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Coronal Cavity Magnetic Fields Inferred by DKIST/CryoNIRSP

  • Authors: Elizabeth M. Wraback, Samaiyah Farid, Thomas A. Schad, Urszula Bąk-Stȩślicka, Giuliana de Toma, Yuhong Fan, Sarah E. Gibson, Mari Paz Miralles, Jie Zhang, Suman K. Dhakal

Elizabeth M. Wraback et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 4.

Panels (A)–(D) show the Stokes I, Q, U, and V spectra, respectively, along a single slit position for the 2025 August 8 cavity, based on the purple line through the cavity at 15″ in scanning direction, as shown in Figure 3(A). The cyan lines represent a single location on the slit (at 55″ along the slit), as shown in Panels (E)–(H), which include the corrected observed (black) and fitted (red) Stokes I, Q, U, and V profiles, respectively. Panel (E) includes the Gaussian profile for the coronal line emission (green). We indicate the line center as the vertical gray dashed lines.

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