Jun 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.235..209f&link_type=abstract
In ESA Future Missions in Solar, Heliospheric and Space Plasma Physics p 209-217 (SEE N86-27330 18-12)
Physics
5
Helioseismology, Solar Oscillations, Solar Physics, Solar Spectra, Background Noise, Power Spectra, Soho Mission, Solar Gravitation, Solar Neutrinos
Scientific paper
The use of pressure modes to probe the deepest layers of the Sun's internal structure is discussed. It is noted that models featuring diffusion in the core satisfying neutrino flux are incompatible with helioseismological data. The contribution expected from gravity mode observations is assessed. The levels of solar and atmospheric noise encountered in Doppler and irradiance measurements are considered. Improvements in observational accuracy possible with SOHO project are reviewed.
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