Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mmsai..55..319s&link_type=abstract
(European Physical Society, Ministero della Pubblica Istruzione, and Universita di Catania, EPS Study Conference on Oscillations
Astronomy and Astrophysics
Astronomy
Convective Flow, Solar Magnetic Field, Solar Prominences, Solar Rotation, Dynamic Models, H Alpha Line, Stellar Models
Scientific paper
The systematic upward motions observed in filaments are presently considered in terms of a large scale convective flow, so that the converging or diverging direction of the subphotospheric flow is related to the magnetic pattern suggested by Kuperus and Raadu (1973) and Kippenhahn and Schlueter (1957). This scheme is tested by means of a method for the detection of the giant convection and its properties, through a differential rotation analysis that uses sunspots, faculae and filaments as outliners. The systematic latitudinal motions obtained in the preliminary results indicate the presence of large scale convection. The method may be used to establish a relationship between the magnetic pattern and the global convection.
Malherbe Jean-Marie
Mein E.
Ribes B.
Schmieder Brigitte
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