TEMPORAL EVOLUTION OF MULTIPLE EVAPORATING RIBBON SOURCES IN A SOLAR FLARE
Authors: D. R. Graham, and G. Cauzzi
2015 The Astrophysical Journal Letters807L22.
Provider: AAS Journals
Caption: Figure 4.
SDO/AIA 131 Å images at two times during the impulsive phase, highlighting the geometry of the hot flare loops. The contours show the IRIS SJI 1400 Å 800DN level.