Non linear inversion for the sound speed in the solar interior using BiSON and SOI/MDI p-mode frequencies

Details Non linear inversion for the sound speed in the solar interior using BiSON and SOI/MDI p-mode frequencies Non linear inversion for the sound speed in the solar interior using BiSON and SOI/MDI p-mode frequencies

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.464..531m&link_type=abstract

In: Proceedings of the SOHO 10/GONG 2000 Workshop: Helio- and asteroseismology at the dawn of the millennium, 2-6 October 2000,

Computer Science

Sound

Sun: Interior, Sun: Oscillations

Scientific paper

The results of the global sound-speed inversion obtained with solar p-mode frequencies provided by the recent high-quality observational data (BiSON, SOI/MDI) are presented and discussed. The iterative nonlinear inversion technique used here is a generalization (for the case of exact solution of the adiabatic oscillation equations) of the Born quasiasymptotic approximate inversion developed by Marchenkov et al. (2000).

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