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Simulation of a transient supersonic jet

Simulation of a transient supersonic jet
Simulation of a transient supersonic jet

This study investigates the evolution of under-expanded jets into a quiescent atmosphere using two-dimensional numerical simulation. The test case consists of two chambers separated by a wall with a small orifice. Initial pressure ratios between the two chambers were varied between 88 and 700, and the jet gas type was high pressure air exhausting into a low pressure, quiescent air chamber. During the initial transient, a Mach shock forms by rapid lateral expansion of the gas near the corner of the orifice and is initially absent at the jet centreline. As the flow evolves, the Mach shock becomes fully formed and vortex rings develop by Kelvin-Helmholtz and baroclinic instabilities at the interface of the barrel shocks and the quiescent air. After further flow evolution, the inner structure of the jet, enclosed by a barrel shock and Mach shock, resembles the structure of a steady under-expanded jet.

Australasian Fluid Mechanics Society
Miller, W. A.
ec9c7496-d8a0-4e64-a4c9-71158d323f11
Doolan, C. J.
18643e47-b21b-4e8f-881a-7fe818653042
Prime, Z. D.
e943259e-72ee-45ac-a8b8-f8f8b7ff591d
Kim, M.
18ed9a6f-484f-4a7c-bf24-b630938c1acc
Miller, W. A.
ec9c7496-d8a0-4e64-a4c9-71158d323f11
Doolan, C. J.
18643e47-b21b-4e8f-881a-7fe818653042
Prime, Z. D.
e943259e-72ee-45ac-a8b8-f8f8b7ff591d
Kim, M.
18ed9a6f-484f-4a7c-bf24-b630938c1acc

Miller, W. A., Doolan, C. J., Prime, Z. D. and Kim, M. (2014) Simulation of a transient supersonic jet. In Proceedings of the 19th Australasian Fluid Mechanics Conference, AFMC 2014. Australasian Fluid Mechanics Society..

Record type: Conference or Workshop Item (Paper)

Abstract

This study investigates the evolution of under-expanded jets into a quiescent atmosphere using two-dimensional numerical simulation. The test case consists of two chambers separated by a wall with a small orifice. Initial pressure ratios between the two chambers were varied between 88 and 700, and the jet gas type was high pressure air exhausting into a low pressure, quiescent air chamber. During the initial transient, a Mach shock forms by rapid lateral expansion of the gas near the corner of the orifice and is initially absent at the jet centreline. As the flow evolves, the Mach shock becomes fully formed and vortex rings develop by Kelvin-Helmholtz and baroclinic instabilities at the interface of the barrel shocks and the quiescent air. After further flow evolution, the inner structure of the jet, enclosed by a barrel shock and Mach shock, resembles the structure of a steady under-expanded jet.

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More information

Published date: 2014
Venue - Dates: 19th Australasian Fluid Mechanics Conference, AFMC 2014, , Melbourne, Australia, 2014-12-08 - 2014-12-11

Identifiers

Local EPrints ID: 498706
URI: http://eprints.soton.ac.uk/id/eprint/498706
PURE UUID: 6178ebf0-ee61-4f6c-b396-0726fd38c294
ORCID for M. Kim: ORCID iD orcid.org/0000-0002-6192-312X

Catalogue record

Date deposited: 25 Feb 2025 18:03
Last modified: 26 Feb 2025 02:47

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Contributors

Author: W. A. Miller
Author: C. J. Doolan
Author: Z. D. Prime
Author: M. Kim ORCID iD

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