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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 3.

Example of fitting the line core and line wing with the WFA. Here Bwing = ( −1460 ± 290)G (blue shaded area and blue points) and Bcore = ( −1100 ± 120)G (green shaded area and green points). The observed profile was taken from the inner penumbra of the sunspot.

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