Issue |
A&A
Volume 566, June 2014
|
|
---|---|---|
Article Number | A148 | |
Number of page(s) | 18 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361/201323097 | |
Published online | 30 June 2014 |
Online material
Appendix A: Additional figures
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Fig. A.1
Hα line profiles (solid lines) from the kernel K1 together with a reference profile (black dotted lines) taken from a quiet region at the bottom-left corner of the field of view. The line centre λ0 is denoted by dashed lines. FWHM of those profiles that can fitted by a single-Gaussian function are noted accordingly, and their fitting Gaussian profiles (orange dotted lines) are overplotted. |
Open with DEXTER |
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Fig. A.2
As Fig. A.1, the evolution of Hα line profiles from the kernel K2. |
Open with DEXTER |
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Fig. A.3
As Fig. A.1, the evolution of Hα line profiles from the kernel K3. |
Open with DEXTER |
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Fig. A.4
Evolution of the flare seen in six different channels. Top-left: Hα – 0.8 Å; top-middle: Hα + 0.8 Å; top-right: AIA 304 Å; bottom-left: AIA 171 Å; bottom-middle: AIA 193 Å; bottom-right: AIA 94 Å. (The animation is available online.) |
Open with DEXTER |
Movie of Fig. A.4
Download Video: Formats: mp4 (3.3 MB) | webm (859.5 KB) | ogg (6.5 MB) | Original mov (6.3 MB)
© ESO, 2014
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