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Observational Evidence of Vortex-driven Information Transfer in the Solar Atmosphere: Insights from SUNRISE III

  • Authors: Suzana S. A. Silva, Ioannis Dakanalis, Kostas Tziotziou, Azaymi L. Siu-Tapia, Shahin Jafarzadeh, Shivdev Singh Turkay, Viktor Fedun, 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, Valentín Martínez Pillet, H. N. Smitha, David Orozco Suárez, Bianca Grauf, Michael Carpenter, Alexander Bell, Francisco Javier Bailén, Julian Blanco Rodríguez, Juan Sebastián Castellanos Durán, Edvarda Harnes, Johannes Hoelken, Francisco A. Iglesias, Ryohtaroh T. Ishikawa, Yusuke Kawabata, Takuma Matsumoto, Takayoshi Oba, Hanna Strecker, Dušan Vukadinovic, Maria Balaguer Jiménez, Esteban Sanchis Kilders, Ignacio Torralbo, Christoph Kuckein

Suzana S. A. Silva et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure A1.

First column: synthetic Hβ core at t = 4280seconds with clockwise rotation of 10° h−1. The red square marks the subregion used to assess the impact of rotation on SPOD vortex detection. Second column: SPOD modes, which present the vortex signature, the “yin-yang” pattern as indicated by the thinner dashed line. The top row is the result of SPOD in the original data and the bottom row is the same for rotated data. Third column: same layout as the second column, but showing a less energetic SPOD mode, mode 9.

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