Fig. 6.

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Magnetic field lines taken from the global NLFFF evolutionary model that show the presence of a flux rope (FR1) along the PIL of the large AR complex that is located behind the east solar limb. The panels are plotted using the same coordinate frame as Fig. 5 and the day of the simulation is given in the bottom left of panel a. The blue (red) contours represent negative (positive) photospheric magnetic field. Panel a: entire solar disk as it would be viewed from the farside of the Sun from the L3 perspective with a central meridian longitude of 180° and representative field lines of FR1 (light blue). Panels b and c: close up of the flux rope and the axis of the flux rope in the y − z plane, respectively.
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