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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 3.

SUSI observation centered at 407.0 nm, acquired during a small 8 minute long portion of the full spectral scan on 2024 July 14 (see SUNRISE ID 22_SPOT in Table 1). Upper panel: a single SJ image acquired at 17:16:26 UT, along with the cotemporal restored frame, separated by a black dashed line. The dashed white rectangle marks the approximate area scanned by the slit. Note that the slit, originally visible near the bottom of the white box, was removed using a Fourier filter. Middle panel: single wavelength point at 406.950 nm (see the green lines in Figure 4) of the raster scan, recorded from 17:08:42 to 17:17:01 UT. Versions before and after image restoration are separated by the diagonal black dashed line. The dashed blue line and red cross mark the cut locations used for the slit spectra and single spectrum shown in Figure 4, respectively. The pixel scales along the slit and scan directions are 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩0297 and 0﹩\mathop{.}\limits^{\unicode{x02033}}﹩0307, respectively. Note that the axes scale in the top and middle panels are different. Bottom panel: same as the middle panel but for the wavelength 406.351 nm.

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