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Magnetoacoustic Portals in Quiet-Sun Fluxtubes Revealed by Chromospheric Spectropolarimetry with SUNRISE III/SCIP

  • Authors: Takayoshi Oba, Yukio Katsukawa, Masahito Kubo, Yusuke Kawabata, Takuma Matsumoto, Ryohtaroh T. Ishikawa, Yoshihiro Naito, Toshifumi Shimizu, Hirohisa Hara, Fumihiro Uraguchi, Toshihiro Tsuzuki, Kazuya Shinoda, Tomonori Tamura, Yoshinori Suematsu, Jose Carlos del Toro Iniesta, David Orozco Suárez, Maria Balaguer Jiménez, Azaymi L. Siu-Tapia, Carlos Quintero Noda, Sami K. Solanki, Andreas Lagg, Achim Gandorfer, Pietro Bernasconi, Thomas Berkefeld, Alex Feller, Tino L. Riethmüller, Alberto Álvarez-Herrero, H. N. Smitha, Bianca Grauf, Michael Carpenter, Alexander Bell, Valentín Martínez Pillet, Francisco Javier Bailén, Julian Blanco Rodríguez, Juan Sebastián Castellanos Durán, Edvarda Harnes, Johannes Hölken, Francisco A. Iglesias, Hanna Strecker, Dušan Vukadinović

Takayoshi Oba et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 2.

Panel (a) and (b): two-dimensional distributions of the LOS magnetic field strength observed by TuMag at 03:41:11 and 04:03:03, respectively. The white horizontal line indicates the SCIP slit position. The uniform gray region on the right corresponds to areas not covered by the TuMag observations, where zero values are padded for display purposes. Panels (c) and (d): LOS magnetic field strength along the SCIP slit for the intervals 03:40:52–03:48:31 and 03:48:33–04:04:31, respectively. BFe I 8468, BCa II 8498, and BCa II 8542 are shown in black, green, and blue, respectively. The gray dashed line indicates 0 G. Panel (e) and (f): yt diagrams of vFe I 8468 and vCa II 8542. Panel (g): yt diagram of ICa II 8542. The quantities in panels (e)–(g) show components with phase speeds exceeding 7 km s−1. The two dashed lines in panels (e)–(g) indicate the locations from which the λt diagrams in Figure 3 were extracted.

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