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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 A1.

Response function, ﹩\hat{R}﹩, of Stokes V to Bz in the FALC atmosphere with a 1 kG vertical magnetic field computed with a perturbation of 10 G. The response function is normalized by its maximum value.

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