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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 5.

Loop geometry approximation. The left panel shows the comparison between the spatial variation of BLoS over the green traced path of panel (e) of Figure 1. The green shaded area represents the maximum error commited when ignoring the projection of the horizontal magnetic field into the value of BLoS. The middle panel shows the variation of the height of the loop over the total distance along the loop. The red star marks the location of the apex. The right panel plots the projected outline of the loop over an SDO/AIA 17.1 nm passband image of the main loop structure emanating from the pore and connecting it to the nearby sunspot. The color reflects the height of the loop, and the red star marks the location of the apex.

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