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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 2.

Evolution of the pore coalescence event in the field of view of the blue rectangle of Figure 1. Panels (a)–(c) show the evolution on the 17.1 nm channel of SDO/AIA. The cyan arrows of panel (a) indicate the location of the strongest brightenings during the end of the coalescence (see text). The white and red arrows reflect the approximate location of the loops leading to the condensations marked with the same colors in panel (c) of Figure 1. The green and blue paths of panel (c) reflect the same paths marked in panel (e) of Figure 1. Panels (d)–(f) show the evolution on the continuum of SDO/HMI. The black squares reflect the field of view of the IRIS slit-jaw images on the 283.2 nm passband, which are shown in panels (g)–(i).

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