Mathematics – Logic
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220....3c&link_type=abstract
In ESA The Hydromagnetics of the Sun p 3-12 (SEE N85-25091 14-92)
Mathematics
Logic
2
Helioseismology, Solar Oscillations, Stellar Cores, Solar Interior, Solar Rotation, Stellar Structure, Sun
Scientific paper
The properties of linear, adiabatic solar oscillations are described. Use of helioseismological data to study solar structure is outlined. Internal solar rotation is reviewed. The physics determining the oscillation frequencies is sufficiently simple that a very detailed comparison between observations and theory is possible. This provides tight constraints on the structure of the solar interior, as well as measurements of the variation of the solar rotation with depth.
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