Search for giant elements of convection with the aid of magnetic tracers

Details Search for giant elements of convection with the aid of magnetic tracers Search for giant elements of convection with the aid of magnetic tracers

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987baicz..38...92b&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 38, no. 2, 1987, p. 92-101.

Mathematics

Logic

25

Convection, Magnetic Field Configurations, Magnetic Flux, Solar Rotation, Flow Distribution, H Alpha Line, Meridional Flow, Solar Magnetic Field

Scientific paper

In this communication the author discusses once more the physical reality of typical morphological cellular-like features of the large-scale distribution of weak background magnetic fields measured with low resolution. He has established several characteristic behaviours concerning the dynamics of their development, of their relation to differential rotation, to the frequency and intensity of new magnetic flux sources. Their rotation as a whole, which is slower than the differential rotation of the upper photospheric layers, and their lifetimes speak in favour of their physical reality and their possible relation to giant elements of convection.

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