Helioseismology of sunspots: How sensitive are travel times to the Wilson depression and to the subsurface magnetic field?

H. Schunker, Laurent Gizon, R. H. Cameron, A. C. Birch

Research output: Contribution to journalArticle

Abstract

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.

Original languageEnglish (US)
Article numberA130
JournalAstronomy and Astrophysics
Volume558
DOIs
StatePublished - Oct 31 2013

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helioseismology
sunspots
sunspot
travel time
travel
magnetic field
magnetic fields
wave packets
wave propagation
waveforms
sun
probe
perturbation
geometry
propagation
probes
shift
modeling
effect

Keywords

  • Sun: helioseismology
  • Sunspots

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Helioseismology of sunspots : How sensitive are travel times to the Wilson depression and to the subsurface magnetic field? / Schunker, H.; Gizon, Laurent; Cameron, R. H.; Birch, A. C.

In: Astronomy and Astrophysics, Vol. 558, A130, 31.10.2013.

Research output: Contribution to journalArticle

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