Free Access
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

thumbnail Fig. 3

Same as for Fig. 2 but for 2007 May 19 STEREO-B.

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thumbnail Fig. 4

Same as for Fig. 2 but for 2007 Dec. 07 STEREO-A.

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thumbnail Fig. 5

Same as for Fig. 2 but for 2007 Dec. 07 STEREO-B.

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thumbnail Fig. 6

Same as for Fig. 2 but for 2009 Feb. 12 STEREO-B.

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thumbnail Fig. 7

Same as for Fig. 2 but for 2009 Feb. 13 STEREO-B.

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thumbnail 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.

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thumbnail Fig. 10

Same as Fig. 9 but for the event on 2007 Dec. 07.

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thumbnail 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.

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thumbnail Fig. 13

Same as for Fig. 12 but showing the event on 2007 Dec. 07.

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thumbnail Fig. 14

Similar to Fig. 12, now only showing STEREO-B data for the event on 2009 Feb. 12.

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thumbnail Fig. 15

Similar to Fig. 12, now only showing STEREO-B data for the event on 2009 Feb. 13.

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thumbnail Fig. 17

Same as for Fig. 16 but for the event of 2007 December 07.

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thumbnail 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).

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© ESO, 2011

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