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Delayed, Line-dependent Reorganization of Pore Oscillations Following a Compact C8.2 Flare Observed by SUNRISE III/SUSI

  • Authors: Shahin Jafarzadeh, David B. Jess, Marco Stangalini, Lyndsay Fletcher, Ryan O. Milligan, Paulo J. A. Simões, Peter H. Keys, Sami K. Solanki, H. N. Smitha, Andreas Lagg, Achim Gandorfer, Alex Feller, Francisco A. Iglesias, Tino L. Riethmüller, Bianca Grauf, Johannes Hoelken, Jose Carlos del Toro Iniesta, 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 1010 .

  • Provider: AAS Journals

Caption: Figure 2.

Direct multiline response to the flare, with the spectral lines ordered by their median peak enhancement within the strong-response region. For each line, the left-hand panel shows the pixel-by-pixel ratio ﹩{I}_{{\rm{peak}}}/{I}_{{\rm{pre}}}﹩. All ratio maps use the same color scale. The cyan contour marks the boundary of the same composite strong-response region in every map. The right-hand panel in each row shows the temporal evolution of the median ﹩I/{I}_{{\rm{pre}}}﹩ within this region. The background colors identify the preevent, flare, early postevent, and late postevent intervals, while the vertical dotted line marks the intensity peak at t = 1008.4 s. The first raster began at 21:40:51.5 UTC.

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