Current Helicity in Response to Coronal Mass Ejections
Zheng Sun, Ting Li, Xinkai Bian, Yijun Hou, Ioannis Kontogiannis, Ziqi Wu

TL;DR
This study combines 3D magnetohydrodynamic modeling and observational data to identify a current helicity reversal pattern associated with coronal mass ejections, enhancing understanding and potential prediction of solar eruptions.
Contribution
It reveals a novel helicity reversal pattern linked to CMEs, supported by simulations and observations, improving insight into eruption mechanisms and forecasting.
Findings
58% of cases showed pre-eruption helicity decrease
92% exhibited post-eruption helicity increase
Helicity pattern correlates with current redistribution and flare ribbon separation
Abstract
Coronal mass ejections (CMEs), powerful solar eruptions with massive plasma ejected into the interplanetary space, are caused by the release of the magnetic free enengy stored in coronal electric currents. Photospheric current helicity, defined as the integral of the product of vertical electric current density and vertical magnetic field (), serves as a key parameter in understanding the eruptions. Using a 3D magnetohydrodynamic model, we identify a current helicity reversal pattern associated with the eruption: a pre-eruption decrease and a post-eruption increase. This helicity reversal is attributed to the redistribution of electric currents: before the eruption, currents concentrate toward the polarity inversion line (PIL); after the eruption they move away from the PIL, consistent with the flare ribbon separation, which is caused by the upward progression…
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Taxonomy
TopicsCardiac Arrest and Resuscitation
