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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 B1.

Spectral lines synthesized from RADYN flare atmospheres. Upper panels: Fe II 325.59 nm spectral lines synthesized from a grid of RADYN simulations, normalized to the continuum level. The colors index the temporal progression from 0 to 50 s in the model. Spectral indices (δ) and low-energy cutoffs (Ec) of the considered models are quoted. Lower panels are for the Fe II 329.58 nm spectral line.

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