In a 3D MHD simulation of a coronal hole, magnetic flux cancellation occurs along an internal polarity inversion line during eruptions and blowout jets, producing rising U-shaped field lines.
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Magnetic flux cancellation in a flux-emergence magnetohydrodynamics simulation of coronal hole eruptions and jets
In a 3D MHD simulation of a coronal hole, magnetic flux cancellation occurs along an internal polarity inversion line during eruptions and blowout jets, producing rising U-shaped field lines.