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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 2.

Multiwavelength signatures in the early phase of the flare. Disk-integrated GOES soft X-ray flux (black) and Fermi/GBM hard X-ray flux in three energy bins (shades of blue) are plotted as a function of time. The maroon-colored light curves are the early flare-related impulses that SUSI captured (same as the yellow and orange curves in Figure 1). In the inset, an ASO-S/HXI background-subtracted spectrogram (energy versus time) is shown along with an overlay of the time series of GOES X-ray flux (black). The two vertical dashed lines in the inset mark the temporal boundaries of the main plot.

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