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A Forest of Emission Lines Observed by Sunrise III/SUSI above the Solar Limb

  • Authors: Juan Sebastián Castellanos Durán, Francisco A. Iglesias, Sami K. Solanki, Andreas Lagg, Ivan Milic, H. N. Smitha, Dušan Vukadinović, Tino L. Riethmüller, Achim Gandorfer, Alex Feller, Julian Blanco Rodríguez, David Orozco Suárez, Yukio Katsukawa, Johannes Hölken, Jose Carlos del Toro Iniesta, Shihao Rao, Mariano Sanchez Toledo, Kunal Singh, Pietro Bernasconi, Thomas Berkefeld, Alberto Álvarez-Herrero, Masahito Kubo, Valentín Martínez Pillet, Bianca Grauf, Michael Carpenter, Alexander Bell, Hanna Strecker, Azaymi L. Siu-Tapia, Pablo Santamarina Guerrero, Yusuke Kawabata, Takuma Matsumoto, Ryohtaroh T. Ishikawa, Edvarda Harnes, Takayoshi Oba

Juan Sebastián Castellanos Durán et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 4.

Panel (a) shows the median line-core intensity as a function of limb distance for all lines within the studied wavelength range. The shaded area marks the 5th and 95th percentiles of the line-core intensity for a given height after the limb was straightened. The black line and its corresponding gray band are the limb profile obtained from the pseudocontinuum at 409.13 nm (see the shaded wavelength range in Figure 2). Profiles are color coded by the line depth normalized to the pseudocontinuum taken from the FTS spectrum at the disk center, where one is given for the strongest line, and zero represents the pseudocontinuum level (see inset color scale). (b) The same as in panel (a), but after subtracting the pseudocontinuum profile (i.e., the black line in panel (a)). The inset shows a close-up near the limb.

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