Image Details

Choose export citation format:

Large resolution
Export to PDF PPT Format

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. 8.

Multiple‐loop models for (a) Δt = 51 s and (b) Δt = 17 s. Top panels: Diagrams of flare heat input into the nine loops. Middle panels: Time variations of the maximum temperature. Bottom panels: Light curve of the Ca XIX w line. The dash‐dotted, dashed, and thin solid lines correspond to directly heated (Iheat), evaporated (Ievp), and accumulated (Iacm) components, respectively. The thick solid line is the sum of these components. The vertical dotted lines mark times when the heat input starts in individual loops, and the vertical dashed line represents when the final heat input terminates.

Other Images in This Article

Show More

Copyright and Terms & Conditions