The fine structure of solar granulation

Details The fine structure of solar granulation The fine structure of solar granulation

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991s%26w....30..724h&link_type=abstract

Sterne und Weltraum (ISSN 0039-1263), vol. 30, Dec. 1991, p. 724-728. In German.

Physics

Fine Structure, Line Shape, Solar Granulation, Photosphere, Solar Magnetic Field

Scientific paper

High resolution observations of the solar granulation fine structure are presented. Findings concerning the solar convection, line asymmetry, bisectors resulting from line profiles, velocity and intensity fluctuations, magnetic fields, and flow tubes are discussed. Bisectors exhibit a red asymmetry in the intergrain region and a blue asymmetry in the grain region. Photospheric plasma motions decrease with increasing height. Small flow tubes are brighter than the surrounding photosphere.

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