Original title: Numerical simulations of dynamic processes in the solar corona
Authors: BELOV, Sofya
Document type: Master’s theses
Year: 2022
Language: eng
Abstract: This master's thesis deals with 3D numerical simulations of turbulent flow past magnetic structures in the solar corona, focusing on the phenomenon of vortex shedding. This phenomenon is well known in hydrodynamic conditions. Still, it has not yet been satisfactorily investigated in magnetohydrodynamic (MHD) conditions, such as in the solar atmosphere, where its occurrence has been suggested by several studies and may explain some oscillatory phenomena. Numerical code Lare3d is used for the simulations.
Keywords: coronal loops; coronal mass ejections; kink oscillations; Lare3d; magnetohydrodynamics; numerical simulations; solar corona; solar prominences; vortex shedding
Citation: BELOV, Sofya. Numerical simulations of dynamic processes in the solar corona. České Budějovice, 2022. diplomová práce (Mgr.). JIHOČESKÁ UNIVERZITA V ČESKÝCH BUDĚJOVICÍCH. Přírodovědecká fakulta

Institution: University of South Bohemia in České Budějovice (web)
Document availability information: Fulltext is available in the Digital Repository of University of South Bohemia.
Original record: http://www.jcu.cz/vskp/63053

Permalink: http://www.nusl.cz/ntk/nusl-517545


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Universities and colleges > Public universities > University of South Bohemia in České Budějovice
Academic theses (ETDs) > Master’s theses