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Magnetic flux transport simulations : applications to solar and stellar magnetic fields

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Figure

Figure 1.1: Image showing the structure of the Sun from the inner core, through the radiative and convection zones, past
Figure 1.2: Image showing a 3-part CME taken from the LASCO C3 imager. Visible is the high density central core,surrounding low density cavity and leading CME front, all of which make up this CME’s structure.
Figure 2.3: Plots showing the Legendre polynomials. Graph (a) shows when l=1, (b) has l=2 and (c) has l=3
Figure 2.5: Images showing the spherical harmonics, when l = 2 and m is (a)0, (b)1 and (c)2
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Outline

MHD Equations Test Simulation Run Results Kitt Peak Synoptic Magnetogram Data Two Bipolar Active Regions Instant Day Simulation Simulated Synoptic Magnetograms Several Emerged Bipoles Future Work

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