Published September 2007 | Version v1
Journal article

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

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