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Joint Magneto-seismological and Polarimetric Inference of Coronal Magnetic Fields with uCoMP

  • Authors: Richard J. Morton, Samuel Skirvin

Richard J. Morton and Samuel Skirvin 2026 Research Notes of the AAS 10 .

  • Provider: AAS Journals

Caption: Figure 1.

(a) Spherical triangle geometry defined by ﹩\hat{R}﹩, ﹩\hat{B}﹩, ﹩\hat{k}﹩ with the wave propagation direction ψwave shown in the POS. The shown case is for ﹩{\sigma }_{0}^{2}\lt 0﹩ (when ﹩{\sigma }_{0}^{2}\gt 0﹩ the red and blue arrows would coincide). (b) Atomic alignment ﹩{\sigma }_{0}^{2}﹩ as a function of ne and Te for θB = 30° at r = 1.3 R, computed with pyCELP. The weak Te dependence supports treating temperature as a fixed parameter. (c) Concentration of Fe XIII 1074.7 nm emission from the POS in angular degrees (θobs − 90°). Computed from MAS thermodynamic models with pyCELP. Solid line: median e−1 length over all rays at a given projected height; shaded region: interquartile range. Emission is concentrated within ±20°–30° of the POS.

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