Non-ideal instabilities in sinusoidal shear flows with a streamwise magnetic field
We investigate the linear stability of a sinusoidal shear flow with an initially uniform streamwise magnetic field in the framework of incompressible magnetohydrodynamics (MHD) with finite resistivity and viscosity. This flow is known to be unstable to the Kelvin–Helmholtz instability in the hydrody...
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description | We investigate the linear stability of a sinusoidal shear flow with an initially uniform streamwise magnetic field in the framework of incompressible magnetohydrodynamics (MHD) with finite resistivity and viscosity. This flow is known to be unstable to the Kelvin–Helmholtz instability in the hydrodynamic case. The same is true in ideal MHD, where dissipation is neglected, provided the magnetic field strength does not exceed a critical threshold beyond which magnetic tension stabilizes the flow. Here, we demonstrate that including viscosity and resistivity introduces two new modes of instability. One of these modes, which we refer to as an Alfvénic Dubrulle–Frisch instability, exists for any non-zero magnetic field strength as long as the magnetic Prandtl number ${{{Pm}}} < 1$. We present a reduced model for this instability that reveals its excitation mechanism to be the negative eddy viscosity of periodic shear flows described by Dubrulle & Frisch (Phys. Rev. A, vol. 43, 1991, pp. 5355–5364). Finally, we demonstrate numerically that this mode saturates in a quasi-stationary state dominated by counter-propagating solitons. |
doi_str_mv | 10.1017/jfm.2022.782 |
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This flow is known to be unstable to the Kelvin–Helmholtz instability in the hydrodynamic case. The same is true in ideal MHD, where dissipation is neglected, provided the magnetic field strength does not exceed a critical threshold beyond which magnetic tension stabilizes the flow. Here, we demonstrate that including viscosity and resistivity introduces two new modes of instability. One of these modes, which we refer to as an Alfvénic Dubrulle–Frisch instability, exists for any non-zero magnetic field strength as long as the magnetic Prandtl number ${{{Pm}}} < 1$. We present a reduced model for this instability that reveals its excitation mechanism to be the negative eddy viscosity of periodic shear flows described by Dubrulle & Frisch (Phys. Rev. A, vol. 43, 1991, pp. 5355–5364). Finally, we demonstrate numerically that this mode saturates in a quasi-stationary state dominated by counter-propagating solitons.</description><identifier>ISSN: 0022-1120</identifier><identifier>EISSN: 1469-7645</identifier><identifier>DOI: 10.1017/jfm.2022.782</identifier><language>eng</language><publisher>Cambridge, UK: Cambridge University Press</publisher><subject>Approximation ; Eddy viscosity ; Electrical resistivity ; Field strength ; Flow stability ; Fluid flow ; Incompressible flow ; Instability ; JFM Papers ; Kelvin-helmholtz instability ; Magnetic field ; Magnetic fields ; Magnetohydrodynamics ; Prandtl number ; Shear flow ; Sine waves ; Solitary waves ; Solitons ; Viscosity</subject><ispartof>Journal of fluid mechanics, 2022-10, Vol.949, Article A43</ispartof><rights>The Author(s), 2022. 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Fluid Mech</addtitle><description>We investigate the linear stability of a sinusoidal shear flow with an initially uniform streamwise magnetic field in the framework of incompressible magnetohydrodynamics (MHD) with finite resistivity and viscosity. This flow is known to be unstable to the Kelvin–Helmholtz instability in the hydrodynamic case. The same is true in ideal MHD, where dissipation is neglected, provided the magnetic field strength does not exceed a critical threshold beyond which magnetic tension stabilizes the flow. Here, we demonstrate that including viscosity and resistivity introduces two new modes of instability. One of these modes, which we refer to as an Alfvénic Dubrulle–Frisch instability, exists for any non-zero magnetic field strength as long as the magnetic Prandtl number ${{{Pm}}} < 1$. We present a reduced model for this instability that reveals its excitation mechanism to be the negative eddy viscosity of periodic shear flows described by Dubrulle & Frisch (Phys. Rev. A, vol. 43, 1991, pp. 5355–5364). Finally, we demonstrate numerically that this mode saturates in a quasi-stationary state dominated by counter-propagating solitons.</description><subject>Approximation</subject><subject>Eddy viscosity</subject><subject>Electrical resistivity</subject><subject>Field strength</subject><subject>Flow stability</subject><subject>Fluid flow</subject><subject>Incompressible flow</subject><subject>Instability</subject><subject>JFM Papers</subject><subject>Kelvin-helmholtz instability</subject><subject>Magnetic field</subject><subject>Magnetic fields</subject><subject>Magnetohydrodynamics</subject><subject>Prandtl number</subject><subject>Shear flow</subject><subject>Sine waves</subject><subject>Solitary waves</subject><subject>Solitons</subject><subject>Viscosity</subject><issn>0022-1120</issn><issn>1469-7645</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>8G5</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><sourceid>GUQSH</sourceid><sourceid>M2O</sourceid><recordid>eNptkEtLAzEQx4MoWKs3P0DAq7tmkt3N7lGKLygKoueQ3UzalH3UJKX47Y204MXTMDP_B_wIuQaWAwN5t7FDzhnnuaz5CZlBUTWZrIrylMxYOmcAnJ2TixA2jIFgjZyR99dpzJxB3VM3hqhb17voMKSNBjfuwuRM-oU1ak9tP-0D3bu4ppqG6FEPexeQDno1YnQdtQ57c0nOrO4DXh3nnHw-PnwsnrPl29PL4n6ZdYLxmEFdtLYoC8Zqa1DYkldtAaZDkC2vgUnRtA10opaNaLRA1tXcMgPa1NoCVmJObg65Wz997TBEtZl2fkyViksOpWhkss7J7UHV-SkEj1ZtvRu0_1bA1C81laipX2oqUUvy_CjXQ-udWeFf6r-GH1J5byQ</recordid><startdate>20221025</startdate><enddate>20221025</enddate><creator>Fraser, A.E.</creator><creator>Cresswell, I.G.</creator><creator>Garaud, P.</creator><general>Cambridge University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TB</scope><scope>7U5</scope><scope>7UA</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>8G5</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F1W</scope><scope>FR3</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H8D</scope><scope>H96</scope><scope>HCIFZ</scope><scope>KR7</scope><scope>L.G</scope><scope>L6V</scope><scope>L7M</scope><scope>M2O</scope><scope>M2P</scope><scope>M7S</scope><scope>MBDVC</scope><scope>P5Z</scope><scope>P62</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PTHSS</scope><scope>Q9U</scope><scope>S0W</scope><orcidid>https://orcid.org/0000-0002-6266-8941</orcidid><orcidid>https://orcid.org/0000-0003-4323-2082</orcidid><orcidid>https://orcid.org/0000-0002-4538-7320</orcidid></search><sort><creationdate>20221025</creationdate><title>Non-ideal instabilities in sinusoidal shear flows with a streamwise magnetic field</title><author>Fraser, A.E. ; 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Fluid Mech</addtitle><date>2022-10-25</date><risdate>2022</risdate><volume>949</volume><artnum>A43</artnum><issn>0022-1120</issn><eissn>1469-7645</eissn><abstract>We investigate the linear stability of a sinusoidal shear flow with an initially uniform streamwise magnetic field in the framework of incompressible magnetohydrodynamics (MHD) with finite resistivity and viscosity. This flow is known to be unstable to the Kelvin–Helmholtz instability in the hydrodynamic case. The same is true in ideal MHD, where dissipation is neglected, provided the magnetic field strength does not exceed a critical threshold beyond which magnetic tension stabilizes the flow. Here, we demonstrate that including viscosity and resistivity introduces two new modes of instability. One of these modes, which we refer to as an Alfvénic Dubrulle–Frisch instability, exists for any non-zero magnetic field strength as long as the magnetic Prandtl number ${{{Pm}}} < 1$. We present a reduced model for this instability that reveals its excitation mechanism to be the negative eddy viscosity of periodic shear flows described by Dubrulle & Frisch (Phys. Rev. A, vol. 43, 1991, pp. 5355–5364). Finally, we demonstrate numerically that this mode saturates in a quasi-stationary state dominated by counter-propagating solitons.</abstract><cop>Cambridge, UK</cop><pub>Cambridge University Press</pub><doi>10.1017/jfm.2022.782</doi><tpages>26</tpages><orcidid>https://orcid.org/0000-0002-6266-8941</orcidid><orcidid>https://orcid.org/0000-0003-4323-2082</orcidid><orcidid>https://orcid.org/0000-0002-4538-7320</orcidid></addata></record> |
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subjects | Approximation Eddy viscosity Electrical resistivity Field strength Flow stability Fluid flow Incompressible flow Instability JFM Papers Kelvin-helmholtz instability Magnetic field Magnetic fields Magnetohydrodynamics Prandtl number Shear flow Sine waves Solitary waves Solitons Viscosity |
title | Non-ideal instabilities in sinusoidal shear flows with a streamwise magnetic field |
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