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Magnetically Structured Oscillatory Power along an Active-region Transect in Near-UV SUNRISE III/SUSI Spectroscopy

  • Authors: 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

Shahin Jafarzadeh et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 2.

Stacked, line-resolved band-integrated RGWS power along the slit for three frequency ranges (left to right): 2–4 mHz, 4–6 mHz, and 6–12 mHz. Rows correspond to the 30 selected spectral line diagnostics (ordered by increasing wavelength). Each row is normalized to its own maximum along the slit, so the color scale highlights where along the slit each line concentrates power within the given band rather than comparing absolute power between different lines. A slit-jaw context strip above each panel marks the slit position and facilitates identification of umbra, penumbra, plage, and pore segments.

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