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• W2897060489 abstract "In the light of recent CRISP/SST observations we aim to study transverse oscillations of a finely structured flux tube. With the use of PLUTO code, we numerically solve ideal magnetohydrodynamic equations in three-dimensional Cartesian geometry. With a pressure signal we generate a finely structured magnetic flux tube that consists of a central strand and four off-central strands. This flux tube is perturbed by a periodic driver in the azimuthal component of velocity. This driver results in transverse oscillations that propagate upward along these strands. The central strand experiences torsional Alfvén waves, while the off-central strands exhibit fast magnetoacoustic kink oscillations. The latter are guided by the off-central strands, which are regions of depression in Alfvén speed." @default.
• W2897060489 created "2018-10-26" @default.
• W2897060489 creator A5003000013 @default.
• W2897060489 creator A5030950569 @default.
• W2897060489 date "2018-10-10" @default.
• W2897060489 modified "2023-10-18" @default.
• W2897060489 title "Numerical Simulations of Transverse Oscillations of a Finely Structured Solar Flux Tube" @default.
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• W2897060489 doi "https://doi.org/10.3847/1538-4357/aadd00" @default.
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