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The Evolution of the Reconnection Flux during the Eruption of Magnetic Flux Ropes

  • Authors: Samriddhi Sankar Maity, Piyali Chatterjee, Ranadeep Sarkar, Ijas S. Mytheen

Samriddhi Sankar Maity et al 2026 The Astrophysical Journal 1000 .

  • Provider: AAS Journals

Caption: Figure 5.

(a) Height–time profile of the core of the flux rope before and after the first eruption at t = 27.9 hr. The height is calculated by tracking the dark region (flux rope) in the central meridional plane. (b) Same as (a), but for the second eruption at t = 34.7 hr. Time evolution of velocity, (c)–(d), and acceleration, (e)–(f), for both eruptions in the simulation. The red (blue) circles are used to represent simulation data before (after) the eruption.

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