Steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere
The noncollisional interaction between conducting obstacles and magnetized plasma winds can be found in different scenarios, from the interaction occurring between regions inside galaxy clusters to the interaction between the solar wind and Mars, Venus, and active comets, or even the interaction bet...
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| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v789_n1_p_Romanelli |
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todo:paper_0004637X_v789_n1_p_Romanelli2023-10-03T14:02:34Z Steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere Romanelli, N. Gómez, D. Bertucci, C. Delva, M. conduction magnetohydrodynamics (MHD) plasmas The noncollisional interaction between conducting obstacles and magnetized plasma winds can be found in different scenarios, from the interaction occurring between regions inside galaxy clusters to the interaction between the solar wind and Mars, Venus, and active comets, or even the interaction between Titan and the Saturnian magnetospheric flow. These objects generate, through several current systems, perturbations in the streaming magnetic field leading to its draping around the obstacle's effective conducting surface. Recent observational results suggest that several properties associated with magnetic field draping, such as the location of the polarity reversal layer of the induced magnetotail, are affected by variations in the conditions of the streaming magnetic field. To improve our understanding of these phenomena, we perform a characterization of several magnetic field draping signatures by analytically solving an ideal problem in which a perfectly conducting magnetized plasma (with frozen-in magnetic field conditions) flows around a spherical body for various orientations of the streaming magnetic field. In particular, we compute the shift of the inverse polarity reversal layer as the orientation of the background magnetic field is changed. © 2014. The American Astronomical Society. All rights reserved. Fil:Romanelli, N. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Bertucci, C. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_0004637X_v789_n1_p_Romanelli |
| institution |
Universidad de Buenos Aires |
| institution_str |
I-28 |
| repository_str |
R-134 |
| collection |
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
| topic |
conduction magnetohydrodynamics (MHD) plasmas |
| spellingShingle |
conduction magnetohydrodynamics (MHD) plasmas Romanelli, N. Gómez, D. Bertucci, C. Delva, M. Steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere |
| topic_facet |
conduction magnetohydrodynamics (MHD) plasmas |
| description |
The noncollisional interaction between conducting obstacles and magnetized plasma winds can be found in different scenarios, from the interaction occurring between regions inside galaxy clusters to the interaction between the solar wind and Mars, Venus, and active comets, or even the interaction between Titan and the Saturnian magnetospheric flow. These objects generate, through several current systems, perturbations in the streaming magnetic field leading to its draping around the obstacle's effective conducting surface. Recent observational results suggest that several properties associated with magnetic field draping, such as the location of the polarity reversal layer of the induced magnetotail, are affected by variations in the conditions of the streaming magnetic field. To improve our understanding of these phenomena, we perform a characterization of several magnetic field draping signatures by analytically solving an ideal problem in which a perfectly conducting magnetized plasma (with frozen-in magnetic field conditions) flows around a spherical body for various orientations of the streaming magnetic field. In particular, we compute the shift of the inverse polarity reversal layer as the orientation of the background magnetic field is changed. © 2014. The American Astronomical Society. All rights reserved. |
| format |
JOUR |
| author |
Romanelli, N. Gómez, D. Bertucci, C. Delva, M. |
| author_facet |
Romanelli, N. Gómez, D. Bertucci, C. Delva, M. |
| author_sort |
Romanelli, N. |
| title |
Steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere |
| title_short |
Steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere |
| title_full |
Steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere |
| title_fullStr |
Steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere |
| title_full_unstemmed |
Steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere |
| title_sort |
steady-state magnetohydrodynamic flow around an unmagnetized conducting sphere |
| url |
http://hdl.handle.net/20.500.12110/paper_0004637X_v789_n1_p_Romanelli |
| work_keys_str_mv |
AT romanellin steadystatemagnetohydrodynamicflowaroundanunmagnetizedconductingsphere AT gomezd steadystatemagnetohydrodynamicflowaroundanunmagnetizedconductingsphere AT bertuccic steadystatemagnetohydrodynamicflowaroundanunmagnetizedconductingsphere AT delvam steadystatemagnetohydrodynamicflowaroundanunmagnetizedconductingsphere |
| _version_ |
1807318238126669824 |