Figure 1 from Comparison of the Scaling Properties of EUV Intensity Fluctuations in Coronal Hole and Quiet-Sun Regions

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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 1.

Logarithm of the intensity (in DN) for three low-latitude coronal holes and adjacent QS regions in the 193 Å (top panels) and 171 Å (bottom panels) emission: CH1 (2017 April 16; left), CH2 (2017 April 21; middle), CH3 (2017 February 21; right). The boundaries denoted by the black line are specified at 45 DN, 55 DN, and 65 DN of the 193 Å intensity, respectively.

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