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...s in high temperature, low resistivity toroidal plasmas|journal=Physics of Plasmas|language=en|volume=8|issue=1|pages=103–109|doi=10.1063/1.1331098|issn=1070- ...

...n the [[interstellar medium]] inside of galaxies. Moreover, gas throughout space is [[turbulent]] implying it has density structure on all spatial scales. [[Category:Space plasmas]] ...

...tios is an important tool to obtain information about laboratory and space plasmas. In emission [[spectroscopy]], the '''intensity of spectral lines''' can pr ...is:<ref>{{cite book |last=Salzmann |first=D. |title=Atomic Physics in Hot Plasmas |publisher=[[Oxford University Press]] |year=1998 |isbn=978-0-19-510930-6 | ...

...processes acting on the resonant electrons and ions, which requires phase space analyses. Since the latter is stochastic, transient and rather filamentary ...tructures are also known under [[Bernstein–Greene–Kruskal modes]] or phase space [[electron]] and [[ion]] holes, or double layers, respectively. ...

...tailoring of both [[positron]] and [[antiproton]] (i.e. [[antiparticle]]) plasmas for a variety of end uses. Single-component plasmas (SCP), which are a type of [[Non-neutral plasmas|nonneutral plasma]], have many uses, including studying a variety of plasma ...

| known_for = Single-component and [[Non-neutral plasmas|non-neutral plasma]] research, [[Penning–Malmberg trap]], collisionless dam ...s]] in 1964,<ref name=":1" /> as well as for his research on [[non-neutral plasmas]] and the development of the [[Penning–Malmberg trap]].<ref name=":2" /><re ...

...ted by suitable boundary conditions, it describes the entire configuration space of possible events the ion fluid is capable of, both globally and locally. ...expansion into vacuum, i.e. a plasma that is confined initially in a half-space and is released at t=0 to occupy in course of time the second half.<ref na ...

...tle=A simple diffusion model showing anomalous scaling |journal=Physics of Plasmas |volume=15 |pages=082308 |year=2008 |issue=8 |doi=10.1063/1.2969429|bibcode ...

{{Short description|Space propulsion system using plasma}} ...t, allowing the nozzle to adapt to different propulsive requirements and [[space mission]]s. Magnetic nozzles are the fundamental acceleration stage of seve ...

...ar=1994|title=Determination of the noninductive current profile in tokamak plasmas|url=https://zenodo.org/record/1233899|journal=Physical Review Letters|volum ...psilon_0</math> is the [[Vacuum permittivity|electric permittivity of free space]], <math>k_\text{B}</math> is the [[Boltzmann constant]], and <math>T_\text ...

...ionization degree microplasmas such as atmospheric pressure laser-induced plasmas.<ref>{{Cite journal |last=Patel |first=Adam |date=2021 |title=Thomson and c ...regime. The linear oscillation of unbound electrons in a relatively-small space gives rise to a short-dipole radiation pattern. ...

...first2=Kenneth|date=1999-06-20|title=FRC fusion propulsion system for deep space exploration results from the Star Thrust Experiment (STX)|journal=35th Join ...onfiguration with rotating magnetic field current drive|journal=Physics of Plasmas|language=en|volume=7|issue=5|pages=1945–1950|doi=10.1063/1.874019|bibcode=2 ...

...[partial differential equation]] of first order in time and third order in space. Similar to a [[Korteweg–De Vries equation]] (KdV),<ref name="myref1" /> it ...ion holes or phase space vortices in collision-free plasmas such as space plasmas,<ref name="myref3" /> ...

...(or more) 'X-points' can be created. An X-point is defined as a point in space at which the poloidal field has zero magnitude. The magnetic [[flux surfac ...

.... B. (1970). Small-scale fluctuations of relic radiation. Astrophysics and Space Science, 7, 3-19.</ref> ...P. W. (2021). Simplified derivation of the Kompaneets equation. Physics of Plasmas, 28(9).</ref> ...

...he unique example of [[Astronomical X-ray source|X-ray source]], since hot plasmas are present wherever in the Universe: from stellar coronae to thin [[galact ...|name-list-style=amp | title = Calculated X-radiation from optically thin plasmas. III – Abundance effects on continuum emission ...

...uency]], and <math>\nabla</math> the [[gradient]], taken in flat Euclidean space in ''n'' dimensions. The <math>\eta_j</math> are the interaction coefficie |title=Space-time evolution of nonlinear three-wave interactions. I. Interaction in a ho ...

...cs)#Thermal vs. nonthermal (cold) plasmas|non-thermal]] [[Plasma (physics)|plasmas]] used in [[MHD converter]]s. It was first theoretically discovered in 1962 | title = Hall instability of current carrying slightly ionized plasmas ...

...the world's most sophisticated fusion devices and now to studying the way plasmas interact with the inside wall and materials of fusion devices. In fact, it ...nal Meeting on Theoretical and Experimental Aspects of Heating of Toroidal Plasmas, Grenoble France, 28 June 1976, 8311643</ref> ...

[[Category:Space plasmas]] [[Category:Waves in plasmas]] ...