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Magnetic Rayleigh–Taylor Interchange Shapes Chiral Barbs in Solar Prominences

  • Authors: Hongyang Luo, Yuhong Fan

Hongyang Luo and Yuhong Fan 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure D1.

(a) Radial-velocity keogram along a fixed line aligned with the prominence spine near its lower boundary. Red and blue indicate upflows and downflows. (b) Spatial Fourier power of the velocity in (a), normalized to the maximum over the full map. The cyan curve marks the peak at each time within the displayed wavenumber range.

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