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Magnetohydrodynamic simulations of the ejection of a magnetic flux rope

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Figure

Fig. 1. Configuration of the magnetic field after 19 days of evolutionusing the model of Mackay & van Ballegooijen (2006a)
Fig. 3. Magnetic field configuration used as the initial condition in theMHD simulations of the erupting flux rope
Fig. 4. Radial component of the Lorentz Force on thecentre of the bipole atdashed black lines mark the contours of negative radial component ofthe Lorentz force at r − φ plane at the a) t = 0 τAlf and b) t = 23.20 τAlf
Fig.7e the blue and yellow magnetic field lines denote magneticfield lines that in the initial condition connect between the outeredges and central part of the LHS bipole
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