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Expanding Magnetic Canopy Structure and Parasitic Polarities in a Quiet-Sun Network Element Observed by SUNRISE III/SCIP

  • Authors: Ryan J. Campbell, Carlos Quintero Noda, Mihalis Mathioudakis, Manuel Collados, Jack McFall, David B. Jess, Sami K. Solanki, Andreas Lagg, Achim Gandorfer, Jose Carlos del Toro Iniesta, Yukio Katsukawa, Pietro Bernasconi, Thomas Berkefeld, Alex Feller, Tino L. Riethmüller, Alberto Álvarez-Herrero, Masahito Kubo, H. N. Smitha, David Orozco Suárez, Bianca Grauf, Michael Carpenter, Alexander Bell, Valentín Martínez Pillet, Francisco Javier Bailén, Julian Blanco Rodríguez, Juan Sebastián Castellanos Durán, Edvarda Harnes, Johannes Hölken, Francisco A. Iglesias, Ryohtaroh T. Ishikawa, Yusuke Kawabata, Takuma Matsumoto, Takayoshi Oba, Azaymi L. Siu-Tapia, Hanna Strecker, Dušan Vukadinović, Hirohisa Hara, Toshifumi Shimizu

Ryan J. Campbell et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 5.

Example Stokes profile fits for a boundary pixel identified as exhibiting a three-lobed Stokes V profile in the Fe I 8468 Å line. The inversion reproduces the multilobed Stokes V signature in the Fe line, while the Ca lines remain two-lobed in Stokes V. The inferred stratification indicates that the observed asymmetry is consistent with strong LOS velocity (and magnetic) gradients.

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