Jun 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989qjras..30..125t&link_type=abstract
Royal Astronomical Society, Quarterly Journal (ISSN 0035-8738), vol. 30, June 1989, p. 125-161.
Other
4
Helioseismology, Solar Activity Effects, Solar Neutrinos, Stellar Evolution, Stellar Models, Late Stars, Solar Corona, Solar Flares, Solar Magnetic Field, Starspots, Stellar Rotation
Scientific paper
The structure and evolution of the sun and the physical processes acting in its interior and on the surface are discussed in a general overview of recent observational and theoretical investigations. The emphasis is on the information gained about the sun by observing other stars and vice versa. Topics addressed include sunspot migration patterns, solar cycles, the solar density and temperature distributions, the production and detection of solar neutrinos, and the possible role of weakly interacting massive particles. Consideration is given to the production of the solar magnetic field, its dominant role in controlling surface behavior, and correlations between surface phenomena and global stellar properties. Typical observational data are summarized in graphs.
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