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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 3.

Estimated LOS magnetic field in the 2025 August 8 (top row) and 2025 October 5 (bottom row) cavities and their embedded prominences, masked to show only 3σ significant observations (first column). The second column shows the signed red-wing amplitude of the antisymmetric Stokes V profile. Each plot shows the egg fits to the cavity, for context. The purple lines represent the slit positions shown in Figures 4 and 5 panels (A)–(D), respectively. The cyan boxes represent the location of the spectra shown in Figures 4 and 5 panels (E)–(H), respectively. For the 2025 October 5 cavity, we outline the prominence in green based on the continuum signal in the Fe XIII observation.

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