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Quantifying Turbulence as Captured in the Inner Corona in White-light Total Solar Eclipse Images

  • Authors: Zachary Bailey, Shadia Rifai Habbal, Riddhi Bandyopadhyay, Shaheda Begum Shaik

Zachary Bailey et al 2026 The Astrophysical Journal Letters 1002 .

  • Provider: AAS Journals

Caption: Figure 3.

Physical sizes within the three subregions shown in Figure 2. Here, we show four different sizes of boxes, the full region size at 2.7 × 105 km (k = 2.3 × 10−5 km−1), half the region size at 1.4 × 105 km (k = 4.8 × 10−5 km−1), and boxes near the limits of our spectral slope measurements at 6.3 × 104 km (k = 10−4 km−1), and 6.3 × 103 km (k = 10−3 km−1). We mark the two smallest boxes with their size in k-space as they are representative of the range of sizes we are probing in our linear fits.

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