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Figure 1: A sample image pair from the Dutch Open Telescope (DOT). Left: G-band image. Right: co-temporal and co-spatial Ca II H image, clipped to improve contrast. The network is readily identified in the Ca II H image as regions with enhanced brightness. In the G-band image these areas contain many tiny bright points, often arranged in strings (filigree) within intergranular lanes. These are NBPs. Close inspection shows the presence of isolated IBPs in the internetwork regions. |
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Figure 2:
Example of a magnetic
patch, visualized by partial Ca II H images (x-y cutouts, top row),
the associated Ca II H x-t slices ( middle row), and the
corresponding x-t slices from the IBP map sequence ( bottom row).
The images shown here are a selection of the data at intervals of
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Figure 3: The temporal average of the Ca II H image sequence over its one-hour duration with the internetwork mask contours overlaid in white. The Ca II H image intensity was scaled logarithmically in order to show contrast in the internetwork. The internetwork mask is computed by taking a 50-pixel boxcar average and thresholding at the mean value. |
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Figure 4:
Integrated x-ycutout, and x-t and y-t slices corresponding to those in
Fig. 2 of the binary IBP map sequences for the
Ca II H ( left) and G band ( right), showing only those IBPs
that group into the central patch. Careful comparison with the
rightmost panel in the bottom row of Fig. 2 shows
that several IBPs present there are part of another patch, such as at
the leftmost edge of the cutout around
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Figure 5:
The average Ca II H image with IBPs
identified in the Ca II H sequence overlaid in white. The IBPs appear
to group in patches that outline edges of cell-like structures, such as
around
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Figure 6: Histograms of IBP lifetimes. Solid: G-band IBP lifetimes. Dotted: Ca II H IBP lifetimes. IBPs with lifetimes shorter than 4 time steps (80 s) are rejected by our processing. |
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