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Multilobed Stokes V Profiles of the Fe I 407.17 nm Line Observed by SUNRISE III

  • Authors: Edvarda Harnes, H. N. Smitha, Andreas Lagg, Damien Przybylski, Alex Feller, Francisco A. Iglesias, Sami K. Solanki, Achim Gandorfer, Tino L. Riethmüller, Johannes Hölken, Juan Sebastián Castellanos Durán, Dušan Vukadinovic, Jose Carlos del Toro Iniesta, Yukio Katsukawa, Pietro Bernasconi, Thomas Berkefeld, Alberto Álvarez-Herrero, Masahito Kubo, David Orozco Suárez, Bianca Grauf, Michael Carpenter, Alexander Bell, Valentín Martínez Pillet, Francisco Javier Bailén, Julian Blanco Rodríguez, Ryohtaroh T. Ishikawa, Yusuke Kawabata, Takuma Matsumoto, Takayoshi Oba, Azaymi L. Siu-Tapia, Hanna Strecker

Edvarda Harnes et al 2026 The Astrophysical Journal Letters 1011 .

  • Provider: AAS Journals

Caption: Figure 4.

Results of the application of the WFA. Panel (a): LOS magnetic field strength retrieved from the core wavelengths. Panel (b): LOS magnetic field strength retrieved from the wing wavelengths. Panel (c): rms error from the fitted BLOS in the core to the samples, scaled with the magnitude of the retrieved LOS magnetic field. Panel (d): same as panel c, but for the wings. Panel (e): difference of the retrieved ∣BLOS∣ in the wings and the core. In all panels, the black contour outlines the outer edge of the penumbra, and the red lines outline the umbra. The markers correspond to the locations of the selected profiles in Figure 2.

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