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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 4.

Results of the WFA applied to Event 1. The red and cyan contours on the WFA maps are the same as those in Figure 2, indicating the intensity enhancements in the Ca II red wing and Ca II blue wing (panels (e) and (f) of Figure 2), respectively. The magenta line is oriented so as to cross the two opposite-polarity patches of the photospheric LOS magnetic field (e.g., panel (d)). The 1D spatial profiles of the line-of-sight magnetic field along the magenta line are displayed in panels (f) and (g). The spatial coordinates are given in arcsec and correspond to those of Figure 1.

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