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Three-dimensional Simulations of Magnetohydrodynamic Waves in Magnetized Solar Atmosphere

Vigeesh, G. and Fedun, V. and Hasan, S. S. and Erdélyi, Róbert (2012) Three-dimensional Simulations of Magnetohydrodynamic Waves in Magnetized Solar Atmosphere. The Astrophysical Journal, 755 (18). pp. 1-11. ISSN 0004-637X

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Abstract

We present results of three-dimensional numerical simulations of magnetohydrodynamic (MHD) wave propagation in a solar magnetic flux tube. Our study aims at understanding the properties of a range of MHD wave modes generated by different photospheric motions. We consider two scenarios observed in the lower solar photosphere, namely, granular buffeting and vortex-like motion, among the simplest mechanism for the generation of waves within a strong, localized magnetic flux concentration. We show that granular buffeting is likely to generate stronger slow and fast magnetoacoustic waves as compared to swirly motions. Correspondingly, the energy flux transported differs as a result of the driving motions. We also demonstrate that the waves generated by granular buffeting are likely to manifest in stronger emission in the chromospheric network. We argue that different mechanisms of wave generation are active during the evolution of a magnetic element in the intergranular lane, resulting in temporally varying emission at chromospheric heights.

Item Type: Article
Uncontrolled Keywords: WAVES; Sun: surface magnetism; Sun: atmosphere; magnetohydrodynamics: MHD; magnetic fields
Subjects: Q Science / természettudomány > QB Astronomy, Astrophysics / csillagászat, asztrofizika
SWORD Depositor: MTMT SWORD
Depositing User: MTMT SWORD
Date Deposited: 29 Sep 2017 07:04
Last Modified: 29 Sep 2017 07:04
URI: http://real.mtak.hu/id/eprint/64307

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