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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. 4.

Top: Time variations of centroid shift (Δλ) and width (δλ) of the Ca XIX w line profiles (case A). The vertical dotted lines mark when each phase starts, and the vertical dashed line represents the time when heat input terminates. Bottom: Δλ‐δλ diagram. The arrows indicate the direction of time evolution. Loop orientations are θ = 0° (thick solid line), θ = 45° and ω = 0° (dotdashed line), and θ = 90° and ω = 90° (thin solid line).

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