Výsledky vyhledávání - "Ogbonna, J. E."

The magnetized spherical couette system: From numerics to experiments

Autor: Garcia Gonzalez, F., Ogbonna, J. E., Gundrum, T., Seilmayer, M., Giesecke, A., Stefani, F.

Publikováno v: The Fourth Russian Conference on Magnetohydrodynamics, RMHD-2021, 20.-22.09.2021, Perm, Russia

The study of magnetohydrodynamic (MHD) instabilities occurring in liquid metals, with imposed differential rotation and magnetic field, is of fundamental importance in the astrophysical context. MHD instabilities are especially relevant in planets or

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______4577::411d9e1119f052413133dde5701e5124
https://www.hzdr.de/publications/Publ-34046-1

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Data for: Experimental investigation of the return flow instability in magnetic spherical Couette flow

Autor: Ogbonna, J. E., Garcia Gonzalez, F., Gundrum, T., Seilmayer, M., Stefani, F.

Publikováno v: Publication date: 2020-09-16 Open accessDOI: 10.14278/rodare.789Versions: 10.14278/rodare.790License: CC-BY-4.0

Experimental data, numerical data, and programming scripts

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______4577::3aff88fc77cd5bcc98bbb606d0af97ff
https://www.hzdr.de/publications/Publ-32239-1

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Convection Caused Symmetry Breaking of Azimuthal Magnetorotational Instability in a Liquid Metal Taylor Couette Flow

Autor: Seilmayer, M., Ogbonna, J. E., Stefani, F.

Publikováno v: Publication date: 2020-06-25 Open accessDOI: 10.14278/rodare.380Versions: 10.14278/rodare.381License: CC-BY-4.0

This are the experimental and numerical results for the publication "Convection Caused Symmetry Breaking of Azimuthal Magnetorotational Instability in a Liquid Metal Taylor Couette Flow ". It contains pictures, experimental results, tex files, COMSOL

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______4577::30fafbaa3ed08e8d9419cbd9cf0aac6e
https://www.hzdr.de/publications/Publ-31238-1

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Experimental investigation of magnetorotational instability in hydromagnetic Taylor-Couette flows

Autor: Ogbonna, J. E., Seilmayer, M., Stefani, F.

Publikováno v: 9th European Postgraduate Fluid Dynamics Conference, 16.-19.07.2019, Ilmenau, Deutschland

Magnetorotational instability (MRI) is believed to be largely responsible for the formation of protostars and black holes by introducing turbulence and facilitating an outward angular momentum transport in accretion disks. MRI is replicable in Taylor

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______4577::72d2919a9b1eb8e20aaddd6316ac6c4d
https://www.hzdr.de/publications/Publ-29181-1

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