The electron-electron instability in a spherical plasma structure with an intermediate double layer
Creators
- 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
- DOI
- 10.1063/1.1564597;
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.