Physics of plasmas

By L. C. Woods. 2003

1,116 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atomic and Molecular Physics, and Optics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/76e4370c9dd595a7ee6f5f3b77b71945ee71e0a1

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Citations in the corpus

Landau Damping: Paraproducts and Gevrey Regularity (2013, background): “However, it was noted by Vlasov [85] that collisions are relatively weak in plasmas (see also [17]) and hence, for many phenomena, it makes sense to consider only mean-field electromagnetic fields.”
Alfvén Waves and Turbulence in the Solar Atmosphere and Solar Wind (2007, methodology): “…which should effectively favor the development of a turbulent cascade in planes perpendicular to the direction of wave propagation (along the magnetic field), has been found (Zank et al. 1996; Matthaeus et al. 1998, 1999;Dmitruk et al. 2001a, 2002;Dmitruk&Matthaeus 2003; Oughton et al. 2001, 2004).”
Simulating cosmic rays in clusters of galaxies – II. A unified scheme for radio haloes and relics with predictions of the γ-ray emission (2007, background): “Furthermore, shearing motions induced by oblique shocks stretch these field lines which leads to a larger magnetic coherence length of two-dimensional field configurations (Schekochihin & Cowley 2006).”
Global existence for the Euler-Maxwell system (2011, background): “There are different models to describe the state of a plasma depending on several parameters such as the Debey length, the plasma frequency, the collision frequencies between the different species... Formal derivation of these models can be found in Plasma Physics textbooks (see for instance Bellan ”
Generalized Squashing Factors for Covariant Description of Magnetic Connectivity in the Solar Corona (2007, background): “They serve as preferred sites for the formation of current sheets and the corresponding accumulation of the free magnetic energy (Sweet 1969; Baum & Bratenahl 1980; Syrovatskii 1981; Lau & Finn 1990; Longcope & Cowley 1996; Priest & Titov 1996; Priest & Forbes 2000; Longcope 2001).”
Non-spherical core collapse supernovae. I. Neutrino-driven convection, Rayleigh-Taylor instabilities, and the formation and propagation of metal clumps (2003, methodology): “Further insight might, however, be gained by laser experiments (Robey et al. 2001; Kane et al. 2001; Drake et al. 2002; Klein et al. 2003, and the references therein), and hydrodynamic code validation experiments as those described by Fishbine (2002) and Zoldi (2002) before well-resolved 3D…”
Ecological collapse and the emergence of travelling waves at the onset of shear turbulence (2015, background): “The specific system has three trophic levels: nutrient (E), Prey (B) and Predator (A), which correspond in the fluid system to laminar flow, turbulence and zonal flow respectively.”
Density limits in toroidal plasmas (2002, background): “Techniques for wall conditioning [6] [7] [8] [9] [10] [11] [12] [13] [14] [15] have been developed which enable operation at higher densities.”
Oscillations and Waves in Solar Spicules (2009, background): “…the actual mathematical form of the governing equation and its solution for kink and longitudinal oscillations in a gravitationally stratified and anchored magnetic flux tube is very similar, see e.g. Sutmann et al. (1998); Musielak and Ulmschneider (2001); Ballai et al. (2006) for more details.”
On the stability threshold for the 3D Couette flow in Sobolev regularity (2015, background): “[14, 47, 38]), also plays a role in suppressing certain nonlinear effects.”
Non-linear MHD simulations of edge localized modes (ELMs) (2009, background): “Using this representation both the variables and their derivatives are continuous.”
Sharp reduction of the secondary electron emission yield from grooved surfaces (2008, background): “Historically, much of the work done to suppress multipacting was developed in the klystron industry [1,2,3].”