The potential of solar high-degree modes for structure inversion

Details The potential of solar high-degree modes for structure inversion The potential of solar high-degree modes for structure inversion

Apr 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..193..345r&link_type=abstract

Solar Physics, v. 193, Issue 1/2, p. 345-356 (2000).

Physics

15

Scientific paper

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 Γ_1 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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