Magnetoconvection.pdf

Magnetoconvection PDF

N. O. Weiss

Date de parution

Magnetoconvection refers to the thermal driving of flow within an electrically conducting fluid in the presence of an imposed magnetic field. In rapidly rotating systems like the Earth's fluid outer core, magnetoconvection offers a key insight into the intricate interaction between the effects of … Magnetoconvection | SpringerLink

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9780521190558 ISBN
Magnetoconvection.pdf

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Notes actuelles

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Sofya Voigtuh

Magnetoconvection I; Participants; Speakers; Timetable; Date: Thursday 9th September 2004 - 11:25 to 12:35. Venue: INI Seminar Room 1. Event: [MSIW01] Magnetohydrodynamics of Stellar Interiors. Abstract: In these lectures I give a description, starting from basic concepts, of the effects of magnetic fields on convection and of convection on the fields. The principal motivation for studying Magneto-convection | Request PDF

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Mattio Müllers

magnetoconvection dans les ferrofluides - Futura

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Noels Schulzen

Magnetoconvection. Authors; Authors and affiliations; T. Emonet; F. Cattaneo; N. O. Weiss; Chapter. 4 Citations; 192 Downloads; Part of the NATO Science Series book series (NAII, volume 26) Abstract. We present results from a systematic numerical survey of the interaction between turbulent convection and magnetic fields, as the net vertical magnetic flux through a large aspect ratio theses.fr – Nicolas Gillet , Magnéto-convection dans une ...

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Jason Leghmann

Magnetoconvection refers to the thermal driving of flow within an electrically conducting fluid in the presence of an imposed magnetic field. In rapidly rotating systems like the Earth's fluid outer core, magnetoconvection offers a key insight into the intricate interaction between the effects of …

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Jessica Kolhmann

Magnetoconvection - University of California, Berkeley Magnetoconvection in Stellar Interiors. I have recently become interested in several specific aspects of the theory of turbulent convection and magnetoconvection; namely, the process of magnetic flux transport in the solar convection zone, and the generation of magnetic fields via a local dynamo (a process independent of the presence or absence of an interface layer separating the