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3D Magnetic Structures of Ellerman Bombs Revealed by SUNRISE III/SCIP

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

Yusuke Kawabata et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 1.

Examples of Stokes I maps in the continuum (averaged over 8474.0–8475.5 Å), the K I 7698 Å line core, and the Ca II 8542 Å line core, acquired with SUNRISE III/SCIP. Panels (a)–(c) show the second scan (10:17–10:29 UT), in which Event 2 was identified; the green rectangle in each top-row panel marks the field of view of Event 2. Panels (d)–(f) show the 17th scan (13:16–13:28 UT), in which Event 1 was identified; the yellow rectangle in each bottom-row panel marks the field of view of Event 1. The white dashed rectangle (visible near the upper-left of each panel) marks the quiet-Sun reference region used for computing the mean quiet-Sun Stokes I profile. The x- and y-axes are given in arcsec and correspond to the scanning and slit directions, respectively. An animation of this figure, covering the 20 completed scans (10:05–14:04 UT), is available.

(An animation of this figure is available in the online article.)

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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