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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. 6.

Light curve of the Ca XIX w line. Flare heating flux is fixed at F0 (=5.4 × 109 ergs cm−2 s−1) for cases A and B, and at 5F0 for cases C, D, and E. The dash‐dotted, dashed, and thin solid lines correspond to directly heated (Iheat), evaporated (Ievp), and accumulated (Iacm) plasma components, respectively. The thick solid line is the sum of these components. The dotted line is the maximum temperature at the apex. The vertical dotted line marks when each phase starts, and the vertical dashed line represents when the heat input terminates. Note the various vertical scales.

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