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TEMPORAL EVOLUTION OF MULTIPLE EVAPORATING RIBBON SOURCES IN A SOLAR FLARE

  • Authors: D. R. Graham, and G. Cauzzi

2015 The Astrophysical Journal Letters 807 L22.

  • Provider: AAS Journals

Caption: Figure 1.

IRIS 1400 Å slit-jaw images (SJI) showing the evolution of the flaring region. The full field of view is seen in the larger left panel, and the four smaller panels display the ribbon evolution in the central area (white box) during the impulsive phase. Note that the 1400 Å SJI images saturate at times, but the spectra analyzed remain below this level.

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