Abstract
It is likely that precise and reliable frequencies of high-degree modes will soon be available from the SOI/MDI experiment. Here we examine the ability of such modes (with l > 300) to resolve the solar structure in the near-surface region. In particular, we investigate inversions to determine the adiabatic exponent Γ1 as a test of the solar equation of state, as well as the potential of such data to constrain the solar envelope helium abundance.
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Rabello-Soares, M.C., Basu, S., Christensen-Dalsgaard, J., Di Mauro, M.P. (2000). The Potential of Solar High-Degree Modes for Structure Inversion. In: Duvall, T.L., Harvey, J.W., Kosovichev, A.G., Švestka, Z. (eds) Helioseismic Diagnostics of Solar Convection and Activity. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4377-6_38
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DOI: https://doi.org/10.1007/978-94-011-4377-6_38
Publisher Name: Springer, Dordrecht
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