Shelyag, Sergiy, Cally, Paul S., Reid, Aaron and Mathioudakis, Mihalis (2013) Alfven waves in simulations of solar photospheric vortices. The Astrophysical Journal Letters, 776 (1). L4. ISSN 2041-8205
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Abstract
Using advanced numerical magneto-hydrodynamic simulations of the magnetized solar photosphere, including non-gray radiative transport and a non-ideal equation of state, we analyze plasma motions in photospheric magnetic vortices. We demonstrate that apparent vortex-like motions in photospheric magnetic field concentrations do not exhibit "tornado"-like behavior or a "bath-tub" effect. While at each time instance the velocity field lines in the upper layers of the solar photosphere show swirls, the test particles moving with the time-dependent velocity field do not demonstrate such structures. Instead, they move in a wave-like fashion with rapidly changing and oscillating velocity field, determined mainly by magnetic tension in the magnetized intergranular downflows. Using time-distance diagrams, we identify horizontal motions in the magnetic flux tubes as torsional Alfvén perturbations propagating along the nearly vertical magnetic field lines with local Alfvén speed.
Item Type: | Article |
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Subjects: | F300 Physics F500 Astronomy G100 Mathematics |
Department: | Faculties > Engineering and Environment > Mathematics, Physics and Electrical Engineering |
Depositing User: | Sergiy Shelyag |
Date Deposited: | 23 May 2016 09:28 |
Last Modified: | 01 Aug 2021 10:35 |
URI: | http://nrl.northumbria.ac.uk/id/eprint/26895 |
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