Fig. 5 from Single and Multiple Solar Flare Loops: Hydrodynamics and Ca XIX Resonance Line Emission

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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. 5.

Same as Fig. 2 but for case B (τ_heat = 44 s < τ_c). Differences from case A appear after phase II. Note the various vertical scales of the line emission.

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