Helioseismological inverse problem: Diagnostics of the structure of the lower solar atmosphere

Details Helioseismological inverse problem: Diagnostics of the structure of the lower solar atmosphere Helioseismological inverse problem: Diagnostics of the structure of the lower solar atmosphere

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..487b&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 487-491 (SEE N89-25819 19-92)

Computer Science

Sound

13

Helioseismology, Solar Atmosphere, Sound Waves, Stellar Structure, Acoustic Properties, Phase Shift, Solar Oscillations, Wave Reflection

Scientific paper

The 5 min solar oscillation frequencies were used to obtain information about the phase shift corresponding to the reflection of the internal acoustic waves from the outer solar layers. The results of the reconstruction of the frequency dependence of the phase shift from the experimental data are described. This information provides an efficient seismic diagnostic of the structure of the outer regions of the convection zone and lower solar atmosphere. The method of direct computation of frequency dependence of the phase shift for a solar envelope model is described.

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