On Deflection of Solar Coronal Mass Ejections by the Ambient Coronal Magnetic Field Configuration
Jingjing Wang, J. Todd Hoeksema, Siqing Liu

TL;DR
This study analyzes how the ambient coronal magnetic field influences the deflection of solar CMEs, finding that the magnetic field configuration, especially the heliospheric current sheet, plays a major role in CME trajectories.
Contribution
It provides a comprehensive analysis of 44 halo-CMEs, demonstrating the significant influence of magnetic field configuration on CME deflection, with improved agreement after excluding high-uncertainty cases.
Findings
80% of CMEs' deflections align with ambient magnetic field configurations.
71% of deflected CMEs are directed toward the heliospheric current sheet.
Agreement increases to 94% when high-uncertainty CMEs are excluded.
Abstract
Solar Coronal Mass Ejections (CMEs) are sometimes deflected during their propagation. This deflection may be the consequence of interaction between a CME and a coronal hole or the solar wind. We analyze 44 halo-CMEs whose deflection angle exceeds 90 degrees. The coronal magnetic field configuration is computed from daily synoptic maps of magnetic field from SOHO/MDI and SDO/HMI using a Potential Field Source Surface (PFSS) model. By comparing the ambient magnetic field configuration and the measured position angles (MPA) of the CMEs, we conclude that the deflection of 80% of the CMEs (35 of 44) are consistent with the ambient magnetic field configuration, agreeing with previous studies. Of these 35, 71% are deflected toward the heliospheric current sheet (HCS), and 29 degrees toward a pseudo-streamer (PS), the boundary between the same-polarity magnetic field regions. This implies that…
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