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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 1.

Panel (a): LOS magnetogram taken by SDO/HMI at 03:41:08 on 2024 July 16th. The white square outlines the region covered by TuMag. The color scale is shared with the other magnetograms shown in panels (b) and (d). Panel (b): enlarged view of the LOS magnetogram in panel (a), rotated clockwise by 17.1 degrees so that the axes are aligned with those of SCIP and TuMag. The coordinates are relative values with respect to the southern end of the SCIP slit. Panel (c): SCIP-SJ image acquired at 03:40:52.537. The dashed white rectangular box indicates the overlapped region of the TuMag magnetogram (before phase-diversity reconstruction), corresponding to the full field of view in panels (b) and (d). Panel (d): coaligned LOS magnetograph by TuMag. The vertical white line is overlaid for reference to mark the SCIP-slit position, inferred by comparing the SCIP-SJ image in panel (c) with a TuMag intensity image (not shown).

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