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Single and Multiple Solar Flare Loops: Hydrodynamics and Ca XIX Resonance Line Emission

  • Authors: Kuniko Hori, Takaaki Yokoyama, Takeo Kosugi, and Kazunari Shibata

Hori et al. 1998 The Astrophysical Journal 500 492.

  • Provider: AAS Journals

Caption: Fig. 10.

Schematic light curve of the Yohkoh/BCS Ca XIX channel flux during a flare. Expectations for distribution of evaporated and accumulated plasma components are shown for both the light curve (Ievp and Iacm) and the line profile (φevp and φacm). Cartoons at the bottom show a model of the flare heating process in multiple loops. The sizes of circles located at the individual loop apexes correspond to the total input energy.

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