Helioseismic investigation of the solar envelope

Details Helioseismic investigation of the solar envelope Helioseismic investigation of the solar envelope

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..879d&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

Sun: Helioseismology, Sun: Oscillations, Sun: Interior

Scientific paper

It has already been demonstrated that the solar envelope can be probed with sufficiently high spatial resolution through inversion of high-degree acoustic modes, which unfortunately appear strongly affected by uncertainties of the surface layers. In order to suppress those uncertainties, we introdue the use of a suitable procedure to be adopted in the helioseismic inversions of high-degree modes and show new results on the properties of the Sun's interior.

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