Titlebook: Solar Phenomena in Stars and Stellar Systems; Proceedings of the N Roger M. Bonnet,Andrea K. Dupree Conference proceedings 1981 D. Reidel P

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The Sun as a Star: Solar Phenomena and Stellar Applicationsone of the best ways to infer the earlier history of the Sun, as well as its future history. In this review we shall concentrate on phenomena common to the Sun and solar-type (main sequence) stars with different fundamental properties such as mass, age, and rotation.

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Cabg318

The Sun as a Star: Solar Phenomena and Stellar Applications as an astrophysical object, for its sameness to other stars suggests that in studying the Sun, we are studying at close hand common, rather than unusual stellar phenomena. Conversely, comparative study of the Sun and other solar-type stars is an invaluable tool for solar physics, for two reasons: F

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The Spontaneous Concentration of Magnetic Field in the Photosphere of the Sunnewly emerging active regions the separate tubes cluster together to produce the sunspot phenomenon, with the magnetic field compressed further, to 2–4 kilogauss. Magnetic fields are concentrated by compressive forces which must equal the magnetic pressure B./8π in the flux tubes. In the surface of

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Solar and Stellar Oscillationscurence, what kind of questions the theoretician asks to the observer and what kind of tools the latter is using to look for the answers, A selected review of the most striking results obtained in the last few years in solar seismology and the present status of their consequences on solar models is

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Implicit

Convection Zones in Sun and Stars38), devoted specifically to the problems of stellar convection, and that of London (Ontario) in 1979 (IAU Colloquium 51), which dealt more broadly with stellar turbulence. In both meetings, there was an active exchange between people respectively working in stellar and solar physics, much in the sp

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