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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 4.

WFA results. The first and second panels show the BLoS maps around the pore for the first and second raster scans of SCIP, respectively. The colored circles mark the locations of the representative profiles shown in Figure 3, with matching colors between the two figures. The contours outline the largest contiguous regions where the condensations were observed. The field corresponds to the area inside the magenta rectangles of panels (b) and (c) of Figure 1. For clarity, smaller regions are not outlined. The right panel shows the distribution of BLoS for the pixels inside these contours that show spectral signatures of coronal-rain condensations.

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