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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 6.

Identification of the CS and field lines of the flux rope from different viewing angles. The CS (in white) traced from the temperature isosurface with a value ﹩{\mathrm{log}}_{10}T=6.6﹩ is shown in panel (a). The height of the CS isosurface (white) from the lower boundary is about 1.4R. The field lines passing through such sheets give the RC flux. The sigmoid field lines are shown in panels (b) and (c). The time in all these panels is at t = 27.32 hr.

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