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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. 12.

Time evolution of VDEM profiles for two multiple‐loop models: (a) case ﹩\mathrm{A}\,^{\prime }_{1}﹩ and (b) case ﹩\mathrm{B}\,^{\prime }_{1}﹩ (θ = 0°). The VDEM is normalized to unit loop cross‐sectional area and has the units of ergs s−1 cm−2 (km s−1)−1. The velocity space resolution (Δvls) is set to be 3 km s−1 (which is less than ~5 km s−1, the wavelength bin size of the Yohkoh/BCS Ca XIX channel).

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