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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 1.

Lower atmospheric small-scale response in the pre- and impulsive phases of the flare. Left: SUSI slit-jaw image covering a footpoint region of the flare. The various colored boxes point to locations of flare ribbons. Right: normalized emission as a function of time, averaged over the corresponding colored boxes identified in the left panel. The gray curve is the background-subtracted ASO-S/HXI hard X-ray flux in the 26–34 keV energy range. In the inset, we show the zoomed-in view of the yellow and orange light curves.

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