Effect of ionization distribution on the low frequency oscillations mode in Hall thrusters
Creators
- 1. Harbin Institute of Technology, Mail Box 3047, Harbin (China)
Description
It is found that the discharge parameters have notable effects on the mode of discharge current low frequency oscillation in Hall thrusters, but different discharge parameters might form the similar low frequency oscillation mode. In order to study the mechanism of oscillation mode formation, the ionization distribution in the discharge channel was measured experimentally, and one-dimensional quasi-neutrality hydrodynamic model was used to study the relationship between ionization distribution and the oscillation mode. Researches show that the low frequency oscillation with a narrow and condensed ionization distribution has the mode of lower amplitude and scattered frequency. The low frequency oscillation amplitude would become high and have dominative frequency component with the relative wide ionization distribution. Therefore, it can be concluded that the difference of ionization distribution characteristics is the main reason of the oscillation mode variation, and discharge parameters are only the external control parameters of ionization distribution characteristics.
Additional details
Identifiers
- DOI
- 10.1063/1.3676160;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 19
- Journal Issue
- 1
- Journal Page Range
- p. 012107-012107.6
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44003000
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- AMPLITUDES; DISTRIBUTION; ELECTRIC DISCHARGES; HYDRODYNAMIC MODEL; IONIZATION; MAGNETOHYDRODYNAMICS; OSCILLATION MODES; OSCILLATIONS; PLASMA; PLASMA WAVES; THRUSTERS
- Descriptors DEC
- FLUID MECHANICS; HYDRODYNAMICS; MATHEMATICAL MODELS; MECHANICS; PARTICLE MODELS; STATISTICAL MODELS; THERMODYNAMIC MODEL
Optional Information
- Notes
- (c) 2012 American Institute of Physics