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arXiv · 2607.26353

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

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
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Abstract

The balloon-borne stratospheric solar observatory Sunrise III successfully completed 6.5 days of observations in July 2024. One of its focal-plane instruments, the Sunrise Chromospheric Infrared spectroPolarimeter (SCIP), is a slit-scanning spectropolarimeter that simultaneously measures full Stokes profiles of multiple spectral lines in the 850 nm and 770 nm bands. SCIP obtained an unprecedented data set of a quiet-sun region near disk center, covering a $58'' \times 58''$ field of view. With an integration time of 10 s per slit position, the scan was completed in 107 minutes without interruption, achieving remarkably stable polarimetric precision of 0.03-0.04% (1$\sigma$) of the continuum level. The multi-wavelength SCIP observations reveal that the chromospheric line-of-sight (LOS) magnetic field exhibits thread-like, elongated structures over the internetwork regions, with no obvious photospheric counterpart directly below. These threads are typically narrower than $1''$ and are embedded within the canopy fields extending from the network regions. Their LOS field strengths derived from the weak-field approximation are typically 10-20 G weaker than the surrounding canopy. In particularly clear cases, the magnetic polarity of the threads is opposite to that of the adjacent canopy. These findings suggest that the canopy field is not simply an expanding structure originating from network regions, but instead has a complex three-dimensional configuration containing numerous localized substructures. These observations provide new constraints on the quiet-sun magnetic topology from the photosphere to the chromosphere.

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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. 2026-07-28. Three-dimensional Magnetic Field Structure of a Quiet-Sun Region Revealed by Sunrise III/SCIP. https://doi.org/10.3847/2041-8213/ae909b

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