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Origin of Small-scale Evaporation Flows Deep in the Chromosphere During a Solar Flare

  • Authors: L. P. Chitta, H. N. Smitha, Francisco A. Iglesias, Tino L. Riethmüller, Alex Feller, Wei Chen, Andreas Lagg, Achim Gandorfer, Johannes Hölken, Sami K. Solanki, Jose Carlos del Toro Iniesta, Yukio Katsukawa, Pietro Bernasconi, Thomas Berkefeld, Alberto Álvarez-Herrero, Masahito Kubo, David Orozco Suárez, Bianca Grauf, Michael Carpenter, Alexander Bell, Valentín Martínez Pillet, Francisco Javier Bailén, Julián Blanco Rodríguez, Juan Sebastián Castellanos Durán, Edvarda Harnes, Ryohtaroh T. Ishikawa, Yusuke Kawabata, Takuma Matsumoto, Takayoshi Oba, Azaymi L. Siu-Tapia, Hanna Strecker, Dušan Vukadinovic

L. P. Chitta et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure B2.

Spectral line formation with height. Contribution functions, normalized to the initial quiet-Sun values, as a function of height are plotted for the grid of RADYN simulations (upper panels: Fe II 325.59 nm line core; lower panels: Fe II 329.58 nm line core). The colors have the same meaning as in Figure B1.

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