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The Origins of Hot Plasma in the Solar Corona
Science, 2011The solar corona is heated by jets of plasma propelled upward from the region immediately above the Sun’s surface.
B, De Pontieu +8 more
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Cosmic Research, 2001
This review deals with basic results of experimental and theoretical studies (numerical simulations included) of the distributions, composition, and dynamics of particles of a hot plasma in the geomagnetosphere. Attention is drawn mainly to the ring current and the plasma sheet of the magnetotail, which play a key role in physics of the magnetosphere ...
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This review deals with basic results of experimental and theoretical studies (numerical simulations included) of the distributions, composition, and dynamics of particles of a hot plasma in the geomagnetosphere. Attention is drawn mainly to the ring current and the plasma sheet of the magnetotail, which play a key role in physics of the magnetosphere ...
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Injection of Hot Particles in the Plasma Flame
Journal of Thermal Spray Technology, 2000This study deals with experimental and theoretical investigations of preheating of the particles injected into a flame during the process of atmospheric plasma spraying (APS). Prior to the injection in the flame, the particles, delivered from the powder feeder, were heated in a carrier gas.
Albin Czernichowski +2 more
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2016
Section 10.1 describes Landau damping and cyclotron damping. Dielectric tensor of bi-Maxwellian hot plasma (10.59) and (10.60) are derived step by step in Sects. 10.2–10.5. Section 10.6 explains mathematical property of plasma dispersion function \(Z_\mathrm{p}(\zeta )\). Dispersion relation of electrostatic wave in homogeneous and inhomogeneous plasma
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Section 10.1 describes Landau damping and cyclotron damping. Dielectric tensor of bi-Maxwellian hot plasma (10.59) and (10.60) are derived step by step in Sects. 10.2–10.5. Section 10.6 explains mathematical property of plasma dispersion function \(Z_\mathrm{p}(\zeta )\). Dispersion relation of electrostatic wave in homogeneous and inhomogeneous plasma
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Physica Scripta, 1982
A survey is given of some recent developments in plasma physics, especially in theoretical plasma physics.
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A survey is given of some recent developments in plasma physics, especially in theoretical plasma physics.
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1998
Abstract In this chapter we will investigate the effects of the thermal motion of ions and electrons on the propagation of h.f. waves in plasmas. As a preliminary, it is useful to introduce notations for the dielectric tensor components and for the hot-plasma dispersion relation which take into account the considerations made in Section ...
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Abstract In this chapter we will investigate the effects of the thermal motion of ions and electrons on the propagation of h.f. waves in plasmas. As a preliminary, it is useful to introduce notations for the dielectric tensor components and for the hot-plasma dispersion relation which take into account the considerations made in Section ...
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Characterization of hot dense plasma with plasma parameters
Radiation Physics and Chemistry, 2018Abstract Characterization of hot dense plasma (HDP) with its parameters temperature, electron density, skin depth, plasma frequency is demonstrated in this work. The dependence of HDP parameters on temperature and electron density is discussed.
Narendra Singh, Arun Goyal, S. Chaurasia
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Hot-Electron Plasma by Beam-Plasma Interaction
Physical Review Letters, 1963A 5-kev d-c electron beam interacting with a plasma of deuterium yielded x-ray photons with energies up to 250 kev from the plasma region. An electron temperature of 32 kev and an electron density of 4 x 10/sup ''/ electrons cm/sup - 3/ are inferred from the total photon flux and its energy distribution.
I. Alexeff +4 more
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1990
The processes of ionization and recombination in hot (T ≳ 0.1 MK) astrophysical plasmas are considered, emphasizing the case of optically thin plasmas. A detailed comparison among different computations is made for the coronal model. The emergent radiation spectra are treated as a function of electron temperature.
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The processes of ionization and recombination in hot (T ≳ 0.1 MK) astrophysical plasmas are considered, emphasizing the case of optically thin plasmas. A detailed comparison among different computations is made for the coronal model. The emergent radiation spectra are treated as a function of electron temperature.
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Hot plasma effects in gas discharge plasma
Physics of Plasmas, 2005The subject of this paper is an abbreviated review of a recent study of rf discharges operating at low pressures where hot electron and nonlinear effects are essential. In this operational regime anomalous skin effect and collisionless electron heating may occur.
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