Experimental study on the characteristics of low power microwave plasma jet within local vacuum environment
- 1. College of Astronautics, Northwestern Polytechnic University, Xi'an 710072 (China)
Description
A microwave plasma jet based on a coaxial cavity can be generated in atmosphere and vacuum environments. It is shown that with argon gas and a power range of 53-60 W, cavity efficiency ranges from 54% to 68%. The electron density distribution and the microwave return loss of the confined plasma jet adjacent to a metal object and their dependency on argon mass flow rate and power have been studied by applying emission/Langmuir probe and spatial reflected wave diagnostic equipments in a low scatter vacuum environment. The results show that the electron density ranges from 8.8x1014 to 7.53x1016/m3, and the electron density on the centerline of the jet decreases exponentially from the nozzle exit plane, but its distribution off the centerline is in an upheaved curve. Increasing mass flow rate at constant power and increasing power at constant mass flow rate increase electron density mildly. From typical measurements of microwave return loss, it is noted that the plasma jet attenuates microwaves in a 6 to 8 GHz range
Additional details
Identifiers
- DOI
- 10.1063/1.2773704;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 14
- Journal Issue
- 9
- Journal Page Range
- p. 093508-093508.7
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39084098
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ARGON; DISTRIBUTION; ELECTRON DENSITY; ENERGY LOSSES; FLOW RATE; GHZ RANGE; LANGMUIR PROBE; MICROWAVE RADIATION; PLASMA; PLASMA DENSITY; PLASMA DIAGNOSTICS; PLASMA JETS
- Descriptors DEC
- ELECTRIC PROBES; ELECTROMAGNETIC RADIATION; ELEMENTS; FLUIDS; FREQUENCY RANGE; GASES; LOSSES; NONMETALS; PROBES; RADIATIONS; RARE GASES
Optional Information
- Notes
- (c) 2007 American Institute of Physics