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Three-dimensional Magnetic Field Structure of a Quiet-Sun Region Revealed by SUNRISE III/SCIP

  • Authors: Masahito Kubo, Yukio Katsukawa, Yusuke Kawabata, Takayoshi Oba, Hirohisa Hara, Toshifumi Shimizu, Ryohtaroh T. Ishikawa, Takuma Matsumoto, Yoshihiro Naito, Fumihiro Uraguchi, Toshihiro Tsuzuki, Kazuya Shinoda, Tomonori Tamura, Yoshinori Suematsu, Jose Carlos del Toro Iniesta, David Orozco Suárez, Maria Balaguer Jiménez, 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, Azaymi L. Siu-Tapia, Hanna Strecker, Dušan Vukadinović, Patrick A. Ondratschek

Masahito Kubo et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 1.

(a) SDO/HMI full-disk LOS magnetogram (Gauss) at 05:38:53 UT on 2024 July 11. The green box indicates the FOV in panels (b) and (c). (b) Enlarged SDO/HMI magnetogram of the region in panel (a). Axes are defined with respect to the disk center along the X and Y directions. The cyan box marks the SCIP FOV. (c) SDO/AIA 171 Å image (DN) at 05:39:33 UT, with the same FOV as panel (b). Green arrow marks a stable dark coronal feature within the ROI2 FOV (see Section 3.3 for details).

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