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Flares Producing Well-organized Post-flare Arcades (Slinkies) Have Early Precursors

  • Authors: M. P. Ryutova, Z. Frank, H. Hagenaar, and T. Berger

Ryutova et al. 2011 The Astrophysical Journal 733 125.

  • Provider: AAS Journals

Caption: Figure 10.

Evolution of coronal loops for different initial conditions. Left panel: the μ > 0 regime corresponds to Poincaré limit cycle; coronal loops with the initial current amplitude higher than critical value, I 0/ I cr > 2, quickly approach the quasi-stable state impulsively releasing the excess of energy. Loops with the initial current amplitude I 0/ I cr < 2 gradually gain energy. Right panel: at μ < 0 loops with the initial current amplitude, I 0/ I cr > 2, show the explosive growth of currents; higher are the initial currents, shorter is the "explosive" time (major flare). Loops with the initial current I 0/ I cr < 2 are in a gradually decaying state (after Ryutova 2006). Inset shows stabilization of explosive phase and formation of long-living self-organized state characterized by μ sime 0 (cf. GOES X-ray plot in Figure  10).

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