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Kelvin-Helmholtz instability in a compressible dust fluid flow
We report the first experimental observations of a single-mode Kelvin-Helmholtz instability in a flowing dusty plasma in which the flow is compressible in nature. The experiments are performed in an inverted [Formula: see text] -shaped dusty plasma experimental device in a DC glow discharge Argon pl...
Autores principales: | , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2023
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9998883/ https://www.ncbi.nlm.nih.gov/pubmed/36894592 http://dx.doi.org/10.1038/s41598-023-30992-3 |
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author | Kumar, Krishan Bandyopadhyay, P. Singh, Swarnima Dharodi, Vikram S. Sen, A. |
author_facet | Kumar, Krishan Bandyopadhyay, P. Singh, Swarnima Dharodi, Vikram S. Sen, A. |
author_sort | Kumar, Krishan |
collection | PubMed |
description | We report the first experimental observations of a single-mode Kelvin-Helmholtz instability in a flowing dusty plasma in which the flow is compressible in nature. The experiments are performed in an inverted [Formula: see text] -shaped dusty plasma experimental device in a DC glow discharge Argon plasma environment. A gas pulse valve is installed in the experimental chamber to initiate directional motion to a particular dust layer. The shear generated at the interface of the moving and stationary layers leads to the excitation of the Kelvin-Helmholtz instability giving rise to a vortex structure at the interface. The growth rate of the instability is seen to decrease with an increase in the gas flow velocity in the valve and the concomitant increase in the compressibility of the dust flow. The shear velocity is further increased by making the stationary layer to flow in an opposite direction. The magnitude of the vorticity is seen to become stronger while the vortex becomes smaller with such an increase of the shear velocity. A molecular dynamics simulation provides good theoretical support to the experimental findings. |
format | Online Article Text |
id | pubmed-9998883 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2023 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-99988832023-03-11 Kelvin-Helmholtz instability in a compressible dust fluid flow Kumar, Krishan Bandyopadhyay, P. Singh, Swarnima Dharodi, Vikram S. Sen, A. Sci Rep Article We report the first experimental observations of a single-mode Kelvin-Helmholtz instability in a flowing dusty plasma in which the flow is compressible in nature. The experiments are performed in an inverted [Formula: see text] -shaped dusty plasma experimental device in a DC glow discharge Argon plasma environment. A gas pulse valve is installed in the experimental chamber to initiate directional motion to a particular dust layer. The shear generated at the interface of the moving and stationary layers leads to the excitation of the Kelvin-Helmholtz instability giving rise to a vortex structure at the interface. The growth rate of the instability is seen to decrease with an increase in the gas flow velocity in the valve and the concomitant increase in the compressibility of the dust flow. The shear velocity is further increased by making the stationary layer to flow in an opposite direction. The magnitude of the vorticity is seen to become stronger while the vortex becomes smaller with such an increase of the shear velocity. A molecular dynamics simulation provides good theoretical support to the experimental findings. Nature Publishing Group UK 2023-03-09 /pmc/articles/PMC9998883/ /pubmed/36894592 http://dx.doi.org/10.1038/s41598-023-30992-3 Text en © The Author(s) 2023 https://creativecommons.org/licenses/by/4.0/Open AccessThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Article Kumar, Krishan Bandyopadhyay, P. Singh, Swarnima Dharodi, Vikram S. Sen, A. Kelvin-Helmholtz instability in a compressible dust fluid flow |
title | Kelvin-Helmholtz instability in a compressible dust fluid flow |
title_full | Kelvin-Helmholtz instability in a compressible dust fluid flow |
title_fullStr | Kelvin-Helmholtz instability in a compressible dust fluid flow |
title_full_unstemmed | Kelvin-Helmholtz instability in a compressible dust fluid flow |
title_short | Kelvin-Helmholtz instability in a compressible dust fluid flow |
title_sort | kelvin-helmholtz instability in a compressible dust fluid flow |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9998883/ https://www.ncbi.nlm.nih.gov/pubmed/36894592 http://dx.doi.org/10.1038/s41598-023-30992-3 |
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