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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 2.

Examples of time series of 193 Å intensities (top) and corresponding probability density functions (PDFs; bottom) for single-pixel signals in the CH1 and QS1 regions. (Left) A pixel in the coronal hole; (right) a pixel in the neighboring quiet-Sun region. The mean, kurtosis and skewness of the PDFs are: 16.0, 3.12, 0.18 (CH); 81.9, 2.55, 0.32 (QS).

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