Rise times of horizontal magnetic flux tubes in the convection zone of the sun
Solutions of the equations describing the motion of a straight horizontal magnetic flux tube in the convection zone of the sun including inertial term and radiative exchange with the surroundings are presented. Cases where the tube is initially both in thermal or in mechanical equilibrium with the surroundings are considered. It is shown that the
Moreno-Insertis, F.
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6
1983