a full ionized gas at about 1% ionization." [9]

In a plasma where the degree of ionization is high, charged particle collisions dominate. In plasmas with a low degree of ionization, collisions between charged particles and neutrals dominate. The degree of ionization which determines when a gas becomes a plasma will vary between different types if plasma, and may be as little as 10-6:

"Among the many types of plasma, those commonly employed for plasma processing are low temperature, low density, non-equilibrium, collision dominated-environments. By low temperature, we mean "cold" plasmas with a temperature normally ranging from 300K and 600K, by low density we mean plasmas with neutral gas number densities of approximately 1013 to 1016 molecules cm-3 (pressure between ~ 0.1 to 103 Pa) which are weakly ionized between 10-6 to 10-1"[10]

Also:

".. Coulomb collisions will dominate over collisions with neutrals in any plasma that is even just a few percent ionized. Only if the ionization level is very low (<10-3) can neutral collisions dominate."[11]

Alfvén and Arrhenius also note:

"The transition between a fully ionized plasma and a partially ionized plasma, and vice versa, is often discontinuous (Lehnert, 1970b)[12]. When the input energy to the plasma increases gradually, the degree of ionization jumps suddenly from a fraction of 1 percent to full ionization. Under certain conditions, the border between a fully ionized and a weakly ionized plasma is very sharp."[13]

Fully ionized plasma

A fully ionized plasma has a degree of ionization approaching 1 (ie. 100%). Examples include the Solar Wind (interplanetery medium), stellar interiors (the Sun's core), fusion plasmas

Partially ionized plasma (weakly ionized gas)

A partially ionized plasma has a degree of ionization that is less than 1. Examples include the ionosphere (2x10-3)[14], gas discharge tubes.

The aurora may exhibition properties of a weakly ionized gas and a weakly ionized plasma:

"If we observe an aurora in the night sky we get a conspicuous and spectacular demonstration of the difference between gas and plasma behavior. Faint aurorae are often diffuse and spread over large areas. They fit reasonably well into the picture of an ionized gas. The degree of ionization is so I low that the medium still has some of the physical properties of a gas that is homogeneous over large volumes. However, in certain other cases (e.g., when the auroral intensity increases), the aurora becomes highly inhomogeneous, consisting of a multitude of rays, thin arcs, and draperies a conspicuous illustration of the basic properties of most magnetized plasmas."[13]

Associate Professor of Physics, Richard Fitzpatrick, writes:

"Note that plasma-like behaviour ensues after a remarkably small fraction of the gas has undergone ionization. Thus, fractionally ionized gases exhibit most of the exotic phenomena characteristic of fully ionized gases."[15]

Collisional plasmas

Collisional plasma

Non-collisional plasma

Neutral plasmas

Neutral plasma

Non-neutral plasma

Plasmas densities

High density plasma

Medium density plasma

Low density plasma

Magnetic plasmas

Magnetic plasma

Non-magnetic plasma

Complex plasmas

Dusty plasmas and grain plasmas

A dusty plasma is a plasma containing nanometer or micrometer-sized particles suspended in it. A grain plasma contains larger particles than dusty plasmas. Examples include comets, planetary rings, exposed dusty surfaces, and the zodiacal dust cloud.[16]

Colloidal plasmas, Liquid plasmas and Plasma crystals

"A macroscopic Coulomb crystal of solid particles in a plasma has been observed. Images of a cloud of 7-μm "dust" particles, which are charged and levitated in a weakly ionized argon plasma, reveal a hexagonal crystal structure. The crystal is visible to the unaided eye."[17]

"Colloidal plasmas may "condense" under certain conditions into liquid and crystalline states, while retaining their essential plasma properties. This "plasma condensation" therefore leads to new states of matter: "liquid plasmas" and "plasma crystals." The experimental discovery was first reported in 1994".[18]

"Liquid and crystalline phases can be formed in so-called complex plasmas — plasmas enriched with solid particles in the nano- to micrometre range. The particles absorb electrons and ions and charge negatively up to a few volts. Due to their high mass compared to that of electrons and ions the particles dominate the processes in the plasma and can be observed on the most fundamental — the kinetic level. Through the strong Coulomb interaction between the particles it is possible that the particle clouds form fluid and crystalline structures. The latter is called 'plasma crystal'."[19]

Active and passive plasmas

Hannes Alfvén writes:

"Passive plasma regions, which can be described by classical hydrodynamic theory. They transmit waves and high energy charged particles but if the field-aligned currents exceed a certain value they are transferred into.
Active plasma regions: These carry field-aligned currents which give them filamentary or sheet structure with thickness down to a few cyclotron radii (ionic or even electronic). They transmit energy from one region to another and produce electric double layers which accelerate particles to high energies. Active regions cannot be described by hydromagnetic theories. Boundary conditions are essential and may be introduced by circuit theory"[20]

Alfvén continues:

Passive plasma

"These regions may transmit different kinds of plasma waves and flow of high energy particles. There may be transient currents perpendicular to the magnetic field changing the state of motion of the plasma but not necessarily associated with strong electric fields and currents parallel to the magnetic field. A plasma of this kind fills most of space."

Active plasma

"Besides the passive plasma regions there are also small but very important regions where filamentary and sheet currents flow (Alfvén, 1977a)[21]. By transferring energy and producing sharp borders between different regions of passive plasmas, they are of decisive importance to the overall behaviour of plasmas in space. There are two different - but somewhat related - types of such regions which we shall call plasma cables and boundary current sheets."

Ideal and non-ideal plasmas

An ideal plasma is one in which Coulomb collisions are negligible, otherwise the plasma is non-ideal.

"At low densities, a low-temperature, partly ionized plasma can be regarded as a mixture of ideal gases of electrons, atoms and ions. The particles travel at thermal velocities, mainly along straight paths, and collide with each other only occasionally. In other words, the free path times prove greater than those of interparticle interaction. With an increase in density, mean distances between the particles decrease and the particles start spending even more time interacting with each other, that is, in the fields of surrounding particles. Under these conditions, the mean energy of interparticle interaction increases. When this energy becomes comparable with the mean kinetic energy of thermal motion, the plasma becomes non-ideal."[22]


High Energy Density Plasmas (HED plasmas)

Footnotes

  1. ^ Kiyotaka Wasa, Shigeru Hayakawa, Handbook of Sputter Deposition Technology: Principles, Technology and Applications (Materials Science and Process Technology Series), (1992), William Andrew Inc., 304 pages, ISBN 0815512805 (page 95)
  2. ^ Maher I. Boulos, Pierre Fauchais, Emil Pfender, Thermal Plasmas: Fundamentals and Applications (1994) Springer, ISBN 0306446073 (p.6) ACADEMIC BOOK
  3. ^ Souheng Wu, Polymer Interface and Adhesion CRC Press, ISBN 0824715330, (page 299) ACADEMIC BOOK
  4. ^ Marcel Goossens, An Introduction to Plasma Astrophysics and Magnetohydrodynamics (2003) Springer, 216 pages, ISBN 1402014333, (page 25) ACADEMIC BOOK
  5. ^ The Sun to the Earth -- And Beyond: Panel Reports, National Research Council (U.S.) (2003) 246 pages, ISBN 0309089727 (p.59) FULL TEXT ACADEMIC BOOK
  6. ^ A. J. van Roosmalen, J. A. G. Baggerman, S. J. H. Brader, Dry Etching for VLSI, Springer, 254 pages, ISBN 0306438356 (page. 14)
  7. ^ T. Killian, T. Pattard, T. Pohl, and J. Rost, "Ultracold neutral plasmas", Physics Reports 449, 77 (2007).
  8. ^ Steven L. Rolston, "Ultracold neutral plasmas", Trends, July 14, 2008, American Physical Society
  9. ^ Umran S. Inan, Marek Gołkowski, Principles of Plasma Physics for Engineers and Scientists, Publ. Cambridge University Press, 2011, ISBN 0521193729, 9780521193726, 284 pages (page 4)
  10. ^ Loucas G. Christophorou, James Kenneth Olthoff, Fundamental Electron Interactions With Plasma Processing Gases, (2004) in Section 3.1 Low-temperature, Low-Density, Non-Equilibrium Plasmas, 76 pages, ISBN 0306480379 (page 39)
  11. ^ Robert J. Goldston, Paul Harding Rutherford, Introduction to Plasma Physics, "Fully and Partially Ionized Plasmas" (page 164)
  12. ^ Lehnert, B., "Minimum temperature and power effect of cosmical plasmas interacting with neutral gas", Cosmic Electrodynamics (1970) 1:397.
  13. ^ a b Hannes Alfvén and Gustaf Arrhenius, Evolution of the Solar System, (1976) Part C, Plasma and Condensation, "15. Plasma Physics and Hetegony FULL TEXT
  14. ^ Francis Delobeau, The Environment of the Earth, (1971) 132 pages, ISBN 902770208X (page 13)
  15. ^ Richard Fitzpatrick, Introduction to Plasma Physics: A graduate level course,FULL TEXT "Introduction: 1.2 What is plasma?" p.6 ACADEMIC BOOK
  16. ^ Horanyi Mihaly, and Mitchell Colin J., "Dusty Plasmas in Space: 6. Saturn's Rings: A Dusty Plasma Laboratory", Journal of Plasma and Fusion Research, Vol.82; No. 2; Page 98-102 (2006)
  17. ^ H. Thomas et al, "Plasma Crystal: Coulomb Crystallization in a Dusty Plasma", Phys. Rev. Lett. 73, 652 - 655 (1994)
  18. ^ G. E. Morfill, H. M. Thomas, U. Konopka, and M. Zuzic, "The plasma condensation: Liquid and crystalline plasmas", Physics of Plasmas 6, 1769 (1999);
  19. ^ Gregor E Morfill et al, "A review of liquid and crystalline plasmas—new physical states of matter?", 2002 Plasma Phys. Control. Fusion 44 B263-B277
  20. ^ Hannes Alfvén, "Plasma in laboratory and space",FULL TEXT Journal de Physique Colloques 40, C7 (1979) C7-1-C7-19
  21. ^ Hannes Alfvén, "Electric Currents in Cosmic Plasmas", Reviews of Geophysics and Space Physics, vol. 15, Aug. 1977, p. 271-284.
  22. ^ V. E. Fortov, Igor T. Iakubov, The physics of non-ideal plasma, World Scientific, 2000, ISBN 9810233051, ISBN 9789810233051, 403 pages. (Page 1)
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