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Fig. 9
Structure of the coronal magnetic field lines with ⟨ ĝ2 ⟩ = −0.5 and ⟨ ĝ3 ⟩ = 1.6, and the corresponding HCS position projected on the source surface at 3.25 R⊙ for the interest period of observations between March 2007 and April 2008. Inwards magnetic field lines are plotted in red, outwards in blue.
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