Production of the Solar Magnetic Fine-Structure by Convection

Details Production of the Solar Magnetic Fine-Structure by Convection Production of the Solar Magnetic Fine-Structure by Convection

Oct 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970soph...14..274w&link_type=abstract

Solar Physics, Volume 14, Issue 2, pp.274-279

Physics

5

Scientific paper

Motion of the gas in supergranular convection will produce twisted flux
tubes. A simple energy calculation shows that for a wide variety of
assumptions a tube of field strength ˜ 100 G will be given about
one twist and will have a diameter ˜ 1000 2000 km. This agrees
with observations of magnetic fine-structure on the sun.

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