Volume 558, October 2013
|Number of page(s)||5|
|Published online||16 October 2013|
Helioseismology of sunspots: how sensitive are travel times to the Wilson depression and to the subsurface magnetic field?
Max-Planck-Institut für Sonnensystemforschung,
2 Institut für Astrophysik, Georg-August-Universität Göttingen, 37077 Göttingen, Germany
Accepted: 21 June 2013
To assess the ability of helioseismology to probe the subsurface structure and magnetic field of sunspots, we need to determine how helioseismic travel times depend on perturbations to sunspot models. Here we numerically simulate the propagation of f, p1, and p2 wave packets through magnetic sunspot models. Among the models we considered, a ±50 km change in the height of the Wilson depression and a change in the subsurface magnetic field geometry can both be detected above the observational noise level. We also find that the travel-time shifts due to changes in a sunspot model must be modeled by computing the effects of changing the reference sunspot model, and not by computing the effects of changing the subsurface structure in the quiet-Sun model. For p1 modes, the latter is wrong by a factor of four. In conclusion, numerical modeling of MHD wave propagation is an essential tool for interpreting the effects of sunspots on seismic waveforms.
Key words: Sun: helioseismology / sunspots
© ESO, 2013
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