Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008apj...681..664g&link_type=abstract
The Astrophysical Journal, Volume 681, Issue 1, pp. 664-671.
Astronomy and Astrophysics
Astronomy
7
Sun: Helioseismology, Sun: Magnetic Fields, Sun: Sunspots
Scientific paper
The interaction of p-modes (acoustic waves) with a magnetic flux tube is investigated. A set of linearized MHD equations is solved numerically in a two-dimensional domain with cylindrical geometry. The wave functions for p-modes are calculated in and around magnetic flux tubes using eigenfunctions from the unperturbed solution as a boundary condition. The amplitudes of the oscillations are found to be suppressed in the magnetized region with the suppression decreasing with depth. It is also found that the absorption of p-modes strongly depends on the degree l as well as the flux tube radius and the magnetic field strength. Convergence of magnetic field may be necessary in order to fit simultaneously the observed phase shifts and absorption coefficients.
Gordovskyy Mykola
Jain Rekha
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