Stokes Diagnostics of Magneto-Acoustic Wave Propagation in the Magnetic Network on the Sun |
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| Authors: | G Vigeesh O Steiner S S Hasan |
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| Institution: | 1.Block II Koramangala,Indian Institute of Astrophysics,Bangalore,India;2.Kiepenheuer-Institut für Sonnenphysik,Freiburg,Germany |
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| Abstract: | The solar atmosphere is magnetically structured and highly dynamic. Owing to the dynamic nature of the regions in which the
magnetic structures exist, waves can be excited in them. Numerical investigations of wave propagation in small-scale magnetic
flux concentrations in the magnetic network on the Sun have shown that the nature of the excited modes depends on the value
of plasma β (the ratio of gas to magnetic pressure) where the driving motion occurs. Considering that these waves should give rise to
observable characteristic signatures, we have attempted a study of synthesised emergent spectra from numerical simulations
of magneto-acoustic wave propagation. We find that the signatures of wave propagation in a magnetic element can be detected
when the spatial resolution is sufficiently high to clearly resolve it, enabling observations in different regions within
the flux concentration. The possibility to probe various lines of sight around the flux concentration bears the potential
to reveal different modes of the magnetohydrodynamic waves and mode conversion. We highlight the feasibility of using the
Stokes-V asymmetries as a diagnostic tool to study the wave propagation within magnetic flux concentrations. These quantities can
possibly be compared with existing and new observations in order to place constraints on different wave excitation mechanisms. |
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