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Experimental pub crawl from Rayleigh–Bénard to magnetostrophic convection
The interplay between convective, rotational and magnetic forces defines the dynamics within the electrically conducting regions of planets and stars. Yet their triadic effects are separated from one another in most studies, arguably due to the richness of each subset. In a single laboratory experim...
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Published in: | Journal of fluid mechanics 2022-05, Vol.939, Article R1 |
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creator | Grannan, Alexander M. Cheng, Jonathan S. Aggarwal, Ashna Hawkins, Emily K. Xu, Yufan Horn, Susanne Sánchez-Álvarez, Jose Aurnou, Jonathan M. |
description | The interplay between convective, rotational and magnetic forces defines the dynamics within the electrically conducting regions of planets and stars. Yet their triadic effects are separated from one another in most studies, arguably due to the richness of each subset. In a single laboratory experiment, we apply a fixed heat flux, two different magnetic field strengths and one rotation rate, allowing us to chart a continuous path through Rayleigh–Bénard convection (RBC), two regimes of magnetoconvection, rotating convection and two regimes of rotating magnetoconvection, before finishing back at RBC. Dynamically rapid transitions are determined to exist between jump rope vortex states, thermoelectrically driven magnetoprecessional modes, mixed wall- and oscillatory-mode rotating convection and a novel magnetostrophic wall mode. Thus, our laboratory ‘pub crawl’ provides a coherent intercomparison of the broadly varying responses arising as a function of the magnetorotational forces imposed on a liquid-metal convection system. |
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(ANL), Argonne, IL (United States)</creatorcontrib><description>The interplay between convective, rotational and magnetic forces defines the dynamics within the electrically conducting regions of planets and stars. Yet their triadic effects are separated from one another in most studies, arguably due to the richness of each subset. In a single laboratory experiment, we apply a fixed heat flux, two different magnetic field strengths and one rotation rate, allowing us to chart a continuous path through Rayleigh–Bénard convection (RBC), two regimes of magnetoconvection, rotating convection and two regimes of rotating magnetoconvection, before finishing back at RBC. Dynamically rapid transitions are determined to exist between jump rope vortex states, thermoelectrically driven magnetoprecessional modes, mixed wall- and oscillatory-mode rotating convection and a novel magnetostrophic wall mode. Thus, our laboratory ‘pub crawl’ provides a coherent intercomparison of the broadly varying responses arising as a function of the magnetorotational forces imposed on a liquid-metal convection system.</description><identifier>ISSN: 0022-1120</identifier><identifier>EISSN: 1469-7645</identifier><identifier>DOI: 10.1017/jfm.2022.204</identifier><language>eng</language><publisher>Cambridge, UK: Cambridge University Press</publisher><subject>Bénard convection ; Convection ; Convection modes ; ENGINEERING ; Estimates ; Experiments ; Fluid mechanics ; Forces ; Heat ; Heat flux ; Heat transfer ; Intercomparison ; JFM Rapids ; Liquid metals ; Magnetic field ; Magnetic fields ; Magnetic flux ; magneto convection ; Metals ; Rayleigh number ; Rayleigh-Benard convection ; Reynolds number ; rotating flows ; Rotation ; Sensors</subject><ispartof>Journal of fluid mechanics, 2022-05, Vol.939, Article R1</ispartof><rights>The Author(s), 2022. Published by Cambridge University Press</rights><rights>The Author(s), 2022. Published by Cambridge University Press. This work is licensed under the Creative Commons Attribution – Non-Commercial – Share Alike License https://creativecommons.org/licenses/by-nc-sa/4.0/ (the “License”). 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(ANL), Argonne, IL (United States)</creatorcontrib><title>Experimental pub crawl from Rayleigh–Bénard to magnetostrophic convection</title><title>Journal of fluid mechanics</title><addtitle>J. Fluid Mech</addtitle><description>The interplay between convective, rotational and magnetic forces defines the dynamics within the electrically conducting regions of planets and stars. Yet their triadic effects are separated from one another in most studies, arguably due to the richness of each subset. In a single laboratory experiment, we apply a fixed heat flux, two different magnetic field strengths and one rotation rate, allowing us to chart a continuous path through Rayleigh–Bénard convection (RBC), two regimes of magnetoconvection, rotating convection and two regimes of rotating magnetoconvection, before finishing back at RBC. Dynamically rapid transitions are determined to exist between jump rope vortex states, thermoelectrically driven magnetoprecessional modes, mixed wall- and oscillatory-mode rotating convection and a novel magnetostrophic wall mode. Thus, our laboratory ‘pub crawl’ provides a coherent intercomparison of the broadly varying responses arising as a function of the magnetorotational forces imposed on a liquid-metal convection system.</description><subject>Bénard convection</subject><subject>Convection</subject><subject>Convection modes</subject><subject>ENGINEERING</subject><subject>Estimates</subject><subject>Experiments</subject><subject>Fluid mechanics</subject><subject>Forces</subject><subject>Heat</subject><subject>Heat flux</subject><subject>Heat transfer</subject><subject>Intercomparison</subject><subject>JFM Rapids</subject><subject>Liquid metals</subject><subject>Magnetic field</subject><subject>Magnetic fields</subject><subject>Magnetic flux</subject><subject>magneto convection</subject><subject>Metals</subject><subject>Rayleigh number</subject><subject>Rayleigh-Benard convection</subject><subject>Reynolds number</subject><subject>rotating flows</subject><subject>Rotation</subject><subject>Sensors</subject><issn>0022-1120</issn><issn>1469-7645</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNptkMtKAzEUhoMoWKs7H2DQrVNzm2Sy1FIvUBBE1yGTJu2UmcmYpGp3voNP4XP4Jj6JKS24cXMOHL7z8_MBcIrgCEHEL5e2HWGIcRp0DwwQZSLnjBb7YADTOUcIw0NwFMISQkSg4AMwnbz3xtet6aJqsn5VZdqrtyaz3rXZo1o3pp4vfj4-r7-_OuVnWXRZq-adiS5E7_pFrTPtulejY-26Y3BgVRPMyW4PwfPN5Gl8l08fbu_HV9NcE8ZjbnSpVUEEwYpow5gl2BbCVERoDWeCVUJAyhAhlleKcqFgwcpSEytQwalmZAjOtrmpRC2DrqPRi1SjSzUkEpgSUibofAv13r2sTIhy6Va-S70kZhSVSMBCJOpiS2nvQvDGyj7ZUH4tEZQbqTJJlRupadCEj3a4aitfz-bmL_Xfh19wgnpp</recordid><startdate>20220525</startdate><enddate>20220525</enddate><creator>Grannan, Alexander M.</creator><creator>Cheng, Jonathan S.</creator><creator>Aggarwal, Ashna</creator><creator>Hawkins, Emily K.</creator><creator>Xu, Yufan</creator><creator>Horn, Susanne</creator><creator>Sánchez-Álvarez, Jose</creator><creator>Aurnou, Jonathan M.</creator><general>Cambridge University Press</general><scope>IKXGN</scope><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>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><scope>OIOZB</scope><scope>OTOTI</scope><orcidid>https://orcid.org/0000-0002-8642-2962</orcidid><orcidid>https://orcid.org/0000-0002-2326-9614</orcidid><orcidid>https://orcid.org/0000-0001-9123-124X</orcidid><orcidid>https://orcid.org/0000-0002-6145-1927</orcidid><orcidid>https://orcid.org/0000-0001-8471-3777</orcidid><orcidid>https://orcid.org/0000-0002-7945-3250</orcidid><orcidid>https://orcid.org/0000-0002-7737-3265</orcidid><orcidid>https://orcid.org/0000-0001-5961-454X</orcidid><orcidid>https://orcid.org/000000019123124X</orcidid><orcidid>https://orcid.org/0000000184713777</orcidid><orcidid>https://orcid.org/000000015961454X</orcidid><orcidid>https://orcid.org/0000000279453250</orcidid><orcidid>https://orcid.org/0000000286422962</orcidid><orcidid>https://orcid.org/0000000223269614</orcidid><orcidid>https://orcid.org/0000000277373265</orcidid><orcidid>https://orcid.org/0000000261451927</orcidid></search><sort><creationdate>20220525</creationdate><title>Experimental pub crawl from Rayleigh–Bénard to magnetostrophic convection</title><author>Grannan, Alexander M. ; 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(ANL), Argonne, IL (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Experimental pub crawl from Rayleigh–Bénard to magnetostrophic convection</atitle><jtitle>Journal of fluid mechanics</jtitle><addtitle>J. Fluid Mech</addtitle><date>2022-05-25</date><risdate>2022</risdate><volume>939</volume><artnum>R1</artnum><issn>0022-1120</issn><eissn>1469-7645</eissn><abstract>The interplay between convective, rotational and magnetic forces defines the dynamics within the electrically conducting regions of planets and stars. Yet their triadic effects are separated from one another in most studies, arguably due to the richness of each subset. 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subjects | Bénard convection Convection Convection modes ENGINEERING Estimates Experiments Fluid mechanics Forces Heat Heat flux Heat transfer Intercomparison JFM Rapids Liquid metals Magnetic field Magnetic fields Magnetic flux magneto convection Metals Rayleigh number Rayleigh-Benard convection Reynolds number rotating flows Rotation Sensors |
title | Experimental pub crawl from Rayleigh–Bénard to magnetostrophic convection |
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