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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 2.

Power spectrum analysis of subregions 11, 17, and 19 from Figure 1. Subregion 11 ia a closed-field region, subregion 17 is a mixed region, and subregion 19 is an open-field region. For each case, the figures are arranged as follows. (A) Zoomed-in view of the subregion. (B) The corresponding 2D power spectrum where the center corresponds to k = (0, 0) km−1. Axis labels for k and k are overlaid, with their lengths representing the anisotropy. (C) Smoothed 2D power spectrum with isobars (contours of equal power) overlaid to highlight anisotropy. (D) 1D power spectra for k (blue) and k (orange). Dashed lines show the fitted slopes for each direction, matching the color of their respective spectra. The regions used for the fits are shown between the vertical lines of the corresponding color.

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