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Measuring the Expansion of Solar Magnetic Fields with Multiline Inversions from Sunrise III

  • Authors: Juan Carlos Trelles Arjona, María Jesús Martínez González, Christoph Kuckein, Sergio Javier González Manrique, Manuel Collados, 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 Vukadinovic, Hirohisa Hara, Toshifumi Shimizu

Juan Carlos Trelles Arjona et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 3.

Vector magnetic field inferred from the simultaneous multiline inversions. The columns correspond to five equally spaced optical depth layers from ﹩\mathrm{log}\tau =-0.5﹩ to –4.5. From top to bottom, the panels show the magnetic-field strength (B), inclination (γ), and azimuth (ϕ), respectively. The magnetic-field strength maps are normalized independently at each optical depth layer by the reference value Bscale, indicated above each panel. The red, green, and blue circles in the inclination maps indicate Pores 1, 2, and 3, respectively. No 180∘ azimuth disambiguation has been applied; the azimuth maps correspond directly to the values returned by the inversion. The sequence illustrates the spatially coherent evolution of the inferred magnetic-field vector across the sampled optical depth range.

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