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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 8.

Additional examples of three quiet-Sun network elements identified within the SCIP field of view. The top row shows continuum intensity, the second row shows the inferred magnetic field strength, and the third and fourth rows show the magnetic inclination at ﹩\mathrm{log}\tau =0﹩ and ﹩\mathrm{log}\tau =-2.5﹩, respectively. All quantities are derived from the multiline inversions. Similar to the network element analyzed in detail throughout this work, each region exhibits a compact magnetic concentration surrounded by smaller-scale patches of differing magnetic inclination.

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