Image Details

Choose export citation format:

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 4.

(a) LOS magnetic field strength, (b) line-core intensity, and (c) Doppler velocity along the green solid line in Figure 3. The horizontal axis represents the distance d along the cut, with zero corresponding to the left end of the green solid line. The typical 1σ uncertainty in the LOS field strength is ≈4.4 G (Appendix A.3). Definition of the Doppler velocity is provided in Appendix  A.1. The positive velocity corresponds to the redshift. The orange dashed line and cyan dashed–dotted line indicate the peak and valley positions of the chromospheric LOS magnetic field (manually identified), respectively.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse