The effect of a magnetic field on individual convective cells

Details The effect of a magnetic field on individual convective cells The effect of a magnetic field on individual convective cells

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974pasau...2..267m&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 8th, Hobart, Australia, May 22-24, 1974.) Astronomical Society of Au

Astronomy and Astrophysics

Astronomy

Convective Heat Transfer, Magnetic Effects, Photosphere, Solar Granulation, Solar Magnetic Field, Astronomical Models, Benard Cells, Heat Flux, Solar Atmosphere, Sunspots

Scientific paper

The darkness of sunspots has been attributed to the inhibition of the normal solar convective processes by the presence of strong magnetic fields. An investigation is conducted of the structure of individual cells of the solar photospheric granulation pattern. A description is given of a situation in which the magnetic field is concentrated by the convective processes along the upper and lower cell boundaries. Under the conditions considered the actual individual cells would show a much stronger field present than the actual strength of the underlying unperturbed field.

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