Magnetically Structured Oscillatory Power Along an Active-Region Transect in Near-UV Sunrise-III/SUSI Spectroscopy

arXiv:2606.14232 · astro-ph.SR · Submitted 2026-06-12 · Read on arXiv

Shahin Jafarzadeh, David B. Jess, Marco Stangalini, Peter H. Keys, Samuel D. T. Grant, Timothy J. Duckenfield, Glen Chambers, Sami K. Solanki, H. N. Smitha, Andreas Lagg, Achim Gandorfer, Alex Feller, Francisco A. Iglesias, Tino L. Riethmüller, Bianca Grauf, Johannes Hoelken, Yukio Katsukawa, Pietro Bernasconi, Thomas Berkefeld, Alberto Álvarez-Herrero, Masahito Kubo, David Orozco Suárez, Michael Carpenter, Alexander Bell, Valentín Martínez Pillet, Francisco Javier Bailén, Julian Blanco Rodríguez, Juan Sebastián Castellanos Durán, Edvarda Harnes, Ryohtaroh T. Ishikawa, Yusuke Kawabata, Takuma Matsumoto, Takayoshi Oba, Azaymi L. Siu-Tapia, Hanna Strecker, Dušan Vukadinović

astro-ph.SR

Submitted: 2026-06-12

Comments: Accepted for publication in The Astrophysical Journal Letters

Journal ref: The Astrophysical Journal Letters, 1005, L65 (2026)

DOI: 10.3847/2041-8213/ae7072

Code: https://github.com/WaLSAteam/WaLSAtools

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 25× in this paper · explained in 2 episodes
• Sunrise-III UV Spectropolarimeter and Imager — 3× in this paper
• Calibration — 2× in this paper · explained in 7 episodes
• Active Regions — 1× in this paper · explained in 1 episode
• Robustness — 1× in this paper · explained in 5 episodes
• Trace — 1× in this paper · explained in 2 episodes
• Wavelet Transform — 1× in this paper · explained in 2 episodes

Sources

• Sunrise III: The Wavefront Correction System
• Compendium solar spectrum formation

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