Progress in sunspot helioseismology

Details Progress in sunspot helioseismology Progress in sunspot helioseismology

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jphcs.271a2001b&link_type=abstract

Journal of Physics: Conference Series, Volume 271, Issue 1, pp. 012001 (2011).

Physics

1

Scientific paper

Local helioseismology is a set of methods that are used to study wave propagation and infer physical conditions in the solar interior. Sunspots are a particularly challenging target for local helioseismology. In this review, I will show that some new methods (magnetoconvection simulations and numerical wave propagation simulations) lead to shallow sunspot models that are apparently inconsistent with traditional inferences from local helioseismology. In addition, I will show that inferences for the depth structure of moat flows are not in general agreement either.

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