Fig. 7 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. 7.

Peak value of I_acm and I_evp as functions of the flare heating duration τ_heat. Here the flare heating flux is fixed at 5F₀. The vertical dotted line represents the time τ_c, which is 29 s under the model conditions. C, D, and E correspond to the results of cases C, D, and E, respectively.

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