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Understanding the Complex Morphology of a Coronal Mass Ejection. II. How Pre-eruptive Conditions Shape Coronal Mass Ejection Evolution

  • Authors: Abril Sahade, Cecilia Mac Cormack, Angelos Vourlidas, Teresa Nieves-Chinchilla, Cooper Downs, Clementina Sasso, Judith T. Karpen

Abril Sahade et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 3.

Solar wind data during October 26–31 provided by PSP, SolO, Wind, and STA, respectively. From top to bottom, we show the total magnetic field [nT], magnetic field component (RTN) [nT], solar wind velocity [km s−1], and density [cm−3]. Dashed gray vertical lines indicate the CME shock arrival.

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