Published May 2003 | Version v1
Journal article

The electron-electron instability in a spherical plasma structure with an intermediate double layer

  • 1. E.T.S.I. Aeronauticos, Universidad Politecnica de Madrid, 28040 Madrid (Spain)

Description

A linear dynamic model of a spherical plasma structure with an intermediate double layer is analyzed in the high-frequency range. The two ion populations tend to stay frozen in their stationary response and this prevents the displacement of the double layer. Different electron modes dominate the plasma dynamics in each quasineutral region. The electrostatic potential and the electron current are the magnitudes most perturbed. The structure develops a reactive electron-electron instability, which is made up of a countable family of eigenmodes. Space-charge effects must be included in the quasineutral regions to determine the eigenmode carrying the maximum growth rate. Except for very small Debye lengths, the fundamental eigenmode governs the instability. The growth rate for the higher harmonics approaches that of an infinite plasma. The instability modes develop mainly on the plasma at the high-potential side of the double layer. The influence of the parameters defining the stationary solution on the instability growth rate is investigated, and the parametric regions of stability are found. The comparison with a couple of experiments on plasma contactors is satisfactory

Additional details

Identifiers

Publishing Information

Journal Title
Physics of Plasmas
Journal Volume
10
Journal Issue
5
Journal Page Range
p. 1351-1363
ISSN
1070-664X
CODEN
PHPAEN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
35033973
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Descriptors DEI
BOUNDARY LAYERS; INSTABILITY GROWTH RATES; PERTURBATION THEORY; PLASMA; PLASMA INSTABILITY; PLASMA SIMULATION; PLASMA WAVES; WALL EFFECTS
Descriptors DEC
INSTABILITY; LAYERS; SIMULATION

Optional Information

Notes
(c) 2003 American Institute of Physics.