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First Apparent Speed Maps of Density Structures in the Solar Corona from 1.2 to 3 R⊙ Derived from Proba-3/ASPIICS White-light Images

  • Authors: Zac Bailey, Shadia R. Habbal, Miloslav Druckmüller, Colby Haggerty

Zac Bailey et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 3.

Panel (A): ridge-score plot for PA = 83﹩\mathop{.}\limits^{{\unicode{x000b0}}}﹩5 described in Section 3.2, with grouped detections overlaid. Colors represent the features’ median height, allowing one to distinguish the linked feature segments identified by the tracking algorithm. Panel (B): corresponding raw H vs. T plot for the 5 minute differenced data, with the fitted trajectory for each segment overlaid. Panels (C) and (D): radial apparent speed profiles of each segment as a function of time and radial distance from the Sun, respectively.

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