The fine structure of the quiet sun

Details The fine structure of the quiet sun The fine structure of the quiet sun

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph..100..237m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 100, Oct. 1985, p. 237-255.

Physics

72

Fine Structure, Solar Flux Density, Solar Granulation, Stellar Models, Brightness Distribution, Line Shape, Magnetic Flux, Photosphere, Solar Cycles, Solar Magnetic Field, Stellar Evolution

Scientific paper

The observed properties of the small-scale features visible in the quiet photosphere - the granulation, of convective origin, and the network bright points, associated with kG magnetic fields - are described. The known properties of the magnetic flux tubes associated with network bright points are also presented. Empirical models derived from the observations are discussed, as well as a few theoretical models of particular importance for the understanding of the origin of the small-scale features of the quiet photosphere. Finally, the observational evidences showing that the structure of the granulation and of the photospheric network are varying over the solar cycle are reported.

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