Reentry Antenna Test (RANT) Program. Volume 2. Linear Plasma Model. Addendum

1970 ◽  
Author(s):  
R. L. Fante ◽  
R. Elkin ◽  
J. Gottesfeld ◽  
R. O'Keefe
Keyword(s):  
Plasma Model ◽  
Linear Plasma

A point plasma model for linear plasma devices based on SOLPS-ITER equations: application to helium plasma

2021 ◽  
Author(s):  
Elena Tonello ◽  
Arianna Formenti ◽  
Gabriele Alberti ◽  
Andrea Uccello ◽  
Matteo Passoni
Keyword(s):  
Helium Plasma ◽  
Plasma Model ◽  
Linear Plasma

scholarly journals Quantifying erosion and retention of silicon carbide due to D plasma irradiation in a high-flux linear plasma device

2021 ◽  
Vol 26 ◽  
pp. 100939
Author(s):  
G. Sinclair ◽  
T. Abrams ◽  
S. Bringuier ◽  
D.M. Thomas ◽  
L. Holland ◽  
...  
Keyword(s):  
Silicon Carbide ◽  
High Flux ◽  
Plasma Irradiation ◽  
Plasma Device ◽  
Linear Plasma

Non-linear plasma wave decay to longer wavelength

2015 ◽  
Author(s):  
F. Anderegg ◽  
M. Affolter ◽  
A. Ashourvan ◽  
D. H. E. Dubin ◽  
F. Valentini ◽  
...  
Keyword(s):  
Plasma Wave ◽  
Wave Decay ◽  
Non Linear ◽  
Linear Plasma

A collisional-radiative SF/sub 6/ arc plasma model using Boltzmann analysis

1997 ◽  
Vol 25 (5) ◽  
pp. 996-1000 ◽  
Author(s):  
G. Cliteur ◽  
K. Suzuki ◽  
H. Ikeda ◽  
S. Yanabu
Keyword(s):  
Arc Plasma ◽  
Plasma Model

Magnetised Wave Collapse in Solar System Plasmas

1993 ◽  
Vol 10 (4) ◽  
pp. 283-286 ◽  
Author(s):  
Andrew Melatos ◽  
Peter Robinson
Keyword(s):  
Solar System ◽  
Wave Packets ◽  
Particle Interactions ◽  
Coherent Wave ◽  
Wave Collapse ◽  
Non Linear ◽  
Acceleration Zone ◽  
The Waves ◽  
Linear Plasma

AbstractClumpy, intense wave packets observed in situ in the Jovian and terrestrial electron foreshocks, and in the Earth’s auroral acceleration zone, point to the existence of non-linear plasma turbulence in these regions. In non-linear turbulence, wave packets collapse to short scales and high fields, stopping only when coherent wave-particle interactions efficiently dissipate the energy in the waves. The purpose of this paper is to examine the shortest scales and highest fields achieved during collapse in a strongly magnetised plasma, and identify parts of the solar system where the magnetised aspects of wave collapse are important.

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