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Comparison of the Scaling Properties of EUV Intensity Fluctuations in Coronal Hole and Quiet-Sun Regions

  • Authors: Ana Cristina Cadavid, Mari Paz Miralles, and Kristine Romich

2019 The Astrophysical Journal 886 143.

  • Provider: AAS Journals

Caption: Figure 7.

Top panels: Hurst exponent maps for the 193 Å signals in each of the three coronal-hole regions (black contour) obtained using R/S analysis. This method is only valid for cases with H ≤ 1; at other sites H takes values greater than 1, which are not well defined. Middle panels: histogram (left) and PDF (right) of H values for the interior pixels in the three coronal holes. Bottom panes: average intensity images with H ∼ 1 pixels in red. The grayscale has been inverted to better visualize these pixels.

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