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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 3.

Mg II intensity spacetime map (inverted B/W color table) with overlays of Mg II downflows at the 30% bisector level at 15 and 30 ﹩\mathrm{km}\ {{\rm{s}}}^{-1}﹩ (red contours). The Fe XXI upflow velocities above 270, 200, and 100 ﹩\mathrm{km}\ {{\rm{s}}}^{-1}﹩ are indicated with yellow, dark blue, and light blue crosses, respectively.

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