Issue |
A&A
Volume 531, July 2011
|
|
---|---|---|
Article Number | A42 | |
Number of page(s) | 15 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361/201015879 | |
Published online | 08 June 2011 |
Online material
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Fig. 3
Same as for Fig. 2 but for 2007 May 19 STEREO-B. |
Open with DEXTER |
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Fig. 4
Same as for Fig. 2 but for 2007 Dec. 07 STEREO-A. |
Open with DEXTER |
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Fig. 5
Same as for Fig. 2 but for 2007 Dec. 07 STEREO-B. |
Open with DEXTER |
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Fig. 6
Same as for Fig. 2 but for 2009 Feb. 12 STEREO-B. |
Open with DEXTER |
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Fig. 7
Same as for Fig. 2 but for 2009 Feb. 13 STEREO-B. |
Open with DEXTER |
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Fig. 8
Left panel: PBD image with arc sector over-plotted. Right panel: intensity profile across arc sector. The intensity profile at a given distance corresponds to the mean intensity across the arc sector at that distance. This is then fitted using a Gaussian model and repeated for the next image. The vertical lines in the right-hand plot and arc lines in the left-hand plot correspond to the 2σ limits of the Gaussian fit. The associated movie (15879_mov.mpeg) shows the procedure used to build these diagrams. |
Open with DEXTER |
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Fig. 10
Same as Fig. 9 but for the event on 2007 Dec. 07. |
Open with DEXTER |
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Fig. 11
Same as Fig. 9 but for the events on 2009 Feb. 12 (top) and 2009 Feb. 13 (bottom), both showing STEREO-B data. |
Open with DEXTER |
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Fig. 13
Same as for Fig. 12 but showing the event on 2007 Dec. 07. |
Open with DEXTER |
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Fig. 14
Similar to Fig. 12, now only showing STEREO-B data for the event on 2009 Feb. 12. |
Open with DEXTER |
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Fig. 15
Similar to Fig. 12, now only showing STEREO-B data for the event on 2009 Feb. 13. |
Open with DEXTER |
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Fig. 17
Same as for Fig. 16 but for the event of 2007 December 07. |
Open with DEXTER |
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Fig. 18
Similar to Fig. 16 but showing the STEREO-B data from the events of 2009 February 12 (left) and 2009 February 13 (right). |
Open with DEXTER |
© ESO, 2011
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