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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 2.

Stokes I and V maps and sample profiles from the SUSI observation. Panel (a) shows the Stokes I averaged over the entire observed wavelength range around 401.1 nm. Panel (b) shows the intensity at the rest wavelength of the line. Panels (c) and (d) show V from the flank of the line core and the wing, respectively. Panels (e)–(g) show the Stokes I, ﹩\frac{\partial I}{\partial \lambda }﹩, and Stokes V for the example points marked in panels (a)–(d). The blue, orange, red, and brown circles in panels (a)–(d) mark the locations of the profiles of the corresponding color in panels (e)–(g). The black dashed profiles are from a reference point in a granule marked with the black square. The vertical dashed lines mark the wavelengths shown in panels (c) and (d), respectively.

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