Stability of Non-Neutral Plasma Cylinder Consisting of Magnetized Cold Electrons and of Small Density Fraction of Ions Born at Rest: Non-Local Analysis
Journal Article
·
· AIP Conference Proceedings
- Institute of Plasma Physics, National Science Center 'Kharkov Institute of Physics and Technology', 61108 Kharkov (Ukraine)
The non-local stability problem of the plasma cylinder, filled with 'cold' magnetized rigidly rotating electrons, and a small density fraction of ions, is solved. The ions are supposed to be born at rest by ionization of background gas. The study is based on the kinetic description of ions. The equilibrium distribution function, taking into account the peculiarity of ions birth, is used. The radial electric field is caused by space charge of non-neutral plasma. The dispersion equation for plasma eigen frequencies is obtained analytically. It is valid within the total admissible range of values of electric and magnetic fields. Normalized eigen frequencies {omega}'/{omega}{sub i} are calculated for the basic azimuth mode m = 1({omega}' {omega}-m{omega}{sub i}{sup +}, {omega}{sub +} = (-{omega}{sub ci}+{omega}{sub i})/2, {omega}{sub i} ({omega}{sub ci}{sup 2}-4eE{sub r}/m{sub i}r){sup 1/2} is called the 'modified' ion cyclotron (MIC) frequency), for the density fraction of ions of atomic nitrogen f N{sub i}/n{sub e} = 0,01 and are presented in graphic form versus parameter 2{omega}{sub pe}{sup 2}/{omega}{sub ce}{sup 2}. The spectra of oscillations {omega}'/{omega}{sub i} consist of the family of electron Trivel-piece--Gould (TG) modes and of the families of MIC modes. The frequencies of MIC modes are located in a small vicinity of harmonics of the MIC frequency {omega}{sub i} above and below the harmonic. The TG modes in non-neutral plasma fall in the region of MIC frequencies {omega}{sub i} and interact strongly with MIC modes. The slow TG modes become unstable near the crossings with non-negative harmonics of MIC frequencies. The instabilities have a resonant character. The lowest radial TG mode has a maximum growth rate at crossing with a zero harmonic of {omega}{sub i} ((Im {omega}'/{omega}{sub i}){sub max}{approx_equal}0,074). The growth rates of MIC modes are much lower ((Im {omega}'/{omega}{sub i}){sub max} < or approx. 0,002). Their instability has a threshold character. The instabilities of TG and MIC modes take place mainly at the values of parameter 2{omega}{sub pe}{sup 2}/{omega}{sub ce}{sup 2}, corresponding to strong radial electric fields ({omega}{sub ci}{sup 2}<<|eE{sub r}/m{sub i}r|), in which the ions are unmagnetized. The oscillations of small amplitude are seen on some frequency dependencies of MIC modes. They are similar to oscillations on dispersion curves of electron waves in metals and are caused by the similarity between the ion equilibrium distribution function and the degenerate Fermi--Dirac one. The results obtained give the solution to the stability problem discussed by R.H. Levy, J.D. Daugherty and O. Buneman [Phys. Fl. 12, 2616-2629 (1969)] for a special case of plasma bounding directly with metal casing and possessing the volumetric eigen modes only.
- OSTI ID:
- 21300435
- Journal Information:
- AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1114; ISSN 0094-243X; ISSN APCPCS
- Country of Publication:
- United States
- Language:
- English
Similar Records
Behaviour and stability of Trivelpiece-Gould modes in non-neutral plasma containing small density fraction of background gas ions
Conditions and growth rate of Rayleigh instability in a Hall thruster under the effect of ion temperature
LONGITUDINAL ION OSCILLATIONS IN A HOT PLASMA
Journal Article
·
Tue Mar 19 00:00:00 EDT 2013
· AIP Conference Proceedings
·
OSTI ID:22113543
Conditions and growth rate of Rayleigh instability in a Hall thruster under the effect of ion temperature
Journal Article
·
Tue Mar 15 00:00:00 EDT 2011
· Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics (Print)
·
OSTI ID:21560079
LONGITUDINAL ION OSCILLATIONS IN A HOT PLASMA
Technical Report
·
Tue Jun 28 00:00:00 EDT 1960
·
OSTI ID:4129223