The Sun's meridional circulation and interior magnetic field
Jeremy McCaslin, CU Boulder.
Advisor: Pascale Garaud, UCSC
Abstract: This effort seeks to explore the fundamental dynamics of a solar model such as that of Gough and McIntyre. Interaction of meridional flows downwelling from the convection zone into the radiative interior with a confined interior magnetic field are explored through a simple Cartesian model and linearized governing equations. Semi-analytical solutions reveal understanding of dynamics that have implications for magnetic confinement and gyroscopic pumping, as well as for stellar mixing.
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