Physics
Scientific paper
Sep 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...38....9m&link_type=abstract
Solar Physics, vol. 38, Sept. 1974, p. 9-13.
Physics
1
Convective Heat Transfer, Magnetic Flux, Solar Flux, Solar Temperature, Astronomical Models, Buoyancy, Internal Energy, Magnetic Effects, Neutrinos, Radiative Heat Transfer, Solar Corpuscular Radiation, Solar Interior, Solar Magnetic Field, Temperature Gradients, Velocity Measurement
Scientific paper
It is found that magnetic convection most probably operates inside the sun. The energy flux which it can carry is five to six orders of magnitude smaller than the total solar flux. The velocity with which magnetic flux rises from the interior of the sun towards the surface is measured. Under conditions where the entire stellar flux is carried by convection, the velocities of magnetic buoyancy are compared with the velocities of convective elements inside stars. Observation shows magnetic convection effects on the internal temperature structure of the sun to be small.
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