Published January 2005 | Version v1
Journal article

Examination of the shock wave regular reflexion phenomenon in a rarefied supersonic plasma flow

  • 1. University of Opole, Oleska 48, Opole (Poland)
  • 2. Laboratoire d'Aerothermique, 1C avenue de la Recherche Scientifique, 45071 Orleans (France)

Description

The flow properties of a low-pressure weakly ionized supersonic argon plasma jet are examined using Fabry-Perot interferometry and laser induced fluorescence spectroscopy. The flow velocity and equilibrium temperature measured at the torch nozzle exit are in close agreement with computational fluid dynamics calculations. The model also predicts the plasma flow to be in a rarefied regime. Departure from thermal equilibrium is indeed observed behind the nozzle where the parallel temperature differs significantly from the perpendicular temperature. The development of the axial velocity component along the jet center stream line reveals the occurrence of the shock wave regular reflexion phenomenon: No Mach disk is formed and the flow experiences successive supersonic-to-supersonic transitions before reaching a subsonic regime. Shock wave regular reflexion is in fact favored under our experimental conditions since the speed ratio is high and the rarefaction degree is pronounced at the nozzle exit

Additional details

Identifiers

Publishing Information

Journal Title
Physics of Plasmas
Journal Volume
12
Journal Issue
1
Journal Page Range
p. 012323-012323.9
ISSN
1070-664X
CODEN
PHPAEN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
36096743
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Descriptors DEI
ARGON; FABRY-PEROT INTERFEROMETER; FLUORESCENCE SPECTROSCOPY; NOZZLES; PLASMA; PLASMA DIAGNOSTICS; PLASMA JETS; SHOCK WAVES; SUPERSONIC FLOW
Descriptors DEC
ELEMENTS; EMISSION SPECTROSCOPY; FLUID FLOW; FLUIDS; GASES; INTERFEROMETERS; MEASURING INSTRUMENTS; NONMETALS; RARE GASES; SPECTROSCOPY

Optional Information

Notes
(c) 2005 American Institute of Physics