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Acceleration and Expansion of a Coronal Mass Ejection in the High Corona: Role of Magnetic Reconnection

  • Authors: Bin Zhuang, Noé Lugaz, Manuela Temmer, Tingyu Gou, Nada Al-Haddad

Bin Zhuang et al 2022 The Astrophysical Journal 933 .

  • Provider: AAS Journals

Caption: Figure 4.

(a)–(c) Variation of the simulated proton speed, number density, and temperature of the solar wind with heliocentric distance, compared with the in situ observational data at 1 au (red asterisks). The horizontal dotted line indicates the distance of 6.5 R . (d) a drag in the drag-based model by using the speed of the CME front based on discrete height–time measurements (filled circle) and a quadratic fit to the height–time measurements (solid curve). (e) Ratio of ∣a drag∣ to a meas. The two dashed curves indicate the lower and upper uncertainties. The vertical dashed lines in panels (d) and (e) indicate the height at 6.5 R .

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