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SUNRISE III: Instrument, Mission, Data, and First Results

  • Authors: Sami K. Solanki, H. N. Smitha, Andreas Lagg, Achim Gandorfer, Jose Carlos del Toro Iniesta, Yukio Katsukawa, Pietro Bernasconi, Thomas Berkefeld, Alex Feller, Tino L. Riethmüller, Alberto Álvarez-Herrero, Masahito Kubo, David Orozco Suárez, Bianca Grauf, Michael Carpenter, Alexander Bell, Valentín Martínez Pillet, Laurent Gizon, Francisco Javier Bailén, Julian Blanco Rodríguez, Juan Sebastián Castellanos Durán, Edvarda Harnes, Johannes Hoelken, Francisco A. Iglesias, Ryohtaroh T. Ishikawa, Yusuke Kawabata, Takuma Matsumoto, Takayoshi Oba, Kunal H. Singh, Azaymi L. Siu-Tapia, Hanna Strecker, Dušan Vukadinovic, Michiel van Noort, Maria Balaguer Jiménez, Esteban Sanchis Kilders, Ignacio Torralbo, Christoph Kuckein, Hirohisa Hara, Toshifumi Shimizu, Reiner Volkmer, Tobias Preis, Nour E. Raouafi, Angelos Vourlidas, Johann Hirzberger, Werner Deutsch, Dietmar Germerott, Klaus Heerlein, Martin Kolleck, Daniel Álvarez García, Antonio C. López Jiménez, Luis R. Bellot Rubio, José Miguel Morales-Fernández, Antonio Jesús Moreno Mantas, Beatriz Aparicio del Moral, Antonio Sánchez Gómez, Eduardo Bailón Martínez, Pablo Santamarina Guerrero, David Hernández Expósito, Angel Tobaruela, José Luis Gasent Blesa, Erich Schulze, Harry Eaton, Geoffrey Palo, Daniel Ayoub, Yoshihiro Naito, Carlos Quintero Noda, Fumihiro Uraguchi, Toshihiro Tsuzuki, Javier Piqueras Carreño

Sami K. Solanki et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 5.

Example TuMag observations obtained on 13 July 2024 during an M5.3-class flare in NOAA AR 13738, showing a frame close to the flare peak. The panels display, from left to right (1) the continuum intensity at +22.7 pm (+227 mÅ) from the Fe I 525.06 nm line, (2) the Mg I 517.26 nm line-core intensity, (3) Stokes V in the Fe I 525.06 nm line wing at −8 pm (−80 mÅ), and (4) Stokes V in the Mg I 517.26 nm line wing at −10 pm (−100 mÅ). All panels are normalized to the average quiet-Sun continuum intensity, IQS. The data have been reconstructed using wave front and PD techniques. Residual instrumental effects may still be present at this stage of the data reduction.

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