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Multithermal Condensations Driven by Pore Coalescence Observed with Sunrise III

  • Authors: Matheus Kriginsky, Adur Pastor Yabar, Ana Belén Griñón-Marín, Jorrit Leenaarts, Jaime de la Cruz Rodríguez, 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, Hirohisa Hara, Toshifumi Shimizu, Takayoshi Oba, Francisco Javier Bailén, Julian Blanco Rodríguez, Juan Sebastián Castellanos Durán, Edvarda Harnes, Johannes Hoelken, Francisco A. Iglesias, Ryohtaroh T. Ishikawa, Yusuke Kawabata, Takuma Matsumoto, Azaymi L. Siu-Tapia, Hanna Strecker, Dušan Vukadinović

Matheus Kriginsky et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure A1.

Representative Stokes I and V profiles for pixels where the coronal-rain component was detected. The first two columns correspond to locations along the green path traced in panel (e) of Figure 1, and the coloring of the spectra identifies the location of each pixel along that path, matching the horizontal marks in panels (f) and (g) of Figure 1. The same system is followed in the rightmost two columns, in that case for the blue path shown in panel (e) of Figure 1. The spectra are normalized by the continuum (Ic).

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