Fig. 6.
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Heliospheric evolution of the flux rope size estimates σx and σy (top panel) and the y-x aspect ratio (bottom panel) for runs A2, A3, A4, A5, and A6, that is, increasing ɛ0. Lighter shades represent increasing parameter values. Run A3 is represented as a dash-dotted line. The light blue (orange) broad line represents the expected ‘kinematic’ trend along x (y).
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